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        <datestamp>2026-09-30T19:17:27Z</datestamp>
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        <oai_dc:dc xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"  xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
          <dc:title>Dense
Low-Energy Landscapes of C&lt;sub&gt;2&lt;/sub&gt;H&lt;sub&gt;6&lt;/sub&gt;S&lt;sub&gt;2&lt;/sub&gt; and
their Implications for Interstellar Sulfur
Chemistry</dc:title>
          <dc:creator>Rafael Flores-Larrañaga (22905742)</dc:creator>
          <dc:creator>Luis Armando Gonzalez-Ortiz (19279037)</dc:creator>
          <dc:creator>Filiberto Ortíz-Chi (19279040)</dc:creator>
          <dc:creator>María Eugenia Castro (10046566)</dc:creator>
          <dc:creator>Francisco J. Melendez (12092780)</dc:creator>
          <dc:creator>Lisset Noriega (12092777)</dc:creator>
          <dc:creator>Gabriel Merino (1413124)</dc:creator>
          <dc:subject>Biophysics</dc:subject>
          <dc:subject>Biochemistry</dc:subject>
          <dc:subject>Evolutionary Biology</dc:subject>
          <dc:subject>Environmental Sciences not elsewhere classified</dc:subject>
          <dc:subject>Chemical Sciences not elsewhere classified</dc:subject>
          <dc:subject>Ecology</dc:subject>
          <dc:subject>Biological Sciences not elsewhere classified</dc:subject>
          <dc:subject>vpt2 calculations reproduce</dc:subject>
          <dc:subject>shallow torsional potentials</dc:subject>
          <dc:subject>mean absolute error</dc:subject>
          <dc:subject>diverse bonding patterns</dc:subject>
          <dc:subject>57 local minima</dc:subject>
          <dc:subject>38 ev ).</dc:subject>
          <dc:subject>10 – 9</dc:subject>
          <dc:subject>polysulfur organic species</dc:subject>
          <dc:subject>interstellar sulfur chemistry</dc:subject>
          <dc:subject>6 &lt;/ sub</dc:subject>
          <dc:subject>2 &lt;/ sub</dc:subject>
          <dc:subject>containing species</dc:subject>
          <dc:subject>whereas geminal</dc:subject>
          <dc:subject>thermodynamically accessible</dc:subject>
          <dc:subject>structural diversity</dc:subject>
          <dc:subject>stable structures</dc:subject>
          <dc:subject>oxygen analogues</dc:subject>
          <dc:subject>narrow interval</dc:subject>
          <dc:subject>molecular inventory</dc:subject>
          <dc:subject>level jun</dc:subject>
          <dc:subject>global minimum</dc:subject>
          <dc:subject>ethyl hydrodisulfide</dc:subject>
          <dc:subject>energy landscapes</dc:subject>
          <dc:subject>dimethyl disulfide</dc:subject>
          <dc:subject>dependent populations</dc:subject>
          <dc:subject>containing structures</dc:subject>
          <dc:subject>conformational flexibility</dc:subject>
          <dc:subject>approximately 0</dc:subject>
          <dc:description>The molecular inventory of sulfur-containing species
in the interstellar
medium remains poorly constrained, particularly for polysulfur organic
species. Here, a comprehensive ab initio exploration of the C&lt;sub&gt;2&lt;/sub&gt;H&lt;sub&gt;6&lt;/sub&gt;S&lt;sub&gt;2&lt;/sub&gt; potential energy surface reveals
a dense low-energy region containing numerous sulfur-containing structures
with diverse bonding patterns and conformational flexibility. High-level
jun-ChS + VPT2 calculations reproduce the available experimental rotational
constants with a mean absolute error of approximately 0.2%, providing
reliable spectroscopic reference data for future laboratory spectroscopic
investigations. A total of 57 local minima were identified, including
seven isomers within 30 kcal·mol&lt;sup&gt;–1&lt;/sup&gt; of the global
minimum. Ethyl hydrodisulfide and dimethyl disulfide are the most
stable structures, whereas geminal and vicinal dithiols remain nearly
degenerate, suggesting that several neutral isomers may be thermodynamically
accessible. In contrast to their oxygen analogues, the low-energy
sulfur isomers exhibit strong energetic crowding and shallow torsional
potentials, generating large conformational manifolds with temperature-dependent
populations. Despite this structural diversity, computed ionization
potentials remain confined to a narrow interval (8.10–9.38
eV).</dc:description>
          <dc:date>2026-09-30T00:00:00Z</dc:date>
          <dc:type>Text</dc:type>
          <dc:type>Journal contribution</dc:type>
          <dc:identifier>10.1021/acsearthspacechem.6c00143.s002</dc:identifier>
          <dc:relation>https://figshare.com/articles/journal_contribution/Dense_Low-Energy_Landscapes_of_C_sub_2_sub_H_sub_6_sub_S_sub_2_sub_and_their_Implications_for_Interstellar_Sulfur_Chemistry/34036712</dc:relation>
          <dc:rights>CC BY-NC 4.0</dc:rights>
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