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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Phys.</journal-id>
<journal-title>Frontiers in Physics</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Phys.</abbrev-journal-title>
<issn pub-type="epub">2296-424X</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="publisher-id">1252725</article-id>
<article-id pub-id-type="doi">10.3389/fphy.2023.1252725</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Physics</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>A strong-field THz light source based on coherent transition radiation</article-title>
<alt-title alt-title-type="left-running-head">Kang et al.</alt-title>
<alt-title alt-title-type="right-running-head">
<ext-link ext-link-type="uri" xlink:href="https://doi.org/10.3389/fphy.2023.1252725">10.3389/fphy.2023.1252725</ext-link>
</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname>Kang</surname>
<given-names>Yin</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/2294407/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Wang</surname>
<given-names>Ruoyu</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Chen</surname>
<given-names>Wei</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Tu</surname>
<given-names>Lingjun</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Zhang</surname>
<given-names>Kaiqing</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/2372405/overview"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Feng</surname>
<given-names>Chao</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1937450/overview"/>
</contrib>
</contrib-group>
<aff id="aff1">
<sup>1</sup>
<institution>Shanghai Institute of Applied Physics</institution>, <institution>Chinese Academy of Sciences</institution>, <addr-line>Shanghai</addr-line>, <country>China</country>
</aff>
<aff id="aff2">
<sup>2</sup>
<institution>University of Chinese Academy of Sciences</institution>, <addr-line>Beijing</addr-line>, <country>China</country>
</aff>
<aff id="aff3">
<sup>3</sup>
<institution>School of Physical Science and Technology, ShanghaiTech University</institution>, <addr-line>Shanghai</addr-line>, <country>China</country>
</aff>
<aff id="aff4">
<sup>4</sup>
<institution>Shanghai Advanced Research Institution</institution>, <institution>Chinese Academy of Sciences</institution>, <addr-line>Shanghai</addr-line>, <country>China</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/2066769/overview">Li Li</ext-link>, Harbin Institute of Technology, China</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/309174/overview">Longqing Cong</ext-link>, Nanyang Technological University, Singapore</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1727128/overview">Anil Kumar Malik</ext-link>, Chaudhary Charan Singh University, India</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Kaiqing Zhang, <email>zhangkq@sari.ac.cn</email>
</corresp>
</author-notes>
<pub-date pub-type="epub">
<day>13</day>
<month>09</month>
<year>2023</year>
</pub-date>
<pub-date pub-type="collection">
<year>2023</year>
</pub-date>
<volume>11</volume>
<elocation-id>1252725</elocation-id>
<history>
<date date-type="received">
<day>04</day>
<month>07</month>
<year>2023</year>
</date>
<date date-type="accepted">
<day>28</day>
<month>08</month>
<year>2023</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2023 Kang, Wang, Chen, Tu, Zhang and Feng.</copyright-statement>
<copyright-year>2023</copyright-year>
<copyright-holder>Kang, Wang, Chen, Tu, Zhang and Feng</copyright-holder>
<license xlink:href="http://creativecommons.org/licenses/by/4.0/">
<p>This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.</p>
</license>
</permissions>
<abstract>
<p>Terahertz (THz) radiation is a powerful tool for exploring various scientific frontiers through THz pump&#x2013;probe experiments. However, different experiments may require THz radiation with different spectral properties, such as broad-band or narrow-band, which are difficult to be generated by a single light source. In this paper, we propose a THz light source that can produce both types of THz radiation by manipulating the longitudinal profile of an electron beam and exploiting coherent transition radiation. We perform theoretical analysis and numerical simulations based on the parameters of the Shanghai soft X-ray Free-Electron Laser facility, and the results show that the proposed light source can generate broad-band THz radiation with a pulse energy of 342&#xa0;&#xb5;J and narrow-band THz radiation with a pulse energy of 91&#xa0;&#xb5;J. The proposed light source can offer more flexibility and versatility for free-electron laser (FEL) users to conduct THz pump&#x2013;probe experiments.</p>
</abstract>
<kwd-group>
<kwd>coherent transition radiation</kwd>
<kwd>strong-field THz radiation</kwd>
<kwd>broad-band and narrow-band THz radiation</kwd>
<kwd>frequency beating</kwd>
<kwd>electron beam manipulation</kwd>
</kwd-group>
<custom-meta-wrap>
<custom-meta>
<meta-name>section-at-acceptance</meta-name>
<meta-value>Optics and Photonics</meta-value>
</custom-meta>
</custom-meta-wrap>
</article-meta>
</front>
<body>
<sec id="s1">
<title>1 Introduction</title>
<p>Terahertz (THz) radiation, which lies between 0.1&#xa0;THz and tens of THz, is widely used in many industrial applications, such as medical imaging, quality testing, and wireless communication [<xref ref-type="bibr" rid="B1">1</xref>, <xref ref-type="bibr" rid="B2">2</xref>]. In recent years, THz radiation has become increasingly important in many scientific frontiers with the development of strong-field THz, which can be used to conduct the so-called THz pump&#x2013;probe experiments. THz users from different scientific fields need THz radiation with different spectral properties: narrow-band THz radiation can manipulate transient substances (lattice vibration, spin precession, and atomic photoionization emission) [<xref ref-type="bibr" rid="B3">3</xref>&#x2013;<xref ref-type="bibr" rid="B7">7</xref>], be used to study the transition from insulators to metals or the ultrafast melting of metals [<xref ref-type="bibr" rid="B8">8</xref>], and achieve quantum control in information science [<xref ref-type="bibr" rid="B9">9</xref>]. However, broad-band THz is more suitable to do the time-domain spectral analysis of materials [<xref ref-type="bibr" rid="B10">10</xref>&#x2013;<xref ref-type="bibr" rid="B12">12</xref>] and study nonlinear physical phenomena [<xref ref-type="bibr" rid="B13">13</xref>] because it has higher peak field strength and contains many characteristic fingerprints of materials between 0.1 and 5&#xa0;THz.</p>
<p>Presently, strong-field THz radiation can be produced by ultrafast laser [<xref ref-type="bibr" rid="B14">14</xref>, <xref ref-type="bibr" rid="B15">15</xref>], laser-produced plasma [<xref ref-type="bibr" rid="B16">16</xref>&#x2013;<xref ref-type="bibr" rid="B21">21</xref>], and an electron accelerator [<xref ref-type="bibr" rid="B22">22</xref>, <xref ref-type="bibr" rid="B23">23</xref>]. Among them, the electron accelerator-based THz light source has been treated as a reliable method to produce strong-field THz radiation with tunable frequency. In recent years, THz radiation in a high-gain free-electron laser (FEL) facility [<xref ref-type="bibr" rid="B24">24</xref>&#x2013;<xref ref-type="bibr" rid="B29">29</xref>] has been one of the main choices for producing strong-field THz radiation, and the FEL facility can generate synchronized high-power X-ray pulse, which has been an excellent experimental platform for THz pump&#x2013;probe experiments. In an FEL facility, THz radiation with a broad spectral bandwidth of about 10% can be obtained by compressing the duration of the electron beam into 1&#xa0;THz period [<xref ref-type="bibr" rid="B24">24</xref>&#x2013;<xref ref-type="bibr" rid="B26">26</xref>]. However, since it is difficult to compress beam length below 100 femtosecond (fs) and the spectral bandwidth is relative broad due to the single THz period, the THz frequency is limited to about 5&#xa0;THz. On the contrary, the electron beam train, produced by direct laser pulse stacking [<xref ref-type="bibr" rid="B30">30</xref>], transverse and longitudinal phase space exchange [<xref ref-type="bibr" rid="B31">31</xref>], dielectric tube wakefield modulation [<xref ref-type="bibr" rid="B32">32</xref>, <xref ref-type="bibr" rid="B33">33</xref>], and space-charge oscillation modulation [<xref ref-type="bibr" rid="B34">34</xref>, <xref ref-type="bibr" rid="B35">35</xref>], can be used to obtain THz radiation with higher frequency and relative narrower bandwidth. However, it is hard to obtain both broad-band and narrow-band THz radiation with the same THz light source.</p>
<p>In this paper, a THz light source has been proposed to generate both broad-band and narrow-band THz pulses by manipulating the longitudinal profile of the electron beam. When the electron beam passes through the interface between media with different dielectric constants, it can produce THz radiation with different spectral properties: broad-band for the single-period beam and narrow-band for the bunch train. The paper is organized as follows: the principles of the method are introduced in <xref ref-type="sec" rid="s2">Section 2</xref>. The simulation results using the parameters of the Shanghai soft X-ray free-electron laser facility (SXFEL) are presented in <xref ref-type="sec" rid="s3">Section 3</xref>. Finally, some concluding comments are given in <xref ref-type="sec" rid="s4">Section 4</xref>.</p>
</sec>
<sec id="s2">
<title>2 Principles and methods</title>
<p>The coherent transition radiation (CTR) is a dipole field radiation generated on both sides of two media due to the collapse and expansion of the dipole field [<xref ref-type="bibr" rid="B36">36</xref>, <xref ref-type="bibr" rid="B37">37</xref>]. The radiation power can be expressed by Larmor&#x2019;s formula <inline-formula id="inf1">
<mml:math id="m1">
<mml:mrow>
<mml:mi>P</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>2</mml:mn>
<mml:msup>
<mml:mi>e</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:msup>
<mml:mi>a</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:msup>
<mml:mi>&#x3b3;</mml:mi>
<mml:mn>4</mml:mn>
</mml:msup>
<mml:mo>/</mml:mo>
<mml:mn>3</mml:mn>
<mml:msup>
<mml:mi>c</mml:mi>
<mml:mn>3</mml:mn>
</mml:msup>
</mml:mrow>
</mml:math>
</inline-formula>, where <italic>e</italic> is the electron charge, <italic>a</italic> is the acceleration, <italic>c</italic> is the speed of light, and <inline-formula id="inf2">
<mml:math id="m2">
<mml:mrow>
<mml:mi>&#x3b3;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> is the relativistic factor [<xref ref-type="bibr" rid="B38">38</xref>]. According to Larmor&#x2019;s formula, the coherent radiation power is proportional to the fourth power of the beam energy so that high-energy electron beams are generally required to produce strong-field THz pulses. The schematic layout of the proposed THz light source is shown in <xref ref-type="fig" rid="F1">Figure 1</xref>. The proposed THz light source can produce both broad-band THz radiation and narrow-band strong-field THz radiation.</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>Schematic layout of the proposed THz light source based on the CTR. The modulation and dispersion sections (in the red box) are turned off and treated as drift sections for the broad-band radiation case.</p>
</caption>
<graphic xlink:href="fphy-11-1252725-g001.tif"/>
</fig>
<sec id="s2-1">
<title>2.1 Transition radiation of the compressed electron beam</title>
<p>In <xref ref-type="fig" rid="F1">Figure 1</xref>, an electron beam with an energy chirp is first generated by Linac 1, and then the electron beam is compressed by the magnetic bunch compressor (BC), where the length of the electron beam can be controlled by adjusting the energy chirp and the intensity of the BC. Generally, the longitudinal structures of the electron beam can be expressed by the following equation:<disp-formula id="e1">
<mml:math id="m3">
<mml:mrow>
<mml:mi>S</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>z</mml:mi>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:mi mathvariant="italic">exp</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mfrac>
<mml:msup>
<mml:mi>z</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:msubsup>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
<mml:mn>2</mml:mn>
</mml:msubsup>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
<mml:mrow>
<mml:msqrt>
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:mi>&#x3c0;</mml:mi>
</mml:mrow>
</mml:msqrt>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfrac>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(1)</label>
</disp-formula>where <italic>Z</italic> is the longitudinal coordinate of the electron beam and <inline-formula id="inf3">
<mml:math id="m4">
<mml:mrow>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> is the length of the electron beam (rms). After that, the compressed electron beam passes through another accelerator section (Linac 2) to reach the final beam energy. The beam then produces transition radiation by passing through a metal foil directly, without the modulation and dispersion sections (chicane) in <xref ref-type="fig" rid="F1">Figure 1</xref>, which are treated as drift sections (turning powers off). We use an aluminum (Al) foil as an example since the material of the foil has little effect on THz transition radiation [<xref ref-type="bibr" rid="B39">39</xref>, <xref ref-type="bibr" rid="B40">40</xref>].</p>
<p>The transition radiation can be divided into forward radiation and backward radiation, which have different formation length <italic>L</italic>. Compared with forward radiation, backward radiation has a much shorter formation length [<xref ref-type="bibr" rid="B41">41</xref>, <xref ref-type="bibr" rid="B42">42</xref>] and is easier to be collected. If only considering backward radiation, the transition radiation of a single electron can be expressed by the Ginzburg&#x2013;Frank formula [<xref ref-type="bibr" rid="B36">36</xref>].<disp-formula id="e2">
<mml:math id="m5">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:msup>
<mml:mi>d</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:msub>
<mml:mi>P</mml:mi>
<mml:mi>e</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi mathvariant="normal">&#x3a9;</mml:mi>
<mml:mi>d</mml:mi>
<mml:mi>k</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:msub>
<mml:mi>r</mml:mi>
<mml:mi>e</mml:mi>
</mml:msub>
<mml:mi>m</mml:mi>
<mml:msup>
<mml:mi>c</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:mrow>
<mml:msup>
<mml:mi>&#x3c0;</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:mfrac>
<mml:mfrac>
<mml:mrow>
<mml:msup>
<mml:mi>&#x3b2;</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:msup>
<mml:mi mathvariant="italic">sin</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
<mml:msup>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mn>1</mml:mn>
<mml:mo>&#x2212;</mml:mo>
<mml:msup>
<mml:mi>&#x3b2;</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:msup>
<mml:mi mathvariant="italic">cos</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:mfrac>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(2)</label>
</disp-formula>where <inline-formula id="inf4">
<mml:math id="m6">
<mml:mrow>
<mml:msub>
<mml:mi>r</mml:mi>
<mml:mi>e</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> is the classical electron radius, <italic>m</italic> is the rest mass of the electron, <inline-formula id="inf5">
<mml:math id="m7">
<mml:mrow>
<mml:mi mathvariant="normal">&#x3a9;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> is the solid angle, <italic>k</italic> is the wave number of radiation, <inline-formula id="inf6">
<mml:math id="m8">
<mml:mrow>
<mml:mi>&#x3b2;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> is the relative speed, and <inline-formula id="inf7">
<mml:math id="m9">
<mml:mrow>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> is the angle measured against the backward radiation. For an electron beam, the form factor of the electron beam <inline-formula id="inf8">
<mml:math id="m10">
<mml:mrow>
<mml:mi>F</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>k</mml:mi>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mfenced open="|" close="|" separators="|">
<mml:mrow>
<mml:mo>&#x222b;</mml:mo>
<mml:msup>
<mml:mi>e</mml:mi>
<mml:mrow>
<mml:mi>i</mml:mi>
<mml:mi>k</mml:mi>
<mml:mi>z</mml:mi>
</mml:mrow>
</mml:msup>
<mml:mi>S</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>z</mml:mi>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi>z</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:mrow>
</mml:math>
</inline-formula> is the square of the Fourier transform result for the normalized longitudinal particle distribution within the electron beam, which greatly affects the intensity of transition radiation. The form factor of the compressed electron beam can be expressed as follows:<disp-formula id="e3">
<mml:math id="m11">
<mml:mrow>
<mml:msub>
<mml:mi>F</mml:mi>
<mml:mi>b</mml:mi>
</mml:msub>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>k</mml:mi>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:msup>
<mml:mi>e</mml:mi>
<mml:msup>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>k</mml:mi>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:msup>
<mml:mo>.</mml:mo>
</mml:mrow>
</mml:math>
<label>(3)</label>
</disp-formula>
</p>
<p>The transition radiation of an electron beam can be expressed by the Nodvick&#x2013;Saxon formula [<xref ref-type="bibr" rid="B43">43</xref>].<disp-formula id="e4">
<mml:math id="m12">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:msup>
<mml:mi>d</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:mi>P</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi mathvariant="normal">&#x3a9;</mml:mi>
<mml:mi>d</mml:mi>
<mml:mi>k</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:msup>
<mml:mi>d</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:msub>
<mml:mi>P</mml:mi>
<mml:mi>e</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi mathvariant="normal">&#x3a9;</mml:mi>
<mml:mi>d</mml:mi>
<mml:mi>k</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mrow>
<mml:mfenced open="[" close="]" separators="|">
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>&#x2b;</mml:mo>
<mml:mi>N</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#xd7;</mml:mo>
<mml:mi>F</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>k</mml:mi>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(4)</label>
</disp-formula>where <italic>N</italic> is the number of the electrons. According to Eq. <xref ref-type="disp-formula" rid="e4">4</xref>, the total radiation intensity can be simplified as <inline-formula id="inf9">
<mml:math id="m13">
<mml:mrow>
<mml:mi>N</mml:mi>
<mml:mfrac>
<mml:mrow>
<mml:msup>
<mml:mi>d</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:msub>
<mml:mi>P</mml:mi>
<mml:mi>e</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi mathvariant="normal">&#x3a9;</mml:mi>
<mml:mi>d</mml:mi>
<mml:mi>k</mml:mi>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
</mml:math>
</inline-formula> for <inline-formula id="inf10">
<mml:math id="m14">
<mml:mrow>
<mml:mi>F</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>k</mml:mi>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>0</mml:mn>
</mml:mrow>
</mml:math>
</inline-formula>, which is called incoherent transition radiation. On the contrary, the total radiation intensity can be simplified as <inline-formula id="inf11">
<mml:math id="m15">
<mml:mrow>
<mml:msup>
<mml:mi>N</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:mfrac>
<mml:mrow>
<mml:msup>
<mml:mi>d</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:msub>
<mml:mi>P</mml:mi>
<mml:mi>e</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi mathvariant="normal">&#x3a9;</mml:mi>
<mml:mi>d</mml:mi>
<mml:mi>k</mml:mi>
</mml:mrow>
</mml:mfrac>
</mml:mrow>
</mml:math>
</inline-formula> for <inline-formula id="inf12">
<mml:math id="m16">
<mml:mrow>
<mml:mi>F</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>k</mml:mi>
<mml:mo>,</mml:mo>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula> 1, which is known as CTR. When substituting Eqs. <xref ref-type="disp-formula" rid="e2">2</xref>, <xref ref-type="disp-formula" rid="e3">3</xref> into Eq. <xref ref-type="disp-formula" rid="e4">4</xref> and only considering CTR, the CTR intensity of the compressed electron beam can be obtained using the following equation:<disp-formula id="e5">
<mml:math id="m17">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:msup>
<mml:mi>d</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:mi>P</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi mathvariant="normal">&#x3a9;</mml:mi>
<mml:mi>d</mml:mi>
<mml:mi>k</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:msup>
<mml:mi>N</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:msup>
<mml:mi>&#x3b2;</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:msub>
<mml:mi>r</mml:mi>
<mml:mi>e</mml:mi>
</mml:msub>
<mml:mi>m</mml:mi>
<mml:msup>
<mml:mi>c</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:mrow>
<mml:msup>
<mml:mi>&#x3c0;</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:mfrac>
<mml:mfrac>
<mml:mrow>
<mml:msup>
<mml:mi mathvariant="italic">sin</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
<mml:msup>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mn>1</mml:mn>
<mml:mo>&#x2212;</mml:mo>
<mml:msup>
<mml:mi>&#x3b2;</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:msup>
<mml:mi mathvariant="italic">cos</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:mfrac>
<mml:mo>&#xd7;</mml:mo>
<mml:msup>
<mml:mi>e</mml:mi>
<mml:msup>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>k</mml:mi>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:msup>
<mml:mo>.</mml:mo>
</mml:mrow>
</mml:math>
<label>(5)</label>
</disp-formula>
</p>
<p>Taking <inline-formula id="inf13">
<mml:math id="m18">
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi mathvariant="normal">&#x3a9;</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mn>2</mml:mn>
<mml:mi>&#x3c0;</mml:mi>
<mml:mi mathvariant="italic">sin</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
<mml:mi>d</mml:mi>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> and integrating wave number <italic>k</italic> of radiation, the angular distribution of the CTR can be expressed as follows:<disp-formula id="e6">
<mml:math id="m19">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi>P</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:msup>
<mml:mi>N</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:msup>
<mml:mi>&#x3b2;</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:msub>
<mml:mi>r</mml:mi>
<mml:mi>e</mml:mi>
</mml:msub>
<mml:mi>m</mml:mi>
<mml:msup>
<mml:mi>c</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:mrow>
<mml:mrow>
<mml:msqrt>
<mml:mi>&#x3c0;</mml:mi>
</mml:msqrt>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#xd7;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:msup>
<mml:mi mathvariant="italic">sin</mml:mi>
<mml:mn>3</mml:mn>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
<mml:msup>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mn>1</mml:mn>
<mml:mo>&#x2212;</mml:mo>
<mml:msup>
<mml:mi>&#x3b2;</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:msup>
<mml:mi mathvariant="italic">cos</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:mfrac>
<mml:mo>.</mml:mo>
</mml:mrow>
</mml:math>
<label>(6)</label>
</disp-formula>
</p>
<p>According to Eq. <xref ref-type="disp-formula" rid="e6">6</xref>, the CTR has a conical distribution with the maximum intensity at angle <inline-formula id="inf14">
<mml:math id="m20">
<mml:mrow>
<mml:mi>&#x3b8;</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:msup>
<mml:mi mathvariant="italic">sin</mml:mi>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msup>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:msqrt>
<mml:mn>3</mml:mn>
</mml:msqrt>
<mml:mo>/</mml:mo>
<mml:msqrt>
<mml:mrow>
<mml:msup>
<mml:mi>&#x3b3;</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msqrt>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
</mml:math>
</inline-formula>. When <inline-formula id="inf15">
<mml:math id="m21">
<mml:mrow>
<mml:mi>&#x3b3;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> is much greater than 1, the <inline-formula id="inf16">
<mml:math id="m22">
<mml:mrow>
<mml:mi>&#x3b8;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> is approximately equal to <inline-formula id="inf17">
<mml:math id="m23">
<mml:mrow>
<mml:msqrt>
<mml:mn>3</mml:mn>
</mml:msqrt>
<mml:mo>/</mml:mo>
<mml:mi>&#x3b3;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>. In addition, taking <inline-formula id="inf18">
<mml:math id="m24">
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi>k</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>2</mml:mn>
<mml:mi>&#x3c0;</mml:mi>
<mml:mo>/</mml:mo>
<mml:msup>
<mml:mi>&#x3bb;</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:mi>d</mml:mi>
<mml:mi>&#x3bb;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> and integrating solid angle <inline-formula id="inf19">
<mml:math id="m25">
<mml:mrow>
<mml:mi mathvariant="normal">&#x3a9;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>, the energy spectrum of the CTR can be expressed as follows:<disp-formula id="e7">
<mml:math id="m26">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi>P</mml:mi>
</mml:mrow>
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi>&#x3bb;</mml:mi>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mrow>
<mml:msup>
<mml:mi>N</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:msub>
<mml:mi>r</mml:mi>
<mml:mi>e</mml:mi>
</mml:msub>
<mml:mi>m</mml:mi>
<mml:msup>
<mml:mi>c</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
<mml:mrow>
<mml:mfenced open="[" close="]" separators="|">
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:mi mathvariant="italic">ln</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:mi>&#x3b3;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>1</mml:mn>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:msqrt>
<mml:mi>&#x3c0;</mml:mi>
</mml:msqrt>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:mfrac>
<mml:mo>&#xd7;</mml:mo>
<mml:mi mathvariant="italic">Erf</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:mi>&#x3c0;</mml:mi>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
<mml:mi>&#x3bb;</mml:mi>
</mml:mfrac>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(7)</label>
</disp-formula>where <inline-formula id="inf20">
<mml:math id="m27">
<mml:mrow>
<mml:mi mathvariant="italic">Erf</mml:mi>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mi>x</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:mo>/</mml:mo>
<mml:msqrt>
<mml:mi>&#x3c0;</mml:mi>
</mml:msqrt>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:msubsup>
<mml:mo>&#x222b;</mml:mo>
<mml:mn>0</mml:mn>
<mml:mi>x</mml:mi>
</mml:msubsup>
<mml:msup>
<mml:mi>e</mml:mi>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:msup>
<mml:mi>&#x3b7;</mml:mi>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:mrow>
</mml:msup>
<mml:mi>d</mml:mi>
<mml:mi>&#x3b7;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> is the error function. From Eq. <xref ref-type="disp-formula" rid="e7">7</xref>, the CTR is a broad-band THz radiation with a center frequency related to length <inline-formula id="inf21">
<mml:math id="m28">
<mml:mrow>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>.</p>
</sec>
<sec id="s2-2">
<title>2.2 Transition radiation of the electron bunch train</title>
<p>To obtain narrow-band THz radiation, the CTR generated by an electron bunch train is also introduced. In <xref ref-type="fig" rid="F1">Figure 1</xref>, an ultrafast laser is stretched by a parallel grating pair to introduce a linear chirp with chirp parameter <inline-formula id="inf22">
<mml:math id="m29">
<mml:mrow>
<mml:mrow>
<mml:mfenced open="|" close="|" separators="|">
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:msub>
<mml:mrow>
<mml:mn>1</mml:mn>
<mml:mo>/</mml:mo>
<mml:mi>&#x3c3;</mml:mi>
</mml:mrow>
<mml:mn>0</mml:mn>
</mml:msub>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mrow>
<mml:mi>o</mml:mi>
<mml:mi>u</mml:mi>
<mml:mi>t</mml:mi>
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</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>, where <inline-formula id="inf23">
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<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mn>0</mml:mn>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> is the initial laser pulse length (rms) and <inline-formula id="inf24">
<mml:math id="m31">
<mml:mrow>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
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<mml:mi>t</mml:mi>
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</mml:msub>
</mml:mrow>
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</inline-formula> is the stretched laser pulse length. Furthermore, the stretched laser pulse is divided into two laser pulses by a beam splitter to introduce tunable time delay <inline-formula id="inf25">
<mml:math id="m32">
<mml:mrow>
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</mml:mrow>
</mml:math>
</inline-formula> by a tunable optical delay line. Finally, the two laser pulses are recombined to obtain a frequency-beating laser pulse with a beating frequency [<xref ref-type="bibr" rid="B28">28</xref>, <xref ref-type="bibr" rid="B29">29</xref>]<disp-formula id="e8">
<mml:math id="m33">
<mml:mrow>
<mml:mi>f</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
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</mml:mrow>
<mml:mi>&#x3c0;</mml:mi>
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<mml:mo>.</mml:mo>
</mml:mrow>
</mml:math>
<label>(8)</label>
</disp-formula>
</p>
<p>According to Eq. <xref ref-type="disp-formula" rid="e8">8</xref>, the beating frequency can be continuously tuned by adjusting chirp parameter <inline-formula id="inf26">
<mml:math id="m34">
<mml:mrow>
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<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:math>
</inline-formula> and time delay <inline-formula id="inf27">
<mml:math id="m35">
<mml:mrow>
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</mml:mrow>
</mml:math>
</inline-formula>.</p>
<p>The electron beam at the exit of Linac 2 is sent into a modulation section together with the frequency-beating laser pulse to interact with each other. Due to the electron phase differences in the initial electron beam, some electrons obtain energy from the frequency-beating laser, while the other electrons transfer energy to the frequency-beating laser during the interaction. The energies of the electrons in the electron beam become different, resulting in periodic energy modulation over the wavelength of the frequency-beating laser [<xref ref-type="bibr" rid="B44">44</xref>, <xref ref-type="bibr" rid="B45">45</xref>]. Then the modulated beam is sent to the chicane to convert the energy modulation into density modulation and obtain a pulse train structure with a THz period, which can be described as <italic>M</italic> Gaussian microbunches with a time interval of <italic>T</italic>. At the same time, the frequency-beating laser pulse is reflected out by an optical mirror. Finally, the electron bunch train passes through the Al foil to generate narrow-band THz radiation. Here, the form factor of the electron bunch train can be expressed as follows [<xref ref-type="bibr" rid="B46">46</xref>, <xref ref-type="bibr" rid="B47">47</xref>]:<disp-formula id="e9">
<mml:math id="m36">
<mml:mrow>
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<mml:mi>F</mml:mi>
<mml:mi>t</mml:mi>
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</mml:mrow>
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<mml:mn>2</mml:mn>
</mml:msup>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(9)</label>
</disp-formula>where <inline-formula id="inf28">
<mml:math id="m37">
<mml:mrow>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> is the length of microbunch in the electron bunch train (rms). According to Eq. <xref ref-type="disp-formula" rid="e9">9</xref>, the form factor has peaks at the resonance wavelength and its harmonics, which can be tuned by manipulating the frequency-beating laser pulse. Substituting Eqs <xref ref-type="disp-formula" rid="e2">2</xref>, <xref ref-type="disp-formula" rid="e9">9</xref> into Eq. <xref ref-type="disp-formula" rid="e4">4</xref>, the CTR intensity of the electron bunch train can be expressed as follows:<disp-formula id="e10">
<mml:math id="m38">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:msup>
<mml:mi>d</mml:mi>
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<label>(10)</label>
</disp-formula>
</p>
<p>Taking <inline-formula id="inf29">
<mml:math id="m39">
<mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi>k</mml:mi>
<mml:mo>&#x3d;</mml:mo>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>2</mml:mn>
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<mml:mo>/</mml:mo>
<mml:msup>
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<mml:mi>d</mml:mi>
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</inline-formula> and integrating solid angle <inline-formula id="inf30">
<mml:math id="m40">
<mml:mrow>
<mml:mi mathvariant="normal">&#x3a9;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>, the energy spectrum of the CTR can be expressed as follows:<disp-formula id="e11">
<mml:math id="m41">
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:mi>d</mml:mi>
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<mml:mrow>
<mml:mfenced open="(" close=")" separators="|">
<mml:mrow>
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<mml:mrow>
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<mml:mi>c</mml:mi>
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<mml:mrow>
<mml:mn>4</mml:mn>
<mml:msup>
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<mml:mn>2</mml:mn>
</mml:msup>
<mml:msubsup>
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<mml:mi>s</mml:mi>
<mml:mn>2</mml:mn>
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</mml:mrow>
</mml:msup>
<mml:mo>.</mml:mo>
</mml:mrow>
</mml:math>
<label>(11)</label>
</disp-formula>
</p>
</sec>
</sec>
<sec sec-type="results" id="s3">
<title>3 Results</title>
<p>To illustrate the performance of the proposed method, simulations with the typical parameters of the SXFEL are performed; the detailed parameters are presented in <xref ref-type="table" rid="T1">Table 1</xref>. We use the ASTRA code [<xref ref-type="bibr" rid="B46">46</xref>] to simulate the beam dynamics in the photoinjector, and the ELEGANT code [<xref ref-type="bibr" rid="B48">48</xref>] to simulate the acceleration and compression processes in the LINAC. The beam dynamics in modulation and dispersion sections are simulated using the FALCON code [<xref ref-type="bibr" rid="B49">49</xref>].</p>
<table-wrap id="T1" position="float">
<label>TABLE 1</label>
<caption>
<p>Parameters of the electron beam and the laser system at the SXFEL.</p>
</caption>
<table>
<thead valign="top">
<tr>
<th align="left">Parameter</th>
<th align="left">Value</th>
<th align="left">Unit</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td colspan="3" align="left">Electron beam</td>
</tr>
<tr>
<td align="left">Energy</td>
<td align="left">1.4</td>
<td align="left">GeV</td>
</tr>
<tr>
<td align="left">Bunch charge</td>
<td align="left">500</td>
<td align="left">pC</td>
</tr>
<tr>
<td align="left">Bunch length (rms)</td>
<td align="left">0.1&#x2013;1.7</td>
<td align="left">ps</td>
</tr>
<tr>
<td align="left">Energy spread (slice)</td>
<td align="left">0.002%</td>
<td align="left">Arb. unit</td>
</tr>
<tr>
<td colspan="3" align="left">Laser</td>
</tr>
<tr>
<td align="left">Laser wavelength</td>
<td align="left">800</td>
<td align="left">nm</td>
</tr>
<tr>
<td align="left">Laser pulse length <inline-formula id="inf31">
<mml:math id="m42">
<mml:mrow>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mn>0</mml:mn>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>
</td>
<td align="left">30</td>
<td align="left">fs</td>
</tr>
<tr>
<td align="left">Laser peak power</td>
<td align="left">19</td>
<td align="left">MW</td>
</tr>
<tr>
<td align="left">Grating line</td>
<td align="left">1800</td>
<td align="left">
<inline-formula id="inf32">
<mml:math id="m43">
<mml:mrow>
<mml:msup>
<mml:mtext>mm</mml:mtext>
<mml:mrow>
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<mml:mn>1</mml:mn>
</mml:mrow>
</mml:msup>
</mml:mrow>
</mml:math>
</inline-formula>
</td>
</tr>
<tr>
<td align="left">Grating pair distance</td>
<td align="left">100</td>
<td align="left">mm</td>
</tr>
<tr>
<td align="left">Incident angle</td>
<td align="left">55</td>
<td align="left">
<inline-formula id="inf33">
<mml:math id="m44">
<mml:mrow>
<mml:mo>&#xb0;</mml:mo>
</mml:mrow>
</mml:math>
</inline-formula>
</td>
</tr>
</tbody>
</table>
</table-wrap>
<sec id="s3-1">
<title>3.1 Broad-band THz radiation generated by the compressed electron beam</title>
<p>In this simulation, an electron beam with a beam energy of 125&#xa0;MeV, a pulse length of 1.7 ps, and a charge of 500&#xa0;pC is produced at the entrance of the BC, and the bunch length can be easily adjusted with a minimum of 100 fs by tuning the current of the BC. The beam is then accelerated to 1.4&#xa0;GeV by Linac 2. Finally, the beam passes through the Al foil with a thickness of several <inline-formula id="inf34">
<mml:math id="m45">
<mml:mrow>
<mml:mi>&#x3bc;</mml:mi>
<mml:mi mathvariant="normal">m</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> to produce the CTR. Here, an ideal longitudinal structure of the electron beam described in Eq. <xref ref-type="disp-formula" rid="e1">1</xref> is adopted, and then the form factors with different pulse lengths are shown in <xref ref-type="fig" rid="F2">Figure 2</xref>.</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>Form factors of the compressed electron beams with different lengths.</p>
</caption>
<graphic xlink:href="fphy-11-1252725-g002.tif"/>
</fig>
<p>According to <xref ref-type="fig" rid="F2">Figure 2</xref>, the form factor will decrease more slowly and have a relative wider bandwidth with the decrease of the beam length, and the CTR generated by the compressed electron beam will have a broad-band spectrum. <xref ref-type="fig" rid="F3">Figure 3</xref> shows the angular distributions of the CTR with a beam length of 100 fs and different energies.</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>Angular distributions of the CTR with a beam length of 100 fs and different energies.</p>
</caption>
<graphic xlink:href="fphy-11-1252725-g003.tif"/>
</fig>
<p>According to <xref ref-type="fig" rid="F3">Figure 3</xref>, the angular distribution has a double-lobe distribution, which conforms to the conical distribution of the CTR. In addition, the intensity of the CTR will decrease and the divergence will increase with decrease in beam energy. For the electron beam with a beam energy of 1.4&#xa0;GeV, the CTR has the maximal intensity at the angle of <inline-formula id="inf35">
<mml:math id="m46">
<mml:mrow>
<mml:mn>6.28</mml:mn>
<mml:mo>&#xd7;</mml:mo>
<mml:msup>
<mml:mn>10</mml:mn>
<mml:mrow>
<mml:mo>&#x2212;</mml:mo>
<mml:mn>4</mml:mn>
</mml:mrow>
</mml:msup>
</mml:mrow>
</mml:math>
</inline-formula> rad and has a good orientation, which is easy to be collected using an off-axis parabolic mirror. <xref ref-type="fig" rid="F4">Figure 4</xref> shows the CTR spectra generated by the electron beams with a beam energy of 1.4&#xa0;GeV and different beam lengths.</p>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>CTR spectra generated by the compressed electron beams with a beam energy of 1.4&#xa0;GeV and different beam lengths.</p>
</caption>
<graphic xlink:href="fphy-11-1252725-g004.tif"/>
</fig>
<p>From <xref ref-type="fig" rid="F4">Figure 4</xref>, if <italic>f</italic> is less than <inline-formula id="inf36">
<mml:math id="m47">
<mml:mrow>
<mml:mi>c</mml:mi>
<mml:mo>/</mml:mo>
<mml:mn>2.35</mml:mn>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>, the CTR intensity increases rapidly and has a maximum at <inline-formula id="inf37">
<mml:math id="m48">
<mml:mrow>
<mml:mi>c</mml:mi>
<mml:mo>/</mml:mo>
<mml:mn>6</mml:mn>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>z</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula>; otherwise, the enhancement effect disappears. The CTR intensity will increase with the decrease in the beam length and the center frequency is also proportional to the beam length; thus, an electron beam with a relative shorter beam length is beneficial to generate CTR radiation with a higher frequency and wider spectral bandwidth. However, compressing the length of the electron beam to below 100 fs generally is a significant challenge. The SXFEL can compress the electron beam to a final bunch length of 100 fs, and the beam can be used to generate CTR radiation with a pulse energy of 342&#xa0;&#xb5;J and a frequency up to 5&#xa0;THz. Moreover, the bunch length of the electron beam at SXFEL can easily be adjusted between 100 fs and 1.7 ps so the broad-band THz radiation can be produced from 0.1 to 5&#xa0;THz.</p>
</sec>
<sec id="s3-2">
<title>3.2 Narrow-band THz radiation generated by the electron bunch train</title>
<p>To obtain THz radiation with a higher frequency and narrow spectral bandwidth, the CTR generated by a frequency-beating laser-modulated electron beam is also introduced. In this simulation, a laser pulse with the central wavelength of 800&#xa0;nm and the initial pulse duration of 30 fs is adopted. The laser pulse is first stretched to 42 ps by the paralleled grating pair, and then a time delay of 40 ps is introduced to obtain the frequency-beating signal at the frequency of 10&#xa0;THz (30 <inline-formula id="inf38">
<mml:math id="m49">
<mml:mrow>
<mml:mi>&#x3bc;</mml:mi>
<mml:mi mathvariant="normal">m</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>). The longitudinal amplitude distributions and spectrum of the frequency-beating laser pulse are shown in <xref ref-type="fig" rid="F5">Figures 5A, B</xref>, where one can observe that the fundamental wavelength is about 30 <inline-formula id="inf39">
<mml:math id="m50">
<mml:mrow>
<mml:mi>&#x3bc;</mml:mi>
<mml:mi mathvariant="normal">m</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>.</p>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>Longitudinal amplitude distributions of the seed laser at 10&#xa0;THz <bold>(A)</bold> and 15&#xa0;THz <bold>(C)</bold>. Spectra of the seed laser at 10&#xa0;THz <bold>(B)</bold> and 15&#xa0;THz <bold>(D)</bold>.</p>
</caption>
<graphic xlink:href="fphy-11-1252725-g005.tif"/>
</fig>
<p>The beating frequency can be tuned by adjusting chirp parameter <inline-formula id="inf40">
<mml:math id="m51">
<mml:mrow>
<mml:mfenced open="|" close="|" separators="|">
<mml:mrow>
<mml:mi>&#x3b1;</mml:mi>
</mml:mrow>
</mml:mfenced>
</mml:mrow>
</mml:math>
</inline-formula> and time delay <inline-formula id="inf41">
<mml:math id="m52">
<mml:mrow>
<mml:mi>&#x3c4;</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula>, which is limited by the initial laser power and pulse length. In theory, the beating frequency can be easily adjusted from 0.1 to 30&#xa0;THz [<xref ref-type="bibr" rid="B29">29</xref>], while the number of modulation periods can decrease with the decrease in the beating frequency for limited electron bunch length, which may broaden the spectral bandwidth. In addition, the fundamental Fourier component decreases from 0.23 to 0.15 when the beating frequency is adjusted from 10 to 15&#xa0;THz according to <xref ref-type="fig" rid="F5">Figures 5C,D</xref>. For a larger beating frequency, a larger time delay &#x3c4; will further decrease the fundamental Fourier component, which can decrease the final radiation power. To obtain a laser pulse with a larger beating frequency and sufficient fundamental Fourier component, higher initial laser power and shorter initial pulse length are required. Therefore, laser pulses with beating frequencies from 5 to 15&#xa0;THz and sufficient fundamental Fourier component can be easily obtained by the frequency-beating technique. As an example, the frequency-beating laser pulse with a frequency of 10&#xa0;THz is used as a seed in the following modulator.</p>
<p>Here, an electron beam with a full pulse length of 2 ps and a beam energy of 1.4&#xa0;GeV at the exit of Linac 2 is adopted to simulate the performance. The frequency-beating laser pulse and the electron beam are sent into the modulation section to interact with each other and obtain the energy modulation with 20 periods at a frequency of 10&#xa0;THz (100 fs). The electron beam passes through the modulator and the chicane with <inline-formula id="inf42">
<mml:math id="m53">
<mml:mrow>
<mml:msub>
<mml:mi>R</mml:mi>
<mml:mn>56</mml:mn>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> of 13.01&#xa0;cm to convert the energy modulation into density modulation. The longitudinal phase spaces after the chicane and corresponding current profile of the electron bunch train are shown in <xref ref-type="fig" rid="F6">Figure 6</xref>.</p>
<fig id="F6" position="float">
<label>FIGURE 6</label>
<caption>
<p>Longitudinal phase space and corresponding current profile of the electron bunch train (left) and local amplification in the phase space of the electron bunch train (right).</p>
</caption>
<graphic xlink:href="fphy-11-1252725-g006.tif"/>
</fig>
<p>From <xref ref-type="fig" rid="F6">Figure 6</xref>, one can find that the electron bunch train includes 20 microbunches, where the pulse length of each microbunch <inline-formula id="inf43">
<mml:math id="m54">
<mml:mrow>
<mml:msub>
<mml:mi>&#x3c3;</mml:mi>
<mml:mi>s</mml:mi>
</mml:msub>
</mml:mrow>
</mml:math>
</inline-formula> is 19.2 fs and time interval <italic>T</italic> is 100 fs. <xref ref-type="fig" rid="F7">Figure 7</xref> shows the form factors of the electron bunch trains with different numbers of microbunches and the CTR spectrum generated by the electron bunch train with 20 microbunches.</p>
<fig id="F7" position="float">
<label>FIGURE 7</label>
<caption>
<p>Form factors of the electron bunch with different numbers of microbunches <bold>(A)</bold> and the CTR spectrum generated by the electron bunch train with 20 microbunches <bold>(B)</bold>.</p>
</caption>
<graphic xlink:href="fphy-11-1252725-g007.tif"/>
</fig>
<p>From <xref ref-type="fig" rid="F7">Figure 7</xref>, one can observe that the form factors have an apparent peak at 10&#xa0;THz with a form factor of 0.23, and the CTR generated by the electron bunch train has a narrow spectral bandwidth. In addition, the spectral bandwidth decreases from 2.69 <inline-formula id="inf44">
<mml:math id="m55">
<mml:mrow>
<mml:mi>&#x3bc;</mml:mi>
<mml:mi mathvariant="normal">m</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> to 0.66 <inline-formula id="inf45">
<mml:math id="m56">
<mml:mrow>
<mml:mi>&#x3bc;</mml:mi>
<mml:mi mathvariant="normal">m</mml:mi>
</mml:mrow>
</mml:math>
</inline-formula> as the number of the microbunches increases; thus, a relative longer electron beam can also decrease the spectral bandwidth. The pulse energy of the CTR generated by the electron bunch train with 20 microbunches can reach 91&#xa0;&#x3bc;J at 10&#xa0;THz. It is worth mentioning that the longitudinal space charge force has limited influence on the frequency-beating laser-modulated electron beam so the method can be adopted for a higher beam charge to generate THz radiation with higher pulse energy. Furthermore, the radiation frequency can be easily tuned from 5 to 15&#xa0;THz by adjusting the beating frequency.</p>
<p>To compare the performance of the actual electron bunch train and the Gaussian microbunches, the form factors of the CTR generated by the actual electron bunch train and the 20 Gaussian microbunches are shown in <xref ref-type="fig" rid="F8">Figure 8</xref>.</p>
<fig id="F8" position="float">
<label>FIGURE 8</label>
<caption>
<p>Form factors of the CTR generated by the actual electron bunch train and the 20 Gaussian microbunches.</p>
</caption>
<graphic xlink:href="fphy-11-1252725-g008.tif"/>
</fig>
<p>
<xref ref-type="fig" rid="F8">Figure 8</xref> shows that the form factor of the actual electron bunch train at the fundamental radiation is 0.22, which is close to the form factor of the Gaussian microbunches (0.23). However, the form factors of these two cases are quite different at the second harmonic. The form factor of the Gaussian microbunches is only 0.003 at the second harmonic, while the form factor of the actual electron bunch train is 0.05. Moreover, the form factor of the actual electron bunch train shifts from 10 to 10.6&#xa0;THz compared with that of the Gaussian microbunches. These differences are caused by several reasons: the actual electron bunch train has a variable time interval, unlike the Gaussian microbunches, and the length of each microbunch of the actual electron bunch train is shorter than that of the Gaussian microbunches. Nevertheless, the CTR of the actual electron bunch train at the fundamental frequency can be estimated using the Gaussian microbunches.</p>
</sec>
</sec>
<sec sec-type="conclusion" id="s4">
<title>4 Conclusion</title>
<p>In this paper, we propose a THz light source that can produce both broad-band and narrow-band THz radiation by manipulating the longitudinal profile of an electron beam and exploiting the CTR. Based on the theoretical analysis and numerical simulations using the typical parameters of the SXFEL, we have shown that the CTR generated by the compressed electron beam can provide broad-band strong-field THz radiation with frequencies from 0.1 to 5&#xa0;THz and a pulse energy up to 342&#xa0;&#x3bc;J; the CTR generated by the electron bunch train obtained by modulating the electron beam with a frequency-beating laser pulse can provide narrow-band strong-field THz radiation from 5 to 15&#xa0;THz, with a pulse energy of 91&#xa0;&#x3bc;J at 10&#xa0;THz. Therefore, the proposed THz light source can generate THz radiation from 0.1 to 15&#xa0;THz by combining beam compression and the frequency-beating laser-modulated electron beam. It is worth noting that the electron bunch train can suppress the influence of space charge force and can possibly carry more charge, resulting in a narrower bandwidth, stronger energy, and higher frequency of the CTR. This kind of a THz light source based on the CTR can effectively enhance the THz radiation capabilities of the SXFEL facility, and offer more flexibility and versatility for advanced THz pump&#x2013;probe experiments.</p>
</sec>
</body>
<back>
<sec sec-type="data-availability" id="s5">
<title>Data availability statement</title>
<p>The raw data supporting the conclusion of this article will be made available by the authors, without undue reservation.</p>
</sec>
<sec id="s6">
<title>Author contributions</title>
<p>YK, RW, KZ, and CF contributed to the conception and design of the study. YK, WC, and LT performed the statistical analysis. YK and KZ wrote the first draft of the manuscript. YK, KZ, and CF contributed to the proofreading and revised the article format. KZ and CF are the supervisors. All authors contributed to the article and approved the submitted version.</p>
</sec>
<sec id="s7">
<title>Funding</title>
<p>This research was supported by the National Natural Science Foundation of China (grant numbers 12105347 and 12275340) and the Shanghai Science and Technology Commission project (grant number 20DZ2210300).</p>
</sec>
<ack>
<p>The authors would like to thank Hao Sun, Weijie Fan, Yaozong Xiao, Yiwen Liu, and Hanxiang Yang for their fruitful discussions on physics and simulations.</p>
</ack>
<sec sec-type="COI-statement" id="s8">
<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="s9">
<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>
<ref-list>
<title>References</title>
<ref id="B1">
<label>1.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Tonouchi</surname>
<given-names>M</given-names>
</name>
</person-group>. <article-title>Cutting-edge terahertz technology</article-title>. <source>Nat Photon</source> (<year>2007</year>) <volume>1</volume>(<issue>2</issue>):<fpage>97</fpage>&#x2013;<lpage>105</lpage>. <pub-id pub-id-type="doi">10.1038/nphoton.2007.3</pub-id>
</citation>
</ref>
<ref id="B2">
<label>2.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Mittleman</surname>
<given-names>DM</given-names>
</name>
</person-group>. <article-title>Perspective: Terahertz science and technology</article-title>. <source>J Appl Phys</source> (<year>2017</year>) <volume>122</volume>(<issue>23</issue>):<fpage>230901</fpage>. <pub-id pub-id-type="doi">10.1063/1.5007683</pub-id>
</citation>
</ref>
<ref id="B3">
<label>3.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Leitenstorfer</surname>
<given-names>A</given-names>
</name>
<name>
<surname>Moskalenko</surname>
<given-names>AS</given-names>
</name>
<name>
<surname>Kampfrath</surname>
<given-names>T</given-names>
</name>
<name>
<surname>Kono</surname>
<given-names>J</given-names>
</name>
<name>
<surname>Castro-Camus</surname>
<given-names>E</given-names>
</name>
<name>
<surname>Peng</surname>
<given-names>K</given-names>
</name>
<etal/>
</person-group> <article-title>The 2023 terahertz science and technology roadmap</article-title>. <source>J Phys D: Appl Phys</source> (<year>2023</year>) <volume>56</volume>(<issue>22</issue>):<fpage>223001</fpage>. <pub-id pub-id-type="doi">10.1088/1361-6463/acbe4c</pub-id>
</citation>
</ref>
<ref id="B4">
<label>4.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Zhang</surname>
<given-names>XC</given-names>
</name>
<name>
<surname>Shkurinov</surname>
<given-names>A</given-names>
</name>
<name>
<surname>Zhang</surname>
<given-names>Y</given-names>
</name>
</person-group>. <article-title>Extreme terahertz science</article-title>. <source>Nat Photon</source> (<year>2017</year>) <volume>11</volume>(<issue>1</issue>):<fpage>16</fpage>&#x2013;<lpage>8</lpage>. <pub-id pub-id-type="doi">10.1038/nphoton.2016.249</pub-id>
</citation>
</ref>
<ref id="B5">
<label>5.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Sal&#xe9;n</surname>
<given-names>P</given-names>
</name>
<name>
<surname>Basini</surname>
<given-names>M</given-names>
</name>
<name>
<surname>Bonetti</surname>
<given-names>S</given-names>
</name>
<name>
<surname>Hebling</surname>
<given-names>J</given-names>
</name>
<name>
<surname>Krasilnikov</surname>
<given-names>M</given-names>
</name>
<name>
<surname>Nikitin</surname>
<given-names>AY</given-names>
</name>
<etal/>
</person-group> <article-title>Matter manipulation with extreme terahertz light: Progress in the enabling THz technology</article-title>. <source>Phys Rep</source> (<year>2019</year>) <volume>836</volume>:<fpage>1</fpage>&#x2013;<lpage>74</lpage>. <pub-id pub-id-type="doi">10.1016/j.physrep.2019.09.002</pub-id>
</citation>
</ref>
<ref id="B6">
<label>6.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Kampfrath</surname>
<given-names>T</given-names>
</name>
<name>
<surname>Tanaka</surname>
<given-names>K</given-names>
</name>
<name>
<surname>Nelson</surname>
<given-names>KA</given-names>
</name>
</person-group>. <article-title>Resonant and nonresonant control over matter and light by intense terahertz transients</article-title>. <source>Nat Photon</source> (<year>2013</year>) <volume>7</volume>(<issue>9</issue>):<fpage>680</fpage>&#x2013;<lpage>90</lpage>. <pub-id pub-id-type="doi">10.1038/nphoton.2013.184</pub-id>
</citation>
</ref>
<ref id="B7">
<label>7.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Schmid</surname>
<given-names>G</given-names>
</name>
<name>
<surname>Schnorr</surname>
<given-names>K</given-names>
</name>
<name>
<surname>Augustin</surname>
<given-names>S</given-names>
</name>
<name>
<surname>Meister</surname>
<given-names>S</given-names>
</name>
<name>
<surname>Lindenblatt</surname>
<given-names>H</given-names>
</name>
<name>
<surname>Trost</surname>
<given-names>F</given-names>
</name>
<etal/>
</person-group> <article-title>Terahertz-field-induced time shifts in atomic photoemission</article-title>. <source>Phys Rev Lett</source> (<year>2019</year>) <volume>122</volume>(<issue>7</issue>):<fpage>073001</fpage>. <pub-id pub-id-type="doi">10.1103/physrevlett.122.073001</pub-id>
</citation>
</ref>
<ref id="B8">
<label>8.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Liu</surname>
<given-names>M</given-names>
</name>
<name>
<surname>Hwang</surname>
<given-names>HY</given-names>
</name>
<name>
<surname>Tao</surname>
<given-names>H</given-names>
</name>
<name>
<surname>Strikwerda</surname>
<given-names>AC</given-names>
</name>
<name>
<surname>Fan</surname>
<given-names>K</given-names>
</name>
<name>
<surname>Keiser</surname>
<given-names>GR</given-names>
</name>
<etal/>
</person-group> <article-title>Terahertz-field-induced insulator-to-metal transition in vanadium dioxide metamaterial</article-title>. <source>Nature</source> (<year>2012</year>) <volume>487</volume>(<issue>7407</issue>):<fpage>345</fpage>&#x2013;<lpage>8</lpage>. <pub-id pub-id-type="doi">10.1038/nature11231</pub-id>
</citation>
</ref>
<ref id="B9">
<label>9.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Schlauderer</surname>
<given-names>S</given-names>
</name>
<name>
<surname>Lange</surname>
<given-names>C</given-names>
</name>
<name>
<surname>Baierl</surname>
<given-names>S</given-names>
</name>
<name>
<surname>Ebnet</surname>
<given-names>T</given-names>
</name>
<name>
<surname>Schmid</surname>
<given-names>CP</given-names>
</name>
<name>
<surname>Valovcin</surname>
<given-names>DC</given-names>
</name>
<etal/>
</person-group> <article-title>Temporal and spectral fingerprints of ultrafast all-coherent spin switching</article-title>. <source>Nature</source> (<year>2019</year>) <volume>569</volume>(<issue>7756</issue>):<fpage>383</fpage>&#x2013;<lpage>7</lpage>. <pub-id pub-id-type="doi">10.1038/s41586-019-1174-7</pub-id>
</citation>
</ref>
<ref id="B10">
<label>10.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>D&#x2019;Angelo</surname>
<given-names>F</given-names>
</name>
<name>
<surname>Mics</surname>
<given-names>Z</given-names>
</name>
<name>
<surname>Bonn</surname>
<given-names>M</given-names>
</name>
<name>
<surname>Turchinovich</surname>
<given-names>D</given-names>
</name>
</person-group>. <article-title>Ultra-broadband THz time-domain spectroscopy of common polymers using THz air photonics</article-title>. <source>Opt express</source> (<year>2014</year>) <volume>22</volume>(<issue>10</issue>):<fpage>12475</fpage>&#x2013;<lpage>85</lpage>. <pub-id pub-id-type="doi">10.1364/oe.22.012475</pub-id>
</citation>
</ref>
<ref id="B11">
<label>11.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Zouaghi</surname>
<given-names>W</given-names>
</name>
<name>
<surname>Thomson</surname>
<given-names>MD</given-names>
</name>
<name>
<surname>Rabia</surname>
<given-names>K</given-names>
</name>
<name>
<surname>Hahn</surname>
<given-names>R</given-names>
</name>
<name>
<surname>Blank</surname>
<given-names>V</given-names>
</name>
<name>
<surname>Roskos</surname>
<given-names>HG</given-names>
</name>
</person-group>. <article-title>Broadband terahertz spectroscopy: Principles, fundamental research and potential for industrial applications</article-title>. <source>Eur J Phys</source> (<year>2013</year>) <volume>34</volume>(<issue>6</issue>):<fpage>S179</fpage>&#x2013;<lpage>99</lpage>. <pub-id pub-id-type="doi">10.1088/0143-0807/34/6/s179</pub-id>
</citation>
</ref>
<ref id="B12">
<label>12.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Roskos</surname>
<given-names>HG</given-names>
</name>
<name>
<surname>Thomson</surname>
<given-names>MD</given-names>
</name>
<name>
<surname>Kre&#xdf;</surname>
<given-names>M</given-names>
</name>
<name>
<surname>L&#xf6;ffler</surname>
<given-names>AT</given-names>
</name>
</person-group>. <article-title>Broadband THz emission from gas plasmas induced by femtosecond optical pulses: From fundamentals to applications</article-title>. <source>Laser Photon Rev</source> (<year>2007</year>) <volume>1</volume>(<issue>4</issue>):<fpage>349</fpage>&#x2013;<lpage>68</lpage>. <pub-id pub-id-type="doi">10.1002/lpor.200710025</pub-id>
</citation>
</ref>
<ref id="B13">
<label>13.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Shen</surname>
<given-names>Y</given-names>
</name>
<name>
<surname>Watanabe</surname>
<given-names>T</given-names>
</name>
<name>
<surname>Arena</surname>
<given-names>DA</given-names>
</name>
<name>
<surname>Kao</surname>
<given-names>CC</given-names>
</name>
<name>
<surname>Murphy</surname>
<given-names>JB</given-names>
</name>
<name>
<surname>Tsang</surname>
<given-names>TY</given-names>
</name>
<etal/>
</person-group> <article-title>Nonlinear cross-phase modulation with intense single-cycle terahertz pulses</article-title>. <source>Phys Rev Lett</source> (<year>2007</year>) <volume>99</volume>(<issue>4</issue>):<fpage>043901</fpage>. <pub-id pub-id-type="doi">10.1103/physrevlett.99.043901</pub-id>
</citation>
</ref>
<ref id="B14">
<label>14.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Vicario</surname>
<given-names>C</given-names>
</name>
<name>
<surname>Monoszlai</surname>
<given-names>B</given-names>
</name>
<name>
<surname>Hauri</surname>
<given-names>CP</given-names>
</name>
</person-group>. <article-title>GV/m single-cycle terahertz fields from a laser-driven large-size partitioned organic crystal</article-title>. <source>Phys Rev Lett</source> (<year>2014</year>) <volume>112</volume>(<issue>21</issue>):<fpage>213901</fpage>. <pub-id pub-id-type="doi">10.1103/physrevlett.112.213901</pub-id>
</citation>
</ref>
<ref id="B15">
<label>15.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Vicario</surname>
<given-names>C</given-names>
</name>
<name>
<surname>Ovchinnikov</surname>
<given-names>AV</given-names>
</name>
<name>
<surname>Ashitkov</surname>
<given-names>SI</given-names>
</name>
<name>
<surname>Agranat</surname>
<given-names>MB</given-names>
</name>
<name>
<surname>Fortov</surname>
<given-names>VE</given-names>
</name>
<name>
<surname>Hauri</surname>
<given-names>CP</given-names>
</name>
</person-group>. <article-title>Generation of 09-mJ THz pulses in DSTMS pumped by a Cr:Mg_2SiO_4 laser</article-title>. <source>Opt Lett</source> (<year>2014</year>) <volume>39</volume>(<issue>23</issue>):<fpage>6632</fpage>&#x2013;<lpage>5</lpage>. <pub-id pub-id-type="doi">10.1364/ol.39.006632</pub-id>
</citation>
</ref>
<ref id="B16">
<label>16.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Kim</surname>
<given-names>KY</given-names>
</name>
<name>
<surname>Taylor</surname>
<given-names>AJ</given-names>
</name>
<name>
<surname>Glownia</surname>
<given-names>JH</given-names>
</name>
<name>
<surname>Rodriguez</surname>
<given-names>G</given-names>
</name>
</person-group>. <article-title>Coherent control of terahertz supercontinuum generation in ultrafast laser&#x2013;gas interactions</article-title>. <source>Nat Photon</source> (<year>2008</year>) <volume>2</volume>(<issue>10</issue>):<fpage>605</fpage>&#x2013;<lpage>9</lpage>. <pub-id pub-id-type="doi">10.1038/nphoton.2008.153</pub-id>
</citation>
</ref>
<ref id="B17">
<label>17.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Clerici</surname>
<given-names>M</given-names>
</name>
<name>
<surname>Peccianti</surname>
<given-names>M</given-names>
</name>
<name>
<surname>Schmidt</surname>
<given-names>BE</given-names>
</name>
<name>
<surname>Caspani</surname>
<given-names>L</given-names>
</name>
<name>
<surname>Shalaby</surname>
<given-names>M</given-names>
</name>
<name>
<surname>Giguere</surname>
<given-names>M</given-names>
</name>
<etal/>
</person-group> <article-title>Wavelength scaling of terahertz generation by gas ionization</article-title>. <source>Phys Rev Lett</source> (<year>2013</year>) <volume>110</volume>(<issue>25</issue>):<fpage>253901</fpage>. <pub-id pub-id-type="doi">10.1103/physrevlett.110.253901</pub-id>
</citation>
</ref>
<ref id="B18">
<label>18.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Malik</surname>
<given-names>HK</given-names>
</name>
<name>
<surname>Malik</surname>
<given-names>AK</given-names>
</name>
</person-group>. <article-title>Tunable and collimated terahertz radiation generation by femtosecond laser pulses</article-title>. <source>Appl Phys Lett</source> (<year>2011</year>) <volume>99</volume>(<issue>25</issue>). <pub-id pub-id-type="doi">10.1063/1.3666855</pub-id>
</citation>
</ref>
<ref id="B19">
<label>19.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Manendra</surname>
<given-names>M</given-names>
</name>
<name>
<surname>Singh</surname>
<given-names>KP</given-names>
</name>
<name>
<surname>Singh</surname>
<given-names>BP</given-names>
</name>
<name>
<surname>Malik</surname>
<given-names>AK</given-names>
</name>
</person-group>. <article-title>Bright terahertz (THz) generation by frequency mixing of dichromatic lasers in inhomogeneous cold plasma: Scaling of THz field</article-title>. <source>Phys Plasmas</source> (<year>2020</year>) <volume>27</volume>(<issue>6</issue>). <pub-id pub-id-type="doi">10.1063/5.0005643</pub-id>
</citation>
</ref>
<ref id="B20">
<label>20.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Manendra</surname>
<given-names>M</given-names>
</name>
<name>
<surname>Singh</surname>
<given-names>KP</given-names>
</name>
<name>
<surname>Bhati</surname>
<given-names>R</given-names>
</name>
<name>
<surname>Malik</surname>
<given-names>AK</given-names>
</name>
</person-group>. <article-title>Efficient terahertz (THz) generation by nonlinear mixing of bicolor top-hat lasers in hot plasma</article-title>. <source>Phys Plasmas</source> (<year>2020</year>) <volume>27</volume>(<issue>2</issue>). <pub-id pub-id-type="doi">10.1063/1.5121913</pub-id>
</citation>
</ref>
<ref id="B21">
<label>21.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Singh</surname>
<given-names>KP</given-names>
</name>
<name>
<surname>Jewariya</surname>
<given-names>M</given-names>
</name>
<name>
<surname>Chaudhary</surname>
<given-names>P</given-names>
</name>
<name>
<surname>Malik</surname>
<given-names>AK</given-names>
</name>
</person-group>. <article-title>Flexible control over polarization tuning using electric wiggler during terahertz generation</article-title>. <source>Opt Lasers Eng</source> (<year>2023</year>) <volume>167</volume>:<fpage>107589</fpage>. <pub-id pub-id-type="doi">10.1016/j.optlaseng.2023.107589</pub-id>
</citation>
</ref>
<ref id="B22">
<label>22.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Gopal</surname>
<given-names>A</given-names>
</name>
<name>
<surname>Herzer</surname>
<given-names>S</given-names>
</name>
<name>
<surname>Schmidt</surname>
<given-names>A</given-names>
</name>
<name>
<surname>Singh</surname>
<given-names>P</given-names>
</name>
<name>
<surname>Reinhard</surname>
<given-names>A</given-names>
</name>
<name>
<surname>Ziegler</surname>
<given-names>W</given-names>
</name>
<etal/>
</person-group> <article-title>Observation of gigawatt-class THz pulses from a compact laser-driven particle accelerator</article-title>. <source>Phys Rev Lett</source> (<year>2013</year>) <volume>111</volume>(<issue>7</issue>):<fpage>074802</fpage>. <pub-id pub-id-type="doi">10.1103/physrevlett.111.074802</pub-id>
</citation>
</ref>
<ref id="B23">
<label>23.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Stojanovic</surname>
<given-names>N</given-names>
</name>
<name>
<surname>Drescher</surname>
<given-names>M</given-names>
</name>
</person-group>. <article-title>Accelerator-and laser-based sources of high-field terahertz pulses</article-title>. <source>J Phys B: At Mol Opt Phys</source> (<year>2013</year>) <volume>46</volume>(<issue>19</issue>):<fpage>192001</fpage>. <pub-id pub-id-type="doi">10.1088/0953-4075/46/19/192001</pub-id>
</citation>
</ref>
<ref id="B24">
<label>24.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Zhang</surname>
<given-names>Z</given-names>
</name>
<name>
<surname>Fisher</surname>
<given-names>AS</given-names>
</name>
<name>
<surname>Hoffmann</surname>
<given-names>MC</given-names>
</name>
<name>
<surname>Jacobson</surname>
<given-names>B</given-names>
</name>
<name>
<surname>Kirchmann</surname>
<given-names>PS</given-names>
</name>
<name>
<surname>Lee</surname>
<given-names>WS</given-names>
</name>
<etal/>
</person-group> <article-title>A high-power, high-repetition-rate THz source for pump&#x2013;probe experiments at Linac Coherent Light Source II</article-title>. <source>J Synchrotron Radiat</source> (<year>2020</year>) <volume>27</volume>(<issue>4</issue>):<fpage>890</fpage>&#x2013;<lpage>901</lpage>. <pub-id pub-id-type="doi">10.1107/s1600577520005147</pub-id>
</citation>
</ref>
<ref id="B25">
<label>25.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Zapolnova</surname>
<given-names>E</given-names>
</name>
<name>
<surname>Golz</surname>
<given-names>T</given-names>
</name>
<name>
<surname>Pan</surname>
<given-names>R</given-names>
</name>
<name>
<surname>Klose</surname>
<given-names>K</given-names>
</name>
<name>
<surname>Schreiber</surname>
<given-names>S</given-names>
</name>
<name>
<surname>Stojanovic</surname>
<given-names>N</given-names>
</name>
</person-group>. <article-title>THz pulse doubler at FLASH: Double pulses for pump&#x2013;probe experiments at X-ray FELs</article-title>. <source>J synchrotron Radiat</source> (<year>2018</year>) <volume>25</volume>(<issue>1</issue>):<fpage>39</fpage>&#x2013;<lpage>43</lpage>. <pub-id pub-id-type="doi">10.1107/s1600577517015442</pub-id>
</citation>
</ref>
<ref id="B26">
<label>26.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Pan</surname>
<given-names>R</given-names>
</name>
<name>
<surname>Zapolnova</surname>
<given-names>E</given-names>
</name>
<name>
<surname>Golz</surname>
<given-names>T</given-names>
</name>
<name>
<surname>Krmpot</surname>
<given-names>AJ</given-names>
</name>
<name>
<surname>Rabasovic</surname>
<given-names>MD</given-names>
</name>
<name>
<surname>Petrovic</surname>
<given-names>J</given-names>
</name>
<etal/>
</person-group> <article-title>Photon diagnostics at the FLASH THz beamline</article-title>. <source>J synchrotron Radiat</source> (<year>2019</year>) <volume>26</volume>(<issue>3</issue>):<fpage>700</fpage>&#x2013;<lpage>7</lpage>. <pub-id pub-id-type="doi">10.1107/s1600577519003412</pub-id>
</citation>
</ref>
<ref id="B27">
<label>27.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Patterson</surname>
<given-names>BD</given-names>
</name>
<name>
<surname>Abela</surname>
<given-names>R</given-names>
</name>
<name>
<surname>Braun</surname>
<given-names>HH</given-names>
</name>
<name>
<surname>Flechsig</surname>
<given-names>U</given-names>
</name>
<name>
<surname>Ganter</surname>
<given-names>R</given-names>
</name>
<name>
<surname>Kim</surname>
<given-names>Y</given-names>
</name>
<etal/>
</person-group> <article-title>Coherent science at the SwissFEL x-ray laser</article-title>. <source>New J Phys</source> (<year>2010</year>) <volume>12</volume>(<issue>3</issue>):<fpage>035012</fpage>. <pub-id pub-id-type="doi">10.1088/1367-2630/12/3/035012</pub-id>
</citation>
</ref>
<ref id="B28">
<label>28.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Zhang</surname>
<given-names>K</given-names>
</name>
<name>
<surname>Kang</surname>
<given-names>Y</given-names>
</name>
<name>
<surname>Liu</surname>
<given-names>T</given-names>
</name>
<name>
<surname>Wang</surname>
<given-names>Z</given-names>
</name>
<name>
<surname>Feng</surname>
<given-names>C</given-names>
</name>
<name>
<surname>Fang</surname>
<given-names>W</given-names>
</name>
<etal/>
</person-group> <article-title>A compact accelerator-based light source for high-power, full-bandwidth tunable coherent THz generation</article-title>. <source>Appl Sci</source> (<year>2021</year>) <volume>11</volume>(<issue>24</issue>):<fpage>11850</fpage>. <pub-id pub-id-type="doi">10.3390/app112411850</pub-id>
</citation>
</ref>
<ref id="B29">
<label>29.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Kang</surname>
<given-names>Y</given-names>
</name>
<name>
<surname>Wang</surname>
<given-names>Z</given-names>
</name>
<name>
<surname>Zhang</surname>
<given-names>K</given-names>
</name>
<name>
<surname>Feng</surname>
<given-names>C</given-names>
</name>
</person-group>. <article-title>Generating high-power, frequency tunable coherent THz pulse in an X-ray free-electron laser for THz pump and X-ray probe experiments</article-title>. <source>Photon</source> (<year>2023</year>) <volume>10</volume>(<issue>2</issue>):<fpage>133</fpage>. <pub-id pub-id-type="doi">10.3390/photonics10020133</pub-id>
</citation>
</ref>
<ref id="B30">
<label>30.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Shen</surname>
<given-names>Y</given-names>
</name>
<name>
<surname>Yang</surname>
<given-names>X</given-names>
</name>
<name>
<surname>Carr</surname>
<given-names>GL</given-names>
</name>
<name>
<surname>Hidaka</surname>
<given-names>Y</given-names>
</name>
<name>
<surname>Murphy</surname>
<given-names>JB</given-names>
</name>
<name>
<surname>Wang</surname>
<given-names>X</given-names>
</name>
</person-group>. <article-title>Tunable few-cycle and multicycle coherent terahertz radiation from relativistic electrons</article-title>. <source>Phys Rev Lett</source> (<year>2011</year>) <volume>107</volume>(<issue>20</issue>):<fpage>204801</fpage>. <pub-id pub-id-type="doi">10.1103/physrevlett.107.204801</pub-id>
</citation>
</ref>
<ref id="B31">
<label>31.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Sun</surname>
<given-names>YE</given-names>
</name>
<name>
<surname>Piot</surname>
<given-names>P</given-names>
</name>
<name>
<surname>Johnson</surname>
<given-names>A</given-names>
</name>
<name>
<surname>Lumpkin</surname>
<given-names>AH</given-names>
</name>
<name>
<surname>Maxwell</surname>
<given-names>TJ</given-names>
</name>
<name>
<surname>Ruan</surname>
<given-names>J</given-names>
</name>
<etal/>
</person-group> <article-title>Tunable subpicosecond electron-bunch-train generation using a transverse-to-longitudinal phase-space exchange technique</article-title>. <source>Phys Rev Lett</source> (<year>2010</year>) <volume>105</volume>(<issue>23</issue>):<fpage>234801</fpage>. <pub-id pub-id-type="doi">10.1103/physrevlett.105.234801</pub-id>
</citation>
</ref>
<ref id="B32">
<label>32.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Antipov</surname>
<given-names>S</given-names>
</name>
<name>
<surname>Babzien</surname>
<given-names>M</given-names>
</name>
<name>
<surname>Jing</surname>
<given-names>C</given-names>
</name>
<name>
<surname>Fedurin</surname>
<given-names>M</given-names>
</name>
<name>
<surname>Gai</surname>
<given-names>W</given-names>
</name>
<name>
<surname>Kanareykin</surname>
<given-names>A</given-names>
</name>
<etal/>
</person-group> <article-title>Subpicosecond bunch train production for a tunable mJ level THz source</article-title>. <source>Phys Rev Lett</source> (<year>2013</year>) <volume>111</volume>(<issue>13</issue>):<fpage>134802</fpage>. <pub-id pub-id-type="doi">10.1103/physrevlett.111.134802</pub-id>
</citation>
</ref>
<ref id="B33">
<label>33.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Lemery</surname>
<given-names>F</given-names>
</name>
<name>
<surname>Piot</surname>
<given-names>P</given-names>
</name>
<name>
<surname>Amatuni</surname>
<given-names>G</given-names>
</name>
<name>
<surname>Boonpornprasert</surname>
<given-names>P</given-names>
</name>
<name>
<surname>Chen</surname>
<given-names>Y</given-names>
</name>
<name>
<surname>Good</surname>
<given-names>J</given-names>
</name>
<etal/>
</person-group> <article-title>Passive ballistic microbunching of nonultrarelativistic electron bunches using electromagnetic wakefields in dielectric-lined waveguides</article-title>. <source>Phys Rev Lett</source> (<year>2019</year>) <volume>122</volume>(<issue>4</issue>):<fpage>044801</fpage>. <pub-id pub-id-type="doi">10.1103/physrevlett.122.044801</pub-id>
</citation>
</ref>
<ref id="B34">
<label>34.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Zhang</surname>
<given-names>Z</given-names>
</name>
<name>
<surname>Yan</surname>
<given-names>L</given-names>
</name>
<name>
<surname>Du</surname>
<given-names>Y</given-names>
</name>
<name>
<surname>Zhou</surname>
<given-names>Z</given-names>
</name>
<name>
<surname>Su</surname>
<given-names>X</given-names>
</name>
<name>
<surname>Zheng</surname>
<given-names>L</given-names>
</name>
<etal/>
</person-group> <article-title>Tunable high-intensity electron bunch train production based on nonlinear longitudinal space charge oscillation</article-title>. <source>Phys Rev Lett</source> (<year>2016</year>) <volume>116</volume>(<issue>18</issue>):<fpage>184801</fpage>. <pub-id pub-id-type="doi">10.1103/physrevlett.116.184801</pub-id>
</citation>
</ref>
<ref id="B35">
<label>35.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Liang</surname>
<given-names>Y</given-names>
</name>
<name>
<surname>Liu</surname>
<given-names>Z</given-names>
</name>
<name>
<surname>Tian</surname>
<given-names>Q</given-names>
</name>
<name>
<surname>Li</surname>
<given-names>T</given-names>
</name>
<name>
<surname>Lin</surname>
<given-names>X</given-names>
</name>
<name>
<surname>Yan</surname>
<given-names>L</given-names>
</name>
<etal/>
</person-group> <article-title>Widely tunable electron bunch trains for the generation of high-power narrowband 1&#x2013;10 THz radiation</article-title>. <source>Nat Photon</source> (<year>2023</year>) <volume>17</volume>:<fpage>259</fpage>&#x2013;<lpage>63</lpage>. <pub-id pub-id-type="doi">10.1038/s41566-022-01131-7</pub-id>
</citation>
</ref>
<ref id="B36">
<label>36.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Ginzburg</surname>
<given-names>VL</given-names>
</name>
<name>
<surname>Frank</surname>
<given-names>IM</given-names>
</name>
</person-group>. <article-title>Radiation of a uniformly moving electron due to its transition from one medium into another</article-title>. <source>J Phys (Ussr)</source> (<year>1945</year>) <volume>9</volume>:<fpage>353</fpage>&#x2013;<lpage>62</lpage>.</citation>
</ref>
<ref id="B37">
<label>37.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Garibian</surname>
<given-names>GM</given-names>
</name>
</person-group>. <article-title>Contribution to the theory of transition radiation</article-title>. <source>Sov Phys JETP</source> (<year>1958</year>) <volume>6</volume>(<issue>6</issue>):<fpage>1079</fpage>.</citation>
</ref>
<ref id="B38">
<label>38.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Carr</surname>
<given-names>GL</given-names>
</name>
<name>
<surname>Martin</surname>
<given-names>MC</given-names>
</name>
<name>
<surname>McKinney</surname>
<given-names>WR</given-names>
</name>
<name>
<surname>Jordan</surname>
<given-names>K</given-names>
</name>
<name>
<surname>Neil</surname>
<given-names>GR</given-names>
</name>
<name>
<surname>Williams</surname>
<given-names>GP</given-names>
</name>
</person-group>. <article-title>High-power terahertz radiation from relativistic electrons</article-title>. <source>Nature</source> (<year>2002</year>) <volume>420</volume>(<issue>6912</issue>):<fpage>153</fpage>&#x2013;<lpage>6</lpage>. <pub-id pub-id-type="doi">10.1038/nature01175</pub-id>
</citation>
</ref>
<ref id="B39">
<label>39.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Shibata</surname>
<given-names>Y</given-names>
</name>
<name>
<surname>Ishi</surname>
<given-names>K</given-names>
</name>
<name>
<surname>Takahashi</surname>
<given-names>T</given-names>
</name>
<name>
<surname>Kanai</surname>
<given-names>T</given-names>
</name>
<name>
<surname>Ikezawa</surname>
<given-names>M</given-names>
</name>
<name>
<surname>Takami</surname>
<given-names>K</given-names>
</name>
<etal/>
</person-group> <article-title>Observation of coherent transition radiation at millimeter and submillimeter wavelengths</article-title>. <source>Phys Rev A</source> (<year>1992</year>) <volume>45</volume>(<issue>12</issue>):<fpage>R8340</fpage>&#x2013;<lpage>3</lpage>. <pub-id pub-id-type="doi">10.1103/physreva.45.r8340</pub-id>
</citation>
</ref>
<ref id="B40">
<label>40.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Wen-Xin</surname>
<given-names>L</given-names>
</name>
<name>
<surname>Wen-Hui</surname>
<given-names>H</given-names>
</name>
<name>
<surname>Ying-Chao</surname>
<given-names>D</given-names>
</name>
<name>
<surname>Li-Xin</surname>
<given-names>Y</given-names>
</name>
<name>
<surname>Dai</surname>
<given-names>W</given-names>
</name>
<name>
<surname>Chuan-Xiang</surname>
<given-names>T</given-names>
</name>
</person-group>. <article-title>Terahertz coherent transition radiation based on an ultrashort electron bunching beam</article-title>. <source>Chin Phys B</source> (<year>2011</year>) <volume>20</volume>(<issue>7</issue>):<fpage>074102</fpage>. <pub-id pub-id-type="doi">10.1088/1674-1056/20/7/074102</pub-id>
</citation>
</ref>
<ref id="B41">
<label>41.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Bass</surname>
<given-names>FG</given-names>
</name>
<name>
<surname>Yakovenko</surname>
<given-names>VM</given-names>
</name>
</person-group>. <article-title>Theory of radiation from a charge passing through an electrically inhomogeneous medium</article-title>. <source>Soviet Phys Uspekhi</source> (<year>1965</year>) <volume>8</volume>(<issue>3</issue>):<fpage>420</fpage>&#x2013;<lpage>44</lpage>. <pub-id pub-id-type="doi">10.1070/pu1965v008n03abeh003054</pub-id>
</citation>
</ref>
<ref id="B42">
<label>42.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Casalbuoni</surname>
<given-names>S</given-names>
</name>
<name>
<surname>Schmidt</surname>
<given-names>B</given-names>
</name>
<name>
<surname>Schm&#xfc;ser</surname>
<given-names>P</given-names>
</name>
<name>
<surname>Arsov</surname>
<given-names>V</given-names>
</name>
<name>
<surname>Wesch</surname>
<given-names>S</given-names>
</name>
</person-group>. <article-title>Ultrabroadband terahertz source and beamline based on coherent transition radiation</article-title>. <source>Phys Rev Spec Topics-Accelerators Beams</source> (<year>2009</year>) <volume>12</volume>(<issue>3</issue>):<fpage>030705</fpage>. <pub-id pub-id-type="doi">10.1103/physrevstab.12.030705</pub-id>
</citation>
</ref>
<ref id="B43">
<label>43.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Nodvick</surname>
<given-names>JS</given-names>
</name>
<name>
<surname>Saxon</surname>
<given-names>DS</given-names>
</name>
</person-group>. <article-title>Suppression of coherent radiation by electrons in a synchrotron</article-title>. <source>Phys Rev</source> (<year>1954</year>) <volume>96</volume>(<issue>1</issue>):<fpage>180</fpage>&#x2013;<lpage>4</lpage>. <pub-id pub-id-type="doi">10.1103/physrev.96.180</pub-id>
</citation>
</ref>
<ref id="B44">
<label>44.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Yu</surname>
<given-names>LH</given-names>
</name>
</person-group>. <article-title>Generation of intense uv radiation by subharmonically seeded single-pass free-electron lasers</article-title>. <source>Phys Rev A</source> (<year>1991</year>) <volume>44</volume>(<issue>8</issue>):<fpage>5178</fpage>&#x2013;<lpage>93</lpage>. <pub-id pub-id-type="doi">10.1103/physreva.44.5178</pub-id>
</citation>
</ref>
<ref id="B45">
<label>45.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Yu</surname>
<given-names>LH</given-names>
</name>
<name>
<surname>Babzien</surname>
<given-names>M</given-names>
</name>
<name>
<surname>Ben-Zvi</surname>
<given-names>I</given-names>
</name>
<name>
<surname>DiMauro</surname>
<given-names>LF</given-names>
</name>
<name>
<surname>Doyuran</surname>
<given-names>A</given-names>
</name>
<name>
<surname>Graves</surname>
<given-names>W</given-names>
</name>
<etal/>
</person-group> <article-title>High-gain harmonic-generation free-electron laser</article-title>. <source>Science</source> (<year>2000</year>) <volume>289</volume>(<issue>5481</issue>):<fpage>932</fpage>&#x2013;<lpage>4</lpage>. <pub-id pub-id-type="doi">10.1126/science.289.5481.932</pub-id>
</citation>
</ref>
<ref id="B46">
<label>46.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Gover</surname>
<given-names>A</given-names>
</name>
</person-group>. <article-title>Superradiant and stimulated-superradiant emission in prebunched electron-beam radiators. I. Formulation</article-title>. <source>Phys Rev Spec Topics-Accelerators Beams</source> (<year>2005</year>) <volume>8</volume>(<issue>3</issue>):<fpage>030701</fpage>. <pub-id pub-id-type="doi">10.1103/physrevstab.8.030701</pub-id>
</citation>
</ref>
<ref id="B47">
<label>47.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Gover</surname>
<given-names>A</given-names>
</name>
<name>
<surname>Dyunin</surname>
<given-names>E</given-names>
</name>
<name>
<surname>Lurie</surname>
<given-names>Y</given-names>
</name>
<name>
<surname>Pinhasi</surname>
<given-names>Y</given-names>
</name>
<name>
<surname>Krongauz</surname>
<given-names>MV</given-names>
</name>
</person-group>. <article-title>Superradiant and stimulated-superradiant emission in prebunched electron-beam radiators. II. Radiation enhancement schemes</article-title>. <source>Phys Rev Spec Topics-Accelerators Beams</source> (<year>2005</year>) <volume>8</volume>(<issue>3</issue>):<fpage>030702</fpage>. <pub-id pub-id-type="doi">10.1103/physrevstab.8.030702</pub-id>
</citation>
</ref>
<ref id="B48">
<label>48.</label>
<citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname>Borland</surname>
<given-names>M</given-names>
</name>
</person-group>. <source>A flexible sdds-compliant code for accelerator simulation</source>. <publisher-loc>Argonne, IL</publisher-loc>: <publisher-name>ANL</publisher-name> (<year>2000</year>).<fpage>60439</fpage>
</citation>
</ref>
<ref id="B49">
<label>49.</label>
<citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname>Zeng</surname>
<given-names>L</given-names>
</name>
<name>
<surname>Feng</surname>
<given-names>C</given-names>
</name>
<name>
<surname>Wang</surname>
<given-names>X</given-names>
</name>
<name>
<surname>Zhang</surname>
<given-names>K</given-names>
</name>
<name>
<surname>Qi</surname>
<given-names>Z</given-names>
</name>
<name>
<surname>Zhao</surname>
<given-names>Z</given-names>
</name>
</person-group>. <article-title>A super-fast free-electron laser simulation code for online optimization</article-title>. <source>Photon</source> (<year>2020</year>) <volume>7</volume>(<issue>4</issue>):<fpage>117</fpage>. <pub-id pub-id-type="doi">10.3390/photonics7040117</pub-id>
</citation>
</ref>
<ref id="B50">
<label>50.</label>
<citation citation-type="book">
<collab>ASTRA</collab>. <source>desy</source> (<year>2023</year>). <comment>Available at: <ext-link ext-link-type="uri" xlink:href="https://www.desy.de/%7Empyflo/">https://www.desy.de/&#x223c;mpyflo/</ext-link> (Accessed June 28, 2023)</comment>.</citation>
</ref>
</ref-list>
</back>
</article>