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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Chem.</journal-id>
<journal-title>Frontiers in Chemistry</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Chem.</abbrev-journal-title>
<issn pub-type="epub">2296-2646</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.3389/fchem.2019.00537</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Chemistry</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>State-Selected Reactivity of Carbon Dioxide Cations (<inline-formula><mml:math id="M1"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>) With Methane</article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name><surname>Ascenzi</surname> <given-names>Daniela</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
<xref ref-type="corresp" rid="c001"><sup>&#x0002A;</sup></xref>
<uri xlink:href="http://loop.frontiersin.org/people/624241/overview"/>
</contrib>
<contrib contrib-type="author">
<name><surname>Romanzin</surname> <given-names>Claire</given-names></name>
<xref ref-type="aff" rid="aff2"><sup>2</sup></xref>
<xref ref-type="aff" rid="aff3"><sup>3</sup></xref>
<uri xlink:href="http://loop.frontiersin.org/people/738681/overview"/>
</contrib>
<contrib contrib-type="author">
<name><surname>Lopes</surname> <given-names>Allan</given-names></name>
<xref ref-type="aff" rid="aff2"><sup>2</sup></xref>
</contrib>
<contrib contrib-type="author">
<name><surname>Tosi</surname> <given-names>Paolo</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
<uri xlink:href="http://loop.frontiersin.org/people/564572/overview"/>
</contrib>
<contrib contrib-type="author">
<name><surname>&#x0017D;abka</surname> <given-names>Jan</given-names></name>
<xref ref-type="aff" rid="aff4"><sup>4</sup></xref>
</contrib>
<contrib contrib-type="author">
<name><surname>Pol&#x000E1;&#x00161;ek</surname> <given-names>Miroslav</given-names></name>
<xref ref-type="aff" rid="aff4"><sup>4</sup></xref>
</contrib>
<contrib contrib-type="author">
<name><surname>Shaffer</surname> <given-names>Christopher J.</given-names></name>
<xref ref-type="aff" rid="aff5"><sup>5</sup></xref>
<xref ref-type="author-notes" rid="fn002"><sup>&#x02020;</sup></xref>
</contrib>
<contrib contrib-type="author">
<name><surname>Alcaraz</surname> <given-names>Christian</given-names></name>
<xref ref-type="aff" rid="aff2"><sup>2</sup></xref>
<xref ref-type="aff" rid="aff3"><sup>3</sup></xref>
<uri xlink:href="http://loop.frontiersin.org/people/624315/overview"/>
</contrib>
</contrib-group>
<aff id="aff1"><sup>1</sup><institution>Department of Physics, University of Trento</institution>, <addr-line>Trento</addr-line>, <country>Italy</country></aff>
<aff id="aff2"><sup>2</sup><institution>Laboratoire de Chimie Physique, B&#x000E2;t. 350, UMR 8000, CNRS-Univ. Paris-Sud and Paris Saclay, Centre Universitaire Paris-Sud</institution>, <addr-line>Orsay</addr-line>, <country>France</country></aff>
<aff id="aff3"><sup>3</sup><institution>Synchrotron SOLEIL, L&#x00027;Orme des Merisiers, Saint-Aubin&#x02014;BP 48</institution>, <addr-line>Gif-sur-Yvette</addr-line>, <country>France</country></aff>
<aff id="aff4"><sup>4</sup><institution>J. Heyrovsk&#x000FD; Institute of Physical Chemistry of the Czech Academy of Sciences</institution>, <addr-line>Prague</addr-line>, <country>Czechia</country></aff>
<aff id="aff5"><sup>5</sup><institution>Institute of Organic Chemistry and Biochemistry of the Czech Academy of Sciences</institution>, <addr-line>Prague</addr-line>, <country>Czechia</country></aff>
<author-notes>
<fn fn-type="edited-by"><p>Edited by: Ramesh L. Gardas, Indian Institute of Technology Madras, India</p></fn>
<fn fn-type="edited-by"><p>Reviewed by: Aparna Shastri, Bhabha Atomic Research Centre (BARC), India; Naved I. Malek, Sardar Vallabhbhai National Institute of Technology Surat, India</p></fn>
<corresp id="c001">&#x0002A;Correspondence: Daniela Ascenzi <email>daniela.ascenzi&#x00040;unitn.it</email></corresp>
<fn fn-type="other" id="fn001"><p>This article was submitted to Physical Chemistry and Chemical Physics, a section of the journal Frontiers in Chemistry</p></fn>
<fn fn-type="present-address" id="fn002"><p>&#x02020;Present address: Christopher J. Shaffer, Sherwin Williams, VAST R&#x00026;D, Minneapolis, MN, United States</p></fn>
</author-notes>
<pub-date pub-type="epub">
<day>02</day>
<month>08</month>
<year>2019</year>
</pub-date>
<pub-date pub-type="collection">
<year>2019</year>
</pub-date>
<volume>7</volume>
<elocation-id>537</elocation-id>
<history>
<date date-type="received">
<day>25</day>
<month>02</month>
<year>2019</year>
</date>
<date date-type="accepted">
<day>15</day>
<month>07</month>
<year>2019</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#x000A9; 2019 Ascenzi, Romanzin, Lopes, Tosi, &#x0017D;abka, Pol&#x000E1;&#x00161;ek, Shaffer and Alcaraz.</copyright-statement>
<copyright-year>2019</copyright-year>
<copyright-holder>Ascenzi, Romanzin, Lopes, Tosi, &#x0017D;abka, Pol&#x000E1;&#x00161;ek, Shaffer and Alcaraz</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>The reactivity of <inline-formula><mml:math id="M2"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> with CD<sub>4</sub> has been experimentally investigated for its relevance in the chemistry of plasmas used for the conversion of CO<sub>2</sub> in carbon-neutral fuels. Non-equilibrium plasmas are currently explored for their capability to activate very stable molecules (such as methane and carbon dioxide) and initiate a series of reactions involving highly reactive species (e.g., radicals and ions) eventually leading to the desired products. Energy, in the form of kinetic or internal excitation of reagents, influences chemical reactions. However, putting the same amount of energy in a different form may affect the reactivity differently. In this paper, we investigate the reaction of <inline-formula><mml:math id="M3"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> with methane by changing either the kinetic energy of <inline-formula><mml:math id="M4"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> or its vibrational excitation. The experiments were performed by a guided ion beam apparatus coupled to synchrotron radiation in the VUV energy range to produce vibrationally excited ions. We find that the reactivity depends on the reagent collision energy, but not so much on the vibrational excitation of <inline-formula><mml:math id="M5"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>. Concerning the product branching ratios (<inline-formula><mml:math id="M6"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>/<inline-formula><mml:math id="M7"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>/DOCO<sup>&#x0002B;</sup>) there is substantial disagreement among the values reported in the literature. We find that the dominant channel is the production of <inline-formula><mml:math id="M8"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>, followed by DOCO<sup>&#x0002B;</sup> and <inline-formula><mml:math id="M9"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>, as a minor endothermic channel.</p></abstract> 
<kwd-group>
<kwd>vibrational excitation</kwd>
<kwd>plasma</kwd>
<kwd>astrochemistry</kwd>
<kwd>Mars atmosphere</kwd>
<kwd>synchrotron radiation</kwd>
<kwd>ion-molecule reaction</kwd>
<kwd>CO<sub>2</sub> dissociation</kwd>
</kwd-group>
<counts>
<fig-count count="5"/>
<table-count count="2"/>
<equation-count count="13"/>
<ref-count count="45"/>
<page-count count="9"/>
<word-count count="7909"/>
</counts>
</article-meta> 
</front>
<body>
<sec sec-type="intro" id="s1">
<title>Introduction</title>
<p>The chemistry of the <inline-formula><mml:math id="M10"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> cation attracts much attention because of the presence of this ion in planetary atmospheres (with particular reference to the Earth and Mars Matta et al., <xref ref-type="bibr" rid="B29">2013</xref>; Tenewitz et al., <xref ref-type="bibr" rid="B41">2018</xref> as well as in laboratory plasmas for energetic and environmental applications Snoeckx and Bogaerts, <xref ref-type="bibr" rid="B39">2017</xref>). In the latter field, the efficient conversion of greenhouse gases into value-added chemicals is a central topic in current research on renewable and sustainable energies (Wang et al., <xref ref-type="bibr" rid="B45">2017</xref>). In particular, the hydrogenation of CO<sub>2</sub> by technologies based on green electricity allows both the storage of renewable energy in value-added compounds and recycling CO<sub>2</sub>, thus paving the way to decarbonise the energy system. Non-thermal plasmas have been explored for their capability to activate very stable molecules with the potential of achieving a higher energy efficiency compared to purely thermal processes (Scapinello et al., <xref ref-type="bibr" rid="B36">2016</xref>; Martini et al., <xref ref-type="bibr" rid="B28">2018</xref>). To improve the performances and to control the outcome of plasma-based processes, insight into the physical and chemical mechanisms at play is desired. According to a chemical kinetic model of the plasma-based dry reforming (Snoeckx et al., <xref ref-type="bibr" rid="B38">2013</xref>), a key role is played by the reaction of <inline-formula><mml:math id="M11"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> with CH<sub>4</sub>. However, as described below, there is considerable uncertainty on the branching ratio, so that a reinvestigation of the reaction is desirable. Also, because vibrationally excited levels of <inline-formula><mml:math id="M12"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> can be populated in plasmas, this study aims at investigating the effect of the vibrational excitation of the <inline-formula><mml:math id="M13"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> cation on the reaction with CH<sub>4</sub>.</p>
<p>Energy, in the form of kinetic or internal motion of the reagents, is the driving force of chemical reactions. However, putting the same amount of energy in a different form (i.e., translational, vibrational, rotational or electronic energy) may affect the reactivity differently. For ion-molecule reactions, some state-selected experiments have shown that for endothermic charge-transfer (CT) processes, vibrational excitation is more effective than translational energy in driving the reactions (Viggiano and Morris, <xref ref-type="bibr" rid="B43">1996</xref>). However, in other cases, the effect of vibrational excitation is more varied (see for example Candori et al., <xref ref-type="bibr" rid="B11">2003</xref>; Boyle et al., <xref ref-type="bibr" rid="B10">2011</xref>; Chang et al., <xref ref-type="bibr" rid="B12">2012</xref>; Bell and Anderson, <xref ref-type="bibr" rid="B6">2013a</xref>,<xref ref-type="bibr" rid="B7">b</xref>; Bell et al., <xref ref-type="bibr" rid="B8">2014</xref> and reference therein).</p>
<p>The effect of the internal excitation of <inline-formula><mml:math id="M14"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> in reactions with small molecules has been addressed in previous studies. It was found that the vibrational excitation of <inline-formula><mml:math id="M15"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> increases the reactivity with O<sub>2</sub> and NO (Alge et al., <xref ref-type="bibr" rid="B3">1981</xref>; Durup-Ferguson et al., <xref ref-type="bibr" rid="B17">1983</xref>; Derai et al., <xref ref-type="bibr" rid="B16">1985</xref>; Ferguson et al., <xref ref-type="bibr" rid="B19">1992</xref>; Nicolas et al., <xref ref-type="bibr" rid="B32">2002</xref>), while it decreases the rate coefficient for the reaction with H<sub>2</sub> (Albritton, <xref ref-type="bibr" rid="B1">1979</xref>; Borodi et al., <xref ref-type="bibr" rid="B9">2009</xref>). However, no previous studies exist in which the <inline-formula><mml:math id="M16"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> cation is generated with a precise amount of internal energy (i.e., state-selection of a specific vibrational state) and reacted with CH<sub>4</sub>.</p>
</sec>
<sec id="s2">
<title>Previous Studies of the <inline-formula><mml:math id="M17"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> &#x0002B; CH<sub>4</sub> Reaction</title>
<p>The reaction of <inline-formula><mml:math id="M18"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> with methane in the gas phase has been studied by several groups, with the earliest experimental results dating back to the late 60s (Anicich, <xref ref-type="bibr" rid="B4">2003</xref>). Rate constant and product branching ratio measurements were made using drift techniques, either flow drift tubes (FDT) (Rakshit and Warneck, <xref ref-type="bibr" rid="B33">1980</xref>; Durup-Ferguson et al., <xref ref-type="bibr" rid="B17">1983</xref>) or selected ion flow tube (SIFT) (Smith et al., <xref ref-type="bibr" rid="B37">1978</xref>; Copp et al., <xref ref-type="bibr" rid="B14">1982</xref>), ion cyclotron resonance (ICR) techniques (Huntress et al., <xref ref-type="bibr" rid="B24">1980</xref>) and ion beam methods (Tsuji et al., <xref ref-type="bibr" rid="B42">1994</xref>). Earlier determinations where done using high-pressure mass spectrometry (HPMS) (Harrison and Myher, <xref ref-type="bibr" rid="B21">1967</xref>; Chong and Franklin, <xref ref-type="bibr" rid="B13">1971</xref>; Kasper and Franklin, <xref ref-type="bibr" rid="B25">1972</xref>) and electron space charge traps (SCT) (Ryan and Harland, <xref ref-type="bibr" rid="B35">1974</xref>). The most relevant results are summarized in <xref ref-type="table" rid="T1">Table 1</xref>.</p>
<table-wrap position="float" id="T1">
<label>Table 1</label>
<caption><p>Summary of existing experimental determinations of rate constants and branching ratios for the reaction of <inline-formula><mml:math id="M19"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> with CH<sub>4</sub>.</p></caption>
<table frame="hsides" rules="groups">
<thead>
<tr>
<th/>
<th valign="top" align="center" colspan="3" style="border-bottom: thin solid #000000;"><bold>Product branching ratios</bold></th>
<th/>
<th/>
</tr>
<tr>
<th valign="top" align="left"><bold><italic>k</italic> (cm<sup>3</sup>&#x000B7;molecule<sup>&#x02212;1</sup>&#x000B7;s<sup>&#x02212;1</sup>)<xref ref-type="table-fn" rid="TN1"><sup>a</sup></xref></bold></th>
<th valign="top" align="center"><bold><inline-formula><mml:math id="M20"><mml:msubsup><mml:mrow><mml:mtext>CH</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula></bold></th>
<th valign="top" align="center"><bold>HOCO<sup><bold>&#x0002B;</bold></sup></bold></th>
<th valign="top" align="left"><bold>Others</bold></th>
<th valign="top" align="center"><bold>Method</bold></th>
<th valign="top" align="left"><bold>References</bold></th>
</tr>
</thead>
<tbody>
<tr>
<td valign="top" align="left">(9.60 &#x000B1; 3.8)&#x000D7; 10<sup>&#x02212;10</sup></td>
<td valign="top" align="center">0.28 &#x000B1; 0.01</td>
<td valign="top" align="center">0.72 &#x000B1; 0.01</td>
<td/>
<td valign="top" align="center">Beam</td>
<td valign="top" align="left">Tsuji et al., <xref ref-type="bibr" rid="B42">1994</xref></td>
</tr>
<tr>
<td valign="top" align="left">(1.0 &#x000B1; 0.3)&#x000D7; 10<sup>&#x02212;9</sup></td>
<td valign="top" align="center">1.0</td>
<td/>
<td/>
<td valign="top" align="center">FDT</td>
<td valign="top" align="left">Durup-Ferguson et al., <xref ref-type="bibr" rid="B17">1983</xref></td>
</tr>
<tr>
<td valign="top" align="left">(1.1 &#x000B1; 0.2)&#x000D7; 10<sup>&#x02212;9</sup></td>
<td valign="top" align="center">0.5 &#x000B1; 0.1</td>
<td valign="top" align="center">0.5 &#x000B1; 0.1</td>
<td/>
<td valign="top" align="center">SIFT</td>
<td valign="top" align="left">Copp et al., <xref ref-type="bibr" rid="B14">1982</xref></td>
</tr>
<tr>
<td valign="top" align="left">(1.0 &#x000B1; 0.1)&#x000D7; 10<sup>&#x02212;9</sup></td>
<td valign="top" align="center">0.25</td>
<td valign="top" align="center">0.75</td>
<td/>
<td valign="top" align="center">ICR</td>
<td valign="top" align="left">Huntress et al., <xref ref-type="bibr" rid="B24">1980</xref></td>
</tr>
<tr>
<td valign="top" align="left">(9.00 &#x000B1; 1.8)&#x000D7; 10<sup>&#x02212;10</sup></td>
<td/>
<td valign="top" align="center">1.00</td>
<td/>
<td valign="top" align="center">DT</td>
<td valign="top" align="left">Rakshit and Warneck, <xref ref-type="bibr" rid="B33">1980</xref></td>
</tr>
<tr>
<td valign="top" align="left">1.0&#x000D7; 10<sup>&#x02212;9</sup></td>
<td valign="top" align="center">0.60</td>
<td valign="top" align="center">0.40</td>
<td/>
<td valign="top" align="center">SIFT</td>
<td valign="top" align="left">Smith et al., <xref ref-type="bibr" rid="B37">1978</xref></td>
</tr>
<tr>
<td valign="top" align="left">(1.15 &#x000B1; 0.1)&#x000D7; 10<sup>&#x02212;9</sup></td>
<td valign="top" align="center">0.30</td>
<td valign="top" align="center">0.70</td>
<td/>
<td valign="top" align="center">SCT</td>
<td valign="top" align="left">Ryan and Harland, <xref ref-type="bibr" rid="B35">1974</xref></td>
</tr>
<tr>
<td valign="top" align="left">2.31&#x000D7; 10<sup>&#x02212;9</sup></td>
<td/>
<td valign="top" align="center">&#x0003E;0.99</td>
<td valign="top" align="left">HCO<sup>&#x0002B;</sup> &#x0003C;0.01</td>
<td valign="top" align="center">HPMS</td>
<td valign="top" align="left">Kasper and Franklin, <xref ref-type="bibr" rid="B25">1972</xref></td>
</tr>
<tr>
<td valign="top" align="left">1.2&#x000D7; 10<sup>&#x02212;9</sup></td>
<td/>
<td valign="top" align="center">1.00<xref ref-type="table-fn" rid="TN2"><sup>b</sup></xref></td>
<td/>
<td valign="top" align="center">MS</td>
<td valign="top" align="left">Harrison and Myher, <xref ref-type="bibr" rid="B21">1967</xref></td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn id="TN1">
<label>a</label>
<p><italic>Rate constants at thermal energy</italic>.</p></fn> 
<fn id="TN2">
<label>b</label>
<p><italic>Reaction with CD<sub>4</sub> to give CO<sub>2</sub>D<sup>&#x0002B;</sup> exclusively</italic>.</p></fn>
</table-wrap-foot>
</table-wrap>
<p>It has been shown that the reaction proceeds at thermal energy with a rate constant close to the Langevin collision rate constant <italic>k</italic><sub><italic>L</italic></sub> &#x0003D; 1.1 &#x000D7; 10<sup>&#x02212;9</sup> cm<sup>3</sup>&#x000B7;molecule<sup>&#x02212;1</sup>&#x000B7;s<sup>&#x02212;1</sup> (Durup-Ferguson et al., <xref ref-type="bibr" rid="B17">1983</xref>). There is fair agreement (within the experimental errors) among the total rate constants measured at thermal energies (in the range 280&#x02013;340 K for the data reported in <xref ref-type="table" rid="T1">Table 1</xref>), with the exception of the HPMS study by Kasper and Franklin (<xref ref-type="bibr" rid="B25">1972</xref>), that gives a rate constant value more than a factor two higher than the others. The values for the branching ratios are quite scattered, with HOCO<sup>&#x0002B;</sup> being dominant in all studies except (Durup-Ferguson et al., <xref ref-type="bibr" rid="B17">1983</xref>), where the CT is the only observed channel.</p>
</sec>
<sec sec-type="materials and methods" id="s3">
<title>Materials and Methods</title>
<p>The experiments have been performed using the CERISES apparatus, an associated experiment to the SOLEIL synchrotron radiation facility. Since the set-up was described in details previously (see Alcaraz et al., <xref ref-type="bibr" rid="B2">2004</xref>; Cunha de Miranda et al., <xref ref-type="bibr" rid="B15">2015</xref>), only the most relevant details will be given here. CERISES is a guided ion beam tandem mass spectrometer composed of two octopoles located between two quadrupole mass spectrometers in a Q1-O1-O2-Q2 configuration that permits investigation of bi-molecular reactions of mass-selected ions. By measuring the yields of parent- and product-ions, absolute reaction cross sections, branching ratios and product velocity distributions as a function of the collision energy are derived.</p>
<p>Vibrational state selection of <inline-formula><mml:math id="M21"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> is performed via the Threshold Photoelectron Photoion Coincidence (TPEPICO) method (Baer and Guyon, <xref ref-type="bibr" rid="B5">1986</xref>) using the ion source of CERISES and the DESIRS beamline. The undulator based DESIRS beamline (Nahon et al., <xref ref-type="bibr" rid="B31">2012</xref>) provides tunable radiation in the vacuum ultraviolet (VUV) range from about 5 eV to 40 eV. Photons at the desired wavelength are selected and scanned simultaneously with the undulator peak energy by a normal incidence monochromator equipped with a low dispersion uncoated SiC grating (200 grooves/mm) optimized to provide photon flux in the 10<sup>12</sup> photon/s to 10<sup>13</sup> photon/s range with an energy resolution down to 1 meV in the 5 eV to 20 eV range. In the present experiments, the photon energies (<italic>E</italic><sub><italic>phot</italic></sub>) required to produce the parent ion by photoionisation are in the range 13.7&#x02013;18.3 eV. Depending on the operation mode, the monochromator slits were set in the range 25 to 400 &#x003BC;m, corresponding, at these photon energies, to a resolution of 3 to 44 meV.</p>
<p>In the TPEPICO mode, the <inline-formula><mml:math id="M22"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> ions are extracted in coincidence with threshold photoelectrons. Threshold photoelectrons are filtered first through geometrical discrimination of energetic photoelectrons by using a small extraction field of &#x02248; 1 V/cm and an extraction hole of 2 mm in diameter. Further time discrimination of energetic photoelectrons is made possible by recording the photoelectron arrival time on the detector and setting a time gate of 10 ns corresponding to the arrival time of threshold photoelectrons. The overall resolution of threshold electrons is about 25 meV. The source pressure and VUV flux are set to limit the false coincidence (FC) rate in the order of 10%. The FC are measured for each TPEPICO point for parent and product ions by replacing the true photoelectron signal by an arbitrary trigger. The FC contribution is then subtracted from the ion count signal. Some measurements have been carried out in the DC mode, i.e., without state-selection but with parent ions in a distribution of excitation that can vary with the photon energy.</p>
<p>Prior to the reactivity experiment, the threshold photoelectron spectrum of CO<sub>2</sub> has been measured using the CERISES set up in the 13.7&#x02013;18.3 eV photon energy range corresponding to the <inline-formula><mml:math id="M23"><mml:msup><mml:mrow><mml:mtext>X</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:msub><mml:mrow><mml:mo>&#x003A0;</mml:mo></mml:mrow><mml:mrow><mml:mtext>g</mml:mtext></mml:mrow></mml:msub></mml:math></inline-formula>(3/2, 1/2) ground state (I.E. &#x0003D; 13.778 eV), the first excited state A <sup>2</sup>&#x003A0; <sub>u</sub>(3/2, 1/2) with I.E. &#x0003D; 17.313 eV, up to the beginning of the B<sup>2</sup><inline-formula><mml:math id="M24"><mml:munderover accentunder="false" accent="false"><mml:mrow><mml:mo>&#x02211;</mml:mo></mml:mrow><mml:mrow><mml:mtext>u</mml:mtext></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:munderover></mml:math></inline-formula> state of the ion (I.E. &#x0003D; 18.076 eV). For high-resolution VUV TPES spectra of CO<sub>2</sub> with the complete assignment of the spectral features to specific internal modes of the <inline-formula><mml:math id="M25"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> ion, the reader is referred to the papers by Baer and Guyon (<xref ref-type="bibr" rid="B5">1986</xref>); Merkt et al. (<xref ref-type="bibr" rid="B30">1993</xref>); Liu et al. (<xref ref-type="bibr" rid="B26">2000a</xref>,<xref ref-type="bibr" rid="B27">b</xref>). In <xref ref-type="fig" rid="F1">Figure 1</xref> we report our measured TPES spectrum in the VUV region where reactivity experiments have been performed. The red dashed lines indicate the photon energies chosen for the production of state-selected <inline-formula><mml:math id="M26"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> in the TPEPICO mode, while the black arrows point to the photon energies at which reactivity studies have been performed in the DC mode (without state-selection).</p>
<fig id="F1" position="float">
<label>Figure 1</label>
<caption><p>TPEPICO spectrum of CO<sub>2</sub> recorded using the CERISES set-up at the DESIRS beamline of the SOLEIL synchrotron. Black solid arrows indicate the photon energies (<italic>E</italic><sub><italic>phot</italic></sub>) at which reactivity studies in the DC mode have been performed, while red dashed lines indicate the energies chosen for experiments in the coincidence mode, i.e., with selective internal excitation of the <inline-formula><mml:math id="M27"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> cation (see section Results and Discussion).</p></caption>
<graphic xlink:href="fchem-07-00537-g0001.tif"/>
</fig>
<p>Following the assignment of Liu et al. (<xref ref-type="bibr" rid="B26">2000a</xref>), the photoelectron band at <italic>E</italic><sub><italic>phot</italic></sub> &#x0003D; 13.78 eV corresponds to the transition <inline-formula><mml:math id="M28"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>(0,0,0) <inline-formula><mml:math id="M29"><mml:msup><mml:mrow><mml:mtext>X</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:msub><mml:mrow><mml:mo>&#x003A0;</mml:mo></mml:mrow><mml:mrow><mml:mtext>g</mml:mtext><mml:mo>,</mml:mo><mml:mn>3</mml:mn><mml:mo>/</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> &#x02190; CO<sub>2</sub>(0,0,0) <inline-formula><mml:math id="M30"><mml:msup><mml:mrow><mml:mtext>X</mml:mtext></mml:mrow><mml:mrow><mml:mn>1</mml:mn></mml:mrow></mml:msup><mml:msubsup><mml:mrow><mml:mo>&#x003A3;</mml:mo></mml:mrow><mml:mrow><mml:mtext>g</mml:mtext></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>, hence producing the <inline-formula><mml:math id="M31"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> cation in its electronic ground state with no vibrational excitation, hereafter indicated as (0,0,0). The band at <italic>E</italic><sub><italic>phot</italic></sub> &#x0003D; 13.84 eV corresponds to one of the four vibronic components of the transition <inline-formula><mml:math id="M32"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>(0,1,0) <inline-formula><mml:math id="M33"><mml:msup><mml:mrow><mml:mtext>X</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:msub><mml:mrow><mml:mo>&#x003A0;</mml:mo></mml:mrow><mml:mrow><mml:mtext>g</mml:mtext></mml:mrow></mml:msub></mml:math></inline-formula> &#x02190; CO<sub>2</sub>(0,0,0) X<sup>1</sup><inline-formula><mml:math id="M34"><mml:munderover accentunder="false" accent="false"><mml:mrow><mml:mo>&#x02211;</mml:mo></mml:mrow><mml:mrow><mml:mtext>g</mml:mtext></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:munderover></mml:math></inline-formula>, more precisely either the <inline-formula><mml:math id="M35"><mml:msub><mml:mrow><mml:mmultiscripts><mml:mo>&#x00394;</mml:mo><mml:mprescripts/><mml:none/><mml:mn>2</mml:mn></mml:mmultiscripts></mml:mrow><mml:mrow><mml:mn>5</mml:mn><mml:mo>/</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> or <sup>2</sup>&#x003A3;<sup>&#x0002B;</sup> component that we cannot distinguish at our limited resolution (see Liu et al., <xref ref-type="bibr" rid="B26">2000a</xref> paper for the attribution of the four components), thus generating the <inline-formula><mml:math id="M36"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> cation in its electronic ground state with one quantum of vibrational excitation in the bending &#x003BD;<sub>2</sub> mode, hereafter indicated as (0,1,0). The band at <italic>E</italic><sub><italic>phot</italic></sub> &#x0003D; 13.95 eV corresponds to the overlap of two transitions, namely <inline-formula><mml:math id="M37"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>(1,0,0) X <inline-formula><mml:math id="M38"><mml:msub><mml:mrow><mml:mmultiscripts><mml:mi>&#x220F;</mml:mi><mml:mprescripts/><mml:none/><mml:mn>2</mml:mn></mml:mmultiscripts></mml:mrow><mml:mrow><mml:mtext>g</mml:mtext><mml:mo>,</mml:mo><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> &#x02190; CO<sub>2</sub>(0,0,0) X <inline-formula><mml:math id="M39"><mml:msubsup><mml:mrow><mml:mmultiscripts><mml:mo>&#x003A3;</mml:mo><mml:mprescripts/><mml:none/><mml:mn>1</mml:mn></mml:mmultiscripts></mml:mrow><mml:mtext>g</mml:mtext><mml:mo>+</mml:mo></mml:msubsup></mml:math></inline-formula> and <inline-formula><mml:math id="M40"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>(0,0,1) X <inline-formula><mml:math id="M41"><mml:msub><mml:mrow><mml:mmultiscripts><mml:mi>&#x220F;</mml:mi><mml:mprescripts/><mml:none/><mml:mn>2</mml:mn></mml:mmultiscripts></mml:mrow><mml:mrow><mml:mtext>g</mml:mtext><mml:mo>,</mml:mo><mml:mn>3</mml:mn><mml:mo>/</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> &#x02190; CO<sub>2</sub>(0,0,0) <inline-formula><mml:math id="M42"><mml:msup><mml:mrow><mml:mtext>X</mml:mtext></mml:mrow><mml:mrow><mml:mn>1</mml:mn></mml:mrow></mml:msup><mml:msubsup><mml:mrow><mml:mo>&#x003A3;</mml:mo></mml:mrow><mml:mrow><mml:mtext>g</mml:mtext></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>, and therefore leads to <inline-formula><mml:math id="M43"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> in the X state with one quantum of vibrational excitation in either the symmetric (&#x003BD;<sub>1</sub>) or the antisymmetric (&#x003BD;<sub>3</sub>) stretching vibration, hereafter indicated as (1,0,0) &#x0002B; (0,0,1).</p>
<p>A sufficient number of ion counts on the threshold electron signal have been observed to perform reactivity experiments with the state-selected cations at the three photon energies (red lines in <xref ref-type="fig" rid="F1">Figure 1</xref>) corresponding to the vibronic bands giving <inline-formula><mml:math id="M44"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> with either no or low vibrational excitation. The intensity of other vibronic bands corresponding to higher internal excitation of <inline-formula><mml:math id="M45"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> was not sufficient to study reactivity in coincidence. For this reason, we decided to perform some measurements not in the coincidence mode, i.e., without pure state-selection but with parent ions in a distribution of excitation that can vary with the photon energy. Two photon-energies were chosen: at <italic>E</italic><sub><italic>phot</italic></sub> &#x0003D; 13.48 eV, corresponding to the <inline-formula><mml:math id="M46"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>(0,0,0) <inline-formula><mml:math id="M47"><mml:msup><mml:mrow><mml:mtext>X</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:msub><mml:mrow><mml:mo>&#x003A0;</mml:mo></mml:mrow><mml:mrow><mml:mtext>g</mml:mtext><mml:mo>,</mml:mo><mml:mn>3</mml:mn><mml:mo>/</mml:mo><mml:mn>2</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> &#x02190; CO<sub>2</sub>(0,0,0) <inline-formula><mml:math id="M48"><mml:msup><mml:mrow><mml:mtext>X</mml:mtext></mml:mrow><mml:mrow><mml:mn>1</mml:mn></mml:mrow></mml:msup><mml:msubsup><mml:mrow><mml:mo>&#x003A3;</mml:mo></mml:mrow><mml:mrow><mml:mtext>g</mml:mtext></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> transition, the <inline-formula><mml:math id="M49"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> cation will be produced with no vibrational excitation; at <italic>E</italic><sub><italic>phot</italic></sub> &#x0003D; 16.48 eV, corresponding to a strong resonant autoionization transition via Rydberg states converging to the <inline-formula><mml:math id="M50"><mml:mover accent="true"><mml:mrow><mml:mi>B</mml:mi></mml:mrow><mml:mo>&#x0007E;</mml:mo></mml:mover></mml:math></inline-formula> state of <inline-formula><mml:math id="M51"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>, the latter will be produced in the X electronic state but with a broad distribution of internal energies, hence in a mixture of low and high vibrational excitation (see Baer and Guyon, <xref ref-type="bibr" rid="B5">1986</xref> for details).</p>
<p>Deuterated methane (CD<sub>4</sub>) was used for the reactivity study, to avoid partial mass overlap between the strong parent ion peak at <italic>m/z</italic> 44 and the one due to the product of the H-atom transfer process at <italic>m/z</italic> 45. CD<sub>4</sub> pressure in the scattering cell was kept in the range 1&#x02013;2 &#x000D7; 10<sup>&#x02212;4</sup> mbar throughout the experiments. Some considerations on possible isotope effects arising when CD<sub>4</sub> is replaced by CH<sub>4</sub> are addressed in the Conclusions.</p>
</sec>
<sec id="s4">
<title>Results and Discussion</title>
<sec>
<title>Results in the DC Mode</title>
<p>As already mentioned in the previous section, in the DC mode we have measured absolute values of the cross sections as a function of the collision energy <italic>E</italic><sub><italic>CM</italic></sub> at two selected photon energies: <italic>E</italic><sub><italic>phot</italic></sub> &#x0003D; 13.78 eV (no vibrational excitation of the <inline-formula><mml:math id="M52"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> cation) and <italic>E</italic><sub><italic>phot</italic></sub> &#x0003D; 16.48 eV (some excitation to high vibrational levels). The main reaction products observed are due to the CT and deuterium-atom-transfer channels (1) and (2), respectively:</p>
<disp-formula id="E1"><label>(1)</label><mml:math id="M53"><mml:msubsup><mml:mtext>CO</mml:mtext><mml:mtext>2</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msubsup><mml:msub><mml:mtext>+CD</mml:mtext><mml:mtext>4</mml:mtext></mml:msub><mml:mo>&#x02192;</mml:mo><mml:msub><mml:mtext>CO</mml:mtext><mml:mtext>2</mml:mtext></mml:msub><mml:msubsup><mml:mtext>+CD</mml:mtext><mml:mtext>4</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msubsup></mml:math></disp-formula>
<disp-formula id="E2"><label>(2)</label><mml:math id="M54"><mml:mo>&#x02192;</mml:mo><mml:msubsup><mml:mtext>DCO</mml:mtext><mml:mtext>2</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msubsup><mml:msub><mml:mtext>+CD</mml:mtext><mml:mtext>3</mml:mtext></mml:msub></mml:math></disp-formula>
<p>Also, small amounts of <inline-formula><mml:math id="M55"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>, and minimal amounts of CD<sub>3</sub><inline-formula><mml:math id="M56"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> are detected and attributed to the following channels (3), (4) and (5):</p>
<disp-formula id="E3"><label>(3)</label><mml:math id="M57"><mml:msubsup><mml:mtext>CO</mml:mtext><mml:mtext>2</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msubsup><mml:msub><mml:mtext>+CD</mml:mtext><mml:mtext>4</mml:mtext></mml:msub><mml:mo>&#x02192;</mml:mo><mml:msubsup><mml:mtext>CD</mml:mtext><mml:mtext>3</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msubsup><mml:mtext>+DOCO</mml:mtext></mml:math></disp-formula>
<disp-formula id="E4"><label>(4)</label><mml:math id="M58"><mml:mo>&#x02192;</mml:mo><mml:msubsup><mml:mtext>CD</mml:mtext><mml:mtext>3</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msubsup><mml:msub><mml:mtext>+D+CO</mml:mtext><mml:mtext>2</mml:mtext></mml:msub></mml:math></disp-formula>
<disp-formula id="E5"><label>(5)</label><mml:math id="M59"><mml:mo>&#x02192;</mml:mo><mml:msub><mml:mtext>CD</mml:mtext><mml:mtext>3</mml:mtext></mml:msub><mml:msubsup><mml:mtext>CO</mml:mtext><mml:mtext>2</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msubsup><mml:mtext>+D</mml:mtext></mml:math></disp-formula>
<p>Using literature values (taken from NIST Chemistry Webbook<xref ref-type="fn" rid="fn0001"><sup>1</sup></xref>, with the exception of some products as specified in the following) for the standard enthalpies of formations (&#x00394;<sub>f</sub><italic>H</italic>&#x000B0;) of reagents and products we can assess that both channels (1) and (2) are exothermic, while channels (3) and (4) are endothermic. In particular, the CT channel (1) has a reaction enthalpy &#x00394;<sub>r</sub><italic>H</italic>&#x000B0; &#x0003D; &#x02212;1.17 eV, while &#x00394;<sub>r</sub><italic>H</italic>&#x000B0; for (2) is equal to &#x02212;1.26 eV, assuming that HOCO<sup>&#x0002B;</sup> has the structure of the hydroxyformyl cation (Holmes et al., <xref ref-type="bibr" rid="B22">2006</xref>). The production of <inline-formula><mml:math id="M60"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> can derive either from D<sup>&#x02212;</sup> transfer process (3) or from dissociative CT (4). In the former case, the DOCO radical might be formed in association with the methyl cation, and the overall process is calculated to be endothermic by about 0.56 eV, using the heat of formation of HOCO as reported in Francisco et al. (<xref ref-type="bibr" rid="B20">2010</xref>). In the latter case, the methyl cation derives from dissociation of the CT product and the process is endothermic by about 0.61 eV.</p>
<p>The CD<sub>3</sub><inline-formula><mml:math id="M61"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> formation can be due to D loss from the ion-molecule adduct <inline-formula><mml:math id="M62"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>-CD<sub>4</sub> (reaction 5). We can attempt to estimate the reaction enthalpy of (5) assuming that CD<sub>3</sub><inline-formula><mml:math id="M63"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> has the structure of the methoxycarbonyl cation [an average value for its heat of formation &#x00394;<sub>f</sub><italic>H</italic>&#x000B0;(CH<sub>3</sub>OCO<sup>&#x0002B;</sup>) is 5.57&#x000B1;0.19 eV, as reported in Holmes et al., <xref ref-type="bibr" rid="B22">2006</xref>] to get &#x00394;<sub>r</sub><italic>H</italic>&#x000B0; &#x0003D; &#x02212;1.10 eV. We note in passing that the adduct <inline-formula><mml:math id="M64"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>-CD<sub>4</sub> was not observed, as expected, as the CD<sub>4</sub> pressure in the scattering cell used throughout the experiments (about 2 &#x000D7; 10<sup>&#x02212;4</sup> mbar) was too low to allow for secondary collisions for its stabilization.</p>
<p>Cross sections for products <inline-formula><mml:math id="M65"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>, DOCO<sup>&#x0002B;</sup> and <inline-formula><mml:math id="M66"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> as well as <inline-formula><mml:math id="M67"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (from secondary reactions of the primary <inline-formula><mml:math id="M68"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> and DOCO<sup>&#x0002B;</sup> products) measured as a function of the collision energy when the reagent <inline-formula><mml:math id="M69"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> ion is in its ground vibrational state (i.e., at <italic>E</italic><sub><italic>phot</italic></sub> &#x0003D; 13.78 eV) are reported in <xref ref-type="fig" rid="F2">Figure 2</xref>, while results for <italic>E</italic><sub><italic>phot</italic></sub> &#x0003D; 16.48 eV are shown in <xref ref-type="fig" rid="F3">Figure 3</xref>. The cross section for <inline-formula><mml:math id="M70"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> was measured to correct the absolute value of the cross section for reactions (1) and (2) due to product ion losses via the highly efficient secondary reactions operative at the deuterated methane pressures used:</p>
<disp-formula id="E6"><label>(6)</label><mml:math id="M71"><mml:msubsup><mml:mtext>CD</mml:mtext><mml:mtext>4</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msubsup><mml:msub><mml:mtext>+CD</mml:mtext><mml:mtext>4</mml:mtext></mml:msub><mml:mo>&#x02192;</mml:mo><mml:msubsup><mml:mtext>CD</mml:mtext><mml:mtext>5</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msubsup><mml:msub><mml:mtext>+CD</mml:mtext><mml:mtext>3</mml:mtext></mml:msub></mml:math></disp-formula>
<disp-formula id="E7"><label>(7)</label><mml:math id="M72"><mml:msup><mml:mtext>DOCO</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msup><mml:msub><mml:mtext>+CH</mml:mtext><mml:mtext>4</mml:mtext></mml:msub><mml:mo>&#x02192;</mml:mo><mml:msubsup><mml:mtext>CD</mml:mtext><mml:mtext>5</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msubsup><mml:msub><mml:mtext>+CO</mml:mtext><mml:mtext>2</mml:mtext></mml:msub></mml:math></disp-formula>
<p>with <italic>k</italic> &#x0003D; 1.1 &#x000D7; 10<sup>&#x02212;9</sup> cm<sup>3</sup>&#x000B7;molecule<sup>&#x02212;1</sup>&#x000B7;sec<sup>&#x02212;1</sup> for reaction (6) (Anicich, <xref ref-type="bibr" rid="B4">2003</xref>) and <italic>k</italic> &#x0003D; 7.2 &#x000D7; 10<sup>&#x02212;10</sup> cm<sup>3</sup>&#x000B7;molecule<sup>&#x02212;1</sup>&#x000B7;sec<sup>&#x02212;1</sup> for reaction (7) (Anicich, <xref ref-type="bibr" rid="B4">2003</xref>). The measured <inline-formula><mml:math id="M73"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> yields have been redistributed among the <inline-formula><mml:math id="M74"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> and DOCO<sup>&#x0002B;</sup> products on the basis of the <inline-formula><mml:math id="M75"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>/DOCO<sup>&#x0002B;</sup> yield ratio (that changes with collision energy from &#x0007E;2 at low energies up to &#x0007E;7 at high energies) and of the different rate coefficients for reactions (6) and (7). In <xref ref-type="fig" rid="F2">Figures 2</xref>, <xref ref-type="fig" rid="F3">3</xref> the uncorrected and corrected cross sections for <inline-formula><mml:math id="M76"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> are labeled as &#x0201C;<inline-formula><mml:math id="M77"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>&#x0201D; and &#x0201C;<inline-formula><mml:math id="M78"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> corr&#x0201D; respectively, and the same notation is used for DOCO<sup>&#x0002B;</sup>.</p>
<fig id="F2" position="float">
<label>Figure 2</label>
<caption><p>Reactive cross sections for products <inline-formula><mml:math id="M79"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (uncorrected, black circles), DOCO<sup>&#x0002B;</sup> (uncorrected, red squares), <inline-formula><mml:math id="M80"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (green diamonds), and <inline-formula><mml:math id="M81"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (blue triangles) measured as a function of the collision energy (<italic>E</italic><sub><italic>CM</italic></sub>) in the DC mode at a photon energy <italic>E</italic><sub><italic>phot</italic></sub> &#x0003D; 13.78 eV. The open black circles and open red squares are the <inline-formula><mml:math id="M82"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> and DOCO<sup>&#x0002B;</sup> cross sections corrected to include the contribution of secondary reactions leading to <inline-formula><mml:math id="M83"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>. The dotted line represents the <inline-formula><mml:math id="M84"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> cross sections corrected for the instrumental effect due to decreased collection efficiency at low <italic>E</italic><sub><italic>CM</italic></sub> (see text for details). Error bars on all the data are about 30%: for the sake of clarity only two error bars are reported, at arbitrarily chosen low and high collision energy values.</p></caption>
<graphic xlink:href="fchem-07-00537-g0002.tif"/>
</fig>
<fig id="F3" position="float">
<label>Figure 3</label>
<caption><p>Reactive cross sections for products <inline-formula><mml:math id="M85"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (uncorrected, black circles), DOCO<sup>&#x0002B;</sup> (uncorrected, red squares), <inline-formula><mml:math id="M86"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (green diamonds), and CD<sub>3</sub><inline-formula><mml:math id="M87"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (magenta triangles) measured as a function of the collision energy (<italic>E</italic><sub><italic>CM</italic></sub>) in the DC mode at a photon energy <italic>E</italic><sub><italic>phot</italic></sub> &#x0003D; 16.48 eV. The open black circles and open red squares are the <inline-formula><mml:math id="M88"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> and DOCO<sup>&#x0002B;</sup> cross sections corrected to include the contribution of secondary reactions leading to <inline-formula><mml:math id="M89"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (data not shown). The dotted line represents the <inline-formula><mml:math id="M90"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> cross sections corrected for the instrumental effect due to decreased collection efficiency at low <italic>E</italic><sub><italic>CM</italic></sub> (see text for details). Error bars on all the data are about 30%: for the sake of clarity only two error bars are reported, at arbitrarily chosen low and high collision energy values.</p></caption>
<graphic xlink:href="fchem-07-00537-g0003.tif"/>
</fig>
<p>The sudden increase in the cross section shown for <inline-formula><mml:math id="M91"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> and <inline-formula><mml:math id="M92"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> products at <italic>E</italic><sub><italic>CM</italic></sub> &#x0007E; 0.3 eV (clearly visible in the data of <xref ref-type="fig" rid="F2">Figure 2</xref>, but also present in the data of <xref ref-type="fig" rid="F3">Figure 3</xref>) is an instrumental effect due to a decrease in the collection efficiency for &#x0201C;slow&#x0201D; products. In particular, when product ions are produced at very low velocities in the lab frame, they have a chance to move backwards in the 1st octopole (O1) in the opposite direction from the parent ions, and they then face the last electrode before this octopole, L3, which is set to a potential of &#x02212;0.4 V. As these ions are produced in O1, their fate depends on their initial kinetic energy and the relative values of the O1 and L3 potentials. At high collision energies, the mean potential of O1 is very low (negative values) and all product ions going back in O1 are reflected on L3 and later detected. At low collision energies, the O1 potential can be higher than that of L3, and backward product ions can be lost, accounting for the step in the product yield observed below collision energies of &#x0007E;0.3 eV. To correct for such effect, we have rescaled the data measured at <italic>E</italic><sub><italic>CM</italic></sub> &#x02264; 0.3 eV by a fixed multiplication factor, chosen equal to 1.12 to match the data measured at <italic>E</italic><sub><italic>CM</italic></sub> &#x0003C; 0.3 eV with those measured at higher collision energy. Implicit in this way of rescaling data is the assumption that the number of product ions lost at low collision energy is independent on the collision energy. The corrected data (reported only for <inline-formula><mml:math id="M93"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> cross sections corrected for the presence of secondary reactions leading to <inline-formula><mml:math id="M94"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>) are shown as dashed lines in <xref ref-type="fig" rid="F2">Figures 2</xref>, <xref ref-type="fig" rid="F3">3</xref>.</p>
<p>According to the above-mentioned thermochemistry, the formation of <inline-formula><mml:math id="M95"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> via either (3) or (4) is endothermic and the cross-section for its formation, when <inline-formula><mml:math id="M96"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> is generated with no vibrational excitation (see green diamonds in <xref ref-type="fig" rid="F2">Figure 2</xref>), shows the expected threshold behavior, with an appearance energy compatible with the endothermicity. Above threshold, the cross section increases accordingly with collision energy. The small amount of signal observed below the threshold is an artifact due to the tail of the very intense mass peak at 20 <italic>m/z</italic> (<inline-formula><mml:math id="M97"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>). Data measured at <italic>E</italic><sub><italic>phot</italic></sub> &#x0003D; 16.48 eV show non-negligible cross sections even at low <italic>E</italic><sub><italic>CM</italic></sub>, thus indicating that vibrational excitation of the <inline-formula><mml:math id="M98"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> cation can promote the endothermic channel.</p>
<p>At <italic>E</italic><sub><italic>phot</italic></sub> &#x0003D; 13.78 eV and at the CD<sub>4</sub> pressure used, the yield of CD<sub>3</sub><inline-formula><mml:math id="M99"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> was below the detection limit, while at <italic>E</italic><sub><italic>phot</italic></sub> &#x0003D; 16.48 eV it was possible to measure a cross section for this very minor channel (data for CD<sub>3</sub><inline-formula><mml:math id="M100"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> in <xref ref-type="fig" rid="F3">Figure 3</xref> are multiplied by 300 to be able to show them in the same scale of the other products).</p>
<p>In <xref ref-type="table" rid="T2">Table 2</xref> results at the two photon energies are summarized by reporting the branching ratios (BRs) for the observed product channels and the energy-dependent rate constants. BR for the <italic>i</italic>-th channel have been calculated from the absolute cross sections according to the expression:</p>
<disp-formula id="E8"><mml:math id="M101"><mml:mi>B</mml:mi><mml:mi>R</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mo>=</mml:mo><mml:mfrac><mml:mrow><mml:msub><mml:mi>&#x003C3;</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mstyle displaystyle='true'><mml:mo>&#x02211;</mml:mo><mml:mrow><mml:msub><mml:mi>&#x003C3;</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:mstyle></mml:mrow></mml:mfrac></mml:math></disp-formula>
<p>The energy-dependent total rate constants <italic>k</italic><sub><italic>tot</italic></sub>(<italic>E</italic><sub><italic>ave</italic></sub>) have been estimated using the expression <italic>k</italic><sub><italic>tot</italic></sub>(<italic>E</italic><sub><italic>ave</italic></sub>) &#x0003D; &#x02329;V&#x0232A; &#x000B7; &#x003C3;<sub>tot</sub>, were &#x003C3;<sub>tot</sub> is the total reaction cross section (i.e., &#x02211;&#x003C3;<sub><italic>i</italic></sub>), as measured in this work (see data in <xref ref-type="fig" rid="F3">Figures 3</xref>, <xref ref-type="fig" rid="F4">4</xref>) and &#x0003C; v&#x0003E; is the average relative velocity that can be estimated from the collision energy <italic>E</italic><sub><italic>CM</italic></sub> (see Ervin and Armentrout, <xref ref-type="bibr" rid="B18">1985</xref> and Nicolas et al., <xref ref-type="bibr" rid="B32">2002</xref> for a more detailed treatment). While the total rate constants do not change (within the error bars) when increasing the amount of internal excitation of the <inline-formula><mml:math id="M102"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> cation (compare the values at different photon energies but same <italic>E</italic><sub><italic>ave</italic></sub>), a slight change in the BRs is observed when increasing the collision energy, which favors the production of <inline-formula><mml:math id="M103"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (and <inline-formula><mml:math id="M104"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>) over that of DOCO<sup>&#x0002B;</sup>.</p>
<table-wrap position="float" id="T2">
<label>Table 2</label>
<caption><p>Energy-dependent rate constants and branching ratios (BRs) for the title reaction measured in the DC mode at two different values of photon energies (<italic>E</italic><sub><italic>phot</italic></sub>) and average collision energies (<italic>E</italic><sub><italic>ave</italic></sub>).</p></caption>
<table frame="hsides" rules="groups">
<thead>
<tr>
<th/>
<th valign="top" align="center" colspan="2" style="border-bottom: thin solid #000000;"><bold><italic>E<sub>phot</sub></italic> &#x0003D; 13.78 eV</bold></th>
<th valign="top" align="center" colspan="2" style="border-bottom: thin solid #000000;"><bold><italic>E<sub>phot</sub></italic> &#x0003D; 16.48 eV</bold></th>
</tr>
<tr>
<th/>
<th valign="top" align="center"><bold><italic>E<sub><bold><italic>ave</italic></bold></sub></italic> &#x0003D; 0.1 eV</bold></th>
<th valign="top" align="center"><bold><italic>E<sub><bold><italic>ave</italic></bold></sub></italic> &#x0003D; 1.9 eV</bold></th>
<th valign="top" align="center"><bold><italic>E<sub><bold><italic>ave</italic></bold></sub></italic> &#x0003D; 0.1 eV</bold></th>
<th valign="top" align="center"><bold><italic>E<sub><bold><italic>ave</italic></bold></sub></italic> &#x0003D; 1.7 eV</bold></th>
</tr>
</thead>
<tbody>
<tr>
<td valign="top" align="left"><italic>k<sub><italic>tot</italic></sub></italic>(<italic>E<sub><italic>ave</italic></sub></italic>)<xref ref-type="table-fn" rid="TN3"><sup>a</sup></xref></td>
<td valign="top" align="center">(1.8 &#x000B1; 0.5) &#x000D7; 10<sup>&#x02212;9</sup></td>
<td valign="top" align="center">(4.9 &#x000B1; 1.5) &#x000D7; 10<sup>&#x02212;9</sup></td>
<td valign="top" align="center">(1.8 &#x000B1; 0.5) &#x000D7; 10<sup>&#x02212;9</sup></td>
<td valign="top" align="center">(4.7 &#x000B1; 1.4) &#x000D7; 10<sup>&#x02212;9</sup></td>
</tr>
<tr>
<td/>
<td valign="top" align="center" colspan="4"><bold>Branching ratios (BRs)</bold></td>
</tr>
<tr>
<td valign="top" align="left"><inline-formula><mml:math id="M105"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula></td>
<td valign="top" align="center">0.63 &#x000B1; 0.06</td>
<td valign="top" align="center">0.82 &#x000B1; 0.08</td>
<td valign="top" align="center">0.62 &#x000B1; 0.06</td>
<td valign="top" align="center">0.84 &#x000B1; 0.08</td>
</tr>
<tr>
<td valign="top" align="left">DOCO<sup>&#x0002B;</sup></td>
<td valign="top" align="center">0.36 &#x000B1; 0.04</td>
<td valign="top" align="center">0.08 &#x000B1; 0.008</td>
<td valign="top" align="center">0.36 &#x000B1; 0.036</td>
<td valign="top" align="center">0.10 &#x000B1; 0.009</td>
</tr>
<tr>
<td valign="top" align="left"><inline-formula><mml:math id="M106"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula></td>
<td valign="top" align="center">(8.9 &#x000B1; 0.9) &#x000D7; 10<sup>&#x02212;3</sup></td>
<td valign="top" align="center">0.10 &#x000B1; 0.01</td>
<td valign="top" align="center">(2.0 &#x000B1; 0.2) &#x000D7; 10<sup>&#x02212;2</sup></td>
<td valign="top" align="center">(6.4 &#x000B1; 0.6) &#x000D7; 10<sup>&#x02212;2</sup></td>
</tr>
<tr>
<td valign="top" align="left">CD<sub>3</sub><inline-formula><mml:math id="M107"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula></td>
<td valign="top" align="center">n.d.</td>
<td valign="top" align="center">n.d.</td>
<td valign="top" align="center">&#x0003C;10<sup>&#x02212;3</sup></td>
<td valign="top" align="center">&#x0003C;10<sup>&#x02212;4</sup></td>
</tr>
</tbody>
</table>
<table-wrap-foot>
<fn id="TN3">
<label>a</label>
<p><italic>Total (i.e., summed over all the product channels) rate constant (in cm<sup>3</sup>&#x000B7;molecule<sup>-1</sup>&#x000B7;s<sup>-1</sup>) at the specified average collision energy E<sub>ave</sub>, estimated as detailed in the text</italic>.</p></fn>
</table-wrap-foot>
</table-wrap>
<fig id="F4" position="float">
<label>Figure 4</label>
<caption><p>Reactive cross sections for products <inline-formula><mml:math id="M108"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (uncorrected, black circles), DOCO<sup>&#x0002B;</sup> (red squares), <inline-formula><mml:math id="M109"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (green diamonds), and <inline-formula><mml:math id="M110"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (blue triangles) measured as a function of the vibrational excitation of the <inline-formula><mml:math id="M111"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> reagent (<italic>E</italic><sub><italic>INT</italic></sub>) at a fixed collision energy <italic>E</italic><sub><italic>CM</italic></sub> &#x0003D; 0.17 &#x000B1; 0.02 eV. The open circles are the <inline-formula><mml:math id="M112"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> cross sections corrected for the contribution of secondary reactions leading to <inline-formula><mml:math id="M113"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>. Lines connecting points are only a guide for the eyes.</p></caption>
<graphic xlink:href="fchem-07-00537-g0004.tif"/>
</fig>
<p>Interestingly, our results for the branching ratios (see <xref ref-type="table" rid="T2">Table 2</xref>) show reaction (1) to be the dominant channel at all the explored collision energies, in net disagreement with some of the existing values for the branching ratios (see <xref ref-type="table" rid="T1">Table 1</xref>). As already mentioned, in fact, in the literature there is a spread of the branching ratios for reaction (1) and (2) ranging from 1:0 (Durup-Ferguson et al., <xref ref-type="bibr" rid="B17">1983</xref>) to 0.6:0.4 (Smith et al., <xref ref-type="bibr" rid="B37">1978</xref>), to 0.5:0.5 (Copp et al., <xref ref-type="bibr" rid="B14">1982</xref>), to 0.28:0.72 (Tsuji et al., <xref ref-type="bibr" rid="B42">1994</xref>) and 0.25:0.75 (Huntress et al., <xref ref-type="bibr" rid="B24">1980</xref>), and finally to 0:1 (Harrison and Myher, <xref ref-type="bibr" rid="B21">1967</xref>; Rakshit and Warneck, <xref ref-type="bibr" rid="B33">1980</xref>). We provide here some explanations for the differences observed between our experiment and previous ones:</p>
<p>1. In addition to working with CD<sub>4</sub>, in our experiment we perform a mass selection of the parent ion before reaction. In this way, we eliminate the contribution due to the <sup>13</sup><inline-formula><mml:math id="M114"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> parent ion that appears at the same <italic>m/z</italic> as the HOCO<sup>&#x0002B;</sup> product (from residual not fully deuterated methane) and represents &#x0007E;1% of the parent ion intensity. Additionally, our experimental procedure consists in measuring both parent and product ion yields first with the target gas in the collision cell, secondly with the target gas in the chamber. In this way, we correct for any contribution of &#x0201C;impurities&#x0201D; coming from the source at the same mass as the product (namely <sup>13</sup><inline-formula><mml:math id="M115"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>/HOCO<sup>&#x0002B;</sup>). In one of the earlier papers (Tsuji et al., <xref ref-type="bibr" rid="B42">1994</xref>), the experiment is performed without parent ion mass selection, and no correction for <sup>13</sup><inline-formula><mml:math id="M116"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> is mentioned. Hence the claimed HOCO<sup>&#x0002B;</sup> branching ratio (0.72) is most likely overestimated. In Durup-Ferguson et al. (<xref ref-type="bibr" rid="B17">1983</xref>), the parent ion mass selection is performed, although no indication is given about the mass resolution. In Rakshit and Warneck (<xref ref-type="bibr" rid="B33">1980</xref>), a mixing of <inline-formula><mml:math id="M117"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>, CO<sub>2</sub><inline-formula><mml:math id="M118"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> and H<sub>2</sub>O<sup>&#x0002B;</sup> parent ions are used. The values from Huntress et al. (<xref ref-type="bibr" rid="B24">1980</xref>) are given without any experimental details, for which a reference is given to an earlier paper (Huntress, <xref ref-type="bibr" rid="B23">1977</xref>) where the ICR set-up is described. However, the earlier paper does not contain data for the title reaction, and it is impossible to infer whether and how the <sup>13</sup><inline-formula><mml:math id="M119"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> contribution was taken into account.</p>
<p>2. In our experiment, we keep the target gas pressure as low as possible to limit the number of secondary reactions. Some of the earlier works (Harrison and Myher, <xref ref-type="bibr" rid="B21">1967</xref>; Kasper and Franklin, <xref ref-type="bibr" rid="B25">1972</xref>; Tsuji et al., <xref ref-type="bibr" rid="B42">1994</xref>) have a pressure in the reaction cell higher than ours by a factor 30-50, with about the same cell length. Such differences may lead to underestimating the BR for <inline-formula><mml:math id="M120"><mml:msubsup><mml:mrow><mml:mtext>CH</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> if secondary reactions are not adequately accounted for (as done in our study).</p>
<p>3. In our experiment, we use a pure target gas, while some of the earlier works perform mass spectrometry studies in mixtures of gases. If some CO<sub>2</sub> is present in the region where <inline-formula><mml:math id="M121"><mml:msubsup><mml:mrow><mml:mtext>CH</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> products are generated by the <inline-formula><mml:math id="M122"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> &#x0002B; CH<sub>4</sub> reaction, the <inline-formula><mml:math id="M123"><mml:msubsup><mml:mrow><mml:mtext>CH</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> will be easily consumed by the efficient reaction <inline-formula><mml:math id="M124"><mml:msubsup><mml:mrow><mml:mtext>CH</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> &#x0002B; CO<sub>2</sub> &#x02192; HOCO<sup>&#x0002B;</sup> &#x0002B; CH<sub>3</sub> (<italic>k</italic> &#x0003D; 1.2 &#x000D7; 10<sup>&#x02212;9</sup> cm<sup>3</sup>&#x000B7;molecule<sup>&#x02212;1</sup>&#x000B7;s<sup>&#x02212;1</sup>) that will produce HOCO<sup>&#x0002B;</sup>, leading to a negative bias in the <inline-formula><mml:math id="M125"><mml:msubsup><mml:mrow><mml:mtext>CH</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>/HOCO<sup>&#x0002B;</sup> ratio. This is an issue in Rakshit and Warneck (<xref ref-type="bibr" rid="B33">1980</xref>) as highlighted by Copp et al. (<xref ref-type="bibr" rid="B14">1982</xref>), where CO<sub>2</sub> is present in the reaction cell, as well as in Ryan and Harland (<xref ref-type="bibr" rid="B35">1974</xref>), where mixing of CH4 and CO<sub>2</sub> occurs in the reaction region, in Tsuji et al. (<xref ref-type="bibr" rid="B42">1994</xref>), Harrison and Myher (<xref ref-type="bibr" rid="B21">1967</xref>) and Kasper and Franklin (<xref ref-type="bibr" rid="B25">1972</xref>).</p>
<p>4. In our experiments we mass select ionic products. Hence we can directly give BRs among different channels. In some of the flow/drift tube experiments, the reaction rate constants are measured by observing the decline of the primary ion signal upon addition of the neutral gas. For instance, in Durup-Ferguson et al. (<xref ref-type="bibr" rid="B17">1983</xref>) no mention is made about the mass detection of products, as if the authors have assumed the exclusive formation of <inline-formula><mml:math id="M126"><mml:msubsup><mml:mrow><mml:mtext>CH</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> via non-dissociative CT, not considering the possibility that HOCO<sup>&#x0002B;</sup> might be produced.</p>
</sec>
<sec>
<title>Results in the TPEPICO Mode</title>
<p>In the TPEPICO mode, we recorded cross sections for the reaction of <inline-formula><mml:math id="M127"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> ions in the (0,0,0) ground state and in two vibrationally excited states: (0,1,0) with one quantum of bending vibration and [(1,0,0) &#x0002B; (0,0,1)] corresponding to a combination of the symmetric and antisymmetric stretching vibration. Cross sections were measured for products <inline-formula><mml:math id="M128"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>, DOCO<sup>&#x0002B;</sup> and <inline-formula><mml:math id="M129"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> as well as <inline-formula><mml:math id="M130"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (from secondary reactions of the primary <inline-formula><mml:math id="M131"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> products, see above). The ion yield for product CD<sub>3</sub><inline-formula><mml:math id="M132"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> was too low to be detectable in coincidence. For most of the other products, reactive cross sections were measured at two different collision energies <italic>E</italic><sub><italic>CM</italic></sub> &#x0003D; 0.17 &#x000B1; 0.02 eV and 1.34 &#x000B1; 0.01 eV and results are shown in <xref ref-type="fig" rid="F4">Figures 4</xref>, <xref ref-type="fig" rid="F5">5</xref>. Despite the larger uncertainties (due to the low S/N ratio in the coincidence mode) cross section measurements are consistent with results obtained in the DC mode. In particular, when converting cross sections reported in <xref ref-type="fig" rid="F4">Figure 4</xref> for <inline-formula><mml:math id="M133"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> at low collision energy and in the (0,0,0) ground state we obtain the following BRs: <inline-formula><mml:math id="M134"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (0.75 &#x000B1; 0.25), DOCO<sup>&#x0002B;</sup> (0.25 &#x000B1; 0.11) and <inline-formula><mml:math id="M135"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (0.00 &#x000B1; 0.03), entirely consistent, within the error bars, with the data obtained in the DC mode (see <xref ref-type="table" rid="T2">Table 2</xref>, second column from the left).</p>
<fig id="F5" position="float">
<label>Figure 5</label>
<caption><p>Reactive cross sections for products <inline-formula><mml:math id="M136"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (uncorrected, black circles), DOCO<sup>&#x0002B;</sup> (red squares), <inline-formula><mml:math id="M137"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (green diamonds), and <inline-formula><mml:math id="M138"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> (blue triangles) measured as a function of the vibrational excitation of the <inline-formula><mml:math id="M139"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> reagent (<italic>E</italic><sub><italic>INT</italic></sub>) at a fixed collision energy <italic>E</italic><sub><italic>CM</italic></sub> &#x0003D; 1.34 &#x000B1; 0.01 eV. The open circles are the <inline-formula><mml:math id="M140"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> cross sections corrected for the contribution of secondary reactions leading to <inline-formula><mml:math id="M141"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>.</p></caption>
<graphic xlink:href="fchem-07-00537-g0005.tif"/>
</fig>
<p>In addition, the TPEPICO results confirm that cross sections for the exothermic CT (1) and deuterium-atom-transfer (2) channels change very little with increasing vibrational excitation, and the increase is more evident in data taken at high collision energy (<xref ref-type="fig" rid="F5">Figure 5</xref>). Cross sections for the endothermic channel leading to <inline-formula><mml:math id="M142"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> increase with collision energy but they do not seem to depend strongly on the internal excitation of the ionic parent, at least for the low internal excitations here explored (i.e., maximum one quantum of vibrational excitation).</p>
<p>The observed small dependence of reactions (1) and (2) from <inline-formula><mml:math id="M143"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> vibrational excitation requires some consideration. First of all, we note that our result is in agreement with a previous study (Durup-Ferguson et al., <xref ref-type="bibr" rid="B17">1983</xref>) in which a drift tube technique is used, and the dependence of the reaction rate constant on the internal energy of the ions is examined by varying the mass of the buffer gas. Despite the limitations of the technique compared to our truly state-selection method, in Durup-Ferguson et al. (<xref ref-type="bibr" rid="B17">1983</xref>) the non-dissociative CT giving <inline-formula><mml:math id="M144"><mml:msubsup><mml:mrow><mml:mtext>CH</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> plus CO<sub>2</sub> is found to occur at near the collision rate and to have little energy dependence and no measurable vibrational dependence.</p>
<p>We also note that, differently from the CH<sub>4</sub> case, vibrational excitation of <inline-formula><mml:math id="M145"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> ions was found to enhance the CT reaction probability with O<sub>2</sub> (Durup-Ferguson et al., <xref ref-type="bibr" rid="B17">1983</xref>; Ferguson et al., <xref ref-type="bibr" rid="B19">1992</xref>; Viggiano and Morris, <xref ref-type="bibr" rid="B43">1996</xref>; Nicolas et al., <xref ref-type="bibr" rid="B32">2002</xref>). To rationalize such results, it should be considered that the two systems present several differences:</p>
<list list-type="bullet">
<list-item><p>CT channels have different exothermicities (&#x02212;1.17 eV for CH<sub>4</sub> and &#x02212;1.71 for O<sub>2</sub>).</p></list-item>
<list-item><p>The CT rate constant is substantially larger for CH<sub>4</sub> (<italic>k</italic> &#x0003D; 0.3&#x02013;1 &#x000D7; 10<sup>&#x02212;9</sup> cm<sup>3</sup>&#x000B7;molecule<sup>&#x02212;1</sup>&#x000B7;s<sup>&#x02212;1</sup>, see values in our <xref ref-type="table" rid="T1">Table 1</xref>) than for O<sub>2</sub> (<italic>k</italic> &#x0007E; 5 &#x000D7; 10<sup>&#x02212;11</sup> cm<sup>3</sup>&#x000B7;molecule<sup>&#x02212;1</sup>&#x000B7;s<sup>&#x02212;1</sup>).</p></list-item>
</list>
<p>The inefficiency of the CT with O<sub>2</sub> is attributed to the non-resonant character of the reaction, i.e., to the fact that Franck-Condon factors for O<sub>2</sub> ionization at the ionization potential of CO<sub>2</sub> (13.78 eV) are close to zero (see for instance Wacks, <xref ref-type="bibr" rid="B44">1964</xref>). On the other hand, it is known that for CH<sub>4</sub> the Franck-Condon factors are low at the ionization threshold and increase reaching a maximum in the region 13.5&#x02013;14.5 eV (see for instance Stockbauer and Inghram, <xref ref-type="bibr" rid="B40">1971</xref>). Thus, while in the CH<sub>4</sub> case CT can occur efficiently at long range via the direct mechanism previously described, for O<sub>2</sub> it should involve the formation of a collision complex. As tentatively explained and demonstrated in Ferguson et al. (<xref ref-type="bibr" rid="B19">1992</xref>), in the O<sub>2</sub> case a small amount in the stretching excitation of <inline-formula><mml:math id="M146"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> can lead to an increase in the CT probability. Hence, CH<sub>4</sub> and O<sub>2</sub> are quite different reaction systems, and in the latter case, the effect of <inline-formula><mml:math id="M147"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> excitation could be more pronounced than for a reaction already at the Langevin limit (as in CH<sub>4</sub>).</p>
<p>More generally, the dynamics of CT processes is regulated by crossings among entrance and exit potential energy surfaces. When such crossings are occurring at distances for which the probability of electron transfer from one adiabatic PES to the other is unfavorable, the CT cross section will be very small even for exothermic processes (according to the Landau-Zener model for CT probability). The fact that increasing the vibrational excitation of the cation does not increase the CT cross section can be related to the fact that the crossing probability does not change much when increasing the vibrational excitation of <inline-formula><mml:math id="M148"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>, even though the exothermicity increases. Unfortunately, modeling the dynamics occurring on a <inline-formula><mml:math id="M149"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>- CH<sub>4</sub> multidimensional potential energy surface which includes vibrational excitation of CH<sub>4</sub> is not an easy task, and it is beyond the scope of our paper. We hope that our results will stimulate theoreticians and experts in <italic>ab-initio</italic> calculations to use this system as a test bench for theory.</p>
</sec>
</sec>
<sec sec-type="conclusions" id="s5">
<title>Conclusions</title>
<p>The reactivity of <inline-formula><mml:math id="M150"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> with deuterated methane has been investigated experimentally by guided ion beam mass spectrometric techniques by changing either the kinetic energy of <inline-formula><mml:math id="M151"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> or its vibrational excitation (using synchrotron radiation in the VUV energy range to produce vibrationally excited reagent ions). The main products are <inline-formula><mml:math id="M152"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>, DOCO<sup>&#x0002B;</sup>, and <inline-formula><mml:math id="M153"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> and reactivity is found to depend on the reagent collision energy, but not so much on the vibrational excitation of <inline-formula><mml:math id="M154"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>.</p>
<p>An interesting issue is whether reaction rates and dynamics change or remain the same when CD<sub>4</sub> is replaced by CH<sub>4</sub>. We do not expect charge transfer cross sections to be affected by a strong kinetic isotope effect (KIE). On the other hand, one can foresee a kinetic isotope effect in the H/D atom transfer channel leading to HOCO<sup>&#x0002B;</sup>/DOCO<sup>&#x0002B;</sup>. In particular, according to the semi-classical theory of primary KIE a normal effect (i.e., k<sub>H</sub>/k<sub>D</sub> &#x0003E; 1) is expected in the transfer of an H/D atom due to the vibrational zero-point energy differences for each of the vibrational modes of the reactants and transition state. Despite the limited mass resolution in our experimental set-up, we have managed to perform some tests using CH<sub>4</sub> in the reaction cell and measuring BRs and cross sections at a fixed collision energy of 0.11 eV in the DC mode at a photon energy <italic>E</italic><sub><italic>phot</italic></sub> &#x0003D; 13.78 eV (i.e., same conditions of <xref ref-type="fig" rid="F2">Figure 2</xref>). Products are observed at <italic>m/z</italic> values corresponding to <inline-formula><mml:math id="M155"><mml:msubsup><mml:mrow><mml:mtext>CH</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>, <inline-formula><mml:math id="M156"><mml:msubsup><mml:mrow><mml:mtext>CH</mml:mtext></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>, and HOCO<sup>&#x0002B;</sup>. By correcting for secondary reactions (as detailed in the text) we obtain a BR of 0.74:0.26 &#x0003D; CH4<sup>&#x0002B;</sup>: HOCO<sup>&#x0002B;</sup> and a total cross section of 199 (&#x000B1;30%) &#x000C5;<sup>2</sup>, corresponding to an energy-dependent rate constant of (2.68 &#x000B1; 0.8) &#x000D7; 10<sup>&#x02212;9</sup> cm<sup>3</sup>&#x000B7;molecule<sup>&#x02212;1</sup>&#x000B7;s<sup>&#x02212;1</sup> to be compared with the CD<sub>4</sub> value of (1.8 &#x000B1; 0.5) &#x000D7; 10<sup>&#x02212;9</sup> at similar <italic>E</italic><sub><italic>ave</italic></sub> (see our results in <xref ref-type="table" rid="T2">Table 2</xref>) and the BR of 0.63:0.36 &#x0003D; <inline-formula><mml:math id="M157"><mml:msubsup><mml:mrow><mml:mtext>CD</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>: DOCO<sup>&#x0002B;</sup>. This means a positive KIE k<sub>H</sub>/k<sub>D</sub> &#x0003D; 1.5(&#x000B1;0.6). On the other hand, our results show that when CD<sub>4</sub> is replaced by the lighter isotopolog, the CT is more favored than the H atom transfer. This effect can be explained assuming that the different vibrational spacings in CD<sub>4</sub>/CH<sub>4</sub> might change the Franck-Condon factors and the efficiencies of non-adiabatic transition probability among the entrance and exit potential energy surfaces. We note that in a similar reacting system CN<sup>&#x0002B;</sup> plus CH<sub>4</sub>/CD<sub>4</sub> a KIE in the total rate coefficient similar to the one observed in our case has been reported, namely k<sub>H</sub>/k<sub>D</sub> &#x0003D; 1.55 (&#x000B1;0.66) (Raksit et al., <xref ref-type="bibr" rid="B34">1984</xref>).</p>
<p>To put our results into the context of plasma chemistry used for the conversion of CO<sub>2</sub> in carbon-neutral fuels (Snoeckx et al., <xref ref-type="bibr" rid="B38">2013</xref>; Snoeckx and Bogaerts, <xref ref-type="bibr" rid="B39">2017</xref>), both the products (<inline-formula><mml:math id="M158"><mml:msubsup><mml:mrow><mml:mtext>CH</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> and HOCO<sup>&#x0002B;</sup>) of the reaction of <inline-formula><mml:math id="M159"><mml:msubsup><mml:mrow><mml:mtext>CO</mml:mtext></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> with CH<sub>4</sub> eventually lead to the production of <inline-formula><mml:math id="M160"><mml:msubsup><mml:mrow><mml:mtext>CH</mml:mtext></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> and CH<sub>3</sub>, as shown in the following scheme:</p>
<p><graphic xlink:href="fchem-07-00537-e0001.tif"/></p>
<disp-formula id="E10"><label>(8)</label><mml:math id="M162"><mml:msubsup><mml:mtext>CH</mml:mtext><mml:mtext>4</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msubsup><mml:mtext>+&#x000A0;</mml:mtext><mml:msub><mml:mtext>CH</mml:mtext><mml:mtext>4</mml:mtext></mml:msub><mml:mo>&#x02192;</mml:mo><mml:msubsup><mml:mtext>CH</mml:mtext><mml:mtext>5</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msubsup><mml:msub><mml:mtext>+&#x000A0;CH</mml:mtext><mml:mtext>3</mml:mtext></mml:msub></mml:math></disp-formula>
<disp-formula id="E11"><label>(9)</label><mml:math id="M163"><mml:msubsup><mml:mtext>CH</mml:mtext><mml:mtext>4</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msubsup><mml:mtext>+&#x000A0;</mml:mtext><mml:msub><mml:mtext>CO</mml:mtext><mml:mtext>2</mml:mtext></mml:msub><mml:mo>&#x02192;</mml:mo><mml:msup><mml:mtext>HOCO</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msup><mml:mtext>+&#x000A0;</mml:mtext><mml:msub><mml:mtext>CH</mml:mtext><mml:mtext>3</mml:mtext></mml:msub></mml:math></disp-formula>
<disp-formula id="E12"><label>(10)</label><mml:math id="M164"><mml:msup><mml:mtext>HOCO</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msup><mml:mtext>+&#x000A0;</mml:mtext><mml:msub><mml:mtext>CH</mml:mtext><mml:mtext>4</mml:mtext></mml:msub><mml:mo>&#x02192;</mml:mo><mml:msubsup><mml:mtext>CH</mml:mtext><mml:mtext>5</mml:mtext><mml:mtext>&#x0002B;</mml:mtext></mml:msubsup><mml:mtext>+&#x000A0;</mml:mtext><mml:msub><mml:mtext>CO</mml:mtext><mml:mtext>2</mml:mtext></mml:msub></mml:math></disp-formula>
<p>Thus the energy initially used to ionize CO<sub>2</sub> is transferred to CH<sub>4</sub> to form <inline-formula><mml:math id="M165"><mml:msubsup><mml:mrow><mml:mtext>CH</mml:mtext></mml:mrow><mml:mrow><mml:mn>4</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula>, <inline-formula><mml:math id="M166"><mml:msubsup><mml:mrow><mml:mtext>CH</mml:mtext></mml:mrow><mml:mrow><mml:mn>5</mml:mn></mml:mrow><mml:mrow><mml:mo>&#x0002B;</mml:mo></mml:mrow></mml:msubsup></mml:math></inline-formula> and CH<sub>3</sub>. Only processes (2) and (9) lead to HOCO<sup>&#x0002B;</sup> that, in addition to react with CH<sub>4</sub>, giving back CO<sub>2</sub>, can also recombine with electrons to yield CO plus OH.</p>
</sec>
<sec sec-type="data-availability" id="s6">
<title>Data Availability</title>
<p>The datasets generated for this study are available on request to the corresponding author.</p>
</sec>
<sec id="s7">
<title>Author Contributions</title>
<p>DA, CA, and PT contributed conception and design of the study. CA, CR, and J&#x0017D; planned and developed the experimental set-up. DA, CR, CA, AL, J&#x0017D;, MP, and CS contributed to data acquisition, data analysis, and interpretation of results. DA wrote the first draft of the manuscript. DA, PT, and CA wrote sections of the manuscript. All authors contributed to manuscript revision, read and approved the submitted version.</p>
<sec>
<title>Conflict of Interest Statement</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>
</body>
<back>
<ack><p>We thank the DESIRS beamline team, L. Nahon, G. Garcia, N. De Oliveira, and J.-F. Gil, for assistance during the synchrotron measurements and the technical staff of SOLEIL for running the facility under projects n&#x000B0; 20140033 and 20150468. CA and CR acknowledge the synchrotron SOLEIL for the support to the associated CERISES setup since 2008 and subsistence expenses during beamtime periods. DA acknowledges financial support from the EU-TNA program during beamtime n&#x000B0; 20140033. J&#x0017D; and MP acknowledge support from the Czech Science Foundation project No. 17-14200S. DA and PT thanks the Department of Physics of the University of Trento for support.</p>
</ack>
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