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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Chem.</journal-id>
<journal-title>Frontiers in Chemistry</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Chem.</abbrev-journal-title>
<issn pub-type="epub">2296-2646</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="publisher-id">751203</article-id>
<article-id pub-id-type="doi">10.3389/fchem.2021.751203</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Chemistry</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>Ab Initio Study of the Large Amplitude Motions of Various Monosubstituted Isotopologues of Methylamine (CH<sub>3</sub>-NH<sub>2</sub>)</article-title>
<alt-title alt-title-type="left-running-head">Al-Mogren and Senent</alt-title>
<alt-title alt-title-type="right-running-head">Methylamine</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname>Al-Mogren</surname>
<given-names>Muneerah Mogren</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/915313/overview"/>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Senent</surname>
<given-names>Mar&#xed;a Luisa</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1369912/overview"/>
</contrib>
</contrib-group>
<aff id="aff1">
<label>
<sup>1</sup>
</label>Chemistry Department, Faculty of Science, King Saud University, <addr-line>Riyadh</addr-line>, <country>Saudi Arabia</country>
</aff>
<aff id="aff2">
<label>
<sup>2</sup>
</label>Departamento de Qu&#xed;mica y F&#xed;sica Te&#xf3;ricas, Instituto de Estructura de La Materia, IEM-CSIC, <addr-line>Madrid</addr-line>, <country>Spain</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/938293/overview">Bouthe&#xef;na Kerkeni</ext-link>, Manouba University, Tunisia</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/685773/overview">Antonio Fernandez-Ramos</ext-link>, Universidad de Santiago de Compostela, Spain</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/949249/overview">Nicola Tasinato</ext-link>, Normal School of Pisa, Italy</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Mar&#xed;a Luisa Senent, <email>ml.senent@csic.es</email>
</corresp>
<fn fn-type="other">
<p>This article was submitted to Astrochemistry, a section of the journal Frontiers in Chemistry</p>
</fn>
</author-notes>
<pub-date pub-type="epub">
<day>23</day>
<month>09</month>
<year>2021</year>
</pub-date>
<pub-date pub-type="collection">
<year>2021</year>
</pub-date>
<volume>9</volume>
<elocation-id>751203</elocation-id>
<history>
<date date-type="received">
<day>31</day>
<month>07</month>
<year>2021</year>
</date>
<date date-type="accepted">
<day>08</day>
<month>09</month>
<year>2021</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2021 Al-Mogren and Senent.</copyright-statement>
<copyright-year>2021</copyright-year>
<copyright-holder>Al-Mogren and Senent</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&#x20;terms.</p>
</license>
</permissions>
<abstract>
<p>CCSD(T)-F12 theory is applied to determine electronic ground state spectroscopic parameters of various isotopologues of methylamine (CH<sub>3</sub>-NH<sub>2</sub>) containing cosmological abundant elements, such as D, <sup>13</sup>C and <sup>15</sup>N. Special attention is given to the far infrared region. The studied isotopologues can be classified in the G<sub>12</sub>, G<sub>6</sub> and G<sub>4</sub> molecular symmetry groups. The rotational and centrifugal distortion constants and the anharmonic fundamentals are determined using second order perturbation theory. Fermi displacements of the vibrational bands are predicted. The low vibrational energy levels corresponding to the large amplitude motions are determine variationally using a flexible three-dimensional model depending on the NH<sub>2</sub> bending and wagging and the CH<sub>3</sub> torsional coordinates. The model has been defined assuming that, in the amine group, the bending and the wagging modes interact strongly. The vibrational levels split into six components corresponding to the six minima of the potential energy surface. The accuracy of the kinetic energy parameters has an important effect on the energies. Strong interactions among the large amplitude motions are observed. Isotopic effects are relevant for the deuterated species.</p>
</abstract>
<kwd-group>
<kwd>methylamine</kwd>
<kwd>LAM</kwd>
<kwd>torsion</kwd>
<kwd>wagging</kwd>
<kwd>
<sup>13</sup>CH<sub>3</sub>NH<sub>2</sub>
</kwd>
<kwd>CH<sub>3</sub>
<sup>15</sup>NH<sub>2</sub>
</kwd>
<kwd>CH<sub>3</sub>NHD</kwd>
<kwd>CH<sub>2</sub>DNH<sub>2</sub>
</kwd>
</kwd-group>
<contract-sponsor id="cn001">Deanship of Scientific Research, King Saud University<named-content content-type="fundref-id">10.13039/501100011665</named-content>
</contract-sponsor>
</article-meta>
</front>
<body>
<sec id="s1">
<title>Introduction</title>
<p>Methylamine (CH<sub>3</sub>-NH<sub>2</sub>) plays important roles in the gas phase chemistry in the terrestrial and extraterrestrial atmospheres. The presence in the Earth&#x2019;s atmosphere has both natural and anthropogenic causes (<xref ref-type="bibr" rid="B18">Ge et&#x20;al., 2011</xref>). In air quality studies, it is considered to be a Volatile Organic Compound (VOC) that can be a precursor of secondary organic aerosols (SOA) in the presence of glyoxal (<xref ref-type="bibr" rid="B11">De Haan et&#x20;al., 2009</xref>). In 1974, it was detected in the interstellar medium and it is contemplated as a relatively abundant species (<xref ref-type="bibr" rid="B25">Kaifu et&#x20;al., 1974</xref>) (<xref ref-type="bibr" rid="B14">Fourikis et&#x20;al., 1974</xref>). Recent studies consider it a precursor of glycine and a building block of life (<xref ref-type="bibr" rid="B49">Ohoshi et&#x20;al., 2019</xref>). Recently, methylamine has been detected in the quasar PKS 1830-211 (<xref ref-type="bibr" rid="B40">Muller et&#x20;al., 2011</xref>) and together with other simple N-bearing species, it has been observed in the hot cores NGC 6334I MM1-3 (<xref ref-type="bibr" rid="B5">B&#xf8;gelund et&#x20;al., 2019</xref>). <xref ref-type="bibr" rid="B15">Fourikis et&#x20;al. (1977)</xref> have reported the probable detection of deuterated methylamine (CH<sub>3</sub>NHD) in Sgr&#x20;B2.</p>
<p>The aim of the present work is the theoretical study of probably detectable methylamine isotopologues. Monosubstituted isotopologues were detected for many astrophysical molecules such as dimethyl-ether and methyl-formate as it is described in the references provided by the papers of <xref ref-type="bibr" rid="B13">Fern&#xe1;ndez et&#x20;al. (2019)</xref> and <xref ref-type="bibr" rid="B17">G&#xe1;mez et&#x20;al. (2019)</xref>. In a recent study of the methylamine main isotopologue, highly correlated ab initio methods were employed to simulate the far infrared spectra (<xref ref-type="bibr" rid="B58">Senent 2018</xref>). The low-lying vibrational energy levels in and their tunneling splitting components were computed, providing relevant information for rotational spectrum assignments, which are mandatory for the detection using radio-astronomy. Very accurate results were obtained by comparing with previous experimental data. A detailed review of previous theoretical and experimental works can be found in <xref ref-type="bibr" rid="B58">Senent (2018)</xref>.</p>
<p>The motivation of many previous studies of methylamine concerns more to the peculiar molecular structure than to its applications (<xref ref-type="bibr" rid="B21">Hamada et&#x20;al., 1982</xref>) (<xref ref-type="bibr" rid="B42">Ohashi &#x26; Hougen 1987</xref>), because it is contemplated as a prototype small non-rigid molecule where two interacting large amplitude motions, the torsion of the methyl group and the NH<sub>2</sub> wagging, govern its internal dynamics (<xref ref-type="bibr" rid="B42">Ohashi &#x26; Hougen 1987</xref>) (<xref ref-type="bibr" rid="B31">Kreglewski 1978</xref>, <xref ref-type="bibr" rid="B30">1989</xref>) (<xref ref-type="bibr" rid="B47">Ohashi &#x26; Toriyama 1994</xref> (<xref ref-type="bibr" rid="B27">Kleiner and Hougen, 2015</xref>). High resolution rovibrational spectra have been measured for the ground and various excited vibrational states, given a special attention to the far infrared region (<xref ref-type="bibr" rid="B3">Belorgeot et&#x20;al., 1982</xref>) (<xref ref-type="bibr" rid="B12">Diallo et&#x20;al., 1985</xref>) (<xref ref-type="bibr" rid="B45">Ohashi et&#x20;al., 1987</xref>, <xref ref-type="bibr" rid="B46">1988</xref>, <xref ref-type="bibr" rid="B48">1989</xref>, <xref ref-type="bibr" rid="B44">1992</xref>) (<xref ref-type="bibr" rid="B24">Ilyushin et&#x20;al., 2005</xref>) (<xref ref-type="bibr" rid="B34">Kreglewski &#x26; Winther 1992</xref>) (<xref ref-type="bibr" rid="B35">Kreglewski &#x26; Wlodarczak 1992</xref>) (<xref ref-type="bibr" rid="B38">Motiyenko et&#x20;al., 2014</xref>) (<xref ref-type="bibr" rid="B41">Nguyen et&#x20;al., 2021</xref>) (<xref ref-type="bibr" rid="B10">Dawadi et&#x20;al., 2013a</xref>; <xref ref-type="bibr" rid="B9">2013b</xref>).</p>
<p>Whereas publications about the methylamine main isotopologue are recurrent, less studies attend to other isotopic species. The microwave spectrum of the monosubstituted species CH<sub>3</sub>NHD (<xref ref-type="bibr" rid="B43">Ohashi et&#x20;al., 1991</xref>), CH<sub>2</sub>DNH<sub>2</sub> (<xref ref-type="bibr" rid="B63">Tamagake &#x26; Tsuboi 1974</xref>), and <sup>13</sup>CH<sub>3</sub>NH<sub>2</sub> (<xref ref-type="bibr" rid="B39">Motiyenko et&#x20;al., 2016</xref>), and the deuterated species, CH<sub>3</sub>ND<sub>2</sub>, CD<sub>3</sub>NH<sub>2</sub>, CD<sub>3</sub>ND<sub>2</sub> (<xref ref-type="bibr" rid="B36">Lide 1954</xref>) (<xref ref-type="bibr" rid="B53">Sastry 1960</xref>) (<xref ref-type="bibr" rid="B62">Takagi &#x26; Kojima 1971</xref>) (<xref ref-type="bibr" rid="B32">Kreglewski et&#x20;al., 1990a</xref>; <xref ref-type="bibr" rid="B33">1990b</xref>) were measured and assigned. The infrared absorption spectrum of <sup>15</sup>N-methylamine was inspected in the gas phase (<xref ref-type="bibr" rid="B23">Hirakawa et&#x20;al., 1972</xref>). Mass resolved excitation spectroscopy and ab initio calculations were employed to analyze the low-lying excited states of CH<sub>3</sub>NH<sub>2</sub>, CH<sub>3</sub>NH2, CD<sub>3</sub>NH<sub>2</sub>, CH<sub>3</sub>ND<sub>2</sub>, and CD<sub>3</sub>ND2 (<xref ref-type="bibr" rid="B64">Taylor &#x26; Bernstein 1995</xref>). The A&#x2190;X excitation spectra of six different deuterated isotopologues including the CH<sub>3</sub>NHD monosubstituted species, were explored (<xref ref-type="bibr" rid="B50">Park et&#x20;al., 2006</xref>).</p>
<p>Previous studies devoted to n-methyl amines describe theoretical techniques and symmetry concepts useful for the present work (<xref ref-type="bibr" rid="B57">Senent &#x26; Smeyers 1996</xref>) (<xref ref-type="bibr" rid="B61">Smeyers et&#x20;al., 1996</xref>, <xref ref-type="bibr" rid="B60">1998</xref>) (<xref ref-type="bibr" rid="B58">Senent 2018</xref>)On the basis of previous ab initio results (<xref ref-type="bibr" rid="B58">Senent 2018</xref>), performed using explicitly correlated coupled cluster theory, CCSD(T)-F12 (<xref ref-type="bibr" rid="B1">Adlet et&#x20;al., 2007</xref>) (<xref ref-type="bibr" rid="B28">Knizia et&#x20;al., 2009</xref>), in this new paper, we attend to several monosubstituted isotopologues containing abundant cosmological elements. Although, to our knowledge, a unique isotopologue CH<sub>3</sub>NHD has been probably detected (<xref ref-type="bibr" rid="B15">Fourikis et&#x20;al., 1977</xref>), other species are considered to be detectable species. Four isotopic species, <sup>13</sup>CH<sub>3</sub>NH<sub>2</sub>, CH<sub>3</sub>
<sup>15</sup>NH<sub>2</sub>, CH<sub>3</sub>NHD, and CH<sub>2</sub>DNH<sub>2</sub>, are studied and compared with the main isotopologue for predicting theoretically isotopic shifts. Recently, interstellar amines and their fragments have been studied using quantum-chemical computations (<xref ref-type="bibr" rid="B52">Salta et&#x20;al., 2020</xref>) (<xref ref-type="bibr" rid="B51">Puzzarini et&#x20;al., 2020</xref>).</p>
<p>An earliest CCSD(T)-F12&#x20;three-dimensional potential energy surface is revisited in the present work (<xref ref-type="bibr" rid="B58">Senent 2018</xref>) because it is mass independent. It is employed for constructing mass dependent effective potential energy surfaces for the different isotopologues. The surfaces present six minima separated by relatively low potential energy barriers. If the minimum interconversion is taken into consideration, the most abundant isotopologue can be classified in the G<sub>12</sub> molecular symmetry group (<xref ref-type="bibr" rid="B42">Ohashi &#x26; Hougen 1987</xref>). The isotopic substitutions carry out changes in the symmetry. Details concerning the followed procedure can be found in our previous paper devoted to the acetone isotopologues (<xref ref-type="bibr" rid="B7">Dalbouha et&#x20;al., 2021</xref>). The effective surfaces allow to construct Hamiltonians depending on three interacting coordinates, two interacting large amplitude motions, the NH<sub>2</sub> wagging and the CH<sub>3</sub> torsion, and the HNH bending. Then, both the bending and wagging of the amine group are treated together. The final levels are computed variationally.</p>
</sec>
<sec sec-type="results|discussion" id="s2">
<title>Results and Discussion</title>
<sec id="s2-1">
<title>Electronic Structure Calculations</title>
<p>The theoretical study of methylamine isotopologues was started from the results of a previous work devoted to the main isotopologue CH<sub>3</sub>NH<sub>2</sub> (<xref ref-type="bibr" rid="B58">Senent 2018</xref>). In this earlier paper, the structural parameters of the minimum energy structure and a three-dimensional ab initio potential energy surface (3D-PES) were computed using explicitly correlated coupled cluster theory with single and double substitutions augmented by a perturbative treatment of triple excitations (CCSD(T)-F12b) (<xref ref-type="bibr" rid="B1">Adlet et&#x20;al., 2007</xref>) (<xref ref-type="bibr" rid="B28">Knizia et&#x20;al., 2009</xref>) using the MOLPRO package default options (<xref ref-type="bibr" rid="B65">Werner et&#x20;al., 2012</xref>). The procedure was applied in connection with the AVTZ-F12 basis set, which contains the Dunning&#x2019;s type aug-cc-pVTZ atomic orbitals (AVTZ) (<xref ref-type="bibr" rid="B26">Kendall et&#x20;al., 1992</xref>) and the corresponding functions for the density fitting and the resolutions of the identity. These previous computed data are mass independent properties that can be used for the different isotopic species.</p>
<p>To determine the core-valence electron correlation effects on the rotational constants, the structure was optimized using CCSD(T) (coupled-cluster theory with single and double substitutions, augmented by a perturbative treatment of triple excitations) (<xref ref-type="bibr" rid="B22">Hampel et&#x20;al., 1992</xref>) and the cc-pCVTZ basis set (CVTZ) (<xref ref-type="bibr" rid="B66">Woon and Dunning Jr 1995</xref>).</p>
<p>The full-dimensional anharmonic force field and the vibrational corrections of the potential energy surface are mass dependent properties that must be computed for each isotopologue. For this reason, new electronic structure calculations have been performed in the present work. That properties were determined using second order M&#xf6;ller-Plesset theory (MP2) (<xref ref-type="bibr" rid="B37">M&#xf8;ller &#x26; Plesset 1934</xref>) implemented in GAUSSIAN (<xref ref-type="bibr" rid="B16">Frisch et&#x20;al., 2016</xref>). Anharmonic force fields allow obtain spectroscopic properties using second order perturbation theory (VPT2) (<xref ref-type="bibr" rid="B2">Barone 2005</xref>) (<xref ref-type="bibr" rid="B4">Bloino et&#x20;al., 2012</xref>). The vibrationally corrected surfaces were employed to construct Hamiltonians for the isotopologues. The energy levels corresponding to the large amplitude vibrations and to the HNH bending mode were computed using a variational procedure implemented in ENEDIM (<xref ref-type="bibr" rid="B55">Senent 1998a</xref>; <xref ref-type="bibr" rid="B54">1998b</xref>, <xref ref-type="bibr" rid="B56">2001</xref>).</p>
</sec>
<sec id="s2-2">
<title>The Symmetry of the Isotopologues</title>
<p>The main isotopologue, as well as <sup>13</sup>CH<sub>3</sub>NH<sub>2</sub> and CH<sub>3</sub> <sup>15</sup>NH<sub>2</sub>, can be classified in the G<sub>12</sub> molecular symmetry group (MSG) (<xref ref-type="bibr" rid="B42">Ohashi &#x26; Hougen 1987</xref>) and in the C<sub>s</sub> point group. However, the H &#x2192;D substitution carries out changes in the symmetry properties. CH<sub>3</sub>NDH must be classified in the C<sub>1</sub> point group and in the G<sub>6</sub> MSG, due to the absence of the symmetry plane. In CDH<sub>2</sub>NH<sub>2,</sub> the D atom can replace the in-plane H atom (C<sub>s</sub>-CDH<sub>2</sub>NH<sub>2</sub>) or one out-of plane H atom (C<sub>1</sub>-CDH<sub>2</sub>NH<sub>2</sub>). If VPT2 is applied and a unique minimum is considered, the molecule is assumed to be semi-rigid and all the vibrations are described as small displacements around the equilibrium. Two different point groups C<sub>1</sub> and C<sub>s</sub> are used. However, if the internal rotation is taken into account, C<sub>s</sub>-CDH<sub>2</sub>NH<sub>2</sub> and C<sub>1</sub>-CDH<sub>2</sub>NH<sub>2</sub> represent different minima of the same potential energy surface and they can be inter-converted. Then, both are classified in the same G<sub>4</sub>&#x20;MSG.</p>
<p>The G<sub>12</sub> MSG contains six irreducible representations, four non-degenerate, A<sub>1</sub>, A<sub>2</sub>, B<sub>1</sub> and B<sub>2</sub>, and two double-degenerate E<sub>1</sub> and E<sub>2</sub>. The G<sub>6</sub> MSG contains three irreducible representations, two non-degenerate, A<sub>1</sub>, and A<sub>2</sub>, and one double-degenerate E. The G<sub>4</sub> MSG contains four non-degenerate irreducible representations, A<sub>1</sub>, A<sub>2</sub>, B<sub>1</sub>, and&#x20;B<sub>2</sub>.</p>
</sec>
<sec id="s2-3">
<title>Rovibrational Parameters</title>
<p>In the earlier paper (<xref ref-type="bibr" rid="B58">Senent 2018</xref>), the CCSD(T)-F12/AVTZ structural parameters of the methylamine equilibrium geometry, are detailed. The structure is shown in <xref ref-type="fig" rid="F1">Figure&#x20;1</xref>, that helps to understand the atom labelling and the isotopic substitutions.</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>Methylamine equilibrium structure.</p>
</caption>
<graphic xlink:href="fchem-09-751203-g001.tif"/>
</fig>
<p>For all the isotopologues, the vibrational ground state rotational constants shown in <xref ref-type="table" rid="T1">Table&#x20;1</xref>, were computed from the CCSD(T)-F12 equilibrium rotational constants using the following equation:<disp-formula id="e1">
<mml:math id="m1">
<mml:mrow>
<mml:msub>
<mml:mtext>B</mml:mtext>
<mml:mtext>0</mml:mtext>
</mml:msub>
<mml:msub>
<mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mtext>&#xa0;B</mml:mtext>
</mml:mrow>
<mml:mrow>
<mml:mtext>e</mml:mtext>
</mml:mrow>
</mml:msub>
<mml:mtext>&#xa0;</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mrow>
<mml:mrow>
<mml:mtext>CCSD</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mtext>T</mml:mtext>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>-</mml:mo>
<mml:mtext>F</mml:mtext>
<mml:mn>12</mml:mn>
</mml:mrow>
<mml:mo>/</mml:mo>
<mml:mrow>
<mml:mtext>AVTZ</mml:mtext>
<mml:mo>-</mml:mo>
<mml:mtext>F</mml:mtext>
<mml:mn>12</mml:mn>
</mml:mrow>
</mml:mrow>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mtext>&#xa0;</mml:mtext>
<mml:mo>&#x2b;</mml:mo>
<mml:mtext>&#xa0;</mml:mtext>
<mml:mo>&#x25b3;</mml:mo>
<mml:msub>
<mml:mtext>B</mml:mtext>
<mml:mtext>e</mml:mtext>
</mml:msub>
<mml:mmultiscripts>
<mml:mrow>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mrow>
<mml:mrow>
<mml:mtext>CCSD</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mtext>T</mml:mtext>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>/</mml:mo>
<mml:mrow>
<mml:mtext>CVTZ</mml:mtext>
</mml:mrow>
</mml:mrow>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mprescripts/>
<mml:none/>
<mml:mrow>
<mml:mtext>core</mml:mtext>
</mml:mrow>
</mml:mmultiscripts>
<mml:mo>&#x2b;</mml:mo>
<mml:mo>&#x25b3;</mml:mo>
<mml:msup>
<mml:mtext>B</mml:mtext>
<mml:mrow>
<mml:mtext>vib</mml:mtext>
</mml:mrow>
</mml:msup>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mrow>
<mml:mrow>
<mml:mtext>MP</mml:mtext>
<mml:mn>2</mml:mn>
</mml:mrow>
<mml:mo>/</mml:mo>
<mml:mrow>
<mml:mtext>AVTZ</mml:mtext>
</mml:mrow>
</mml:mrow>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:math>
<label>(1)</label>
</disp-formula>
</p>
<table-wrap id="T1" position="float">
<label>TABLE 1</label>
<caption>
<p>Rotational constants (in MHz).</p>
</caption>
<table>
<tbody valign="top">
<tr>
<td align="left"/>
<td colspan="2" align="center">CH<sub>3</sub>NH<sub>2</sub> (Cs)</td>
<td colspan="2" align="center">
<sup>13</sup>CH<sub>3</sub>NH<sub>2</sub> (C<sub>s</sub>)</td>
<td align="center">CH<sub>3</sub>
<sup>15</sup>NH<sub>2</sub> (C<sub>s</sub>)</td>
</tr>
<tr>
<td align="left">A<sub>e</sub>
</td>
<td colspan="2" align="char" char=".">103,855.395</td>
<td colspan="2" align="char" char=".">103,851.612</td>
<td align="char" char=".">103,751.743</td>
</tr>
<tr>
<td align="left">B<sub>e</sub>
</td>
<td colspan="2" align="char" char=".">22,803.133</td>
<td colspan="2" align="char" char=".">22,267.093</td>
<td align="char" char=".">22,292.683</td>
</tr>
<tr>
<td align="left">C<sub>e</sub>
</td>
<td colspan="2" align="char" char=".">21,926.385</td>
<td colspan="2" align="char" char=".">21,430.485</td>
<td align="char" char=".">21,458.454</td>
</tr>
<tr>
<td align="left"/>
<td align="center">
<xref ref-type="bibr" rid="B55">Senent (2018a)</xref>
</td>
<td align="center">
<xref ref-type="bibr" rid="B24">Ilyushin et al. (2005)</xref>
</td>
<td align="center">
<italic>This work</italic>
</td>
<td align="center">
<xref ref-type="bibr" rid="B39">Motiyenko et al. (2016)</xref>
</td>
<td align="center">
<italic>This work</italic>
</td>
</tr>
<tr>
<td align="left">A<sub>0</sub>
</td>
<td align="char" char=".">103,067.129</td>
<td align="char" char=".">103,155.749</td>
<td align="char" char=".">103,110.685</td>
<td align="char" char=".">103,158.312</td>
<td align="char" char=".">103,012.808</td>
</tr>
<tr>
<td align="left">B<sub>0</sub>
</td>
<td align="char" char=".">22,588.290</td>
<td align="char" char=".">22,608.305</td>
<td align="char" char=".">22,061.169</td>
<td align="char" char=".">22,080.995</td>
<td align="char" char=".">22,086.384</td>
</tr>
<tr>
<td align="left">C<sub>0</sub>
</td>
<td align="char" char=".">21,710.496</td>
<td align="char" char=".">21,730.428</td>
<td align="char" char=".">21,221.438</td>
<td align="char" char=".">21,242.856</td>
<td align="char" char=".">21,248.664</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
</tr>
<tr>
<td align="left"/>
<td align="center">CH<sub>3</sub>NDH (C1)</td>
<td align="left"/>
<td colspan="2" align="center">C<sub>s</sub>- CDH<sub>2</sub>NH<sub>2</sub>/C<sub>1</sub>- CDH<sub>2</sub>NH<sub>2</sub>
</td>
<td align="left"/>
</tr>
<tr>
<td align="left">A<sub>e</sub>
</td>
<td colspan="2" align="char" char=".">90,053.981</td>
<td colspan="2" align="left">86,604.055/87,207.318</td>
</tr>
<tr>
<td align="left">B<sub>e</sub>
</td>
<td colspan="2" align="char" char=".">21,528.245</td>
<td colspan="2" align="left">20,720.150/21,422.590</td>
<td align="left"/>
</tr>
<tr>
<td align="left">C<sub>e</sub>
</td>
<td colspan="2" align="char" char=".">20,266.914</td>
<td colspan="2" align="left">20,649.766/20,082.096</td>
<td align="left"/>
</tr>
<tr>
<td align="left"/>
<td align="center">Calc</td>
<td align="center">
<xref ref-type="bibr" rid="B43">Ohashi et al. (1991)</xref>
</td>
<td colspan="2" align="center">
<italic>This work</italic>
</td>
<td align="left"/>
</tr>
<tr>
<td align="left">A<sub>0</sub>
</td>
<td align="char" char=".">89,438.271</td>
<td align="char" char=".">89,523.02</td>
<td colspan="2" align="center">86,037.713/86,570.015</td>
<td align="left"/>
</tr>
<tr>
<td align="left">B<sub>0</sub>
</td>
<td align="char" char=".">21,334.679</td>
<td align="char" char=".">21,333.37</td>
<td colspan="2" align="center">20,526.133/21,225.188</td>
<td align="left"/>
</tr>
<tr>
<td align="left">C<sub>0</sub>
</td>
<td align="char" char=".">20,072.203</td>
<td align="char" char=".">20,118.07</td>
<td colspan="2" align="center">20,455.807/19,894.077</td>
<td align="left"/>
</tr>
</tbody>
</table>
</table-wrap>
<p>Here, &#x394;B<sub>e</sub>
<sup>core</sup> collects the core-valence electron correlation effects on the equilibrium structure and &#x394;B<sup>vib</sup> represents the vibrational contribution derived from the second order perturbation theory (VPT2) <italic>&#x3b1;</italic>
<sub>
<italic>r</italic>
</sub>
<sup>
<italic>i</italic>
</sup> vibration-rotation interaction parameters. These last were determined using the MP2/AVTZ cubic force fields and vibrational second order perturbation theory. &#x394;B<sub>e</sub>
<sup>core</sup> was determined from the CCSD(T)/CVTZ parameters B<sub>e</sub> (CV) and B<sub>e</sub>(V), calculated correlating both core and valence electrons (CV) or just the valence electrons (V) in the post-SCF process. Then:<disp-formula id="e2">
<mml:math id="m2">
<mml:mrow>
<mml:mi>&#x394;</mml:mi>
<mml:msubsup>
<mml:mtext>B</mml:mtext>
<mml:mtext>e</mml:mtext>
<mml:mrow>
<mml:mtext>core</mml:mtext>
</mml:mrow>
</mml:msubsup>
<mml:msub>
<mml:mrow>
<mml:mtext>&#xa0;</mml:mtext>
<mml:mo>&#x3d;</mml:mo>
<mml:mtext>&#xa0;B</mml:mtext>
</mml:mrow>
<mml:mtext>e</mml:mtext>
</mml:msub>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>CV</mml:mtext>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:msub>
<mml:mrow>
<mml:mtext>&#xa0;</mml:mtext>
<mml:mo>-</mml:mo>
<mml:mtext>&#xa0;B</mml:mtext>
</mml:mrow>
<mml:mtext>e</mml:mtext>
</mml:msub>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mtext>V</mml:mtext>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:math>
<label>(2)</label>
</disp-formula>
</p>
<p>This approximation has been corroborated in previous studies of other non-rigid molecules providing really accurate parameters, whose deviations with respect available experimental data, represent few MHz (<xref ref-type="bibr" rid="B6">Boussesi et&#x20;al., 2016</xref>) (<xref ref-type="bibr" rid="B8">Dalbouha et&#x20;al., 2016</xref>, <xref ref-type="bibr" rid="B7">2021</xref>). In <xref ref-type="table" rid="T1">Table&#x20;1</xref>, the computed rotational constants of CH<sub>3</sub>NH<sub>2</sub>, <sup>13</sup>CH<sub>3</sub>NH<sub>2,</sub> and CH<sub>3</sub>NDH are compared with available experimental parameters (<xref ref-type="bibr" rid="B24">Ilyushin et&#x20;al., 2005</xref>) (<xref ref-type="bibr" rid="B39">Motiyenko et&#x20;al., 2016</xref>) (<xref ref-type="bibr" rid="B43">Ohashi et&#x20;al., 1991</xref>). The MP2/AVTZ quartic centrifugal distortion constants corresponding to the asymmetrically reduced Hamiltonian, are shown in <xref ref-type="table" rid="T2">Table&#x20;2</xref> where they are compared with previous experimental data (<xref ref-type="bibr" rid="B24">Ilyushin et&#x20;al., 2005</xref>) (<xref ref-type="bibr" rid="B39">Motiyenko et&#x20;al., 2016</xref>) (<xref ref-type="bibr" rid="B43">Ohashi et&#x20;al., 1991</xref>). Disagreements between experimental and computed data can be correlated with the level of ab initio calculations used to compute the anharmonic force field. In addition, in methyl amine, the interaction between the internal and global rotation causes deviations. Isotopic shifts are more reliable.</p>
<table-wrap id="T2" position="float">
<label>TABLE 2</label>
<caption>
<p>MP2/AVTZ quartic (in KHz) centrifugal distortion constants<sup>a</sup> computed using the MP2/AVTZ cubic force fields.</p>
</caption>
<table>
<thead>
<tr>
<td rowspan="2" align="left"/>
<td colspan="2" align="center">CH<sub>3</sub>NH<sub>2</sub> (C<sub>s</sub>)</td>
<td colspan="2" align="center">
<sup>13</sup>CH<sub>3</sub>NH<sub>2</sub> (C<sub>s</sub>)</td>
<td align="center">CH<sub>3</sub>
<sup>15</sup>NH<sub>2</sub> (C<sub>s</sub>)</td>
</tr>
<tr>
<td align="center">
<italic>This work</italic>
</td>
<td align="center">
<xref ref-type="bibr" rid="B24">Ilyushin et al. (2005)</xref>
</td>
<td align="center">
<italic>This work</italic>
</td>
<td align="center">
<xref ref-type="bibr" rid="B39">Motiyenko et al. (2016)</xref>
</td>
<td align="center">
<italic>This work</italic>
</td>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="left">&#x394;<sub>J</sub>
</td>
<td align="char" char=".">38.7083</td>
<td align="char" char="( .">39.4506(18)</td>
<td align="char" char=".">37.3369</td>
<td align="char" char="( .">38.06084(18)</td>
<td align="char" char=".">37.3734</td>
</tr>
<tr>
<td align="left">&#x394;<sub>K</sub>
</td>
<td align="char" char=".">610.0394</td>
<td align="char" char="( .">701.049(24)</td>
<td align="char" char=".">641.8328</td>
<td align="char" char="( .">706.766(12)</td>
<td align="char" char=".">643.7290</td>
</tr>
<tr>
<td align="left">&#x394;<sub>JK</sub>
</td>
<td align="char" char=".">172.7131</td>
<td align="char" char="( .">170.983(15)</td>
<td align="char" char=".">161.3963</td>
<td align="char" char="( .">166.8639(18)</td>
<td align="char" char=".">161.0483</td>
</tr>
<tr>
<td align="left">&#x3b4;<sub>J</sub>
</td>
<td align="char" char=".">1.6377</td>
<td align="char" char="( .">1.75679(17)</td>
<td align="char" char=".">1.5367</td>
<td align="char" char="( .">1.660,274(31)</td>
<td align="char" char=".">1.5536</td>
</tr>
<tr>
<td align="left">&#x3b4;<sub>K</sub>
</td>
<td align="char" char=".">&#x2212;217.5746</td>
<td align="char" char="( .">&#x2212;337.78(14)</td>
<td align="char" char=".">&#x2212;226.9603</td>
<td align="char" char="( .">&#x2212;322.295(13)</td>
<td align="char" char=".">&#x2212;223.0754</td>
</tr>
</tbody>
</table>
<table>
<thead>
<tr>
<td align="left"/>
<td colspan="2" align="center">CH<sub>3</sub>NDH (C<sub>1</sub>)</td>
<td align="center">C<sub>s</sub>- CDH<sub>2</sub>NH<sub>2</sub>/C<sub>1</sub>-&#x20;CDH<sub>2</sub>NH<sub>2</sub>
</td>
<td align="left"/>
</tr>
<tr>
<td align="left"/>
<td align="center">
<italic>This work</italic>
</td>
<td align="center">
<xref ref-type="bibr" rid="B43">Ohashi et al. (1991)</xref>
</td>
<td align="center">
<italic>This work</italic>
</td>
<td align="left"/>
</tr>
</thead>
<tbody>
<tr>
<td align="left">&#x394;<sub>J</sub>
</td>
<td align="char" char=".">33.6435</td>
<td align="char" char="( .">33.22(93)</td>
<td align="center">32.5197/32.9086</td>
<td align="left"/>
</tr>
<tr>
<td align="left">&#x394;<sub>K</sub>
</td>
<td align="char" char=".">454.6168</td>
<td align="char" char="( .">682.0(13)</td>
<td align="center">487.9419/392.1165</td>
<td align="left"/>
</tr>
<tr>
<td align="left">&#x394;<sub>JK</sub>
</td>
<td align="char" char=".">154.6421</td>
<td align="char" char="( .">128.1(94)</td>
<td align="center">142.1828/167.5383</td>
<td align="left"/>
</tr>
<tr>
<td align="left">&#x3b4;<sub>J</sub>
</td>
<td align="char" char=".">2.0344</td>
<td align="left"/>
<td align="center">0.1886/2.3911</td>
<td align="left"/>
</tr>
<tr>
<td align="left">&#x3b4;<sub>K</sub>
</td>
<td align="char" char=".">&#x2212;88.5972</td>
<td align="left"/>
<td align="center">&#x2212;6,125.3195/19.9638</td>
<td align="left"/>
</tr>
</tbody>
</table>
</table-wrap>
<p>The anharmonic fundamental frequencies shown in <xref ref-type="table" rid="T3">Table&#x20;3</xref>, were computed using VPT2 theory (<xref ref-type="bibr" rid="B2">Barone 2005</xref>) (<xref ref-type="bibr" rid="B4">Bloino et&#x20;al., 2012</xref>) implemented in Gaussian (<xref ref-type="bibr" rid="B16">Frisch et&#x20;al., 2016</xref>) and the MP2/AVTZ force fields. The modes are ordered following the criteria used for the main isotopologue that helps to make visible the isotopic shifts. Although VPT2 does not represent the proper treatment for the study of the vibrations responsible for the non-rigidity, it provides a good description of the mid- and near-infrared regions and a useful first description of the far-infrared region. In addition, it allows predict possible band displacements due to Fermi resonances. VPT2 theory ignores the inter-conversion of minima and treats the molecule as a semi-rigid species with a single minimum. If the existence of a single minimum is assumed, the resulting VPT2 properties are different for C<sub>s</sub>-CDH<sub>2</sub>NH<sub>2</sub> than for C<sub>1</sub>-CDH<sub>2</sub>NH<sub>2</sub>.</p>
<table-wrap id="T3" position="float">
<label>TABLE 3</label>
<caption>
<p>Anharmonic fundamental frequencies (in cm<sup>&#x2212;1</sup>) calculated in this work and measured in previous experiments in the gas phase<sup>a</sup>.</p>
</caption>
<table>
<tbody valign="top">
<tr>
<td colspan="2" align="left"/>
<td colspan="2" align="center">
<bold>CH<sub>3</sub>NH<sup>2</sup>
</bold>
</td>
<td align="center">
<bold>
<sup>13</sup>CH<sub>3</sub>NH<sub>2</sub>
</bold>
</td>
<td colspan="2" align="center">
<bold>CH<sub>3</sub>
<sup>15</sup>NH<sub>2</sub>
</bold>
</td>
</tr>
<tr>
<td align="left">
<bold>Mode</bold>
</td>
<td align="center">
<bold>assign.<sup>b</sup>
</bold>
</td>
<td align="center">
<bold>
<xref ref-type="bibr" rid="B58">Senent (2018)</xref>
</bold>
</td>
<td align="center">
<bold>
<xref ref-type="bibr" rid="B59">Shimanouchi (1972)</xref>
</bold>
</td>
<td align="center">
<bold>
<italic>This work</italic>
</bold>
</td>
<td align="center">
<bold>
<italic>This work</italic>
</bold>
</td>
<td align="center">
<bold>Hirakawa et al., 1972</bold>
</td>
</tr>
<tr>
<td rowspan="2" align="left">1</td>
<td rowspan="2" align="center">NH<sub>2</sub> st</td>
<td rowspan="2" align="char" char=".">3,388</td>
<td align="char" char=".">3,361</td>
<td align="char" char=".">3,385</td>
<td align="char" char=".">3,380</td>
<td align="char" char=".">3,354.5</td>
</tr>
<tr>
<td align="char" char=".">3,360</td>
<td align="left"/>
<td align="left"/>
<td align="left"/>
</tr>
<tr>
<td rowspan="2" align="left">2</td>
<td rowspan="2" align="center">CH<sub>3</sub> st</td>
<td rowspan="2" align="char" char=".">3,001</td>
<td align="char" char=".">2,961</td>
<td align="char" char=".">
<bold>2,989</bold>
</td>
<td align="char" char=".">
<bold>3,010</bold>
</td>
<td align="char" char=".">2,961.2</td>
</tr>
<tr>
<td align="char" char=".">2,960</td>
<td align="left"/>
<td align="left"/>
<td align="left"/>
</tr>
<tr>
<td rowspan="2" align="left">3</td>
<td rowspan="2" align="center">CH<sub>3</sub> st</td>
<td rowspan="2" align="char" char=".">
<bold>2,931</bold>
</td>
<td align="char" char=".">2,820</td>
<td align="char" char=".">
<bold>2,909</bold>
</td>
<td align="char" char=".">
<bold>2,916</bold>
</td>
<td align="char" char=".">2,820</td>
</tr>
<tr>
<td align="char" char=".">2,820</td>
<td align="left"/>
<td align="left"/>
<td align="left"/>
</tr>
<tr>
<td align="left">4</td>
<td align="center">NH<sub>2</sub> b</td>
<td align="char" char=".">
<bold>1,610</bold>
</td>
<td align="char" char=".">1,623</td>
<td align="char" char=".">
<bold>1,639</bold>
</td>
<td align="char" char=".">
<bold>1,635</bold>
</td>
<td align="char" char=".">1,618.7</td>
</tr>
<tr>
<td align="left">5</td>
<td align="center">CH<sub>3</sub> b</td>
<td align="char" char=".">1,481</td>
<td align="char" char=".">1,473</td>
<td align="char" char=".">1,476</td>
<td align="char" char=".">1,478</td>
<td align="char" char=".">1,473.6</td>
</tr>
<tr>
<td align="left">6</td>
<td align="center">CH<sub>3</sub> b</td>
<td align="char" char=".">1,453</td>
<td align="char" char=".">1,430</td>
<td align="char" char=".">1,426</td>
<td align="char" char=".">1,433</td>
<td align="char" char=".">1,430.4</td>
</tr>
<tr>
<td align="left">7</td>
<td align="center">HCN b</td>
<td align="char" char=".">1,146</td>
<td align="char" char=".">1,130</td>
<td align="char" char=".">1,127</td>
<td align="char" char=".">1,131</td>
<td align="char" char=".">1,126.2</td>
</tr>
<tr>
<td align="left">8</td>
<td align="center">NC st</td>
<td align="char" char=".">1,055</td>
<td align="char" char=".">1,044</td>
<td align="char" char=".">1,032</td>
<td align="char" char=".">1,037</td>
<td align="char" char=".">1,031.7</td>
</tr>
<tr>
<td align="left">9</td>
<td align="center">NH<sub>2</sub> wag</td>
<td align="char" char=".">781</td>
<td align="char" char=".">780</td>
<td align="char" char=".">787</td>
<td align="char" char=".">783</td>
<td align="char" char=".">775.8</td>
</tr>
<tr>
<td align="left">10</td>
<td align="center">NH<sub>2</sub> st</td>
<td align="char" char=".">3,464</td>
<td align="char" char=".">3,427</td>
<td align="char" char=".">3,462</td>
<td align="char" char=".">3,453</td>
<td align="char" char=".">3,415</td>
</tr>
<tr>
<td align="left">11</td>
<td align="center">CH<sub>3</sub> st</td>
<td align="char" char=".">3,034</td>
<td align="char" char=".">2,985</td>
<td align="char" char=".">3,021</td>
<td align="char" char=".">3,031</td>
<td align="char" char=".">2,985</td>
</tr>
<tr>
<td align="left">12</td>
<td align="center">CH<sub>3</sub> b</td>
<td align="char" char=".">1,481</td>
<td align="char" char=".">1485c</td>
<td align="char" char=".">1,495</td>
<td align="char" char=".">1,495</td>
<td align="char" char=".">1,485</td>
</tr>
<tr>
<td align="left">13</td>
<td align="center">HNC b</td>
<td align="char" char=".">1,315</td>
<td align="left"/>
<td align="char" char=".">
<bold>1,292</bold>
</td>
<td align="char" char=".">
<bold>1,296</bold>
</td>
<td align="left"/>
</tr>
<tr>
<td align="left">14</td>
<td align="center">CH<sub>3</sub> b</td>
<td align="char" char=".">971</td>
<td align="left"/>
<td align="char" char=".">965</td>
<td align="char" char=".">966</td>
<td align="left"/>
</tr>
<tr>
<td align="left">15</td>
<td align="center">CH<sub>3</sub> tor</td>
<td align="char" char=".">288</td>
<td align="char" char=".">268</td>
<td align="char" char=".">274</td>
<td align="char" char=".">274</td>
<td align="left"/>
</tr>
<tr>
<td rowspan="4" align="left"/>
<td rowspan="4" align="left"/>
<td rowspan="4" align="left"/>
<td align="char" char=".">264.58204<sup>d</sup>
</td>
<td rowspan="4" align="left"/>
<td rowspan="4" align="left"/>
<td align="left"/>
</tr>
<tr>
<td align="char" char=".">264.58279<sup>d</sup>
</td>
<td align="left"/>
</tr>
<tr>
<td align="char" char=".">264.58314<sup>e</sup>
</td>
<td align="left"/>
</tr>
<tr>
<td align="char" char=".">264.58337<sup>f</sup>
</td>
<td align="left"/>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="char" char=".">
<bold>CH</bold>
<sub>
<bold>3</bold>
</sub>
<bold>NDH</bold>
</td>
<td colspan="3" align="center">
<bold>Cs-CDH</bold>
<sub>
<bold>2</bold>
</sub>
<bold>NH</bold>
<sub>
<bold>2</bold>
</sub>
<bold>/C1-CDH</bold>
<sub>
<bold>2</bold>
</sub>
<bold>NH</bold>
<sub>
<bold>2</bold>
</sub>
</td>
<td align="left"/>
</tr>
<tr>
<td align="left">
<bold>mode</bold>
</td>
<td align="center">
<bold>assign.<sup>b</sup>
</bold>
</td>
<td align="char" char=".">
<bold>This work</bold>
</td>
<td colspan="3" align="center">
<bold>This work</bold>
</td>
<td align="left"/>
</tr>
<tr>
<td align="left">1</td>
<td align="center">NH<sub>2</sub> st</td>
<td align="char" char=".">2,528</td>
<td colspan="3" align="center">3,384/3,385</td>
<td align="left"/>
</tr>
<tr>
<td align="left">2</td>
<td align="center">CH<sub>3</sub> st</td>
<td align="char" char=".">3,000</td>
<td colspan="3" align="center">
<bold>2,998</bold>/<bold>2,898</bold>
</td>
<td align="left"/>
</tr>
<tr>
<td align="left">3</td>
<td align="center">CH<sub>3</sub> st</td>
<td align="char" char=".">
<bold>2,915</bold>
</td>
<td colspan="3" align="center">
<bold>2,160</bold>/<bold>2,228</bold>
</td>
<td align="left"/>
</tr>
<tr>
<td align="left">4</td>
<td align="center">NH<sub>2</sub> b</td>
<td align="char" char=".">
<bold>1,461</bold>
</td>
<td colspan="3" align="center">1,605/<bold>1,654</bold>
</td>
<td align="left"/>
</tr>
<tr>
<td align="left">5</td>
<td align="center">CH<sub>3</sub> b</td>
<td align="char" char=".">1,478</td>
<td colspan="3" align="center">1,458/1,476</td>
<td align="left"/>
</tr>
<tr>
<td align="left">6</td>
<td align="center">CH<sub>3</sub> b</td>
<td align="char" char=".">1,432</td>
<td colspan="3" align="center">1,337/1,324</td>
<td align="left"/>
</tr>
<tr>
<td align="left">7</td>
<td align="center">HCN b</td>
<td align="char" char=".">
<bold>1,152</bold>
</td>
<td colspan="3" align="center">1,078/1,062</td>
<td align="left"/>
</tr>
<tr>
<td align="left">8</td>
<td align="center">NC st</td>
<td align="char" char=".">1,038</td>
<td colspan="3" align="center">920/1,046</td>
<td align="left"/>
</tr>
<tr>
<td align="left">9</td>
<td align="center">NH<sub>2</sub> wag</td>
<td align="char" char=".">691</td>
<td colspan="3" align="center">767/780</td>
<td align="left"/>
</tr>
<tr>
<td align="left">10</td>
<td align="center">NH<sub>2</sub> st</td>
<td align="char" char=".">3,422</td>
<td colspan="3" align="center">3,462/3,462</td>
<td align="left"/>
</tr>
<tr>
<td align="left">11</td>
<td align="center">CH<sub>3</sub> st</td>
<td align="char" char=".">3,032</td>
<td colspan="3" align="center">3,025/3,010</td>
<td align="left"/>
</tr>
<tr>
<td align="left">12</td>
<td align="center">CH<sub>3</sub> b</td>
<td align="char" char=".">1,496</td>
<td colspan="3" align="center">1,373/<bold>1,356</bold>
</td>
<td align="left"/>
</tr>
<tr>
<td align="left">13</td>
<td align="center">HNC b</td>
<td align="char" char=".">1,219</td>
<td colspan="3" align="center">
<bold>1,246</bold>/1,228</td>
<td align="left"/>
</tr>
<tr>
<td align="left">14</td>
<td align="center">CH<sub>3</sub> b</td>
<td align="char" char=".">878</td>
<td colspan="3" align="center">937/845</td>
<td align="left"/>
</tr>
<tr>
<td align="left">15</td>
<td align="center">CH<sub>3</sub> tor</td>
<td align="char" char=".">247</td>
<td colspan="3" align="center">265/262</td>
<td align="left"/>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn>
<p>a) Emphasized in bold the transitions displaced by Fermi resonances.</p>
</fn>
<fn>
<p>b) st &#x3d; stretching; b &#x3d; bending; w &#x3d; wagging; tor &#x3d; torsion.</p>
</fn>
<fn>
<p>c) <xref ref-type="bibr" rid="B23">Hirakawa et al., 1972</xref>; d) <xref ref-type="bibr" rid="B48">Ohashi et al., 1989</xref>; e) <xref ref-type="bibr" rid="B35">Kreglewski &#x26; Wlodarczak 1992</xref>; f) <xref ref-type="bibr" rid="B19">Gulaczyk et al., 2017</xref>.</p>
</fn>
</table-wrap-foot>
</table-wrap>
<p>The frequencies corresponding to the main isotopologue are compared with experimental data measured in the gas phase (<xref ref-type="bibr" rid="B48">Ohashi et&#x20;al., 1989</xref>) (<xref ref-type="bibr" rid="B35">Kreglewski &#x26; Wlodarczak 1992</xref>) (<xref ref-type="bibr" rid="B19">Gulaczyk et&#x20;al., 2017</xref>) (<xref ref-type="bibr" rid="B23">Hirakawa et&#x20;al., 1972</xref>) [58]. Previous results are available for CH<sub>3</sub>
<sup>15</sup>NH<sub>2</sub> (<xref ref-type="bibr" rid="B23">Hirakawa et&#x20;al., 1972</xref>). Deviation for several modes are significant, whereas the isotopic shits computed at the MP2 level of theory are reliable.</p>
<p>In <xref ref-type="table" rid="T3">Table&#x20;3</xref>, emphasized in bold, are the fundamental frequencies for which resonances can be relevant. Displacements due to the Fermi interactions were found to be relevant for the &#x3bd;<sub>3</sub> fundamental (CH<sub>3</sub> st), that interacts with two overtones (2&#x3bd;<sub>6</sub> and 2&#x3bd;<sub>12</sub>). The NH<sub>2</sub> bending fundamental is predicted to interact strongly with the NH<sub>2</sub> wagging overtone. Since both amine vibrations behave as inseparable modes, the variational model used for exploring the far infrared region, includes explicitly the bending coordinate.</p>
</sec>
<sec id="s2-4">
<title>The far Infrared Spectrum</title>
<p>As was assumed in the previous paper devoted to the main isotopologue (<xref ref-type="bibr" rid="B58">Senent 2018</xref>), the low-lying vibrational energy levels corresponding to the two large amplitude motions, the methyl torsion (&#x3b8;) and the amine NH<sub>2</sub> wagging (&#x3b1;) can be determined by solving variationally a three-dimensional Hamiltonian where a third coordinate, the HNH bending angle (&#x3b2;), is considered to be an independent variable. The Hamiltonian obeys the formula:<disp-formula id="e3">
<mml:math id="m3">
<mml:mrow>
<mml:mi>H</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>&#x3b2;</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mo>&#x2212;</mml:mo>
<mml:munderover>
<mml:mstyle displaystyle="true">
<mml:mo>&#x2211;</mml:mo>
</mml:mstyle>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mn>3</mml:mn>
</mml:munderover>
<mml:munderover>
<mml:mstyle displaystyle="true">
<mml:mo>&#x2211;</mml:mo>
</mml:mstyle>
<mml:mrow>
<mml:mi>j</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
<mml:mn>3</mml:mn>
</mml:munderover>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mfrac>
<mml:mo>&#x2202;</mml:mo>
<mml:mrow>
<mml:mo>&#x2202;</mml:mo>
<mml:msub>
<mml:mi>q</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:msub>
<mml:mi>B</mml:mi>
<mml:mrow>
<mml:msub>
<mml:mi>q</mml:mi>
<mml:mi>i</mml:mi>
</mml:msub>
<mml:msub>
<mml:mi>q</mml:mi>
<mml:mi>j</mml:mi>
</mml:msub>
</mml:mrow>
</mml:msub>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>&#x3b2;</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mfrac>
<mml:mo>&#x2202;</mml:mo>
<mml:mrow>
<mml:mo>&#x2202;</mml:mo>
<mml:msub>
<mml:mi>q</mml:mi>
<mml:mi>j</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x2b;</mml:mo>
<mml:msup>
<mml:mi>V</mml:mi>
<mml:mrow>
<mml:mi>e</mml:mi>
<mml:mi>f</mml:mi>
<mml:mi>f</mml:mi>
</mml:mrow>
</mml:msup>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>&#x3b2;</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:math>
<label>(3)</label>
</disp-formula>
</p>
<p>This Hamiltonian was defined by taking into consideration the predictions of the test of resonances described in the previous section and in the previous paper (<xref ref-type="bibr" rid="B58">Senent 2018</xref>). Significant interactions between the NH<sub>2</sub> bending and wagging vibrational modes were predicted. This fact suggests the prerequisite of a 3D-model. In <xref ref-type="disp-formula" rid="e3">Eq. 3</xref>, <inline-formula id="inf1">
<mml:math id="m4">
<mml:mrow>
<mml:msub>
<mml:mi>B</mml:mi>
<mml:mrow>
<mml:mi>q</mml:mi>
<mml:mi>i</mml:mi>
<mml:mi>q</mml:mi>
<mml:mi>j</mml:mi>
</mml:mrow>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> and V<sup>eff</sup> represent the kinetic energy parameters and the effective potential defined as the sum of three contributions:<disp-formula id="e4">
<mml:math id="m5">
<mml:mrow>
<mml:msup>
<mml:mtext>V</mml:mtext>
<mml:mrow>
<mml:mtext>eff</mml:mtext>
</mml:mrow>
</mml:msup>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
<mml:mtext>,</mml:mtext>
<mml:mi>&#x3b1;</mml:mi>
<mml:mtext>,</mml:mtext>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mtext>&#xa0;&#xa0;</mml:mtext>
<mml:mo>&#x3d;</mml:mo>
<mml:mtext>V</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
<mml:mtext>,</mml:mtext>
<mml:mi>&#x3b1;</mml:mi>
<mml:mtext>,</mml:mtext>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mtext>&#xa0;</mml:mtext>
<mml:mo>&#x2b;</mml:mo>
<mml:mtext>&#xa0;V</mml:mtext>
<mml:mo>&#x2032;</mml:mo>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
<mml:mtext>,</mml:mtext>
<mml:mi>&#x3b1;</mml:mi>
<mml:mtext>,</mml:mtext>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:msup>
<mml:mrow>
<mml:mo>&#x2b;</mml:mo>
<mml:mtext>V</mml:mtext>
</mml:mrow>
<mml:mrow>
<mml:mtext>ZPVE</mml:mtext>
</mml:mrow>
</mml:msup>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
<mml:mtext>,</mml:mtext>
<mml:mi>&#x3b1;</mml:mi>
<mml:mtext>,</mml:mtext>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:math>
<label>(4)</label>
</disp-formula>
</p>
<p>Here, V(<inline-formula id="inf2">
<mml:math id="m6">
<mml:mrow>
<mml:mtext>&#x3b2;</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#xa0;</mml:mo>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>) is the mass independent ab initio three-dimensional potential energy surface; V&#x2019;(<inline-formula id="inf3">
<mml:math id="m7">
<mml:mrow>
<mml:mtext>&#x3b2;</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#xa0;</mml:mo>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>) and V<sup>ZPVE</sup>(<inline-formula id="inf4">
<mml:math id="m8">
<mml:mrow>
<mml:mtext>&#x3b2;</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#xa0;</mml:mo>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>) represent the Podolsky pseudopotential and the zero point vibrational energy correction (<xref ref-type="bibr" rid="B7">Dalbouha et&#x20;al., 2021</xref>). The two last contributions must be computed for all the isotopologues because they are mass dependent properties. &#x3b2;, &#x3b1;, and &#x3b8;, the HNH bending, the NH2 wagging and the torsional coordinates, are defined using curvilinear internal coordinates:<disp-formula id="e5">
<mml:math id="m9">
<mml:mrow>
<mml:mtable>
<mml:mtr>
<mml:mtd>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
<mml:msup>
<mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mtext>HNH</mml:mtext>
<mml:mo>-</mml:mo>
<mml:mtext>HNH</mml:mtext>
</mml:mrow>
<mml:mtext>e</mml:mtext>
</mml:msup>
</mml:mrow>
</mml:mtd>
</mml:mtr>
<mml:mtr>
<mml:mtd>
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>180</mml:mn>
<mml:mtext>.0</mml:mtext>
<mml:mo>-</mml:mo>
<mml:mi mathvariant="normal">&#x3b3;</mml:mi>
</mml:mrow>
</mml:mtd>
</mml:mtr>
<mml:mtr>
<mml:mtd>
<mml:mrow>
<mml:mi mathvariant="normal">&#x3b8;</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mrow>
<mml:mrow>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>H</mml:mtext>
<mml:mn>5</mml:mn>
<mml:mtext>C</mml:mtext>
<mml:mn>4</mml:mn>
<mml:mtext>N</mml:mtext>
<mml:mn>1</mml:mn>
<mml:mtext>X</mml:mtext>
<mml:mo>&#x2b;</mml:mo>
<mml:mtext>H6C4N1X</mml:mtext>
<mml:mo>&#x2b;</mml:mo>
<mml:mtext>H7C4N1X&#xa0;</mml:mtext>
<mml:mo>-</mml:mo>
<mml:mn>2</mml:mn>
<mml:mi>&#x3a0;</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>/</mml:mo>
<mml:mn>3</mml:mn>
</mml:mrow>
</mml:mrow>
</mml:mtd>
</mml:mtr>
</mml:mtable>
</mml:mrow>
</mml:math>
<label>(5)</label>
</disp-formula>
</p>
<p>HNH<sup>e</sup> is the value of the HNH bending angle corresponding to the equilibrium geometry; &#x3b3; represents the angle between the C-N bond and the HNH plane (see <xref ref-type="fig" rid="F1">Figure&#x20;1</xref>); X denotes a ghost atom lying in the HNH plane perpendicular to the HNH angle bisector. The set of internal coordinates were chosen taking into consideration the procedure for the determination of the 3D-PES which demands a partial optimization of the geometry. Three internal coordinates, NHN, &#x3b3; and H5C4N1X distinguish the selected conformations whereas twelve &#x201c;dependent coordinates&#x201d; are allowed to be relaxed in all the structures.</p>
<p>The ab initio three-dimensional potential energy surface, V(<inline-formula id="inf5">
<mml:math id="m10">
<mml:mrow>
<mml:mtext>&#x3b2;</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#xa0;</mml:mo>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>), was computed for the study of the main isotopologue (<xref ref-type="bibr" rid="B58">Senent 2018</xref>). It was constructed using the CCSD(T)-F12/AVTZ energies of 131 geometries defined for selected values of the independent coordinates that were fitted to the following series:<disp-formula id="e6">
<mml:math id="m11">
<mml:mrow>
<mml:mi>V</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mo>&#xa0;</mml:mo>
<mml:mstyle displaystyle="true">
<mml:munder>
<mml:mo>&#x2211;</mml:mo>
<mml:mrow>
<mml:mi>K</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>L</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>M</mml:mi>
</mml:mrow>
</mml:munder>
<mml:mrow>
<mml:msubsup>
<mml:mi>A</mml:mi>
<mml:mrow>
<mml:mi>K</mml:mi>
<mml:mi>M</mml:mi>
<mml:mi>L</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>C</mml:mi>
<mml:mi>C</mml:mi>
</mml:mrow>
</mml:msubsup>
<mml:msup>
<mml:mi>&#x3b2;</mml:mi>
<mml:mi>K</mml:mi>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>cos</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>L</mml:mi>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>cos</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mn>6</mml:mn>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>M</mml:mi>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:msubsup>
<mml:mi>A</mml:mi>
<mml:mrow>
<mml:mi>K</mml:mi>
<mml:mi>M</mml:mi>
<mml:mi>L</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>S</mml:mi>
<mml:mi>S</mml:mi>
</mml:mrow>
</mml:msubsup>
<mml:msup>
<mml:mi>&#x3b2;</mml:mi>
<mml:mi>K</mml:mi>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>sin</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>L</mml:mi>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>sin</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mn>3</mml:mn>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mn>2</mml:mn>
<mml:mi>M</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:mn>1</mml:mn>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
</mml:mstyle>
</mml:mrow>
</mml:math>
<label>(6)</label>
</disp-formula>
</p>
<p>This analytical expression transforms as the totally symmetric representation of the G<sub>12</sub> MSG. Formally identical expressions can be employed for V&#x2019;, V<sup>ZPVE</sup>, V<sup>eff</sup>(<inline-formula id="inf6">
<mml:math id="m12">
<mml:mrow>
<mml:mtext>&#x3b2;</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#xa0;</mml:mo>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>) and the diagonal kinetic energy parameters B<sub>qiqi</sub> of the main isotopologue, <sup>13</sup>CH<sub>3</sub>NH<sub>2</sub> and CH<sub>3</sub>
<sup>15</sup>NH<sub>2</sub>. However, since the H &#x2192;D substitution carries out symmetry changes, the effective potential V<sup>eff</sup>(<inline-formula id="inf7">
<mml:math id="m13">
<mml:mrow>
<mml:mtext>&#x3b2;</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#xa0;</mml:mo>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>) and the diagonal kinetic parameters must be expressed using less-symmetric analytical expressions. For CH<sub>3</sub>NDH (G<sub>6</sub>):<disp-formula id="e7">
<mml:math id="m14">
<mml:mrow>
<mml:msup>
<mml:mi>V</mml:mi>
<mml:mrow>
<mml:mi>e</mml:mi>
<mml:mi>f</mml:mi>
<mml:mi>f</mml:mi>
</mml:mrow>
</mml:msup>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mo>&#xa0;</mml:mo>
<mml:mstyle displaystyle="true">
<mml:munder>
<mml:mo>&#x2211;</mml:mo>
<mml:mrow>
<mml:mi>K</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>L</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>M</mml:mi>
</mml:mrow>
</mml:munder>
<mml:mrow>
<mml:msubsup>
<mml:mi>A</mml:mi>
<mml:mrow>
<mml:mi>K</mml:mi>
<mml:mi>M</mml:mi>
<mml:mi>L</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>C</mml:mi>
<mml:mi>C</mml:mi>
</mml:mrow>
</mml:msubsup>
<mml:msup>
<mml:mi>&#x3b2;</mml:mi>
<mml:mi>K</mml:mi>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>cos</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>L</mml:mi>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>cos</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mn>3</mml:mn>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>M</mml:mi>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:msubsup>
<mml:mi>A</mml:mi>
<mml:mrow>
<mml:mi>K</mml:mi>
<mml:mi>M</mml:mi>
<mml:mi>L</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>S</mml:mi>
<mml:mi>S</mml:mi>
</mml:mrow>
</mml:msubsup>
<mml:msup>
<mml:mi>&#x3b2;</mml:mi>
<mml:mi>K</mml:mi>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>sin</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>L</mml:mi>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>sin</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mn>3</mml:mn>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>M</mml:mi>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
</mml:mstyle>
</mml:mrow>
</mml:math>
<label>(7)</label>
</disp-formula>and for CDH<sub>2</sub>NH<sub>2</sub> (G<sub>4</sub>)<disp-formula id="e8">
<mml:math id="m15">
<mml:mrow>
<mml:msup>
<mml:mi>V</mml:mi>
<mml:mrow>
<mml:mi>e</mml:mi>
<mml:mi>f</mml:mi>
<mml:mi>f</mml:mi>
</mml:mrow>
</mml:msup>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mo>&#xa0;</mml:mo>
<mml:mstyle displaystyle="true">
<mml:munder>
<mml:mo>&#x2211;</mml:mo>
<mml:mrow>
<mml:mi>K</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>L</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>M</mml:mi>
</mml:mrow>
</mml:munder>
<mml:mrow>
<mml:msubsup>
<mml:mi>A</mml:mi>
<mml:mrow>
<mml:mi>K</mml:mi>
<mml:mi>M</mml:mi>
<mml:mi>L</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>C</mml:mi>
<mml:mi>C</mml:mi>
</mml:mrow>
</mml:msubsup>
<mml:msup>
<mml:mi>&#x3b2;</mml:mi>
<mml:mi>K</mml:mi>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>cos</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>L</mml:mi>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>cos</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mn>2</mml:mn>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>M</mml:mi>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:msubsup>
<mml:mi>A</mml:mi>
<mml:mrow>
<mml:mi>K</mml:mi>
<mml:mi>M</mml:mi>
<mml:mi>L</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>S</mml:mi>
<mml:mi>S</mml:mi>
</mml:mrow>
</mml:msubsup>
<mml:msup>
<mml:mi>&#x3b2;</mml:mi>
<mml:mi>K</mml:mi>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>sin</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>L</mml:mi>
<mml:mi>&#x3b1;</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>sin</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mn>2</mml:mn>
<mml:mi>M</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:mn>1</mml:mn>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
</mml:mstyle>
</mml:mrow>
</mml:math>
<label>(8)</label>
</disp-formula>
</p>
<p>To construct the effective potential using <xref ref-type="disp-formula" rid="e4">Eq. 4</xref>, two mass-dependent properties V&#x2032; and V<sup>ZPVE</sup> must be computed for all the isotopologues and for all the geometries. The V&#x2019; pseudopotential is very small. However, V<sup>ZPVE</sup> has important effects on the levels. It was determined within the harmonic approximation at the MP2/AVTZ level of theory. To obtain the mass-dependent properties of the low-symmetry varieties, more than 131 geometries and more than 131 sets of harmonic frequencies need to be computed. For example, in the case of CDH<sub>2</sub>NH<sub>2</sub>, 131x3 geometries are required because the three hydrogen atoms of the methyl group are not identical.</p>
<p>The ground vibrational state potential energy surface contains six equivalent minima corresponding to a single conformer. The contours of <xref ref-type="fig" rid="F2">Figures 2</xref>, <xref ref-type="fig" rid="F3">3</xref> represents layers of the 3D-surface of the main isotopologue containing the minimum energy structure. <xref ref-type="fig" rid="F2">Figure&#x20;2</xref> corresponds to V<sup>eff</sup> (&#x3b1;, &#x3b2;; &#x3b8; &#x3d; 270&#xb0;) and <xref ref-type="fig" rid="F3">Figure&#x20;3</xref> to V<sup>eff</sup> (&#x3b1;, &#x3b8;; &#x3b2; &#x3d; 106&#xb0;). Figures emphasize the coupling between coordinates.</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>V<sup>eff</sup> (&#x3b1;, &#x3b2;; &#x3b8; &#x3d; 270&#x00B0;) two dimensional potential energy surface (in cm<sup>&#x2212;1</sup>).</p>
</caption>
<graphic xlink:href="fchem-09-751203-g002.tif"/>
</fig>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>V<sup>eff</sup> (&#x3b1;, &#x3b8;; &#x3b2; &#x3d; 106&#x00B0;) two dimensional potential energy surface (in cm<sup>&#x2212;1</sup>).</p>
</caption>
<graphic xlink:href="fchem-09-751203-g003.tif"/>
</fig>
<p>The kinetic energy parameters were also computed for all the selected geometries and for all the isotopologues. The number of selected geometries required for their computation in the deuterated forms was 171 and 393 for CH<sub>3</sub>NDH and CDH<sub>2</sub>NH<sub>2</sub>, respectively. For all the symmetries, the diagonal terms B<sub>&#x3b2;&#x3b2;</sub>, B<sub>&#x3b1;&#x3b1;</sub>, and B<sub>&#x3b8;&#x3b8;</sub> transform as the totally symmetric representation A<sub>1</sub>. However, the symmetry properties of the off-diagonal elements vary with the&#x20;MSG:</p>
<p>B<sub>&#x3b1;&#x3b8;</sub> transforms as B<sub>1</sub> (G<sub>12</sub>, G<sub>4</sub>) and A<sub>1</sub>(G<sub>6</sub>)</p>
<p>B<sub>&#x3b1;&#x3b2;</sub> transforms as B<sub>2</sub> (G<sub>12</sub>, G<sub>4</sub>) and A<sub>2</sub>(G<sub>6</sub>)</p>
<p>B<sub>&#x3b8;&#x3b2;</sub> transforms as A<sub>2</sub> (G<sub>12</sub>, G<sub>4</sub>,&#x20;G<sub>6</sub>)</p>
<p>The non-zero coefficients A<sub>000</sub>(B<sub>qiqz</sub>) of the kinetic energy expressions are shown in <xref ref-type="table" rid="T4">Table&#x20;4</xref>. For the main isotopologue, they are compared with previous data (<xref ref-type="bibr" rid="B46">Ohashi et&#x20;al., 1988</xref>, <xref ref-type="bibr" rid="B44">1992</xref>), although in works based in experiments, these coefficients are considered to be constants. The potential energy barriers, V<sup>tor</sup> and V<sup>inv</sup> were estimated using the effective potentials. For the main isotopologue, they are in reasonable good agreement with previous data (<xref ref-type="bibr" rid="B46">Ohashi et&#x20;al., 1988</xref>, <xref ref-type="bibr" rid="B44">1992</xref>) (<xref ref-type="bibr" rid="B29">Kreglewski 1993</xref>). Isotopic shifts of all the potential parameters are only important for the deuterated&#x20;forms.</p>
<table-wrap id="T4" position="float">
<label>TABLE 4</label>
<caption>
<p>CCSD(T)-F12/AVTZ potential energy barriers (in cm<sup>&#x2212;1</sup>).</p>
</caption>
<table>
<thead valign="top">
<tr>
<th rowspan="2" align="left"/>
<th colspan="2" align="center">CH<sub>3</sub>-NH<sub>2</sub>
</th>
<th align="center">
<sup>13</sup>CH<sub>3</sub>-NH<sub>2</sub>
</th>
<th align="center">CH<sub>3</sub>-<sup>15</sup>NH<sub>2</sub>
</th>
<th align="center">CH<sub>3</sub>-NDH</th>
<th align="center">CDH<sub>2</sub>-NH<sub>2</sub>
</th>
</tr>
<tr>
<th align="center">
<italic>This work</italic>
</th>
<th align="center">
<italic>Previous works</italic>
</th>
<th align="center">
<italic>This work</italic>
</th>
<th align="center">
<italic>This work</italic>
</th>
<th align="center">
<italic>This work</italic>
</th>
<th align="center">
<italic>This work</italic>
</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="left">V<sup>tor</sup>
</td>
<td align="char" char=".">703</td>
<td align="char" char="( .">684.71(1)<sup>a</sup>
</td>
<td align="char" char=".">704</td>
<td align="char" char=".">704</td>
<td align="char" char=".">692</td>
<td align="char" char=".">691</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="char" char="( .">681.0(5)<sup>b</sup>
</td>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="char" char=".">714.55<sup>c</sup>
</td>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
</tr>
<tr>
<td align="left">V<sup>inv</sup>
</td>
<td align="char" char=".">1907</td>
<td align="char" char=".">1931.26<sup>c</sup>
</td>
<td align="char" char=".">1927</td>
<td align="char" char=".">1926</td>
<td align="char" char=".">1890</td>
<td align="char" char=".">1907</td>
</tr>
<tr>
<td align="left">A<sub>000</sub>(B<sub>&#x3b2;&#x3b2;</sub>)</td>
<td align="char" char=".">34.8345</td>
<td align="left"/>
<td align="char" char=".">34.8021</td>
<td align="char" char=".">34.7823</td>
<td align="char" char=".">25.9961</td>
<td align="char" char=".">35.1168</td>
</tr>
<tr>
<td align="left">A<sub>000</sub>(B<sub>&#x3b1;&#x3b1;</sub>)</td>
<td align="char" char=".">24.9448</td>
<td align="left"/>
<td align="char" char=".">24.9168</td>
<td align="char" char=".">24.7859</td>
<td align="char" char=".">26.9749</td>
<td align="char" char=".">20.3891</td>
</tr>
<tr>
<td align="left">A<sub>000</sub>(B<sub>&#x3b8;&#x3b8;</sub>)</td>
<td align="char" char=".">19.0289</td>
<td align="char" char="( .">15.1130(2)<sup>a</sup>
</td>
<td align="char" char=".">19.0349</td>
<td align="char" char=".">19.1537</td>
<td align="char" char=".">19.4989</td>
<td align="char" char=".">20.7992</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="char" char="( .">15.03(1)<sup>b</sup>
</td>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
</tr>
<tr>
<td align="left">A<sub>000</sub>(B<sub>&#x3b1;&#x3b8;</sub>)</td>
<td align="char" char=".">0.0</td>
<td align="left"/>
<td align="char" char=".">0.0</td>
<td align="char" char=".">0.0</td>
<td align="char" char=".">5.0554</td>
<td align="char" char=".">&#x2212;0.0129</td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn>
<p>a) <xref ref-type="bibr" rid="B46">Ohashi et al., 1988</xref>; b) <xref ref-type="bibr" rid="B44">Ohashi et al., 1992</xref>; c) <xref ref-type="bibr" rid="B29">Kreglewski 1993</xref>.</p>
</fn>
</table-wrap-foot>
</table-wrap>
<p>Symmetry adapted series were employed as trial functions for the variational calculations. Products of harmonic oscillator solutions X<sub>K</sub> (for the bending coordinate) and double Fourier series (for the wagging and torsional coordinates) were employed. <xref ref-type="table" rid="T5">Table&#x20;5</xref> shows the symmetry eigenvectors. The convergence of the low energy levels requires long basis sets leading to Hamiltonian matrices of 18,755 x18,755 elements. In the case of the G<sub>12</sub> species, the matrices factorize by symmetry into eight blocks which dimensions are 1815 (A<sub>1</sub>, B<sub>2</sub>), 1,518 (B<sub>1</sub>), 1,507 (A<sub>2</sub>), and 3,025 (E<sub>1x</sub>, E<sub>1y</sub>, E<sub>2x</sub> and E<sub>2y</sub>). For the G<sub>6</sub> species, the corresponding submatrix dimensions were 3,333 (A<sub>1</sub>), 3,322 (A<sub>2</sub>), and 6,050 (E), whereas for the G<sub>4</sub> species, the dimensions were 4,840 (A<sub>1</sub>, B<sub>2</sub>), 4,543 (B<sub>1</sub>), and 4,532&#x20;(A<sub>2</sub>).</p>
<table-wrap id="T5" position="float">
<label>TABLE 5</label>
<caption>
<p>Symmetry eigenvectors.<sup>a</sup>.</p>
</caption>
<table>
<tbody valign="top">
<tr>
<td colspan="2" align="left">
<bold>G<sub>12</sub>
</bold>
</td>
</tr>
<tr>
<td align="left">
<bold>A<sub>1</sub>
</bold>
</td>
<td align="center">
<bold>E<sub>1x</sub>
</bold>
</td>
</tr>
<tr>
<td align="left">X<sub>K</sub> cos (L&#x3b1;) cos6M&#x3b8;</td>
<td align="center">X<sub>K</sub> cos (L&#x3b1;) cos (6M &#xb1; 1)&#x3b8;</td>
</tr>
<tr>
<td align="left">X<sub>K</sub> sin (L&#x3b1;) sin(6M &#x2b; 3)&#x3b8;</td>
<td align="center">X<sub>K</sub> sin (L&#x3b1;) sin (6M &#xb1; 2)&#x3b8;</td>
</tr>
<tr>
<td align="left">
<bold>B<sub>1</sub>
</bold>
</td>
<td align="center">
<bold>E<sub>1y</sub>
</bold>
</td>
</tr>
<tr>
<td align="left">X<sub>K</sub> cos (L&#x3b1;) cos(6M &#x2b; 3)&#x3b8;</td>
<td align="center">X<sub>K</sub> sin (L&#x3b1;) cos (6M &#xb1; 2)&#x3b8;</td>
</tr>
<tr>
<td align="left">X<sub>K</sub> sin (L&#x3b1;) sin6M&#x3b8;</td>
<td align="center">X<sub>K</sub> cos (L&#x3b1;) sin (6M &#xb1; 1)&#x3b8;</td>
</tr>
<tr>
<td align="left">
<bold>B<sub>2</sub>
</bold>
</td>
<td align="center">
<bold>E<sub>2x</sub>
</bold>
</td>
</tr>
<tr>
<td align="left">X<sub>K</sub> sin (L&#x3b1;) cos6M&#x3b8;</td>
<td align="center">X<sub>K</sub> cos (L&#x3b1;) cos (6M &#xb1; 2)&#x3b8;</td>
</tr>
<tr>
<td align="left">X<sub>K</sub> cos (L&#x3b1;) sin(6M &#x2b; 3)&#x3b8;</td>
<td align="center">X<sub>K</sub> sin (L&#x3b1;) sin (6M &#xb1; 1)&#x3b8;</td>
</tr>
<tr>
<td align="left">
<bold>A<sub>2</sub>
</bold>
</td>
<td align="center">
<bold>E<sub>2y</sub>
</bold>
</td>
</tr>
<tr>
<td align="left">X<sub>K</sub> sin (L&#x3b1;) cos(6M &#x2b; 3)&#x3b8;</td>
<td align="center">X<sub>K</sub> sin (L&#x3b1;) cos (6M &#xb1; 1)&#x3b8;</td>
</tr>
<tr>
<td align="left">X<sub>K</sub> cos (L&#x3b1;) sin6M&#x3b8;</td>
<td align="center">X<sub>K</sub> cos (L&#x3b1;) sin (6M &#xb1; 2)&#x3b8;</td>
</tr>
<tr>
<td colspan="2" align="left">
<bold>G</bold>
<sub>
<bold>6</bold>
</sub>
</td>
</tr>
<tr>
<td align="left">
<bold>A1</bold>
</td>
<td align="center">
<bold>Ex</bold>
</td>
</tr>
<tr>
<td align="left">X<sub>K</sub> cos (L&#x3b1;) cos3M&#x3b8;</td>
<td align="center">X<sub>K</sub> cos (L&#x3b1;) cos(3M &#xb1; 1)&#x3b8;</td>
</tr>
<tr>
<td align="left">X<sub>K</sub> sin (L&#x3b1;) sin3M&#x3b8;</td>
<td align="center">X<sub>K</sub> sin (L&#x3b1;) sin(3M &#xb1; 1)&#x3b8;</td>
</tr>
<tr>
<td align="left">
<bold>A2</bold>
</td>
<td align="center">
<bold>Ey</bold>
</td>
</tr>
<tr>
<td align="left">X<sub>K</sub> sin (L&#x3b1;) cos3M&#x3b8;</td>
<td align="center">X<sub>K</sub> sin (L&#x3b1;) cos(3M &#xb1; 1)&#x3b8;</td>
</tr>
<tr>
<td align="left">X<sub>K</sub> cos (L&#x3b1;) sin3M&#x3b8;</td>
<td align="center">X<sub>K</sub> cos (L&#x3b1;) sin(3M &#xb1; 1)&#x3b8;</td>
</tr>
<tr>
<td colspan="2" align="left">
<bold>G</bold>
<sub>
<bold>4</bold>
</sub>
</td>
</tr>
<tr>
<td align="left">
<bold>A<sub>1</sub>
</bold>
</td>
<td align="center">
<bold>B<sub>2</sub>
</bold>
</td>
</tr>
<tr>
<td align="left">X<sub>K</sub> cos (L&#x3b1;) cos2M&#x3b8;</td>
<td align="center">X<sub>K</sub> sin (L&#x3b1;) cos2M&#x3b8;</td>
</tr>
<tr>
<td align="left">X<sub>K</sub> sin (L&#x3b1;) sin(2M &#x2b; 1)&#x3b8;</td>
<td align="center">X<sub>K</sub> cos (L&#x3b1;) sin(2M &#x2b; 1)&#x3b8;</td>
</tr>
<tr>
<td align="left">
<bold>B<sub>1</sub>
</bold>
</td>
<td align="center">
<bold>A<sub>2</sub>
</bold>
</td>
</tr>
<tr>
<td align="left">X<sub>K</sub> cos (L&#x3b1;) cos(2M &#x2b; 1)&#x3b8;</td>
<td align="center">X<sub>K</sub> sin (L&#x3b1;) cos(2M &#x2b; 1)&#x3b8;</td>
</tr>
<tr>
<td align="left">X<sub>K</sub> sin (L&#x3b1;) sin2M&#x3b8;</td>
<td align="center">X<sub>K</sub> cos (L&#x3b1;) sin2M&#x3b8;</td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn>
<p>a) K, L, M &#x3d; 0, 1, 2, 3,...</p>
</fn>
</table-wrap-foot>
</table-wrap>
<p>The resulting energy levels are shown in <xref ref-type="table" rid="T6">Table&#x20;6</xref> and they are classified using symmetry and the v<sub>7</sub>, v<sub>9</sub> and v<sub>15</sub> quantum numbers. For the main isotopologue, the energies are compared with those of <xref ref-type="bibr" rid="B30">Kreglewski (1989)</xref> obtained from experimental parameters. The computed levels denote a slight improvement with respect to the work of <xref ref-type="bibr" rid="B58">Senent (2018)</xref>, after using longer expansions for the kinetic energy parameters. The aim was to increase precision considering that isotopic shifts are relatively small. We observed that the vibrational energies are very sensitive to the kinetic contributions. It can be pointed out that their computations in the deuterated forms is not straightforward.</p>
<table-wrap id="T6" position="float">
<label>TABLE 6</label>
<caption>
<p>CCSD(T)-F12 energy levels corresponding to the large amplitude vibration and to the HNH bending mode (in cm<sup>&#x2212;1</sup>). For the main isotopologue, the energies compared with previous data obtained using a two-dimensional model.</p>
</caption>
<table>
<thead>
<tr>
<td rowspan="2" align="left">
<bold>&#x28b;<sub>NN&#x3d;7,9,15</sub>
</bold>
</td>
<td align="left"/>
<td colspan="2" align="center">
<bold>CH<sub>3</sub>NH<sub>2</sub> (G<sub>12</sub>)</bold>
</td>
<td colspan="1" align="center">
<bold>
<sup>13</sup>CH<sub>3</sub>-NH<sub>2</sub> (G<sub>12</sub>)</bold>
</td>
<td colspan="1" align="center">
<bold>CH<sub>3</sub>-<sup>15</sup>NH<sub>2</sub> (G<sub>12</sub>)</bold>
</td>
<td colspan="2" align="center">
<bold>CH<sub>3</sub>-NDH (G<sub>6</sub>)</bold>
</td>
<td colspan="2" align="center">
<bold>CDH<sub>2</sub>-NH<sub>2</sub> (G<sub>4</sub>)</bold>
</td>
</tr>
<tr>
<td align="left"/>
<td align="center">
<bold>
<italic>This work</italic>
</bold>
</td>
<td align="center">
<bold>
<xref ref-type="bibr" rid="B30">Kreglewski (1989)</xref>
</bold>
</td>
<td align="left"/>
<td align="left"/>
<td colspan="2" align="center">
<bold>
<italic>This work</italic>
</bold>
</td>
<td colspan="2" align="left"/>
</tr>
</thead>
<tbody valign="top">
<tr>
<td align="left"/>
<td align="center">
<italic>3D</italic>
</td>
<td align="center">
<italic>2D</italic>
</td>
<td align="left"/>
<td align="left"/>
<td colspan="2" align="center">
<italic>3D</italic>
</td>
<td align="left"/>
<td align="left"/>
</tr>
<tr>
<td rowspan="6" align="left">0 0 0</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">0.000</td>
<td align="center">0.000</td>
<td align="center">0.000</td>
<td align="center">0.000</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">0.000</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">0.000</td>
</tr>
<tr>
<td align="center">B<sub>2</sub>
</td>
<td align="center">0.163</td>
<td align="center">0.078</td>
<td align="center">0.167</td>
<td align="center">0.153</td>
<td align="center">A<sub>2</sub>
</td>
<td align="center">0.071</td>
<td align="center">B<sub>2</sub>
</td>
<td align="center">0.015</td>
</tr>
<tr>
<td align="center">E<sub>1</sub>
</td>
<td align="center">0.325</td>
<td align="center">0.283</td>
<td align="center">0.328</td>
<td align="center">0.322</td>
<td align="center">E</td>
<td align="center">0.117</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">1.491</td>
</tr>
<tr>
<td align="center">E<sub>2</sub>
</td>
<td align="center">0.407</td>
<td align="center">0.338</td>
<td align="center">0.412</td>
<td align="center">0.398</td>
<td align="center">E</td>
<td align="center">0.167</td>
<td align="center">B<sub>2</sub>
</td>
<td align="center">1.542</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">B<sub>1</sub>
</td>
<td align="center">1.605</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">A<sub>2</sub>
</td>
<td align="center">1.672</td>
</tr>
<tr>
<td rowspan="6" align="left">0 0 1</td>
<td align="center">B<sub>1</sub>
</td>
<td align="center">265.572</td>
<td align="center">269.88</td>
<td align="center">264.441</td>
<td align="center">264.428</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">236.260</td>
<td align="center">A<sub>2</sub>
</td>
<td align="center">254.110</td>
</tr>
<tr>
<td align="center">A<sub>2</sub>
</td>
<td align="center">266.117</td>
<td align="center">270.20</td>
<td align="center">264.995</td>
<td align="center">264.936</td>
<td align="center">A<sub>2</sub>
</td>
<td align="center">236.470</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">254.315</td>
</tr>
<tr>
<td align="center">E<sub>1</sub>
</td>
<td align="center">259.316</td>
<td align="center">260.94</td>
<td align="center">258.241</td>
<td align="center">258.260</td>
<td align="center">E</td>
<td align="center">233.470</td>
<td align="center">B<sub>1</sub>
</td>
<td align="center">254.384</td>
</tr>
<tr>
<td align="center">E<sub>2</sub>
</td>
<td align="center">259.066</td>
<td align="center">261.18</td>
<td align="center">257.987</td>
<td align="center">258.027</td>
<td align="center">E</td>
<td align="center">233.571</td>
<td align="center">B<sub>2</sub>
</td>
<td align="center">254.589</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">B<sub>1</sub>
</td>
<td align="center">259.182</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">A<sub>2</sub>
</td>
<td align="center">259.774</td>
</tr>
<tr>
<td rowspan="6" align="left">0 0 2</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">447.074</td>
<td align="center">419.47</td>
<td align="center">446.642</td>
<td align="center">447.022</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">416.671</td>
<td align="center">B<sub>2</sub>
</td>
<td align="center">436.260</td>
</tr>
<tr>
<td align="center">B<sub>2</sub>
</td>
<td align="center">447.418</td>
<td align="center">420.17</td>
<td align="center">446.981</td>
<td align="center">447.347</td>
<td align="center">A<sub>2</sub>
</td>
<td align="center">416.888</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">436.350</td>
</tr>
<tr>
<td align="center">E<sub>1</sub>
</td>
<td align="center">484.483</td>
<td align="center">464.93</td>
<td align="center">485.819</td>
<td align="center">485.980</td>
<td align="center">E</td>
<td align="center">439.614</td>
<td align="center">B<sub>2</sub>
</td>
<td align="center">436.868</td>
</tr>
<tr>
<td align="center">E<sub>2</sub>
</td>
<td align="center">486.661</td>
<td align="center">464.36</td>
<td align="center">485.990</td>
<td align="center">486.150</td>
<td align="center">E</td>
<td align="center">439.790</td>
<td align="center">B<sub>1&#x2b;</sub>
</td>
<td align="center">469.827</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">A<sub>2</sub>
</td>
<td align="center">470.213</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">A<sub>1</sub>
</td>
<td align="center">470.501</td>
</tr>
<tr>
<td rowspan="6" align="left">0 1 0</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">771.083</td>
<td align="center">729.39</td>
<td align="center">776.413</td>
<td align="center">763.689</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">715.178</td>
<td align="center">B<sub>2</sub>
</td>
<td align="center">767.484</td>
</tr>
<tr>
<td align="center">B<sub>2</sub>
</td>
<td align="center">775.011</td>
<td align="center">727.36</td>
<td align="center">777.617</td>
<td align="center">769.602</td>
<td align="center">A<sub>2</sub>
</td>
<td align="center">718.848</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">767.952</td>
</tr>
<tr>
<td align="center">E<sub>1</sub>
</td>
<td align="center">773.482</td>
<td align="center">769.96</td>
<td align="center">778.819</td>
<td align="center">765.948</td>
<td align="center">E</td>
<td align="center">715.901</td>
<td align="center">B<sub>1</sub>
</td>
<td align="center">772.529</td>
</tr>
<tr>
<td align="center">E<sub>2</sub>
</td>
<td align="center">777.407</td>
<td align="center">766.97</td>
<td align="center">782.846</td>
<td align="center">769.669</td>
<td align="center">E</td>
<td align="center">718.291</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">774.561</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">A<sub>2</sub>
</td>
<td align="center">775.594</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">B<sub>2</sub>
</td>
<td align="center">779.235</td>
</tr>
<tr>
<td rowspan="6" align="left">0 0 3</td>
<td align="center">B<sub>1</sub>
</td>
<td align="center">764.073</td>
<td align="center">732.43</td>
<td align="center">763.519</td>
<td align="center">763.290</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">664.079</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">598.372</td>
</tr>
<tr>
<td align="center">A<sub>2</sub>
</td>
<td align="center">764.112</td>
<td align="center">733.47</td>
<td align="center">763.543</td>
<td align="center">763.344</td>
<td align="center">A<sub>2</sub>
</td>
<td align="center">664.202</td>
<td align="center">B<sub>2</sub>
</td>
<td align="center">598.567</td>
</tr>
<tr>
<td align="center">E<sub>1</sub>
</td>
<td align="center">623.966</td>
<td align="center">586.69</td>
<td align="center">623.904</td>
<td align="center">624.147</td>
<td align="center">E</td>
<td align="center">566.925</td>
<td align="center">A<sub>2</sub>
</td>
<td align="center">599.434</td>
</tr>
<tr>
<td align="center">E<sub>2</sub>
</td>
<td align="center">623.909</td>
<td align="center">587.55</td>
<td align="center">623.863</td>
<td align="center">624.088</td>
<td align="center">E</td>
<td align="center">567.015</td>
<td align="center">B<sub>1</sub>
</td>
<td align="center">599.613</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">B<sub>1</sub>
</td>
<td align="center">724.376</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">A<sub>2</sub>
</td>
<td align="center">724.454</td>
</tr>
<tr>
<td rowspan="6" align="left">0 0 4</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">779.811</td>
<td align="center">776.16</td>
<td align="center">779.725</td>
<td align="center">779.716</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">689.459</td>
<td align="center">B<sub>2</sub>
</td>
<td align="center">737.897</td>
</tr>
<tr>
<td align="center">B<sub>2</sub>
</td>
<td align="center">783.640</td>
<td align="center">783.91</td>
<td align="center">786.487</td>
<td align="center">781.134</td>
<td align="center">A<sub>2</sub>
</td>
<td align="center">689.207</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">739.049</td>
</tr>
<tr>
<td align="center">E<sub>1</sub>
</td>
<td align="center">961.292</td>
<td align="center">917.30</td>
<td align="center">960.940</td>
<td align="center">960.471</td>
<td align="center">E</td>
<td align="center">825.383</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">905.008</td>
</tr>
<tr>
<td align="center">E<sub>2</sub>
</td>
<td align="center">960.857</td>
<td align="center">919.24</td>
<td align="center">960.579</td>
<td align="center">959.974</td>
<td align="center">E</td>
<td align="center">825.524</td>
<td align="center">B<sub>2</sub>
</td>
<td align="center">905.345</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">A<sub>2</sub>
</td>
<td align="center">905.499</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">B<sub>1</sub>
</td>
<td align="center">905.780</td>
</tr>
<tr>
<td rowspan="6" align="left">0 1 1</td>
<td align="center">B<sub>1</sub>
</td>
<td align="center">1,013.573</td>
<td align="center">1,018.95</td>
<td align="center">1,017.495</td>
<td align="center">1,005.532</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">935.768</td>
<td align="center">A<sub>2</sub>
</td>
<td align="center">997.758</td>
</tr>
<tr>
<td align="center">A<sub>2</sub>
</td>
<td align="center">1,036.858</td>
<td align="center">1,038.29</td>
<td align="center">1,041.180</td>
<td align="center">1,027.452</td>
<td align="center">A<sub>2</sub>
</td>
<td align="center">945.547</td>
<td align="center">B<sub>1</sub>
</td>
<td align="center">1,000.853</td>
</tr>
<tr>
<td align="center">E<sub>1</sub>
</td>
<td align="center">1,018.895</td>
<td align="center">1,008.94</td>
<td align="center">1,023.138</td>
<td align="center">1,010.215</td>
<td align="center">E</td>
<td align="center">933.720</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">1,001.672</td>
</tr>
<tr>
<td align="center">E<sub>2</sub>
</td>
<td align="center">1,009.382</td>
<td align="center">1,010.33</td>
<td align="center">1,013.343</td>
<td align="center">1,001.258</td>
<td align="center">E</td>
<td align="center">938.159</td>
<td align="center">B<sub>1</sub>
</td>
<td align="center">1,008.420</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">B<sub>2</sub>
</td>
<td align="center">1,011.166</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">A<sub>2</sub>
</td>
<td align="center">1,026.022</td>
</tr>
<tr>
<td rowspan="6" align="left">0 1 2</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">1,164.413</td>
<td align="left"/>
<td align="center">1,169.282</td>
<td align="center">1,157.813</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">1,091.240</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">1,147.762</td>
</tr>
<tr>
<td align="center">B<sub>2</sub>
</td>
<td align="center">1,178.154</td>
<td align="left"/>
<td align="center">1,182.743</td>
<td align="center">1,171.147</td>
<td align="center">A<sub>2</sub>
</td>
<td align="center">1,102.316</td>
<td align="center">B<sub>2</sub>
</td>
<td align="center">1,164.196</td>
</tr>
<tr>
<td align="center">E<sub>1</sub>
</td>
<td align="center">1,183.366</td>
<td align="left"/>
<td align="center">1,182.979</td>
<td align="center">1,181.927</td>
<td align="center">E</td>
<td align="center">1,122.545</td>
<td align="center">B<sub>2</sub>
</td>
<td align="center">1,195.131</td>
</tr>
<tr>
<td align="center">E<sub>2</sub>
</td>
<td align="center">1,183.676</td>
<td align="left"/>
<td align="center">1,183.288</td>
<td align="center">1,182.336</td>
<td align="center">E</td>
<td align="center">1,131.506</td>
<td align="center">B<sub>1</sub>
</td>
<td align="center">1,195.903</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">A<sub>1</sub>
</td>
<td align="center">1,202.220</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">A<sub>2</sub>
</td>
<td align="center">1,207.561</td>
</tr>
<tr>
<td rowspan="6" align="left">0 2 0</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">1,383.962</td>
<td align="left"/>
<td align="center">1,389.035</td>
<td align="center">1,372.966</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">1,255.006</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">1,382.358</td>
</tr>
<tr>
<td align="center">B<sub>2</sub>
</td>
<td align="center">1,423.217</td>
<td align="left"/>
<td align="center">1,427.359</td>
<td align="center">1,414.927</td>
<td align="center">A<sub>2</sub>
</td>
<td align="center">1,271.686</td>
<td align="center">B<sub>2</sub>
</td>
<td align="center">1,393.998</td>
</tr>
<tr>
<td align="center">E<sub>1</sub>
</td>
<td align="center">1,408.533</td>
<td align="left"/>
<td align="center">1,414.258</td>
<td align="center">1,398.004</td>
<td align="center">E</td>
<td align="center">1,267.221</td>
<td align="center">B<sub>1</sub>
</td>
<td align="center">1,404.544</td>
</tr>
<tr>
<td align="center">E<sub>2</sub>
</td>
<td align="center">1,443.195</td>
<td align="left"/>
<td align="center">1,448.522</td>
<td align="center">1,431.945</td>
<td align="center">E</td>
<td align="center">1,280.415</td>
<td align="center">B<sub>2</sub>
</td>
<td align="center">1,409.878</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">A<sub>1</sub>
</td>
<td align="center">1,431.111</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">A<sub>2</sub>
</td>
<td align="center">1,432.783</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
</tr>
<tr>
<td align="left">&#x2003;1 0 0</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">1,648.554</td>
<td align="center">1,628.67</td>
<td align="center">1,636.359</td>
<td align="center">1,656.933</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">1,407.586</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">1,643.044</td>
</tr>
<tr>
<td align="left"/>
<td align="center">B<sub>2</sub>
</td>
<td align="center">1,659.193</td>
<td align="center">1,651.28</td>
<td align="center">1,648.221</td>
<td align="center">1,667.223</td>
<td align="center">A<sub>2</sub>
</td>
<td align="center">1,436.635</td>
<td align="center">A<sub>2</sub>
</td>
<td align="center">1,643.704</td>
</tr>
<tr>
<td align="left"/>
<td align="center">E<sub>1</sub>
</td>
<td align="center">1,637.115</td>
<td align="left"/>
<td align="center">1,629.309</td>
<td align="center">1,679.237</td>
<td align="center">E</td>
<td align="center">1,404.920</td>
<td align="center">A<sub>1</sub>
</td>
<td align="center">1,649.293</td>
</tr>
<tr>
<td align="left"/>
<td align="center">E<sub>2</sub>
</td>
<td align="center">1,656.584</td>
<td align="left"/>
<td align="center">1,646.585</td>
<td align="center">1,662.688</td>
<td align="center">E</td>
<td align="center">1,418.014</td>
<td align="center">B<sub>2</sub>
</td>
<td align="center">1,661.305</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">B<sub>2</sub>
</td>
<td align="center">1,670.498</td>
</tr>
<tr>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="left"/>
<td align="center">B<sub>1</sub>
</td>
<td align="center">1,673.893</td>
</tr>
<tr>
<td colspan="2" align="center">&#x2003;ZPVE</td>
<td align="center">1,382.996</td>
<td align="center">561.00</td>
<td align="center">1,381.794</td>
<td align="center">1,383.940</td>
<td colspan="2" align="center">1,191.310</td>
<td colspan="2" align="center">1,370.190</td>
</tr>
</tbody>
</table>
</table-wrap>
<p>Each energy level splits into six components corresponding to the six minima of the potential energy surface. Their distributions are represented in <xref ref-type="fig" rid="F4">Figure&#x20;4</xref>. In the G<sub>12</sub> species, the levels split into two non-degenerate and two double-degenerated sublevels. The components of the ground vibrational state were computed to lie at 0.000 (A<sub>1</sub>), 0.163 (B<sub>2</sub>), 0.325 (E<sub>1</sub>), and 0.407 (E<sub>2</sub>) cm<sup>&#x2212;1</sup>. Very small shifts are found for <sup>13</sup>CH<sub>3</sub>-NH<sub>2</sub>, whereas for CH<sub>3</sub>-<sup>15</sup>NH<sub>2</sub>, the subcomponents are close in energy (0.000 (A<sub>1</sub>), 0.153 (B<sub>2</sub>), 0.322 (E<sub>1</sub>), and 0.398 (E<sub>2</sub>)). The non-degenerated components B<sub>1</sub> and A<sub>2</sub> of the &#x28b;<sub>15</sub> fundamental (0 0&#x20;1) were obtained to lie at 265.572 and 266.117&#x20;cm<sup>&#x2212;1</sup> in the main isotopologue and at 264.441 and 264.995 cm&#x2212;1 in <sup>13</sup>CH<sub>3</sub>-NH<sub>2</sub>, and at 264.428 and 264.936&#x20;cm<sup>&#x2212;1</sup> in CH<sub>3</sub>-<sup>15</sup>NH<sub>2.</sub> For &#x28b;<sub>9,</sub> the corresponding components of the (0 1&#x20;0) level were obtained to lie at 771.083 and 775.011 in the main isotopologue and at 776.413 and 777.617 cm&#x2212;1 in <sup>13</sup>CH<sub>3</sub>-NH<sub>2</sub>, and at 763.413 and 769.602 cm&#x2212;1 in CH<sub>3</sub>-<sup>15</sup>NH<sub>2.</sub> It may be concluded that the effects of isotopic substitutions on the heavy atoms are less relevant for the torsional excitation than for inversion excitations.</p>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>Subcomponents of the (0 0&#x20;0) and (0 01) energy levels.</p>
</caption>
<graphic xlink:href="fchem-09-751203-g004.tif"/>
</fig>
<p>As was expected, isotopic effects on the low-lying energies are more noticeable for the deuterated species. For CH<sub>3</sub>-NDH, the nondegenerate components of the &#x28b;<sub>9</sub> and &#x28b;<sub>15</sub> fundamentals have been computed to be 236.260 and 236.470&#x20;cm<sup>&#x2212;1</sup>, and to be 715.178 and 718.848&#x20;cm<sup>&#x2212;1</sup>. The gaps among subcomponents of the ground vibrational state are smaller than in the hydrogenated species. The isotopic substitution in one methyl group hydrogen breaks ten the degeneracy of the CDH<sub>2</sub>NH<sub>2</sub> levels. The ground vibrational state splits into two A<sub>1</sub>, two B<sub>2</sub>, one B<sub>1</sub> and one A<sub>2</sub> components lying in the 0.000&#x2013;1.672&#x20;cm<sup>&#x2212;1</sup>&#x20;range.</p>
</sec>
</sec>
<sec sec-type="conclusion" id="s3">
<title>Conclusion</title>
<p>This work describes the shifts of spectroscopic parameters and the symmetry changes due to the isotopic substitutions for various probably detectable methylamine isotopologues, <sup>13</sup>CH<sub>3</sub>NH<sub>2</sub>, CH<sub>3</sub>
<sup>15</sup>NH<sub>2</sub>, CH<sub>3</sub>NHD, and CDH<sub>2</sub>ND<sub>2</sub>. A variational procedure and VPT2 theory are employed for describing rovibrational properties with a special attention to the far infrared region. For all the isotopologues, the levels up to 1,500&#xa0;cm<sup>&#x2212;1</sup> over the ground vibrational state are determine variationally and classified using the G<sub>12</sub>, G<sub>6</sub> and G<sub>4</sub> MSG properties. For the main isotopologue, the ground vibrational state splits into six components computed to lie at 0.000 (A<sub>1</sub>), 0.163 (B<sub>2</sub>), 0.325 (E<sub>1</sub>), and 0.407 (E<sub>2</sub>) cm<sup>&#x2212;1</sup>. Very small differences are found for <sup>13</sup>CH<sub>3</sub>-NH<sub>2</sub>, whereas for CH<sub>3</sub>-<sup>15</sup>NH<sub>2</sub>, the computed subcomponents are close in energy (0.000 (A<sub>1</sub>), 0.153 (B<sub>2</sub>), 0.322 (E<sub>1</sub>), and 0.398 (E<sub>2</sub>)). Isotopic shifts are relevant for the deuterated forms, whereas the effects of substitution of heavy atoms are less relevant for the torsional excitation than for inversion excitations. Small variations of the kinetic energy parameters carry out substantial displacements of the levels. It can be pointed out that their computations in the deuterated forms is not straightforward.</p>
</sec>
</body>
<back>
<sec id="s4">
<title>Data Availability Statement</title>
<p>The original contributions presented in the study are included in the article/Supplementary Material, further inquiries can be directed to the corresponding authors.</p>
</sec>
<sec id="s5">
<title>Author Contributions</title>
<p>MA has performed the new ab initio calculations. MS was responsible for the variational calculations, the assignments of the levels, and for writing the manuscript.</p>
</sec>
<sec id="s6">
<title>Funding</title>
<p>The authors would like to extend their sincere appreciation to the Deanship of Scientific Research at King Saud University for funding the research through the Research Group Project No. RG-333. This research was supported by the Ministerio de Ciencia, Innovaci&#xf3;n y Universidades of Spain through the grants EIN 2019-103072 and FIS 2016-76418-P. The author acknowledges the &#x201c;Red Espa&#xf1;ola de Computaci&#xf3;n&#x201d; for the grants AECT-2020-2-0008 and RES-AECT-2020-3-0011.</p>
</sec>
<sec sec-type="COI-statement" id="s7">
<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="s8">
<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>The author acknowledges the CTI (CSIC) and CESGA for computing facilities.</p>
</ack>
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