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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Phys.</journal-id>
<journal-title>Frontiers in Physics</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Phys.</abbrev-journal-title>
<issn pub-type="epub">2296-424X</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="publisher-id">877628</article-id>
<article-id pub-id-type="doi">10.3389/fphy.2022.877628</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Physics</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>Nematicity and Glassy Behavior Probed by Nuclear Magnetic Resonance in Iron-Based Superconductors</article-title>
<alt-title alt-title-type="left-running-head">Curro et al.</alt-title>
<alt-title alt-title-type="right-running-head">NMR and Nematicity</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Curro</surname>
<given-names>N. J.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1134182/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Kissikov</surname>
<given-names>T.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1709490/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Tanatar</surname>
<given-names>M. A.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Prozorov</surname>
<given-names>R.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1700579/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Bud&#x2019;ko</surname>
<given-names>S. L.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Canfield</surname>
<given-names>P. C.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group>
<aff id="aff1">
<sup>1</sup>
<institution>Department of Physics and Astronomy</institution>, <institution>University of California, Davis</institution>, <addr-line>Davis</addr-line>, <addr-line>CA</addr-line>, <country>United States</country>
</aff>
<aff id="aff2">
<sup>2</sup>
<institution>Ames Laboratory U.S. DOE and Department of Physics and Astronomy</institution>, <institution>Iowa State University</institution>, <addr-line>Ames</addr-line>, <addr-line>IA</addr-line>, <country>United States</country>
</aff>
<author-notes>
<fn fn-type="edited-by">
<p>
<bold>Edited by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1376670/overview">Laura Fanfarillo</ext-link>, International School for Advanced Studies (SISSA), Italy</p>
</fn>
<fn fn-type="edited-by">
<p>
<bold>Reviewed by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1687362/overview">Pietro Carretta</ext-link>, University of Pavia, Italy</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1688558/overview">Kenji Ishida</ext-link>, Kyoto University, Japan</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1690328/overview">Rui Zhou</ext-link>, Institute of Physics (CAS), China</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: N. J. Curro, <email>njcurro@ucdavis.edu</email>
</corresp>
<fn fn-type="other">
<p>This article was submitted to Condensed Matter Physics, a section of the journal Frontiers in Physics</p>
</fn>
</author-notes>
<pub-date pub-type="epub">
<day>14</day>
<month>04</month>
<year>2022</year>
</pub-date>
<pub-date pub-type="collection">
<year>2022</year>
</pub-date>
<volume>10</volume>
<elocation-id>877628</elocation-id>
<history>
<date date-type="received">
<day>16</day>
<month>02</month>
<year>2022</year>
</date>
<date date-type="accepted">
<day>21</day>
<month>03</month>
<year>2022</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2022 Curro, Kissikov, Tanatar, Prozorov, Bud&#x2019;ko and Canfield.</copyright-statement>
<copyright-year>2022</copyright-year>
<copyright-holder>Curro, Kissikov, Tanatar, Prozorov, Bud&#x2019;ko and Canfield</copyright-holder>
<license xlink:href="http://creativecommons.org/licenses/by/4.0/">
<p>This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.</p>
</license>
</permissions>
<abstract>
<p>Nuclear magnetic resonance provides a wealth of information about the magnetic and nematic degrees of freedom in the iron-based superconductors. A striking observation is that the spin lattice relaxation rate is inhomogeneous with a standard deviation that correlates with the nematic susceptibility. Moreover, the spin lattice relaxation is strongly affected by uniaxial strain, and in doped samples it depends sensitively upon the history of the applied strain. These observations suggest that quenched strain fields associated with doping atoms induce a nematic glass in the iron pnictide materials.</p>
</abstract>
<kwd-group>
<kwd>nuclear magnetic resonance</kwd>
<kwd>nematicity</kwd>
<kwd>uniaxial strain</kwd>
<kwd>glassy dynamics</kwd>
<kwd>spin lattice relaxation</kwd>
<kwd>quantum materials</kwd>
</kwd-group>
</article-meta>
</front>
<body>
<sec id="s1">
<title>1 Introduction</title>
<p>Electronic nematic order, in which low energy electronic degrees of freedom drive a crystal to spontaneously break discrete rotational symmetry without simultaneously breaking translational symmetry, has attracted broad interest in correlated electron physics [<xref ref-type="bibr" rid="B1">1</xref>]. Much of this interest stems from observations that unconventional superconductivity tends to emerge in materials exhibiting competing ground states with different broken symmetries, including nematic, charge, and/or spin density wave fluctuations [<xref ref-type="bibr" rid="B2">2</xref>&#x2013;<xref ref-type="bibr" rid="B6">6</xref>]. Measurements of the nematic susceptibility in the iron based superconductors indicated the presence of a putative nematic quantum critical point under the dome of superconductivity in these materials [<xref ref-type="bibr" rid="B7">7</xref>, <xref ref-type="bibr" rid="B8">8</xref>]. These observations have suggested a connection between quantum critical nematic fluctuations and the pairing mechanism for superconductivity [<xref ref-type="bibr" rid="B9">9</xref>&#x2013;<xref ref-type="bibr" rid="B13">13</xref>]. It is thus important to understand the nature of the nematic fluctuations and their relationship to the coexisting antiferromagnetism throughout the phase diagram.</p>
<p>Nuclear magnetic resonance (NMR) provides a wealth of information about both the magnetic and nematic degrees of freedom in the iron-based superconductors [<xref ref-type="bibr" rid="B14">14</xref>]. Studies under uniaxial strain offer an important new direction in thermodynamic phase space to explore the physics of nematicity. Such experiments can broadly be separated into those that probe the static properties of the magnetic and nematic order, and those that probe the dynamical properties. The latter set of experiments have yielded some important surprises, such as a change in the spin anisotropy as a function of strain [<xref ref-type="bibr" rid="B15">15</xref>], and the presence of dynamical inhomogeneity when the materials are doped [<xref ref-type="bibr" rid="B16">16</xref>]. Below we discuss how NMR probes these broken symmetries and their fluctuations, and summarize results of experiments under uniaxial strain, both in the undoped and doped materials. These observations are consistent with the emergence of a nematic glass in doped samples, possibly driven by the presence of random strain fields from quenched disorder.</p>
</sec>
<sec id="s2">
<title>2 Coupling to Nuclear Spins</title>
<p>The <sup>75</sup>As nuclei, with 100% abundance and spin <italic>I</italic> &#x3d; 3/2, are excellent sensors of both the nematic and magnetic degrees of freedom in the iron pnictide superconductors. <xref ref-type="fig" rid="F1">Figure 1</xref> shows the unit cell and indicates the hyperfine coupling between the As nuclei and the four nearest neighbor Fe electronic moments. The As also has a significant quadrupolar moment, <italic>Q</italic> &#x3d; 3.14 &#xd7; 10<sup>&#x2212;29</sup>&#xa0;m<sup>2</sup>, which couples to the surrounding electric field gradient (EFG) [<xref ref-type="bibr" rid="B17">17</xref>]. The hyperfine and quadrupolar couplings enable microscopic studies of both the magnetic and nematic susceptibilities of the <italic>electronic</italic> degrees of freedom.</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>
<bold>(A)</bold> BaFe<sub>2</sub>As<sub>2</sub> unit cell. Ba is cyan, Fe is brown and As is green. <bold>(B)</bold> The hyperfine field (green arrows) at the As sites in the antiferromagnetic state, with the Fe moments (red) oriented in the plane.</p>
</caption>
<graphic xlink:href="fphy-10-877628-g001.tif"/>
</fig>
<sec id="s2-1">
<title>2.1 Hyperfine Interaction</title>
<p>The hyperfine coupling is given by:<disp-formula id="e1">
<mml:math id="m1">
<mml:msub>
<mml:mrow>
<mml:mi mathvariant="script">H</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>h</mml:mi>
<mml:mi>y</mml:mi>
<mml:mi>p</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:munder>
<mml:mrow>
<mml:mo>&#x2211;</mml:mo>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>&#x2208;</mml:mo>
<mml:mi>n</mml:mi>
<mml:mo>.</mml:mo>
<mml:mi>n</mml:mi>
<mml:mo>.</mml:mo>
</mml:mrow>
</mml:munder>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mi mathvariant="bold">I</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">&#x302;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mo>&#x22c5;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi mathvariant="double-struck">A</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x22c5;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mi mathvariant="bold">S</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">&#x302;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>,</mml:mo>
</mml:math>
<label>(1)</label>
</disp-formula>where <inline-formula id="inf1">
<mml:math id="m2">
<mml:msub>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mi>I</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">&#x302;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
</mml:mrow>
</mml:msub>
</mml:math>
</inline-formula> are the nuclear spin operators, <inline-formula id="inf2">
<mml:math id="m3">
<mml:msub>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mi mathvariant="bold">S</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">&#x302;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
</mml:mrow>
</mml:msub>
</mml:math>
</inline-formula> are the Fe spins on the four nearest neighbors to the As nucleus, and the hyperfine coupling tensors, <inline-formula id="inf3">
<mml:math id="m4">
<mml:msub>
<mml:mrow>
<mml:mi mathvariant="double-struck">A</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
</mml:mrow>
</mml:msub>
</mml:math>
</inline-formula>, have dipolar symmetry [<xref ref-type="bibr" rid="B18">18</xref>, <xref ref-type="bibr" rid="B19">19</xref>]. In BaFe<sub>2</sub>As<sub>2</sub>, the eigenvalues of the tensor are <italic>A</italic>
<sub>
<italic>aa</italic>
</sub> &#x3d; <italic>A</italic>
<sub>
<italic>bb</italic>
</sub> &#x3d; 6.6&#xa0;kOe/<italic>&#x3bc;</italic>
<sub>
<italic>B</italic>
</sub>, and <italic>A</italic>
<sub>
<italic>cc</italic>
</sub> &#x3d; 4.7&#xa0;kOe/<italic>&#x3bc;</italic>
<sub>
<italic>B</italic>
</sub>, but these values depend on details of the electronic structure and can vary between compounds. They can change as a function of pressure or doping, but the general symmetry of the <inline-formula id="inf4">
<mml:math id="m5">
<mml:msub>
<mml:mrow>
<mml:mi mathvariant="double-struck">A</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
</mml:mrow>
</mml:msub>
</mml:math>
</inline-formula> does not. The magnitude of these values are greater than those for the direct dipole interaction, which reflects the electronic hybridization between the As 4<italic>p</italic> and Fe 3<italic>d</italic> orbitals. The tensor nature of this coupling gives rise to a hyperfine field <bold>H</bold>
<sub>
<italic>hf</italic>
</sub> &#x2225;<bold>c</bold> when the Fe moments lie in the <italic>ab</italic> plane, as illustrated in top row of <xref ref-type="fig" rid="F2">Figure 2</xref>. Alternatively, if the Fe moments ordered parallel to <bold>c</bold>, then <bold>H</bold>
<sub>
<italic>hf</italic>
</sub> lies in the plane, as shown in the middle row of <xref ref-type="fig" rid="F2">Figure 2</xref>.</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>The hyperfine field at the As site (green) for the four degenerate domains with in-plane Fe moments oriented parallel to the ordering vector (<italic>&#x3d5;</italic>
<sub>
<italic>xy</italic>
</sub> nematic order, upper row), with <italic>c</italic>-axis Fe moments (<italic>&#x3d5;</italic>
<sub>
<italic>zz</italic>
</sub> nematic order, middle row) and with in-plane moments oriented perpendicular to the ordering vector (<italic>&#x3d5;</italic>
<sub>
<italic>yx</italic>
</sub> nematic order, bottom row). Red and blue correspond to the two different nematic domains (positive and negative strains). Within each nematic domain, there are two different antiferromagnetic configurations.</p>
</caption>
<graphic xlink:href="fphy-10-877628-g002.tif"/>
</fig>
<p>Other magnetic orderings can be present in the pnictides, beyond the stripe-type spin density wave illustrated in <xref ref-type="fig" rid="F2">Figure 2</xref>. In particular, the spin-vortex crystal configuration, in which the Fe spins form either loop or hedgehog structures, can be stabilized when a glide symmetry across the Fe planes is broken [<xref ref-type="bibr" rid="B20">20</xref>]. This type of order was recently identified in Ni-doped and Co-doped CaKFe<sub>4</sub>As<sub>4</sub> [<xref ref-type="bibr" rid="B21">21</xref>]. There are two crystallographically distinct As sites in this structure, and the hyperfine field either vanishes at both sites for loop spin-vortex crystal order, or is aligned along the <bold>c</bold> axis for one&#xa0;As site and vanishes for the other As site for hedgehog spin-vortex crystal order. In this system, doping induces the latter, which was identified by NMR.</p>
<p>Note that when the Fe is substituted by another transition metal, the symmetry among the hyperfine couplings of the four nearest neighbors is broken, and the hyperfine field vector can acquire a component perpendicular to the <bold>c</bold> axis [<xref ref-type="bibr" rid="B22">22</xref>]. This effect contributes to inhomogeneous broadening in doped samples. In the presence of nematic order, the <italic>C</italic>
<sub>4</sub> symmetry of the lattice is broken, and in principle <italic>A</italic>
<sub>
<italic>aa</italic>
</sub> &#x2260; <italic>A</italic>
<sub>
<italic>bb</italic>
</sub>. This asymmetry has not been observed directly. In FeSe, the Knight shift tensor becomes anisotropic, with <italic>K</italic>
<sub>
<italic>aa</italic>
</sub> &#x2260; <italic>K</italic>
<sub>
<italic>bb</italic>
</sub>, where <italic>K</italic>
<sub>
<italic>&#x3b1;&#x3b1;</italic>
</sub> &#x3d; <italic>A</italic>
<sub>
<italic>&#x3b1;&#x3b1;</italic>
</sub>
<italic>&#x3c7;</italic>
<sub>
<italic>&#x3b1;&#x3b1;</italic>
</sub>, and <italic>&#x3c7;</italic>
<sub>
<italic>&#x3b1;&#x3b1;</italic>
</sub> is the static magnetic susceptibility [<xref ref-type="bibr" rid="B5">5</xref>]. However, in this case the anisotropy is believed to reflect that of the susceptibility, i.e., <italic>&#x3c7;</italic>
<sub>
<italic>aa</italic>
</sub> &#x2260; <italic>&#x3c7;</italic>
<sub>
<italic>bb</italic>
</sub> in the nematic phase, rather than an asymmetry in the hyperfine coupling [<xref ref-type="bibr" rid="B23">23</xref>]. Curiously, <italic>&#x3c7;</italic>
<sub>
<italic>aa</italic>
</sub> &#x3e; <italic>&#x3c7;</italic>
<sub>
<italic>bb</italic>
</sub> in FeSe, but <italic>&#x3c7;</italic>
<sub>
<italic>bb</italic>
</sub> &#x3e; <italic>&#x3c7;</italic>
<sub>
<italic>aa</italic>
</sub> in BaFe<sub>2</sub>As<sub>2</sub>, LaFeAsO, and NaFeAs [<xref ref-type="bibr" rid="B24">24</xref>&#x2013;<xref ref-type="bibr" rid="B26">26</xref>], which may reflect different natures of the nematic order in these materials [<xref ref-type="bibr" rid="B27">27</xref>]. In particular, the nematic order parameter in the latter can be understood in terms of differential occupations between the <italic>d</italic>
<sub>
<italic>yz</italic>
</sub> and <italic>d</italic>
<sub>
<italic>xz</italic>
</sub> orbitals, whereas in the former the nematic order may involve more complex superpositions between 3<italic>d</italic> orbitals, giving rise to bond-centered nematic order [<xref ref-type="bibr" rid="B23">23</xref>, <xref ref-type="bibr" rid="B28">28</xref>, <xref ref-type="bibr" rid="B29">29</xref>]. The sign of the resistivity anisotropies in BaFe<sub>2</sub>As<sub>2</sub> and FeSe match those of the magnetic anisotropies [<xref ref-type="bibr" rid="B24">24</xref>, <xref ref-type="bibr" rid="B30">30</xref>], suggesting a common origin for the two.</p>
</sec>
<sec id="s2-2">
<title>2.2 Quadrupolar Interaction</title>
<p>For nuclei with spin <italic>I</italic> &#x3e; 1/2, the quadrupolar coupling is given by:<disp-formula id="e2">
<mml:math id="m6">
<mml:msub>
<mml:mrow>
<mml:mi mathvariant="script">H</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>Q</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mi>h</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3bd;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>z</mml:mi>
<mml:mi>z</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mrow>
<mml:mn>6</mml:mn>
</mml:mrow>
</mml:mfrac>
<mml:mfenced open="[" close="]">
<mml:mrow>
<mml:mn>3</mml:mn>
<mml:msubsup>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mi>I</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">&#x302;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mrow>
<mml:mi>z</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msubsup>
<mml:mo>&#x2212;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mi>I</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">&#x302;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>&#x3b7;</mml:mi>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:msubsup>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mi>I</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">&#x302;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mrow>
<mml:mi>x</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msubsup>
<mml:mo>&#x2212;</mml:mo>
<mml:msubsup>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mi>I</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">&#x302;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mrow>
<mml:mi>y</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mfenced>
<mml:mo>,</mml:mo>
</mml:math>
<label>(2)</label>
</disp-formula>where the EFG tensor is given by:<disp-formula id="e3">
<mml:math id="m7">
<mml:msub>
<mml:mrow>
<mml:mi>&#x3bd;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
<mml:mi>&#x3b2;</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mi>e</mml:mi>
<mml:mi>Q</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>12</mml:mn>
<mml:mi>h</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mfrac>
<mml:mrow>
<mml:msup>
<mml:mrow>
<mml:mi>&#x2202;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mi>V</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x2202;</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mi>x</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mi>&#x2202;</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mi>x</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfrac>
<mml:mo>,</mml:mo>
</mml:math>
<label>(3)</label>
</disp-formula>and <italic>V</italic> is the electrostatic potential at the As site. This quantity is dominated by the occupation of the As 4<italic>p</italic> orbitals, which in turn are hybridized with the <italic>d</italic>
<sub>
<italic>xz</italic>,<italic>yz</italic>
</sub>-orbitals of the neighboring Fe atoms [<xref ref-type="bibr" rid="B31">31</xref>]. The EFG asymmetry parameter is given by:<disp-formula id="e4">
<mml:math id="m8">
<mml:mi>&#x3b7;</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3bd;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>y</mml:mi>
<mml:mi>y</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3bd;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>x</mml:mi>
<mml:mi>x</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3bd;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>x</mml:mi>
<mml:mi>x</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2b;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3bd;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>y</mml:mi>
<mml:mi>y</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfrac>
<mml:mo>.</mml:mo>
</mml:math>
<label>(4)</label>
</disp-formula>
</p>
<p>This quantity vanishes in the tetragonal phase because the As 4<italic>p</italic>
<sub>
<italic>x</italic>
</sub> and 4<italic>p</italic>
<sub>
<italic>y</italic>
</sub> orbitals are degenerate, hence <italic>&#x3bd;</italic>
<sub>
<italic>xx</italic>
</sub> &#x3d; <italic>&#x3bd;</italic>
<sub>
<italic>yy</italic>
</sub> [<xref ref-type="bibr" rid="B32">32</xref>]. The EFG tensor is always traceless, thus in this case it can be characterized by a single quantity, <italic>&#x3bd;</italic>
<sub>
<italic>zz</italic>
</sub>. The magnitude of <italic>&#x3bd;</italic>
<sub>
<italic>zz</italic>
</sub> depends on the degree of hybridization of the As 4<italic>p</italic>
<sub>
<italic>z</italic>
</sub> orbital, and is sensitive to the <italic>c</italic>-axis length of the unit cell [<xref ref-type="bibr" rid="B33">33</xref>&#x2013;<xref ref-type="bibr" rid="B35">35</xref>] and also varies with temperature [<xref ref-type="bibr" rid="B18">18</xref>, <xref ref-type="bibr" rid="B36">36</xref>&#x2013;<xref ref-type="bibr" rid="B38">38</xref>].</p>
<p>The EFG is strongly affected by doping. Replacing the Fe by another transition metal, or replacing the As by P, will give rise to spatially-varying strain fields that will distort the electrostatic potential and alter the EFG tensor. This effect can lower the symmetry such that <italic>&#x3bd;</italic>
<sub>
<italic>xx</italic>
</sub> &#x2260; <italic>&#x3bd;</italic>
<sub>
<italic>yy</italic>
</sub>, and create non-zero off-diagonal terms of the tensor. In some cases the effect is sufficiently large that separate resonances can be detected for sites that are adjacent to the substitutional site [<xref ref-type="bibr" rid="B31">31</xref>, <xref ref-type="bibr" rid="B39">39</xref>]. This sensitivity to disorder tends to significantly broaden the NMR resonance frequencies in doped samples relative to the parent compound. In doped Ba(Fe,Co)<sub>2</sub>As<sub>2</sub> the width of the quadrupolar satellites is dominated by a variation of <italic>&#x3b7;</italic> that exhibits a Curie-Weiss temperature dependence, which has been associated with the growth of nematic correlations surrounding the dopant atoms [<xref ref-type="bibr" rid="B40">40</xref>]. A similar effect has been observed in FeSe where the magnetic linewidth is broadened by the presence of crystal defects (there is no quadrupolar interaction for Se) [<xref ref-type="bibr" rid="B41">41</xref>]. In this case, the Knight shift anisotropy reflects the growth of an Edwards-Anderson order parameter of the nematicity [<xref ref-type="bibr" rid="B42">42</xref>].</p>
<p>In the presence of long range nematic order, the <italic>C</italic>
<sub>4</sub> symmetry of the EFG tensor is broken and <italic>&#x3bd;</italic>
<sub>
<italic>xx</italic>
</sub> &#x2260; <italic>&#x3bd;</italic>
<sub>
<italic>yy</italic>
</sub> [<xref ref-type="bibr" rid="B43">43</xref>]. In CaFe<sub>2</sub>As<sub>2</sub> <italic>&#x3b7;</italic> reaches 0.4 at low temperature, but in BaFe<sub>2</sub>As<sub>2</sub> and SrFe<sub>2</sub>As<sub>2</sub>, <italic>&#x3b7;</italic> reaches 1.2 and 1.4, respectively, reflecting the fact that <italic>&#x3bd;</italic>
<sub>
<italic>xx</italic>
</sub> and <italic>&#x3bd;</italic>
<sub>
<italic>yy</italic>
</sub> have opposite signs [<xref ref-type="bibr" rid="B33">33</xref>]. Note that it is sometimes customary to define the principal axes of the EFG such that the eigenvalues &#x7c;<italic>V</italic>
<sub>
<italic>zz</italic>
</sub>&#x7c;&#x2265;&#x7c;<italic>V</italic>
<sub>
<italic>yy</italic>
</sub>&#x7c;&#x2265;&#x7c;<italic>V</italic>
<sub>
<italic>xx</italic>
</sub>&#x7c;, so that 0 &#x2264; <italic>&#x3b7;</italic> &#x2264; 1. Here we do not follow this convention, maintaining the <italic>V</italic>
<sub>
<italic>zz</italic>
</sub> associated with the crystal <italic>c</italic> axis as in the tetragonal phase. This choice is the reason that <italic>&#x3b7;</italic> &#x3e; 1, which would correspond to a confusing rotation of orientation of the principal axes under the customary definition. These changes reflect a dramatic rearrangement of the charge distribution around the As nucleus below the structural transition, despite an orthorhombicity of only approximately 1%. The EFG tensor is dominated by the occupations of the As 4<italic>p</italic> orbitals, which in turn are hybridized with the Fe 3<italic>d</italic>
<sub>
<italic>yz</italic>
</sub> and 3<italic>d</italic>
<sub>
<italic>xz</italic>
</sub> orbitals [<xref ref-type="bibr" rid="B31">31</xref>, <xref ref-type="bibr" rid="B32">32</xref>]. These orbitals are degenerate in the tetragonal phase, but develop a splitting on the order of 40&#xa0;meV in the nematic phase [<xref ref-type="bibr" rid="B44">44</xref>]. As a result, the relative occupations of the As <italic>p</italic>
<sub>
<italic>x</italic>
</sub> and <italic>p</italic>
<sub>
<italic>y</italic>
</sub> orbitals change and alter the EFG.</p>
</sec>
<sec id="s2-3">
<title>2.3 NMR Spectra</title>
<p>In order to resolve the in-plane asymmetry that emerges in the Knight shift or EFG tensors, it is important to measure the NMR spectra of carefully oriented single crystals. In an external magnetic field, the As nuclear spins experience the sum of three interactions: <inline-formula id="inf5">
<mml:math id="m9">
<mml:msub>
<mml:mrow>
<mml:mi mathvariant="script">H</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>Z</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2b;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi mathvariant="script">H</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>h</mml:mi>
<mml:mi>y</mml:mi>
<mml:mi>p</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2b;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi mathvariant="script">H</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>Q</mml:mi>
</mml:mrow>
</mml:msub>
</mml:math>
</inline-formula>, where <inline-formula id="inf6">
<mml:math id="m10">
<mml:msub>
<mml:mrow>
<mml:mi mathvariant="script">H</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>Z</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>&#x3b3;</mml:mi>
<mml:mi>&#x210f;</mml:mi>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mi mathvariant="bold">I</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">&#x302;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mo>&#x22c5;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi mathvariant="bold">H</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>0</mml:mn>
</mml:mrow>
</mml:msub>
</mml:math>
</inline-formula> is the Zeeman interaction. The spectrum will consist of three resonances. For sufficiently large Zeeman interaction (<italic>&#x3b3;H</italic>
<sub>0</sub> &#x226b; <italic>&#x3bd;</italic>
<sub>
<italic>&#x3b1;&#x3b1;</italic>
</sub>), the frequencies are given to first order by:<disp-formula id="equ1">
<mml:math id="m11">
<mml:mtable class="eqnarray-star">
<mml:mtr>
<mml:mtd columnalign="right">
<mml:msub>
<mml:mrow>
<mml:mi>f</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>s</mml:mi>
<mml:mi>a</mml:mi>
<mml:mi>t</mml:mi>
<mml:mn>1,2</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mtd>
<mml:mtd columnalign="left">
<mml:mo>&#x3d;</mml:mo>
</mml:mtd>
<mml:mtd columnalign="left">
<mml:mi>&#x3b3;</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mi>H</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>0</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mn>1</mml:mn>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>K</mml:mi>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>&#x3d5;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mfenced>
<mml:mo>&#xb1;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3bd;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>z</mml:mi>
<mml:mi>z</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mn>3</mml:mn>
<mml:mo>&#x2061;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mi>cos</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>&#x3b7;</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mi>sin</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>cos</mml:mi>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:mi>&#x3d5;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mfenced>
</mml:mtd>
</mml:mtr>
<mml:mtr>
<mml:mtd columnalign="right">
<mml:msub>
<mml:mrow>
<mml:mi>f</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>c</mml:mi>
<mml:mi>e</mml:mi>
<mml:mi>n</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mtd>
<mml:mtd columnalign="left">
<mml:mo>&#x3d;</mml:mo>
</mml:mtd>
<mml:mtd columnalign="left">
<mml:mi>&#x3b3;</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mi>H</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>0</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mn>1</mml:mn>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>K</mml:mi>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>&#x3d5;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mfenced>
<mml:mo>&#x2b;</mml:mo>
<mml:mi mathvariant="normal">&#x394;</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mi>f</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>&#x3d5;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mtd>
</mml:mtr>
</mml:mtable>
</mml:math>
<label>(5)</label>
</disp-formula>where <italic>f</italic>
<sub>
<italic>sat</italic>1,2</sub> and <italic>f</italic>
<sub>
<italic>cen</italic>
</sub> are the frequencies of the two satellites and the central transition, <italic>&#x3b8;</italic> is the angle between <bold>H</bold>
<sub>0</sub> and <bold>c</bold>, and <italic>&#x3d5;</italic> is the azimuthal angle of the projection of <bold>H</bold>
<sub>0</sub> in the <italic>ab</italic> plane. The Knight shift is given by:<disp-formula id="e5">
<mml:math id="m12">
<mml:mi>K</mml:mi>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>&#x3d5;</mml:mi>
</mml:mrow>
</mml:mfenced>
<mml:mo>&#x3d;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>z</mml:mi>
<mml:mi>z</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2061;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mi>cos</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>x</mml:mi>
<mml:mi>x</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2061;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mi>sin</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mi>cos</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3d5;</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>K</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>y</mml:mi>
<mml:mi>y</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2061;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mi>sin</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mi>sin</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3d5;</mml:mi>
<mml:mo>.</mml:mo>
</mml:math>
<label>(6)</label>
</disp-formula>
</p>
<p>The second order correction to the central transition is given by:<disp-formula id="e6">
<mml:math id="m13">
<mml:mtable class="eqnarray">
<mml:mtr>
<mml:mtd columnalign="right">
<mml:mi mathvariant="normal">&#x394;</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mi>f</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>&#x3d5;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mtd>
<mml:mtd columnalign="left">
<mml:mo>&#x3d;</mml:mo>
</mml:mtd>
<mml:mtd columnalign="left">
<mml:mfrac>
<mml:mrow>
<mml:msubsup>
<mml:mrow>
<mml:mi>&#x3bd;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>z</mml:mi>
<mml:mi>z</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:mrow>
<mml:mrow>
<mml:mn>96</mml:mn>
<mml:mi>&#x3b3;</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mi>H</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>0</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfrac>
<mml:mfenced open="[" close="">
<mml:mrow>
<mml:mn>7</mml:mn>
<mml:msup>
<mml:mrow>
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<mml:mrow>
<mml:mn>2</mml:mn>
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</mml:msup>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>18</mml:mn>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>6</mml:mn>
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<mml:mrow>
<mml:msup>
<mml:mrow>
<mml:mi>&#x3b7;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
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</mml:msup>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>30</mml:mn>
</mml:mrow>
</mml:mfenced>
<mml:msup>
<mml:mrow>
<mml:mi>cos</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>9</mml:mn>
<mml:mfenced open="(" close=")">
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<mml:mn>18</mml:mn>
<mml:mo>&#x2b;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mi>&#x3b7;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
</mml:mrow>
</mml:mfenced>
<mml:msup>
<mml:mrow>
<mml:mi>cos</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>4</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
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</mml:mtd>
</mml:mtr>
</mml:mtable>
</mml:math>
</disp-formula>
<disp-formula id="e7">
<mml:math id="m14">
<mml:mtable class="eqnarray">
<mml:mtr>
<mml:mtd columnalign="right"/>
<mml:mtd columnalign="left"/>
<mml:mtd columnalign="left">
<mml:mfenced open="" close="]">
<mml:mrow>
<mml:mo>&#x2b;</mml:mo>
<mml:mn>12</mml:mn>
<mml:mi>&#x3b7;</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>cos</mml:mi>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:mi>&#x3d5;</mml:mi>
</mml:mrow>
</mml:mfenced>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mn>9</mml:mn>
<mml:mo>&#x2061;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mi>cos</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>4</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>8</mml:mn>
<mml:mo>&#x2061;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mi>cos</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:mfenced>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>9</mml:mn>
<mml:msup>
<mml:mrow>
<mml:mi>&#x3b7;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>cos</mml:mi>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mn>4</mml:mn>
<mml:mi>&#x3d5;</mml:mi>
</mml:mrow>
</mml:mfenced>
<mml:msup>
<mml:mrow>
<mml:mi>sin</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>4</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
</mml:mfenced>
<mml:mo>.</mml:mo>
</mml:mtd>
</mml:mtr>
</mml:mtable>
</mml:math>
<label>(7)</label>
</disp-formula>
</p>
<p>Measurements of the two satellite transitions as a function of field orientation can be used to extract the Knight shift and EFG tensors.</p>
<p>In the tetragonal phase, there are three distinct resonances for each As in the unit cell (e.g., one As site in AFe<sub>2</sub>As<sub>2</sub>). However, in the nematic phase there are multiple domains in an untwinned crystal, giving rise to extra resonances. If the magnetic field is oriented in the plane, then there may be two sets of resonances associated with these two domains because the azimuthal angle, <italic>&#x3d5;</italic>, differs for each domain, as observed in <xref ref-type="fig" rid="F3">Figure 3</xref>. This behavior is illustrated in <xref ref-type="fig" rid="F4">Figure 4</xref>. In general, there are five distinct transitions (six if the Knight shift is also anisotropic), but in certain directions the spectra from the two domains overlap and three resonances are recovered. Large values of &#x7c;<italic>&#x3b7;</italic>&#x7c; cause the satellites to switch positions from below to above the central transition as the in-plane angle <italic>&#x3d5;</italic> is rotated.</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>Fe-As plane in tetragonal and orthorhombic phase of BaFe<sub>2</sub>As<sub>2</sub>. Orange arrows indicate direction of displacements giving rise to two domains with positive and negative <italic>B</italic>
<sub>2<italic>g</italic>
</sub> strain. Strain is labeled by the unit cell of the tetragonal phase, so uniaxial strain along the [110]<sub>
<italic>T</italic>
</sub> direction of the tetragonal unit cell gives rise to a <italic>B</italic>
<sub>2<italic>g</italic>
</sub> distortion.</p>
</caption>
<graphic xlink:href="fphy-10-877628-g003.tif"/>
</fig>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>Polar plots of the three resonance frequencies of the As for &#x7c;<italic>&#x3b7;</italic>&#x7c; &#x3d; 0.4 <bold>(A)</bold> and for &#x7c;<italic>&#x3b7;</italic>&#x7c; &#x3d; 1.2 <bold>(B)</bold>. Blue and red correspond to two nematic domains with &#xb1; <italic>&#x3b7;</italic>, as a function of in-plane field direction. In this case, we assume <italic>K</italic>
<sub>
<italic>xx</italic>
</sub> &#x3d; <italic>K</italic>
<sub>
<italic>yy</italic>
</sub>. The directions [100] and [010] correspond to the orthorhombic unit cell directions. In general, there are five distinct transitions, but for certain angles the two sets of satellites overlap. When &#x7c;<italic>&#x3b7;</italic>&#x7c; &#x3e; 1, the two satellites for each domain reverse, crossing the central transition.</p>
</caption>
<graphic xlink:href="fphy-10-877628-g004.tif"/>
</fig>
<p>When <italic>&#x3b7;</italic> is non-zero the nuclear spin Hamiltonian does not commute with <inline-formula id="inf7">
<mml:math id="m15">
<mml:msub>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mi>I</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">&#x302;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mrow>
<mml:mi>z</mml:mi>
</mml:mrow>
</mml:msub>
</mml:math>
</inline-formula>, and the eigenstates, &#x7c;<italic>i</italic>&#x27e9;, are superpositions of the &#x7c;<italic>I</italic>
<sub>
<italic>z</italic>
</sub>&#x27e9; states. In such cases it may be possible to observe hidden transitions when the matrix element <inline-formula id="inf8">
<mml:math id="m16">
<mml:mo stretchy="false">&#x2329;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3c8;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo stretchy="false">&#x7c;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mi>I</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">&#x302;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mrow>
<mml:mo>&#xb1;</mml:mo>
</mml:mrow>
</mml:msub>
<mml:mo stretchy="false">&#x7c;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3c8;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>j</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo stretchy="false">&#x232a;</mml:mo>
</mml:math>
</inline-formula> does not vanish. This effect can arise when <italic>&#x3bd;</italic>
<sub>
<italic>zz</italic>
</sub> &#x2273; <italic>&#x3b3;H</italic>, but in almost all cases there is an internal field, <italic>H</italic>
<sub>
<italic>int</italic>
</sub>, that develops in the antiferromagnetic state that accompanies the orthorhombic distortion. Typically <italic>&#x3b3;H</italic>
<sub>
<italic>int</italic>
</sub> &#x226b; <italic>&#x3bd;</italic>
<sub>
<italic>zz</italic>
</sub> is sufficiently large that such hidden transitions should not be evident. For CaFe<sub>2</sub>As<sub>2</sub>, however, <italic>&#x3bd;</italic>
<sub>
<italic>zz</italic>
</sub>/<italic>&#x3b3;H</italic> &#x223c; 0.7 thus it may be possible to observe these transitions for small external fields <italic>H</italic>
<sub>0</sub> applied in the plane, as illustrated in <xref ref-type="fig" rid="F5">Figure 5</xref>. To date no such transitions have been reported.</p>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>Resonance frequencies versus applied magnetic field, <bold>H</bold>
<sub>0</sub>, oriented either along the orthorhombic [100] <bold>(A)</bold> or [110] directions <bold>(B)</bold> assuming an internal field of 2.5&#xa0;T along <italic>c</italic> and an EFG of <italic>&#x3bd;</italic>
<sub>
<italic>zz</italic>
</sub> &#x3d; 12.4&#xa0;MHz with <italic>&#x3b7;</italic> &#x3d; 0.4, corresponding to the case of CaFe<sub>2</sub>As<sub>2</sub>. Red and blue correspond to the two nematic domains. The intensity of the transitions are given by the matrix elements &#x7c;&#x27e8;<italic>i</italic>&#x7c;<italic>I</italic>
<sub>&#x2b;</sub>&#x7c;<italic>j</italic>&#x27e9;&#x7c;<sup>2</sup>, where <italic>i</italic>, <italic>j</italic> correspond to eigenstates of the nuclear spin Hamiltonian. Hidden transitions should be visible for certain field ranges.</p>
</caption>
<graphic xlink:href="fphy-10-877628-g005.tif"/>
</fig>
</sec>
<sec id="s2-4">
<title>2.4 Relaxation Rate</title>
<p>The hyperfine field, <bold>H</bold>
<sub>
<italic>hyp</italic>
</sub>, and the EFG not only give rise to static spectral signatures, but their fluctuations can also drive relaxation of the nuclear spins. The nuclear spin energies are generally several order of magnitude smaller than the relevant electron energies, and thus the nuclear spin ensemble can easily be manipulated to have a non-equilibrium distribution among the energy levels. The nuclear spins will return to thermal equilibrium with the &#x201c;lattice,&#x201d; or the electronic spin system, over a time scale, <italic>T</italic>
<sub>1</sub>, known as the spin-lattice relaxation time. This rate, <inline-formula id="inf9">
<mml:math id="m17">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula>, can be measured with high precision and is determined by the couplings described above in <xref ref-type="sec" rid="s2-1">Section 2.1</xref>, <xref ref-type="sec" rid="s2-2">Section 2.2</xref>. In essence, the nuclear spins act as quantum sensors that probe the noise spectra of the electronic spin and charge degrees of freedom. There are three important spectral densities that may play a role:<disp-formula id="e8">
<mml:math id="m18">
<mml:mtable class="eqnarray">
<mml:mtr>
<mml:mtd columnalign="right">
<mml:mi>J</mml:mi>
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<mml:mrow>
<mml:mi>&#x3c9;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mtd>
<mml:mtd columnalign="left">
<mml:mo>&#x3d;</mml:mo>
</mml:mtd>
<mml:mtd columnalign="left">
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<mml:mrow>
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<mml:mrow>
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</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:mfrac>
<mml:msubsup>
<mml:mrow>
<mml:mo>&#x222b;</mml:mo>
</mml:mrow>
<mml:mrow>
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</mml:mrow>
<mml:mrow>
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</mml:mrow>
</mml:msubsup>
<mml:mfenced open="[" close="]">
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</mml:mrow>
<mml:mrow>
<mml:mo>&#x2b;</mml:mo>
</mml:mrow>
</mml:msub>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>h</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
</mml:mrow>
</mml:msub>
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<mml:msup>
<mml:mrow>
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</mml:mrow>
<mml:mrow>
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<mml:mi>d</mml:mi>
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</mml:mtd>
</mml:mtr>
</mml:mtable>
</mml:math>
<label>(8)</label>
</disp-formula>
<disp-formula id="e9">
<mml:math id="m19">
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<mml:mtd columnalign="right">
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<mml:mrow>
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</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:msup>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mi>&#x3c9;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mtd>
<mml:mtd columnalign="left">
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</mml:mtd>
<mml:mtd columnalign="left">
<mml:msup>
<mml:mrow>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:mi>e</mml:mi>
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</mml:mrow>
<mml:mrow>
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</mml:mrow>
</mml:mfrac>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:msubsup>
<mml:mrow>
<mml:mo>&#x222b;</mml:mo>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x221e;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x221e;</mml:mi>
</mml:mrow>
</mml:msubsup>
<mml:mfenced open="[" close="]">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>V</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2b;</mml:mo>
<mml:mn>1,2</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>V</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1,2</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfenced>
<mml:msup>
<mml:mrow>
<mml:mi>e</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mi>&#x3c9;</mml:mi>
<mml:mi>&#x3c4;</mml:mi>
</mml:mrow>
</mml:msup>
<mml:mi>d</mml:mi>
<mml:mi>&#x3c4;</mml:mi>
</mml:mtd>
</mml:mtr>
</mml:mtable>
</mml:math>
<label>(9)</label>
</disp-formula>where <inline-formula id="inf10">
<mml:math id="m20">
<mml:mfenced open="[" close="]">
<mml:mrow>
<mml:mi>A</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>B</mml:mi>
</mml:mrow>
</mml:mfenced>
<mml:mo>&#x3d;</mml:mo>
<mml:mo stretchy="false">&#x2329;</mml:mo>
<mml:mi>A</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:mi>&#x3c4;</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
<mml:mi>B</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:mn>0</mml:mn>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>B</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:mi>&#x3c4;</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
<mml:mi>A</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:mn>0</mml:mn>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
<mml:mo stretchy="false">&#x232a;</mml:mo>
<mml:mo>/</mml:mo>
<mml:mn>2</mml:mn>
</mml:math>
</inline-formula> is an ensemble average. Here <italic>h</italic>
<sub>&#xb1;</sub> &#x3d; <italic>H</italic>
<sub>
<italic>hyp</italic>,<italic>x</italic>
</sub> &#xb1; <italic>iH</italic>
<sub>
<italic>hyp</italic>,<italic>y</italic>
</sub>, <italic>V</italic> <sub>&#xb1; 1</sub> &#x3d; <italic>V</italic>
<sub>
<italic>xz</italic>
</sub> &#xb1; <italic>iV</italic>
<sub>
<italic>yz</italic>
</sub>, and <italic>V</italic> <sub>&#xb1; 2</sub> &#x3d; (<italic>V</italic>
<sub>
<italic>xx</italic>
</sub> &#x2212; <italic>V</italic>
<sub>
<italic>yy</italic>
</sub>)/2 &#xb1; <italic>iV</italic>
<sub>
<italic>xy</italic>
</sub> [<xref ref-type="bibr" rid="B45">45</xref>]. <italic>J</italic>(<italic>&#x3c9;</italic>) and <italic>J</italic>
<sup>(1,2)</sup>(<italic>&#x3c9;</italic>) are the spectral densities of the hyperfine and EFG fluctuations, respectively. The <inline-formula id="inf11">
<mml:math id="m21">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula> measurements probe these spectral functions at the nuclear resonance frequency, <italic>&#x3c9;</italic>
<sub>
<italic>N</italic>
</sub>, typically on the order of 100&#xa0;MHz (<inline-formula id="inf12">
<mml:math id="m22">
<mml:mo>&#x223c;</mml:mo>
<mml:mn>0.4</mml:mn>
<mml:mi>&#x3bc;</mml:mi>
</mml:math>
</inline-formula>eV). This frequency is nearly vanishing in comparison to the relevant electronic energies, typically on the order of meV. If there is only one type of fluctuation, then <inline-formula id="inf13">
<mml:math id="m23">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula> is directly related to the appropriate spectral density. For example, for pure magnetic fluctuations, (e.g., <italic>V</italic> <sub>&#xb1; 1,2</sub> &#x3d; 0), then <inline-formula id="inf14">
<mml:math id="m24">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
<mml:mo>&#x3d;</mml:mo>
<mml:mi>J</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3c9;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>N</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula>, or if <italic>h</italic>
<sub>&#xb1;</sub> &#x3d; 0 and <italic>V</italic> <sub>&#xb1; 1</sub> &#x3d; 0, then <inline-formula id="inf15">
<mml:math id="m25">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
<mml:mo>&#x3d;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mi>J</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:msup>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3c9;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>N</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula>, or if <italic>h</italic>
<sub>&#xb1;</sub> &#x3d; 0 and <italic>V</italic> <sub>&#xb1; 2</sub> &#x3d; 0 then <inline-formula id="inf16">
<mml:math id="m26">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
<mml:mo>&#x3d;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mi>J</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:msup>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3c9;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>N</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula>. On the other hand, if multiple types of fluctuations are present, then the nuclear spin relaxation is a complex function of multiple spectral functions and it is not straightforward to disentangle the different contributions to <inline-formula id="inf17">
<mml:math id="m27">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula> [<xref ref-type="bibr" rid="B46">46</xref>&#x2013;<xref ref-type="bibr" rid="B48">48</xref>]. It is common for the magnetic fluctuations to dominate, in which case the contribution from quadrupolar contributions can be ignored. However, as we discuss below in <xref ref-type="sec" rid="s2-4-1">Section 2.4.1</xref>, there is a significant quadrupolar contribution to the <inline-formula id="inf18">
<mml:math id="m28">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula> of the As in the pnictides.</p>
<p>When the electronic system is close to an thermodynamic instability, critical fluctuations will slow down and may have a dramatic effect on <inline-formula id="inf19">
<mml:math id="m29">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula>. As an example, consider the case where the magnetic fluctuations exhibit Lorentzian autocorrelation function: <inline-formula id="inf20">
<mml:math id="m30">
<mml:mfenced open="[" close="]">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>h</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2b;</mml:mo>
</mml:mrow>
</mml:msub>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>h</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfenced>
<mml:mo>&#x3d;</mml:mo>
<mml:msubsup>
<mml:mrow>
<mml:mi>h</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>0</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msubsup>
<mml:msup>
<mml:mrow>
<mml:mi>e</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mo stretchy="false">&#x7c;</mml:mo>
<mml:mi>&#x3c4;</mml:mi>
<mml:mo stretchy="false">&#x7c;</mml:mo>
<mml:mo>/</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3c4;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>c</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:msup>
</mml:math>
</inline-formula>, where <italic>&#x3c4;</italic>
<sub>
<italic>c</italic>
</sub> is the correlation time. In this case:<disp-formula id="e10">
<mml:math id="m31">
<mml:mfrac>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:msup>
<mml:mrow>
<mml:mi>&#x3b3;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:msubsup>
<mml:mrow>
<mml:mi>h</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>0</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msubsup>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3c4;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>c</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
<mml:mo>&#x2b;</mml:mo>
<mml:msubsup>
<mml:mrow>
<mml:mi>&#x3c9;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>N</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msubsup>
<mml:msubsup>
<mml:mrow>
<mml:mi>&#x3c4;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>c</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:mrow>
</mml:mfrac>
<mml:mo>.</mml:mo>
</mml:math>
<label>(10)</label>
</disp-formula>
</p>
<p>Usually <italic>&#x3c9;</italic>
<sub>
<italic>N</italic>
</sub>
<italic>&#x3c4;</italic>
<sub>
<italic>c</italic>
</sub> &#x226a; 1, but close to a phase transition where there is critical slowing down, <italic>&#x3c4;</italic>
<sub>
<italic>c</italic>
</sub> can approach infinity as a power law. As a result, <inline-formula id="inf21">
<mml:math id="m32">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula> exhibits a peak at the phase transition temperature, as illustrated in <xref ref-type="fig" rid="F6">Figure 6</xref>. This property has been exploited to investigate the critical dynamics of many correlated electron systems, especially the pnictides [<xref ref-type="bibr" rid="B39">39</xref>, <xref ref-type="bibr" rid="B49">49</xref>].</p>
<fig id="F6" position="float">
<label>FIGURE 6</label>
<caption>
<p>Calculated spin lattice relaxation rate versus temperature using <xref ref-type="disp-formula" rid="e10">Eq. 10</xref> for two different models for the temperature dependence of the autocorrelation time, <italic>&#x3c4;</italic>
<sub>
<italic>c</italic>
</sub>. The blue curve assumes a power law divergence: <italic>&#x3c4;</italic>
<sub>
<italic>c</italic>
</sub> &#x221d;&#x7c;<italic>T</italic> &#x2212; <italic>T</italic>
<sub>0</sub>&#x7c;<sup>&#x2212;2</sup>, appropriate for critical slowing down at a phase transition. The sharp dip around <italic>T</italic>
<sub>0</sub> is usually not observable and there is only a single peak. The purple curve assumes an activated form: <inline-formula id="inf22">
<mml:math id="m33">
<mml:msub>
<mml:mrow>
<mml:mi>&#x3c4;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>c</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x221d;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mi>e</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>E</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>a</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>/</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>k</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>B</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mi>T</mml:mi>
</mml:mrow>
</mml:msup>
</mml:math>
</inline-formula>, where <italic>E</italic>
<sub>
<italic>a</italic>
</sub> is an activation energy, which is appropriate for a glassy system where the degrees of freedom gradually freeze out.</p>
</caption>
<graphic xlink:href="fphy-10-877628-g006.tif"/>
</fig>
<p>As discussed above in <xref ref-type="sec" rid="s2-3">Section 2.3</xref>, the nuclear spin eigenstates become superpositions of the <italic>I</italic>
<sub>
<italic>z</italic>
</sub> states for non-zero values of <italic>&#x3b7;</italic>. In this case, it is important to consider spectral densities other than those described in <xref ref-type="disp-formula" rid="e6">Eqs 6</xref>, <xref ref-type="disp-formula" rid="e7">7</xref> to account for fluctuations in other directions. For example, hyperfine field fluctuations, <italic>H</italic>
<sub>
<italic>hyp</italic>,<italic>z</italic>
</sub>, may play a role in relaxing the nuclear spins. In such cases the form of the relaxation function is more complicated, and <xref ref-type="disp-formula" rid="e8">Eq. 8</xref> will contain more terms.</p>
<sec id="s2-4-1">
<title>2.4.1 Quadrupolar Relaxation From Nematic Fluctuations</title>
<p>Although magnetic relaxation is usually dominant, quadrupolar relaxation should also be present in the pnictides because the EFG changes dramatically at the nematic phase transition. This effect has been investigated in BaFe<sub>2</sub>(As<sub>1&#x2212;<italic>x</italic>
</sub>P<sub>
<italic>x</italic>
</sub>)<sub>2</sub> by comparing the relaxation of the <sup>75</sup>As to <sup>31</sup>P [<xref ref-type="bibr" rid="B43">43</xref>]. The phosphorus isotope has spin <italic>I</italic> &#x3d; 1/2, and does not have a quadrupolar moment. It therefore is only sensitive to magnetic fluctuations, whereas the As probes both magnetic and quadrupolar fluctuations. Importantly, both the As and the P are located in the same crystallographic site, and experience similar hyperfine interactions. In fact, the <sup>75</sup>As exhibits a higher relaxation rate, indicating the presence of a second relaxation channel that is, not probed by the <sup>31</sup>P. Moreover, the extra relaxation increases with decreasing temperature, and exhibits a peak at the nematic ordering temperature. An analysis of the extra relaxation rate suggests that the nematic susceptibility diverges below <italic>T</italic>
<sub>
<italic>N</italic>
</sub> for the lightly doped system, and below <italic>T</italic>
<sub>
<italic>c</italic>
</sub> for the optimally doped system. It was not possible to quantitatively disentangle the contributions from the magnetic and quadrupolar channels separately, primarily because the doping introduced inhomogeneous relaxation, as discussed below in <xref ref-type="sec" rid="s4">Section 4</xref>. The three relaxation channels (one magnetic and two quadrupolar) may also be coupled to one another. For example, a nematic fluctuation can give rise spectral densities <italic>J</italic> (<italic>&#x3c9;</italic>
<sub>
<italic>N</italic>
</sub>), <italic>J</italic>
<sup>(1)</sup>(<italic>&#x3c9;</italic>
<sub>
<italic>N</italic>
</sub>), and <italic>J</italic>
<sup>(2)</sup>(<italic>&#x3c9;</italic>
<sub>
<italic>N</italic>
</sub>). Nevertheless, this work provided direct proof of nematic fluctuations that diverge near the superconducting transition temperature, <italic>T</italic>
<sub>
<italic>c</italic>
</sub>. Theoretical work has suggested that nematic fluctuations may play a role in the superconducting pairing in these materials [<xref ref-type="bibr" rid="B9">9</xref>, <xref ref-type="bibr" rid="B11">11</xref>].</p>
</sec>
</sec>
</sec>
<sec id="s3">
<title>3 Response to Uniaxial Strain</title>
<p>In the iron based superconductors, the electronic nematic degrees of freedom couple to lattice strain with <italic>B</italic>
<sub>2<italic>g</italic>
</sub> symmetry: <italic>&#x25b;</italic>
<sub>
<italic>B</italic>2<italic>g</italic>
</sub> &#x3d; (<italic>&#x25b;</italic>
<sub>
<italic>xx</italic>
</sub> &#x2212; <italic>&#x25b;</italic>
<sub>
<italic>yy</italic>
</sub>)/2, where <italic>x</italic> and <italic>y</italic> are defined with respect to the tetragonal unit cell as illustrated in <xref ref-type="fig" rid="F3">Figure 3</xref> [<xref ref-type="bibr" rid="B4">4</xref>]. This coupling gives rise to a linear response of the electronic nematicity to external strain on a crystal. Uniaxial strain can be applied via different techniques, however in recent years piezoelectric-based strain cells have demonstrated excellent properties that enable one to carefully control the level of strain even at cryogenic temperatures [<xref ref-type="bibr" rid="B50">50</xref>]. Even though piezoelectric actuators do not have linear response to control voltages, the strain can be controlled through feedback control algorithms for the long periods of time necessary for NMR experiments [<xref ref-type="bibr" rid="B51">51</xref>]. The strain is measured by a capacitive dilatometer. Note that even though the device applies a uniaxial stress, <italic>&#x3c3;</italic>
<sub>0</sub>, along the <italic>x</italic> direction, the response of the crystal is not a pure uniaxial strain. Rather, the non-zero stress tensor elements become: <italic>&#x25b;</italic>
<sub>
<italic>xx</italic>
</sub> &#x3d; <italic>&#x3c3;</italic>
<sub>0</sub>/<italic>E</italic> and <italic>&#x25b;</italic>
<sub>
<italic>yy</italic>
</sub> &#x3d; <italic>&#x25b;</italic>
<sub>
<italic>zz</italic>
</sub> &#x3d; &#x2212;<italic>&#x3bd;&#x3c3;</italic>
<sub>0</sub>/<italic>E</italic>, where <italic>E</italic> is the Young&#x2019;s modulus and <italic>&#x3bd;</italic> is the Poisson&#x2019;s ratio of the material. This gives rise to strain in two symmetry channels:<disp-formula id="e11">
<mml:math id="m34">
<mml:mtable class="eqnarray">
<mml:mtr>
<mml:mtd columnalign="right">
<mml:msub>
<mml:mrow>
<mml:mi>&#x3b5;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>B</mml:mi>
<mml:mn>2</mml:mn>
<mml:mi>g</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mtd>
<mml:mtd columnalign="left">
<mml:mo>&#x3d;</mml:mo>
</mml:mtd>
<mml:mtd columnalign="left">
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3b5;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>x</mml:mi>
<mml:mi>x</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3b5;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>y</mml:mi>
<mml:mi>y</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfenced>
<mml:mo>/</mml:mo>
<mml:mn>2</mml:mn>
<mml:mo>&#x3d;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3c3;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>0</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mfrac>
<mml:mrow>
<mml:mn>1</mml:mn>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>&#x3bd;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:mi>E</mml:mi>
</mml:mrow>
</mml:mfrac>
</mml:mtd>
</mml:mtr>
</mml:mtable>
</mml:math>
<label>(11)</label>
</disp-formula>
<disp-formula id="e12">
<mml:math id="m35">
<mml:mtable class="eqnarray">
<mml:mtr>
<mml:mtd columnalign="right">
<mml:msub>
<mml:mrow>
<mml:mi>&#x3b5;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>A</mml:mi>
<mml:mn>1</mml:mn>
<mml:mi>g</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mtd>
<mml:mtd columnalign="left">
<mml:mo>&#x3d;</mml:mo>
</mml:mtd>
<mml:mtd columnalign="left">
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3b5;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>x</mml:mi>
<mml:mi>x</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2b;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3b5;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>y</mml:mi>
<mml:mi>y</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfenced>
<mml:mo>/</mml:mo>
<mml:mn>2</mml:mn>
<mml:mo>&#x3d;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3c3;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>0</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mfrac>
<mml:mrow>
<mml:mn>1</mml:mn>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>&#x3bd;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:mi>E</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>.</mml:mo>
</mml:mtd>
</mml:mtr>
</mml:mtable>
</mml:math>
<label>(12)</label>
</disp-formula>
</p>
<p>On the other hand, the electronic nematicity has a much stronger response to <italic>B</italic>
<sub>2<italic>g</italic>
</sub> strain than <italic>A</italic>
<sub>1<italic>g</italic>
</sub>, thus uniaxial stress is sufficient to probe the intrinsic <italic>B</italic>
<sub>2<italic>g</italic>
</sub> nematic response [<xref ref-type="bibr" rid="B7">7</xref>].</p>
<sec id="s3-1">
<title>3.1 Spectra</title>
<p>In BaFe<sub>2</sub>As<sub>2</sub>, uniaxial strain dramatically alters the EFG tensor and <italic>&#x3b7;</italic> &#x221d;<italic>&#x25b;</italic>
<sub>
<italic>xx</italic>
</sub>, as illustrated in <xref ref-type="fig" rid="F7">Figure 7</xref> [<xref ref-type="bibr" rid="B32">32</xref>]. In the absence of strain, the crystal remains tetragonal down to the nematic transition temperature <italic>T</italic>
<sub>
<italic>s</italic>
</sub> &#x3d; 135&#xa0;K, in which case the EFG tensor spontaneously develops an asymmetry such that <italic>&#x3bd;</italic>
<sub>
<italic>xx</italic>
</sub> &#x2260; <italic>&#x3bd;</italic>
<sub>
<italic>yy</italic>
</sub>. However, in the presence of a finite strain field, <italic>&#x3b7;</italic> becomes finite above <italic>T</italic>
<sub>
<italic>s</italic>
</sub>. In fact, <italic>&#x3b7;</italic> &#x221d;<italic>&#x25b;</italic>
<sub>
<italic>xx</italic>
</sub> and the constant of proportionality is the nematic susceptibility. As seen in <xref ref-type="fig" rid="F7">Figure 7</xref>, the response is largest just above <italic>T</italic>
<sub>
<italic>s</italic>
</sub>, where the nematic susceptibility diverges. This behavior is illustrated in <xref ref-type="fig" rid="F8">Figure 8</xref>, which reveals that <italic>d&#x3b7;</italic>/<italic>d&#x25b;</italic>
<sub>
<italic>xx</italic>
</sub> &#x2248; 300 at <italic>T</italic>
<sub>
<italic>s</italic>
</sub>.</p>
<fig id="F7" position="float">
<label>FIGURE 7</label>
<caption>
<p>The As EFG components, <italic>&#x3bd;</italic>
<sub>
<italic>a</italic>
</sub> &#x3d; <italic>&#x3bd;</italic>
<sub>
<italic>xx</italic>
</sub> and <italic>&#x3bd;</italic>
<sub>
<italic>b</italic>
</sub> &#x3d; <italic>&#x3bd;</italic>
<sub>
<italic>yy</italic>
</sub>, as a function of temperature and uniaxial strain. The color bar indicates <italic>&#x25b;</italic>
<sub>
<italic>xx</italic>
</sub>. The circles are the measured values from [<xref ref-type="bibr" rid="B18">18</xref>].</p>
</caption>
<graphic xlink:href="fphy-10-877628-g007.tif"/>
</fig>
<fig id="F8" position="float">
<label>FIGURE 8</label>
<caption>
<p>The nematic susceptibility measured by the EFG asymmetry parameter, <italic>&#x3b7;</italic> and via elastoresistance measurements in BaFe<sub>2</sub>As<sub>2</sub>. The solid line is a fit to a Curie-Weiss expression. Reproduced from [<xref ref-type="bibr" rid="B32">32</xref>].</p>
</caption>
<graphic xlink:href="fphy-10-877628-g008.tif"/>
</fig>
<p>Uniaxial stress has also been utilized to study the NMR spectra in LaFeAsO and FeSe [<xref ref-type="bibr" rid="B23">23</xref>]. In this case, compressive stress on the order of 10&#x2013;20&#xa0;MPa was applied by tightening a screw. A similar approach in which a crystal is suspended between the prongs of a horseshoe-shaped device was also utilized for NMR studies under tensile strain [<xref ref-type="bibr" rid="B52">52</xref>]. Neither approach directly measures the strain, precluding the possibility for feedback control. Moreover, differential thermal contraction may also give rise to finite strain fields even without applied stresses via the tightening screw. Nevertheless, such approaches can be used to mechanically detwin the crystal in the nematic phase [<xref ref-type="bibr" rid="B53">53</xref>]. If the crystal is cooled in a finite strain field, then a single nematic domain should nucleate below the transition. For a twinned crystal, there should be two sets of resonances as discussed above in <xref ref-type="sec" rid="s2-3">Section 2.3</xref>. In detwinned or partially de-twinned crystals, the relative intensity changes. In FeSe, this approach enabled the identification of which resonance corresponds to which domain [<xref ref-type="bibr" rid="B23">23</xref>].</p>
</sec>
<sec id="s3-2">
<title>3.2 Relaxation Rate</title>
<p>The spin-lattice-relaxation rate varies strongly with uniaxial strain in BaFe<sub>2</sub>As<sub>2</sub>, as shown in <xref ref-type="fig" rid="F9">Figure 9</xref> [<xref ref-type="bibr" rid="B15">15</xref>]. Strain enhances the relaxation rate and the effect is anisotropic: the enhancement is stronger for in-plane fields than for out-of-plane fields. The enhancement can be understood qualitatively by realizing that strain enhances the antiferromagnetic ordering temperature, <italic>T</italic>
<sub>
<italic>N</italic>
</sub>, thus for <italic>T</italic> &#x3e; <italic>T</italic>
<sub>
<italic>N</italic>
</sub>, the correlation length should grow with increasing strain. The correlation time <italic>&#x3c4;</italic>
<sub>
<italic>c</italic>
</sub> grows with increasing correlation length, thus enhancing <inline-formula id="inf23">
<mml:math id="m36">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula> as illustrated in <xref ref-type="fig" rid="F6">Figure 6</xref>.</p>
<fig id="F9" position="float">
<label>FIGURE 9</label>
<caption>
<p>
<inline-formula id="inf24">
<mml:math id="m37">
<mml:msubsup>
<mml:mrow>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mrow>
<mml:mtext>y,&#x2009;z</mml:mtext>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula> versus strain <bold>(A,C)</bold> and versus temperature <bold>(B,D)</bold>. The solid lines are fits to the data. The <italic>y</italic>, <italic>z</italic> subscripts indicate the direction of the applied magnetic field, <bold>H</bold>
<sub>0</sub>. Reproduced from [<xref ref-type="bibr" rid="B15">15</xref>].</p>
</caption>
<graphic xlink:href="fphy-10-877628-g009.tif"/>
</fig>
<p>A more complete picture of the nematicity and the antiferromagnetism can be obtained by analyzing the reciprocal-space structure of the spin susceptibility tensor, <italic>&#x3c7;</italic>
<sub>
<italic>&#x3b1;&#x3b2;</italic>
</sub>(<bold>q</bold>). In the disordered tetragonal phase, <italic>&#x3c7;</italic>
<sub>
<italic>xx</italic>
</sub>(<bold>q</bold>) &#x3d; <italic>&#x3c7;</italic>
<sub>
<italic>yy</italic>
</sub>(<bold>q</bold>), but in the presence of nematicity these components are no longer equal. In the ordered phase, the susceptibility diverges at the antiferromagnetic ordering wavevectors, <bold>Q</bold>
<sub>1</sub> &#x3d; (<italic>&#x3c0;</italic>, 0) in one domain, and <bold>Q</bold>
<sub>2</sub> &#x3d; (0, <italic>&#x3c0;</italic>) in the other domain. A nematic order parameter can defined as <inline-formula id="inf25">
<mml:math id="m38">
<mml:msub>
<mml:mrow>
<mml:mi>&#x3d5;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
<mml:mi>&#x3b2;</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:msubsup>
<mml:mrow>
<mml:mi>&#x3c7;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
<mml:mi>&#x3b1;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi mathvariant="bold">Q</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:msubsup>
<mml:mrow>
<mml:mi>&#x3c7;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
<mml:mi>&#x3b2;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi mathvariant="bold">Q</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> [<xref ref-type="bibr" rid="B15">15</xref>]. By symmetry, the only non-vanishing components are <italic>&#x3d5;</italic>
<sub>
<italic>xy</italic>
</sub>, <italic>&#x3d5;</italic>
<sub>
<italic>yx</italic>
</sub> and <italic>&#x3d5;</italic>
<sub>
<italic>zz</italic>
</sub>. In the ordered state, only <italic>&#x3d5;</italic>
<sub>
<italic>xy</italic>
</sub> condenses, which corresponds to the spins oriented parallel to the antiferromagnetic ordering vector, as shown in the upper row of <xref ref-type="fig" rid="F2">Figure 2</xref>. <italic>&#x3d5;</italic>
<sub>
<italic>zz</italic>
</sub> order is illustrated in the second row of <xref ref-type="fig" rid="F2">Figure 2</xref>. In this case, the spins are oriented along the <italic>c</italic> direction, and the hyperfine field is in-plane. Although this channel does not condense, <italic>&#x3d5;</italic>
<sub>
<italic>zz</italic>
</sub> fluctuations are present and contribute to <inline-formula id="inf26">
<mml:math id="m39">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula>. <italic>&#x3d5;</italic>
<sub>
<italic>yx</italic>
</sub> is illustrated in the bottom row, where the spins are oriented in-plane and are perpendicular to the antiferromagnetic ordering vector. For <italic>&#x3d5;</italic>
<sub>
<italic>yx</italic>
</sub> order the hyperfine field vanishes, so <inline-formula id="inf27">
<mml:math id="m40">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula> is insensitive to these types of fluctuations.</p>
<p>The anisotropy of <inline-formula id="inf28">
<mml:math id="m41">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula> contains key information about these two nematic channels, <italic>&#x3d5;</italic>
<sub>
<italic>xy</italic>
</sub> and <italic>&#x3d5;</italic>
<sub>
<italic>zz</italic>
</sub>. The fluctuations <italic>h</italic>
<sub>
<italic>&#x3b1;</italic>
</sub>(<italic>&#x3c4;</italic>) of the hyperfine field that contribute to the spin-lattice-relaxation rate as described in <xref ref-type="disp-formula" rid="e10">Eq. 10</xref> are perpendicular to the applied field, <bold>H</bold>
<sub>0</sub>. If <bold>H</bold>
<sub>0</sub> &#x2225;<bold>c</bold>, then the in-plane fluctuations driven by <italic>&#x3d5;</italic>
<sub>
<italic>zz</italic>
</sub> fluctuations will dominate <inline-formula id="inf29">
<mml:math id="m42">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula>. If <bold>H</bold>
<sub>0</sub> &#x22a5;<bold>c</bold>, then both <italic>&#x3d5;</italic>
<sub>
<italic>zz</italic>
</sub> and <italic>&#x3d5;</italic>
<sub>
<italic>xy</italic>
</sub> fluctuations will contribute. As seen in <xref ref-type="fig" rid="F9">Figure 9</xref>, <inline-formula id="inf30">
<mml:math id="m43">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula> measured for <bold>H</bold>
<sub>0</sub> &#x22a5;<bold>c</bold> has a much stronger variation with applied strain. This suggests that <italic>&#x3d5;</italic>
<sub>
<italic>zz</italic>
</sub> fluctuations are enhanced under strain more than <italic>&#x3d5;</italic>
<sub>
<italic>xy</italic>
</sub> fluctuations. In fact, a detailed analysis of the nematic susceptibilities, <inline-formula id="inf31">
<mml:math id="m44">
<mml:msubsup>
<mml:mrow>
<mml:mi>&#x3c7;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>x</mml:mi>
<mml:mi>y</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>n</mml:mi>
<mml:mi>e</mml:mi>
<mml:mi>m</mml:mi>
</mml:mrow>
</mml:msubsup>
<mml:mo>&#x3d;</mml:mo>
<mml:mi>&#x2202;</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3d5;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>x</mml:mi>
<mml:mi>y</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>/</mml:mo>
<mml:mi>&#x2202;</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3b5;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>B</mml:mi>
<mml:mn>2</mml:mn>
<mml:mi>g</mml:mi>
</mml:mrow>
</mml:msub>
</mml:math>
</inline-formula> and <inline-formula id="inf32">
<mml:math id="m45">
<mml:msubsup>
<mml:mrow>
<mml:mi>&#x3c7;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>z</mml:mi>
<mml:mi>z</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>n</mml:mi>
<mml:mi>e</mml:mi>
<mml:mi>m</mml:mi>
</mml:mrow>
</mml:msubsup>
<mml:mo>&#x3d;</mml:mo>
<mml:mi>&#x2202;</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3d5;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>z</mml:mi>
<mml:mi>z</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>/</mml:mo>
<mml:mi>&#x2202;</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3b5;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>B</mml:mi>
<mml:mn>2</mml:mn>
<mml:mi>g</mml:mi>
</mml:mrow>
</mml:msub>
</mml:math>
</inline-formula> indicates that the latter is largest, despite the fact that <italic>&#x3d5;</italic>
<sub>
<italic>xy</italic>
</sub> condenses at zero strain [<xref ref-type="bibr" rid="B15">15</xref>]. These results imply that for sufficient strain, the system would order with the spins oriented along the <italic>c</italic>-axis. This interpretation was recently confirmed by polarized inelastic neutron scattering results [<xref ref-type="bibr" rid="B54">54</xref>].</p>
</sec>
</sec>
<sec id="s4">
<title>4 Glassy Behavior</title>
<sec id="s4-1">
<title>4.1 Relaxation</title>
<p>Measurements of the doped pnictides under strain are challenging because the doping introduces both static and dynamic inhomogeneities. The quadrupolar linewidths of the satellites broaden significantly with doping, thus it is more difficult to discern static changes in the resonances due to strain. Measurements of the spin-lattice-relaxation rate are more straightforward and do not require sharp resonances, but doping introduces a distribution of local hyperfine fields and autocorrelation times, <italic>&#x3c4;</italic>
<sub>
<italic>c</italic>
</sub>, so that there is no longer a homogeneous <inline-formula id="inf33">
<mml:math id="m46">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula> value throughout the bulk of the materials [<xref ref-type="bibr" rid="B16">16</xref>].</p>
<sec id="s4-1-1">
<title>4.1.1 Stretched Relaxation</title>
<p>Heterogeneous spin lattice relaxation is directly manifest in the behavior of the magnetization and leads to a stretching exponent. In this case, the nuclear magnetization is described by:<disp-formula id="e13">
<mml:math id="m47">
<mml:msub>
<mml:mrow>
<mml:mi>M</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>z</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mi>t</mml:mi>
</mml:mrow>
</mml:mfenced>
<mml:mo>&#x3d;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>M</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>e</mml:mi>
<mml:mi>q</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2212;</mml:mo>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>M</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>e</mml:mi>
<mml:mi>q</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>M</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>0</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfenced>
<mml:msup>
<mml:mrow>
<mml:mi>e</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mi>t</mml:mi>
<mml:mo>/</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
</mml:mrow>
</mml:msup>
</mml:mrow>
</mml:msup>
<mml:mo>,</mml:mo>
</mml:math>
<label>(13)</label>
</disp-formula>where <italic>M</italic>
<sub>0</sub> is the initial magnetization, <italic>M</italic>
<sub>
<italic>eq</italic>
</sub> is the thermal equilibrium magnetization, and 0 &#x3c; <italic>&#x3b2;</italic> &#x2264; 1 is a stretching exponent [<xref ref-type="bibr" rid="B55">55</xref>]. <italic>&#x3b2;</italic> &#x3d; 1 corresponds to homogeneous relaxation, but in several doped pnictides <italic>&#x3b2;</italic> &#x223c; 0.4&#x2013;0.9 depending on the doping level and temperature [<xref ref-type="bibr" rid="B16">16</xref>, <xref ref-type="bibr" rid="B56">56</xref>&#x2013;<xref ref-type="bibr" rid="B60">60</xref>]. A typical temperature dependence is shown in <xref ref-type="fig" rid="F10">Figure 10</xref> for <italic>x</italic> &#x3d; 0.06. For temperatures greater than approximately 100&#xa0;K, the relaxation is homogeneous, but below this temperature <italic>&#x3b2;</italic> decreases from unity to approximately 0.4 at <italic>T</italic>
<sub>
<italic>N</italic>
</sub>. The exponent <italic>&#x3b2;</italic> is a measure of the width of the distribution of local relaxation rates, <inline-formula id="inf34">
<mml:math id="m48">
<mml:mi mathvariant="script">P</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula>, where <italic>W</italic>
<sub>1</sub> is the relaxation rate. <inline-formula id="inf35">
<mml:math id="m49">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula>, is the median of this distribution and <italic>&#x3b2;</italic> is related to the logarithmic FWHM of <inline-formula id="inf36">
<mml:math id="m50">
<mml:mi mathvariant="script">P</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> [<xref ref-type="bibr" rid="B55">55</xref>]. When <italic>&#x3b2;</italic> &#x3d; 1, the distribution is a delta function, and as <italic>&#x3b2;</italic> decreases the width of <inline-formula id="inf37">
<mml:math id="m51">
<mml:mi mathvariant="script">P</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> increases exponentially. <xref ref-type="fig" rid="F10">Figure 10</xref> indicates that for <italic>x</italic> &#x3d; 0.06 just above <italic>T</italic>
<sub>
<italic>N</italic>
</sub> the distribution of relaxation rates is at least two to three orders of magnitude in width. Additionally, the average correlation time, <italic>&#x3c4;</italic>
<sub>
<italic>c</italic>
</sub>, does not have a power law divergence, but rather an activated or Vogel-Fulcher behavior with temperature, which tends to broaden the peak in <inline-formula id="inf38">
<mml:math id="m52">
<mml:msup>
<mml:mrow>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msup>
</mml:math>
</inline-formula> with temperature, as illustrated in <xref ref-type="fig" rid="F6">Figure 6</xref>.</p>
<fig id="F10" position="float">
<label>FIGURE 10</label>
<caption>
<p>
<bold>(A)</bold> <inline-formula id="inf39">
<mml:math id="m53">
<mml:msup>
<mml:mrow>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msup>
</mml:math>
</inline-formula> and <bold>(B)</bold> <italic>&#x3b2;</italic> versus temperature measured in Ba(Fe<sub>1&#x2212;<italic>x</italic>
</sub>Co<sub>
<italic>x</italic>
</sub>)<sub>2</sub>As<sub>2</sub> with <italic>x</italic> &#x3d; 0.06.</p>
</caption>
<graphic xlink:href="fphy-10-877628-g010.tif"/>
</fig>
</sec>
<sec id="s4-1-2">
<title>4.1.2 Inverse Laplace Transform</title>
<p>Rather than fitting the magnetization with a stretched exponent, as in <xref ref-type="disp-formula" rid="e13">Eq. 13</xref>, it is possible to fit the data assuming a particular form of <inline-formula id="inf40">
<mml:math id="m54">
<mml:mi mathvariant="script">P</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula>. One such approach is via a log-normal distribution, where:<disp-formula id="e14">
<mml:math id="m55">
<mml:mi mathvariant="script">P</mml:mi>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfenced>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:msqrt>
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:mi>&#x3c0;</mml:mi>
</mml:mrow>
</mml:msqrt>
</mml:mrow>
</mml:mfrac>
<mml:msup>
<mml:mrow>
<mml:mi>e</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mi>ln</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>&#x3bc;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mo>/</mml:mo>
<mml:mn>2</mml:mn>
<mml:msup>
<mml:mrow>
<mml:mi>&#x3c3;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
</mml:mrow>
</mml:msup>
<mml:mo>.</mml:mo>
</mml:math>
<label>(14)</label>
</disp-formula>
</p>
<p>In this case the median of the distribution (<inline-formula id="inf41">
<mml:math id="m56">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula>) is <italic>e</italic>
<sup>
<italic>&#x3bc;</italic>
</sup>, and the standard deviation is <inline-formula id="inf42">
<mml:math id="m57">
<mml:msub>
<mml:mrow>
<mml:mi>&#x3c3;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:msqrt>
<mml:mrow>
<mml:msup>
<mml:mrow>
<mml:mi>e</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:mi>&#x3bc;</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mi>&#x3c3;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
</mml:mrow>
</mml:msup>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msup>
<mml:mrow>
<mml:mi>e</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:msup>
<mml:mrow>
<mml:mi>&#x3c3;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
</mml:mrow>
</mml:msup>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:msqrt>
</mml:math>
</inline-formula> <italic>&#x3c3;</italic>
<sub>1</sub> is roughly inversely proportional to <italic>&#x3b2;</italic>. The relaxation in the pnictides is well-captured by this form of the distribution [<xref ref-type="bibr" rid="B16">16</xref>].</p>
<p>An alternative approach is to extract <inline-formula id="inf43">
<mml:math id="m58">
<mml:mi mathvariant="script">P</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> directly from the data, rather than to assume a particular form. This is known as an inverse Laplace transform (ILT), and has been utilized to investigate a range of correlated electron systems [<xref ref-type="bibr" rid="B61">61</xref>&#x2013;<xref ref-type="bibr" rid="B63">63</xref>]. <xref ref-type="fig" rid="F11">Figure 11</xref> displays representative data set with such a fit, and <xref ref-type="fig" rid="F12">Figure 12</xref> shows the distribution versus temperature extracted using this approach in Ba(Fe<sub>1&#x2212;<italic>x</italic>
</sub>Co<sub>
<italic>x</italic>
</sub>)<sub>2</sub>As<sub>2</sub> with <italic>x</italic> &#x3d; 0.059. It is clear that both the median and width of this distribution change in the vicinity of <italic>T</italic>
<sub>
<italic>N</italic>
</sub>, and that the width approaches several orders of magnitude. The ILT approach does not make any a priori assumptions about the distribution, and may uncover features that are not captured by <xref ref-type="disp-formula" rid="e14">Eq. 14</xref>. On the other hand, the ILT requires time series data with high a signal-to-noise ratio, a complicated analysis algorithm, and assumptions about the smoothness of the distribution [<xref ref-type="bibr" rid="B64">64</xref>]. The distribution shown in <xref ref-type="fig" rid="F12">Figure 12</xref> exhibits several structures for <italic>T</italic> &#x226a; <italic>T</italic>
<sub>
<italic>N</italic>
</sub> that are likely artifacts due to the poor signal to noise at these temperatures. Ultimately, the most meaningful information about the distribution appear to be the median and width, which are well-captured by the stretched exponential approach. Note that although the <sup>75</sup>As has <italic>I</italic> &#x3d; 3/2 and hence a multi-exponential relaxation form even for homogeneous relaxation, the stretched exponential approach accurately captures the true distribution of relaxation rates, <inline-formula id="inf44">
<mml:math id="m59">
<mml:mi mathvariant="script">P</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> [<xref ref-type="bibr" rid="B64">64</xref>].</p>
<fig id="F11" position="float">
<label>FIGURE 11</label>
<caption>
<p>Magnetization versus recovery time measured at 50&#xa0;K in Ba (Fe<sub>1&#x2212;<italic>x</italic>
</sub>Co<sub>
<italic>x</italic>
</sub>)<sub>2</sub>As<sub>2</sub> with <italic>x</italic> &#x3d; 0.06. Panel <bold>(A)</bold> shows the raw data, and panel <bold>(B)</bold> shows the data after normalization such that <italic>M</italic>(<italic>&#x221e;</italic>) &#x3d; 1 and <italic>M</italic>(0) &#x3d; &#x2212;1. The solid line shows the fit using the ILT algorithm.</p>
</caption>
<graphic xlink:href="fphy-10-877628-g011.tif"/>
</fig>
<fig id="F12" position="float">
<label>FIGURE 12</label>
<caption>
<p>Distribution of relaxation rates, <inline-formula id="inf45">
<mml:math id="m60">
<mml:mi mathvariant="script">P</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> versus temperature shown as contour lines in Ba(Fe<sub>1&#x2212;<italic>x</italic>
</sub>Co<sub>
<italic>x</italic>
</sub>)<sub>2</sub>As<sub>2</sub> with <italic>x</italic> &#x3d; 0.06, extracted by inverse Laplace transform. Contour lines are shown between <inline-formula id="inf46">
<mml:math id="m61">
<mml:mi mathvariant="script">P</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>0.01</mml:mn>
</mml:math>
</inline-formula> to 0.15 in intervals of 0.01. The solid black circles shows the median of the distribution at teach temperature. The contributions near 10<sup>5</sup> sec<sup>&#x2212;1</sup> are artifacts introduced by normalization errors for early recovery times.</p>
</caption>
<graphic xlink:href="fphy-10-877628-g012.tif"/>
</fig>
</sec>
<sec id="s4-1-3">
<title>4.1.3 Nematicity and Dynamical Heterogeneity</title>
<p>Similar glassy behavior has been observed in the cuprates and been associated with stripe-glass behavior [<xref ref-type="bibr" rid="B65">65</xref>&#x2013;<xref ref-type="bibr" rid="B73">73</xref>]. The cuprates, however, are doped Mott insulators, and the glassy behavior was attributed to intrinsic frustration between the competing effects of Coulomb repulsion and charge segregation [<xref ref-type="bibr" rid="B74">74</xref>&#x2013;<xref ref-type="bibr" rid="B76">76</xref>]. The iron arsenides do not exhibit charge ordering and thus a different mechanism must be driving the glassy dynamics. This behavior is present for a range of doping levels, and is most pronounced near optimal doping where <italic>T</italic>
<sub>
<italic>c</italic>
</sub> reaches a maximum. <xref ref-type="fig" rid="F13">Figure 13</xref> shows a phase diagram for both Cu and Co doping. Like Co, Cu introduces extra electrons but it also suppresses superconductivity [<xref ref-type="bibr" rid="B77">77</xref>]. The color scale indicates the standard deviation of a log-normal distribution fit, <italic>&#x3c3;</italic>
<sub>1</sub>. As shown in <xref ref-type="fig" rid="F13">Figure 13</xref>, the distribution exhibits the greatest width in the vicinity of a putative nematic quantum critical point near <italic>x</italic> &#x223c; 0.07 if there were no superconductivity. This behavior is striking because it bears a similarity to the divergent nematic susceptibility measured by elastoresistance in these materials [<xref ref-type="bibr" rid="B7">7</xref>, <xref ref-type="bibr" rid="B8">8</xref>]. In other words, <italic>the width of the distribution of relaxation rates correlates with the magnitude of the nematic susceptibility</italic>.</p>
<fig id="F13" position="float">
<label>FIGURE 13</label>
<caption>
<p>Phase diagram of Ba(Fe<sub>1&#x2212;<italic>x</italic>
</sub>Cu<sub>
<italic>x</italic>
</sub>)<sub>2</sub>As<sub>2</sub> and Ba(Fe<sub>1&#x2212;<italic>x</italic>
</sub>Co<sub>
<italic>x</italic>
</sub>)<sub>2</sub>As<sub>2</sub> with the width of the distribution, <italic>&#x3c3;</italic>
<sub>1</sub> shown as the color scale. The blue diamonds represent <italic>T</italic>
<sub>
<italic>s</italic>
</sub>, the red circles represent <italic>T</italic>
<sub>
<italic>N</italic>
</sub>, and the green triangles represent <italic>T</italic>
<sub>
<italic>c</italic>
</sub>. Reproduced from [<xref ref-type="bibr" rid="B16">16</xref>].</p>
</caption>
<graphic xlink:href="fphy-10-877628-g013.tif"/>
</fig>
<p>What is the origin of this glassy behavior, and is there a physical connection with the nematic susceptibility? A compelling hypothesis is that the dopants introduce quenched random strain fields that couple to the nematic order parameter and give rise to a distribution of local correlation times, <italic>&#x3c4;</italic>
<sub>
<italic>c</italic>
</sub>. Local strains can nucleate different nematic domains, even in absence of long range nematic order. The result is a nematic glass, in which a distribution of local nematic domains (with different orientations) exist throughout the sample, each fluctuating with a different correlations times. These nematic fluctuations in turn drive spin fluctuations that are reflected in the distribution <inline-formula id="inf47">
<mml:math id="m62">
<mml:mi mathvariant="script">P</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula>.</p>
<p>Another hypothesis for the inhomogeneous dynamics is that static inhomogeneity of the EFG and Knight shift tensors induced by the dopants suppresses spin diffusion among the nuclear spins, so that they do not all relax with a common spin temperature. In principle, dipolar interactions between neighboring nuclear spins <bold>I</bold>
<sub>1</sub> and <bold>I</bold>
<sub>2</sub> may contain terms such as <inline-formula id="inf48">
<mml:math id="m63">
<mml:msub>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mi>I</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">&#x302;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
<mml:mo>&#x2b;</mml:mo>
</mml:mrow>
</mml:msub>
<mml:msub>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mi>I</mml:mi>
</mml:mrow>
<mml:mo stretchy="false">&#x302;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:mo>&#x2212;</mml:mo>
</mml:mrow>
</mml:msub>
</mml:math>
</inline-formula>, which can give rise to mutual spin flips [<xref ref-type="bibr" rid="B78">78</xref>]. This effect could enable nuclei in regions that exhibit fast relaxation to transfer polarization with those in regions with slow relaxation, giving rise to a more homogeneous relaxation throughout the sample. If the static EFG and Knight shift tensors vary spatially, however, then mutual spin flips between neighbors would not conserve energy. In fact, spin diffusion should behave differently for a spin-1/2 versus a spin-3/2 nucleus. For the latter there are only six out of sixteen possible configurations where the two neighbors can undergo a mutual spin flip while conserving energy, whereas there are two out of four possibilities for the former. Thus spin-diffusion should be suppressed for <sup>75</sup>As relative to <sup>31</sup>P, and thus one might expect <italic>&#x3b2;</italic> to be closer to unity for the spin-1/2 <sup>31</sup>P. In fact, both sites exhibit similar values of <italic>&#x3b2;</italic> at all temperatures in BaFe<sub>2</sub>(As,P)<sub>2</sub> [<xref ref-type="bibr" rid="B43">43</xref>]. These results suggest, therefore, that spin diffusion does not play a significant role in the observed glassy dynamics.</p>
</sec>
<sec id="s4-1-4">
<title>4.1.4 Edwards-Anderson Parameter</title>
<p>In a recent paper, Wiecki and collaborators pointed out that the NMR linewidth of <sup>77</sup>Se in FeSe is directly proportional to the Edwards-Anderson parameter in a random-field Ising model of the nematicity [<xref ref-type="bibr" rid="B42">42</xref>]. Crystal defects provide local strain fields, <italic>h</italic>
<sub>
<italic>i</italic>
</sub>, at site <italic>i</italic>, and the enhanced nematic susceptibility gives rise to large spatial variations of local nematicity, <italic>&#x3d5;</italic>
<sub>
<italic>i</italic>
</sub>(<italic>h</italic>
<sub>
<italic>i</italic>
</sub>) (we drop the distinction between <italic>&#x3d5;</italic>
<sub>
<italic>xy</italic>
</sub>, <italic>&#x3d5;</italic>
<sub>
<italic>yx</italic>
</sub> and <italic>&#x3d5;</italic>
<sub>
<italic>zz</italic>
</sub> for simplicity). In this case, the Knight shift is known to vary linearly with <italic>&#x3d5;</italic>, and the second moment of the NMR spectrum is directly proportional to the Edwards-Anderson parameter: <inline-formula id="inf49">
<mml:math id="m64">
<mml:msub>
<mml:mrow>
<mml:mi>q</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>E</mml:mi>
<mml:mi>A</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mo>&#x3d;</mml:mo>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mo stretchy="false">&#x2329;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mi>&#x3d5;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mo stretchy="false">&#x232a;</mml:mo>
</mml:mrow>
<mml:mo>&#x304;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mo stretchy="false">&#x2329;</mml:mo>
<mml:mi>&#x3d5;</mml:mi>
<mml:mo stretchy="false">&#x232a;</mml:mo>
</mml:mrow>
<mml:mo>&#x304;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
</mml:math>
</inline-formula>, where the brackets indicate a thermal average and the overbar indicates an average over disorder configurations.</p>
<p>A similar approach can be utilized to analyze the distribution of relaxation rates, <inline-formula id="inf50">
<mml:math id="m65">
<mml:mi mathvariant="script">P</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula>. In undoped BaFe<sub>2</sub>As<sub>2</sub>, the spin lattice relaxation rate is a function of the nematic order parameter:<disp-formula id="e15">
<mml:math id="m66">
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mi>&#x3d5;</mml:mi>
</mml:mrow>
</mml:mfenced>
<mml:mo>&#x3d;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mn>0</mml:mn>
</mml:mrow>
</mml:mfenced>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>&#x3b1;</mml:mi>
<mml:mi>&#x3d5;</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:mo>&#x22ef;</mml:mo>
<mml:mspace width="0.17em"/>
<mml:mo>,</mml:mo>
</mml:math>
<label>(15)</label>
</disp-formula>where <italic>&#x3b1;</italic> depends the correlation length, and is hence strongly temperature dependent [<xref ref-type="bibr" rid="B15">15</xref>]. In the doped system, we can model the distribution of relaxation rates by assuming a distribution of local strain fields, so that:<disp-formula id="e16">
<mml:math id="m67">
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mi mathvariant="script">P</mml:mi>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x304;</mml:mo>
</mml:mover>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mi>N</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x222b;</mml:mo>
<mml:munderover accentunder="false" accent="false">
<mml:mrow>
<mml:mo>&#x220f;</mml:mo>
</mml:mrow>
<mml:mrow>
<mml:mi>j</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mi>N</mml:mi>
</mml:mrow>
</mml:munderover>
<mml:mi>d</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mi>h</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>j</mml:mi>
</mml:mrow>
</mml:msub>
<mml:msub>
<mml:mrow>
<mml:mi>p</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>&#x3c3;</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>h</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>j</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfenced>
<mml:munderover accentunder="false" accent="false">
<mml:mrow>
<mml:mo>&#x2211;</mml:mo>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mi>N</mml:mi>
</mml:mrow>
</mml:munderover>
<mml:mi>&#x3b4;</mml:mi>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:mn>0</mml:mn>
</mml:mrow>
</mml:mfenced>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>&#x3b1;</mml:mi>
<mml:msub>
<mml:mrow>
<mml:mi>&#x3d5;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mfenced open="(" close=")">
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>h</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>i</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mfenced>
<mml:mo>,</mml:mo>
</mml:math>
<label>(16)</label>
</disp-formula>where <italic>p</italic>
<sub>
<italic>&#x3c3;</italic>
</sub>(<italic>h</italic>
<sub>
<italic>j</italic>
</sub>) is the disorder distribution [<xref ref-type="bibr" rid="B42">42</xref>]. The second moment of <inline-formula id="inf51">
<mml:math id="m68">
<mml:mrow>
<mml:mover accent="true">
<mml:mrow>
<mml:mi mathvariant="script">P</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>&#x304;</mml:mo>
</mml:mover>
</mml:mrow>
</mml:math>
</inline-formula> is <inline-formula id="inf52">
<mml:math id="m69">
<mml:msubsup>
<mml:mrow>
<mml:mi>&#x3c3;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msubsup>
<mml:mo>&#x3d;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
</mml:mrow>
</mml:msup>
<mml:msub>
<mml:mrow>
<mml:mi>q</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>E</mml:mi>
<mml:mi>A</mml:mi>
</mml:mrow>
</mml:msub>
</mml:math>
</inline-formula>, thus the second moment of the distribution measures the Edwards-Anderson order parameter.</p>
<p>As shown in <xref ref-type="fig" rid="F13">Figure 13</xref>, <italic>&#x3c3;</italic>
<sub>1</sub> is a strong function of temperature and doping. The magnitude of this quantity is given in part by the coefficient <italic>&#x3b1;</italic>, reflecting the growth of antiferromagnetic fluctuations. Note, however, that <italic>&#x3c3;</italic>
<sub>1</sub> would be zero if <italic>q</italic>
<sub>
<italic>EA</italic>
</sub> &#x3d; 0. In other words, <italic>&#x3c3;</italic>
<sub>1</sub> is finite because the Edwards-Anderson parameter is non-zero, which indicates the presence of a nematic glass. Higher order corrections to the relationship between <italic>W</italic>
<sub>1</sub> and strain, and the presence of other strain channels due the dopant atoms, are likely to modify the quantitative relationship between <italic>&#x3c3;</italic>
<sub>1</sub> and <italic>q</italic>
<sub>
<italic>EA</italic>
</sub>, and these issues should be addressed in future theoretical work.</p>
</sec>
</sec>
<sec id="s4-2">
<title>4.2 Response to Strain</title>
<p>In principle, an <italic>external</italic> strain field of sufficient magnitude might overcome the local strain fields and give rise to more homogeneous relaxation. This hypothesis was tested in Ba(Fe<sub>1&#x2212;<italic>x</italic>
</sub>Co<sub>
<italic>x</italic>
</sub>)<sub>2</sub>As<sub>2</sub> with <italic>x</italic> &#x3d; 0.048 under tensile strain [<xref ref-type="bibr" rid="B52">52</xref>]. Although the magnitude of <inline-formula id="inf53">
<mml:math id="m70">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula> changed in response to the strain field, no changes were observed to the stretching exponent. This observation suggests that the intrinsic strains around the dopants exceed the homogeneous external strain, so that <inline-formula id="inf54">
<mml:math id="m71">
<mml:mi mathvariant="script">P</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> remains unchanged under strain. In fact, the lattice strain around Co dopants in Ba(Fe<sub>1&#x2212;<italic>x</italic>
</sub>Co<sub>
<italic>x</italic>
</sub>)<sub>2</sub>As<sub>2</sub> can reach several percent [<xref ref-type="bibr" rid="B79">79</xref>]. The applied strain was only a fraction of a percent, thus it is not surprising that no change was observed in the width of the distribution.</p>
</sec>
<sec id="s4-3">
<title>4.3 Strain Hysteresis</title>
<p>Although the width of the <inline-formula id="inf55">
<mml:math id="m72">
<mml:mi mathvariant="script">P</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> does not change with externally applied strain, the median of the distribution does, and in a manner that depends on the strain history. <xref ref-type="fig" rid="F14">Figure 14</xref> illustrates a protocol to investigate such hysteretic effects. A crystal is strain-cooled either under compressive (or tensile) strain from room temperature down to a base temperature. The spin lattice relaxation is then measured for a series of different levels of increasing (or decreasing) strain at constant temperature. The sample is then returned to room temperature (where the relaxation is homogeneous and there is no glassy behavior), and then the process is repeated under the opposite direction. For a fully linear response, the spin lattice relaxation as a function of strain should be independent of whether it was tensile-cooled or compressive-cooled.</p>
<fig id="F14" position="float">
<label>FIGURE 14</label>
<caption>
<p>Protocol for strain hysteresis measurements. The sample is first cooled (red arrows) in a compressive strain field from room temperature. Spin lattice relaxation measurements are then conducted at several different increasing strain levels as the displacement increases. The sample is then returned to room temperature and zero strain. Finally the sample is strain cooled under tensile strain to the same base temperature and measurements are conducted for several values of decreasing displacement. <xref ref-type="fig" rid="F15">Figure 15</xref> compares the measured values for both protocols for various temperatures.</p>
</caption>
<graphic xlink:href="fphy-10-877628-g014.tif"/>
</fig>
<p>
<xref ref-type="fig" rid="F15">Figure 15</xref> shows the results of such a study on Ba(Fe<sub>1&#x2212;<italic>x</italic>
</sub>Co<sub>
<italic>x</italic>
</sub>)<sub>2</sub>As<sub>2</sub> for four different base temperatures for <italic>x</italic> &#x3d; 0.059. As expected, <italic>&#x3b2;</italic> decreases as temperature is reduced, but remains independent of the applied strain, and is the same for both tensile- and compressive-cooling. On the other hand, the median of the distribution, <inline-formula id="inf56">
<mml:math id="m73">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula>, is strain-dependent and is different under the two strain conditions at low temperature.</p>
<fig id="F15" position="float">
<label>FIGURE 15</label>
<caption>
<p>
<inline-formula id="inf57">
<mml:math id="m74">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula> and <italic>&#x3b2;</italic> versus displacement for several different temperatures in Ba(Fe<sub>1&#x2212;<italic>x</italic>
</sub>Co<sub>
<italic>x</italic>
</sub>)<sub>2</sub>As<sub>2</sub> with <italic>x</italic> &#x3d; 0.059. The red and green points represent data obtained during compressive field cooled and tensile field cooled protocols, as illustrated in <xref ref-type="fig" rid="F14">Figure 14</xref>.</p>
</caption>
<graphic xlink:href="fphy-10-877628-g015.tif"/>
</fig>
<p>Note that the horizontal axes in <xref ref-type="fig" rid="F15">Figure 15</xref> are displacement, not strain. Strain is defined as <italic>&#x25b;</italic> &#x3d; (<italic>d</italic> &#x2212; <italic>d</italic>
<sub>0</sub>)/<italic>L</italic>, where <italic>d</italic> is the displacement of the capacitative dilatometer, <italic>d</italic>
<sub>0</sub> is the equilibrium unstrained displacement, and <italic>L</italic> is the sample length. <italic>d</italic>
<sub>0</sub> can be determined at room temperature, but thermal contractions of both the sample and the strain device make it difficult to determine <italic>d</italic>
<sub>0</sub> under cryogenic conditions. It is best to utilize an independent measure of strain, such as the EFG tensor discussed in <xref ref-type="sec" rid="s3-1">Section 3.1</xref>, to find the displacement corresponding to <italic>&#x25b;</italic> &#x3d; 0. Such a calibration was not possible for the <inline-formula id="inf58">
<mml:math id="m75">
<mml:msubsup>
<mml:mrow>
<mml:mi>T</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msubsup>
</mml:math>
</inline-formula> measurements in <xref ref-type="fig" rid="F15">Figure 15</xref>. It is also important to note that the level of strain during the cooling part of the protocol in <xref ref-type="fig" rid="F14">Figure 14</xref> is likely temperature-dependent, rather than constant as illustrated. Again, this is due to differential thermal contractions between the sample and the strain device. The displacement measured by the dilatometer is the quantity that is held constant.</p>
<p>Despite these complications, these measurements reveal that <inline-formula id="inf59">
<mml:math id="m76">
<mml:mi mathvariant="script">P</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula>, and presumably the distribution of local nematic domains, depends on the past history of applied strain. Hysteresis is commonly observed in ordered ferromagnets, in which the static bulk magnetization is hysteretic with the applied field. If the applied field exceeds the coercive field, the magnetization will saturate, and when the applied field is reduced to zero, a remnant magnetization remains. Similar behavior should be expected in an ordered nematic without quenched disorder, in which nematic domains can reorient in an external strain field [<xref ref-type="bibr" rid="B80">80</xref>]. The NMR measurements described here, on the other hand, are in a nematic glass phase with quenched disorder, and probe the distribution of local correlation times of different fluctuating domains. Hysteresis has been studied in magnetic materials with quenched disorder in both the weak-disorder limit in the paramagnetic phase, as well in the strong-disorder limit in the spin glass phase [<xref ref-type="bibr" rid="B81">81</xref>]. The particular domain pattern is likely determined by the combination of local strains and the external strain field applied during the cool down. The fluctuation time of the domains is a complicated function of these strain fields as well as the behavior of their neighboring nematic domains. As the external strain field changes, the local correlation times change, but in such a manner that the median of the distribution of correlation times changes, but not the standard deviation. If the system were homogenous and not glassy, then the nematic domains would be mobile and there would be a single average correlation time. The presence of a distribution of correlation times that is altered by external strain provides evidence for the formation of a nematic glass, in which some domains exhibit very large correlation times, whereas others have short correlation times and may be reoriented by small external strain fields.</p>
</sec>
<sec id="s4-4">
<title>4.4 Theoretical Models</title>
<p>A quantitative theory to connect the measured distribution of the spin-lattice-relaxation rate, <inline-formula id="inf60">
<mml:math id="m77">
<mml:mi mathvariant="script">P</mml:mi>
<mml:mrow>
<mml:mo stretchy="false">(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mi>W</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo stretchy="false">)</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula>, to the nematic domains and their dynamics in the presence of external strain, particularly in the context of the iron pnictides, is highly desirable. Although no such theory yet exists, there are important models that capture elements of the glassy behavior in these materials. Nematic ordering in the presence of random strain fields can be mapped onto the random field Ising model (RFIM) [<xref ref-type="bibr" rid="B80">80</xref>, <xref ref-type="bibr" rid="B82">82</xref>, <xref ref-type="bibr" rid="B83">83</xref>]. Detailed numerical simulations have uncovered a broad distribution of local correlation times, which agrees qualitatively with the observations of stretched relaxation in NMR experiments [<xref ref-type="bibr" rid="B16">16</xref>].</p>
<p>On the other hand, the iron pnictides exhibit both antiferromgnetism and nematicity, and there are two types of spin order for each of two possible nematic domains, as illustrated in <xref ref-type="fig" rid="F2">Figure 2</xref>. Recently, a random Baxter-field model was proposed as an alternative to capture both the nematic and antiferromagnetic fluctuations in the presence of quenched random strain fields [<xref ref-type="bibr" rid="B84">84</xref>]. In this case, there are two Ising variables at each lattice site associated with the magnetic and the nematic degree of freedom. These two variables are coupled due to the next nearest neighbor coupling, <italic>J</italic>
<sub>2</sub>, in the <italic>J</italic>
<sub>1</sub> &#x2212; <italic>J</italic>
<sub>2</sub> model for the iron pnictides [<xref ref-type="bibr" rid="B4">4</xref>]. Random strain fields couple only to the nematic degree of freedom, but the magnetic variable is also affected and consequently the system breaks up into domains of all four configurations illustrated in the top row of <xref ref-type="fig" rid="F2">Figure 2</xref>.</p>
</sec>
</sec>
<sec id="s5">
<title>5 Summary and Conclusion</title>
<p>NMR is a powerful tool to investigate nematicity in the iron based superconductors, providing microscopic insight in the local antiferromagnetic and nematic order parameters. Investigations of the NMR response to uniaxial strain in BaFe<sub>2</sub>As<sub>2</sub> and FeSe have revealed important information about the anisotropy of the dynamical and static spin susceptibilities. In particular, the temperature dependence of the spin fluctuations under strain reflect an unusual piezomagnetic response in which the antiferromagnetically ordered spins can change their orientation direction under sufficient strain.</p>
<p>The doped pnictides have been less studied under strain because static and dynamical heterogeneity present in these materials render interpretation of results more difficult. Strain fields surrounding dopants create random fields that couple to the nematic order parameter, which may have a large response at low temperature. As a result, the NMR spectra broaden significantly, reflecting a distribution of static EFGs, some of which may indicate static local nematic order. More importantly, the NMR spin lattice relaxation rate reveals a broad distribution of local spin fluctuations that gradually freeze out at lower temperatures. This distribution likely reflects the correlated nematic fluctuations breaking up into spatial domains in a nematic glass. This distribution depends on the history of the strain field, but remains broad even at the highest uniaxial strain levels applied. These results suggest that quenched disorder creates large random strain fields.</p>
<p>Future studies on other doped materials may shed important light on the nature of the nematic glass. For example, hole doping by substituting Ba with K may introduce milder levels of local strain fields, in which case external strain might be able to induce homogeneous relaxation. Studies of static hysteretic behavior with strain in the ordered nematic phase may also shed important light on the mesoscopic physics of the domain formation, the coercive strain fields, and remnant nematicity. Unfortunately, NMR studies under strain require small crystals, and the NMR signal in doped samples tends to be suppressed due to the same glassy physics giving rise to the stretched relaxation. These effects conspire to make such experiments on doped samples particularly challenging.</p>
</sec>
</body>
<back>
<sec id="s6">
<title>Data Availability Statement</title>
<p>The raw data supporting the conclusion of this article will be made available by the authors, without undue reservation.</p>
</sec>
<sec id="s7">
<title>Author Contributions</title>
<p>TK acquired the NMR data on crystals grown and characterized by MT, RP, SB and PC, and NC conceived the experiments and wrote the manuscript.</p>
</sec>
<sec id="s8">
<title>Funding</title>
<p>Work at UC Davis was supported by the NSF under Grant No. DMR-1807889, and the UC Laboratory Fees Research Program (LFR-20-653926). Work at Ames Lab (PC, SB, RP, MT for growth and basic characterization of samples) was supported by the U.S. Department of Energy, Office of Basic Energy Science, Division of Materials Sciences and Engineering. Ames Laboratory is operated for the U.S. Department of Energy by Iowa State University under Contract No. DE-AC02-07CH11358.</p>
</sec>
<sec sec-type="COI-statement" id="s9">
<title>Conflict of Interest</title>
<p>The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.</p>
</sec>
<sec sec-type="disclaimer" id="s10">
<title>Publisher&#x2019;s Note</title>
<p>All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.</p>
</sec>
<ack>
<p>We thank Erica Carlson, Karin Dahmen, Stylianos Gregoriou, Lamei Nie and Rafael Fernandes for stimulating discussions.</p>
</ack>
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