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<titleInfo><title>Bottom-up analysis of rovibrational helical dichroism</title></titleInfo>


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<name type="personal">
  <namePart type="given">Mateja</namePart>
  <namePart type="family">Hrast</namePart>
  <role><roleTerm type="text">author</roleTerm> </role><identifier type="local">48dbb294-2a9c-11ef-905d-f56be71f0e5d</identifier></name>
<name type="personal">
  <namePart type="given">Georgios</namePart>
  <namePart type="family">Koutentakis</namePart>
  <role><roleTerm type="text">author</roleTerm> </role><identifier type="local">d7b23d3a-9e21-11ec-b482-f76739596b95</identifier></name>
<name type="personal">
  <namePart type="given">Mikhail</namePart>
  <namePart type="family">Maslov</namePart>
  <role><roleTerm type="text">author</roleTerm> </role><identifier type="local">2E65BB0E-F248-11E8-B48F-1D18A9856A87</identifier><description xsi:type="identifierDefinition" type="orcid">0000-0003-4074-2570</description></name>
<name type="personal">
  <namePart type="given">Mikhail</namePart>
  <namePart type="family">Lemeshko</namePart>
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  <namePart>Coherent Optical Metrology Beyond Electric-Dipole-Allowed Transitions</namePart>
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<abstract lang="eng">We present a general theoretical framework for helical dichroism (HD), establishing an explicit link between chiral resolution and orbital angular momentum (OAM) exchange in light–matter interaction. Tracing microscopic mechanisms of the OAM transfer, we derive rotational selection rules, which establish that HD emerges only from the spin–orbit coupling of light, even for beams without the far-field OAM. Our findings refine the conditions for observing HD, provide a tool to re-examine the outcome of prior experiments, and guide future designs for chiral sensing with structured light.</abstract>

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<originInfo><publisher>American Physical Society</publisher><dateIssued encoding="w3cdtf">2026</dateIssued>
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<language><languageTerm authority="iso639-2b" type="code">eng</languageTerm>
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<relatedItem type="host"><titleInfo><title>Physical Review Letters</title></titleInfo>
  <identifier type="issn">0031-9007</identifier>
  <identifier type="eIssn">1079-7114</identifier>
  <identifier type="arXiv">2505.16393</identifier><identifier type="doi">10.1103/fkf1-1jml</identifier>
<part><detail type="volume"><number>136</number></detail><detail type="issue"><number>5</number></detail>
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<ama>Hrast M, Koutentakis G, Maslov M, Lemeshko M. Bottom-up analysis of rovibrational helical dichroism. &lt;i&gt;Physical Review Letters&lt;/i&gt;. 2026;136(5). doi:&lt;a href=&quot;https://doi.org/10.1103/fkf1-1jml&quot;&gt;10.1103/fkf1-1jml&lt;/a&gt;</ama>
<apa>Hrast, M., Koutentakis, G., Maslov, M., &amp;#38; Lemeshko, M. (2026). Bottom-up analysis of rovibrational helical dichroism. &lt;i&gt;Physical Review Letters&lt;/i&gt;. American Physical Society. &lt;a href=&quot;https://doi.org/10.1103/fkf1-1jml&quot;&gt;https://doi.org/10.1103/fkf1-1jml&lt;/a&gt;</apa>
<ieee>M. Hrast, G. Koutentakis, M. Maslov, and M. Lemeshko, “Bottom-up analysis of rovibrational helical dichroism,” &lt;i&gt;Physical Review Letters&lt;/i&gt;, vol. 136, no. 5. American Physical Society, 2026.</ieee>
<mla>Hrast, Mateja, et al. “Bottom-up Analysis of Rovibrational Helical Dichroism.” &lt;i&gt;Physical Review Letters&lt;/i&gt;, vol. 136, no. 5, 053204, American Physical Society, 2026, doi:&lt;a href=&quot;https://doi.org/10.1103/fkf1-1jml&quot;&gt;10.1103/fkf1-1jml&lt;/a&gt;.</mla>
<short>M. Hrast, G. Koutentakis, M. Maslov, M. Lemeshko, Physical Review Letters 136 (2026).</short>
<chicago>Hrast, Mateja, Georgios Koutentakis, Mikhail Maslov, and Mikhail Lemeshko. “Bottom-up Analysis of Rovibrational Helical Dichroism.” &lt;i&gt;Physical Review Letters&lt;/i&gt;. American Physical Society, 2026. &lt;a href=&quot;https://doi.org/10.1103/fkf1-1jml&quot;&gt;https://doi.org/10.1103/fkf1-1jml&lt;/a&gt;.</chicago>
<ista>Hrast M, Koutentakis G, Maslov M, Lemeshko M. 2026. Bottom-up analysis of rovibrational helical dichroism. Physical Review Letters. 136(5), 053204.</ista>
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