Thermally Initiated Formation of Criegee Intermediate CH 2 OO in the Oxidation of Ethane
Criegee intermediates (CIs) play an important role in atmospheric chemistry as a transient source of the OH radical through their formation by the ozonolysis of unsaturated organic compounds. Here, we report thermally initiated formation of the smallest CI (CH OO) in the oxidation of ethane (CH CH )...
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Veröffentlicht in: | The journal of physical chemistry letters 2024-12, Vol.15 (50), p.12441-12448 |
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creator | Saragi, Rizalina T Seifert, Nathan A Sivaramakrishnan, Raghu Prozument, Kirill |
description | Criegee intermediates (CIs) play an important role in atmospheric chemistry as a transient source of the OH radical through their formation by the ozonolysis of unsaturated organic compounds. Here, we report thermally initiated formation of the smallest CI (CH
OO) in the oxidation of ethane (CH
CH
) that may be relevant to combustion and flames. The SiO
/SiC oxidation microreactor is heated to 1800 K and has a short residence time of ∼100 μs. The CH
OO we observe is likely formed in a lower-temperature region near the microreactor's exit. Plausible mechanisms for CH
OO formation and retention under these conditions mediated by methylperoxy (CH
OO) radicals are discussed. Pure rotational spectra of CH
OO and other intermediates (HO
, CH
CHO, CH
CHOH,
CH
OCH
, CH
CH
CHO, CH
OOH, and HCOOH) are detected with a chirped-pulse Fourier transform millimeter-wave spectrometer operating in the frequency range of 60-90 GHz. Detection occurs in a molecular beam, where the species are supersonically cooled to 5 K. |
doi_str_mv | 10.1021/acs.jpclett.4c02445 |
format | Article |
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OO) in the oxidation of ethane (CH
CH
) that may be relevant to combustion and flames. The SiO
/SiC oxidation microreactor is heated to 1800 K and has a short residence time of ∼100 μs. The CH
OO we observe is likely formed in a lower-temperature region near the microreactor's exit. Plausible mechanisms for CH
OO formation and retention under these conditions mediated by methylperoxy (CH
OO) radicals are discussed. Pure rotational spectra of CH
OO and other intermediates (HO
, CH
CHO, CH
CHOH,
CH
OCH
, CH
CH
CHO, CH
OOH, and HCOOH) are detected with a chirped-pulse Fourier transform millimeter-wave spectrometer operating in the frequency range of 60-90 GHz. Detection occurs in a molecular beam, where the species are supersonically cooled to 5 K.</description><identifier>ISSN: 1948-7185</identifier><identifier>EISSN: 1948-7185</identifier><identifier>DOI: 10.1021/acs.jpclett.4c02445</identifier><identifier>PMID: 39663998</identifier><language>eng</language><publisher>United States</publisher><ispartof>The journal of physical chemistry letters, 2024-12, Vol.15 (50), p.12441-12448</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c678-33bc601947ccc68da1ba4a9cfad3d189e7406b737ce4d238570aa3f7984264dd3</cites><orcidid>0000-0002-1867-1254 ; 0000-0003-4472-357X ; 0000-0003-3045-8429</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,2752,27901,27902</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/39663998$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Saragi, Rizalina T</creatorcontrib><creatorcontrib>Seifert, Nathan A</creatorcontrib><creatorcontrib>Sivaramakrishnan, Raghu</creatorcontrib><creatorcontrib>Prozument, Kirill</creatorcontrib><title>Thermally Initiated Formation of Criegee Intermediate CH 2 OO in the Oxidation of Ethane</title><title>The journal of physical chemistry letters</title><addtitle>J Phys Chem Lett</addtitle><description>Criegee intermediates (CIs) play an important role in atmospheric chemistry as a transient source of the OH radical through their formation by the ozonolysis of unsaturated organic compounds. Here, we report thermally initiated formation of the smallest CI (CH
OO) in the oxidation of ethane (CH
CH
) that may be relevant to combustion and flames. The SiO
/SiC oxidation microreactor is heated to 1800 K and has a short residence time of ∼100 μs. The CH
OO we observe is likely formed in a lower-temperature region near the microreactor's exit. Plausible mechanisms for CH
OO formation and retention under these conditions mediated by methylperoxy (CH
OO) radicals are discussed. Pure rotational spectra of CH
OO and other intermediates (HO
, CH
CHO, CH
CHOH,
CH
OCH
, CH
CH
CHO, CH
OOH, and HCOOH) are detected with a chirped-pulse Fourier transform millimeter-wave spectrometer operating in the frequency range of 60-90 GHz. Detection occurs in a molecular beam, where the species are supersonically cooled to 5 K.</description><issn>1948-7185</issn><issn>1948-7185</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><recordid>eNpNkM1qwzAMgM3YWLtuTzAYfoF0duz45zhC_6CQSw-7BcdWFpc0KYkH69vPpV3ZSULSJ6QPoVdK5pSk9N3Ycb4_2hZCmHNLUs6zOzSlmqtEUpXd_8sn6Gkc94QITZR8RBOmhWBaqyn63DUwHEzbnvCm88GbAA4v-1gKvu9wX-N88PAFENshToI7j-B8jVNcFNh3ODSAix_vbsAiNKaDZ_RQm3aEl2ucod1yscvXybZYbfKPbWKFVAljlRUk3imttUI5QyvDjba1ccxRpUFyIirJpAXuUqYySYxhtdSKp4I7x2aIXdbaoR_HAeryOPiDGU4lJeVZUxk1lVdN5VVTpN4u1PG7ii_dmD8v7BcbbGa5</recordid><startdate>20241219</startdate><enddate>20241219</enddate><creator>Saragi, Rizalina T</creator><creator>Seifert, Nathan A</creator><creator>Sivaramakrishnan, Raghu</creator><creator>Prozument, Kirill</creator><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><orcidid>https://orcid.org/0000-0002-1867-1254</orcidid><orcidid>https://orcid.org/0000-0003-4472-357X</orcidid><orcidid>https://orcid.org/0000-0003-3045-8429</orcidid></search><sort><creationdate>20241219</creationdate><title>Thermally Initiated Formation of Criegee Intermediate CH 2 OO in the Oxidation of Ethane</title><author>Saragi, Rizalina T ; Seifert, Nathan A ; Sivaramakrishnan, Raghu ; Prozument, Kirill</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c678-33bc601947ccc68da1ba4a9cfad3d189e7406b737ce4d238570aa3f7984264dd3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Saragi, Rizalina T</creatorcontrib><creatorcontrib>Seifert, Nathan A</creatorcontrib><creatorcontrib>Sivaramakrishnan, Raghu</creatorcontrib><creatorcontrib>Prozument, Kirill</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><jtitle>The journal of physical chemistry letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Saragi, Rizalina T</au><au>Seifert, Nathan A</au><au>Sivaramakrishnan, Raghu</au><au>Prozument, Kirill</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Thermally Initiated Formation of Criegee Intermediate CH 2 OO in the Oxidation of Ethane</atitle><jtitle>The journal of physical chemistry letters</jtitle><addtitle>J Phys Chem Lett</addtitle><date>2024-12-19</date><risdate>2024</risdate><volume>15</volume><issue>50</issue><spage>12441</spage><epage>12448</epage><pages>12441-12448</pages><issn>1948-7185</issn><eissn>1948-7185</eissn><abstract>Criegee intermediates (CIs) play an important role in atmospheric chemistry as a transient source of the OH radical through their formation by the ozonolysis of unsaturated organic compounds. Here, we report thermally initiated formation of the smallest CI (CH
OO) in the oxidation of ethane (CH
CH
) that may be relevant to combustion and flames. The SiO
/SiC oxidation microreactor is heated to 1800 K and has a short residence time of ∼100 μs. The CH
OO we observe is likely formed in a lower-temperature region near the microreactor's exit. Plausible mechanisms for CH
OO formation and retention under these conditions mediated by methylperoxy (CH
OO) radicals are discussed. Pure rotational spectra of CH
OO and other intermediates (HO
, CH
CHO, CH
CHOH,
CH
OCH
, CH
CH
CHO, CH
OOH, and HCOOH) are detected with a chirped-pulse Fourier transform millimeter-wave spectrometer operating in the frequency range of 60-90 GHz. Detection occurs in a molecular beam, where the species are supersonically cooled to 5 K.</abstract><cop>United States</cop><pmid>39663998</pmid><doi>10.1021/acs.jpclett.4c02445</doi><tpages>8</tpages><orcidid>https://orcid.org/0000-0002-1867-1254</orcidid><orcidid>https://orcid.org/0000-0003-4472-357X</orcidid><orcidid>https://orcid.org/0000-0003-3045-8429</orcidid></addata></record> |
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title | Thermally Initiated Formation of Criegee Intermediate CH 2 OO in the Oxidation of Ethane |
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