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Experimental and Theoretical Studies of Reactions Between H Atoms and Carbanions of Interstellar Relevance
The recent detection of molecular anions in the interstellar medium (ISM) has highlighted the need for laboratory studies of negative ion chemistry. Hydrogen atoms are the most abundant atomic species in the ISM, and the chemistry of H atoms with anions may contribute to molecular synthesis in inter...
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Published in: | The Astrophysical journal 2010-11, Vol.723 (2), p.1325-1330 |
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description | The recent detection of molecular anions in the interstellar medium (ISM) has highlighted the need for laboratory studies of negative ion chemistry. Hydrogen atoms are the most abundant atomic species in the ISM, and the chemistry of H atoms with anions may contribute to molecular synthesis in interstellar clouds. This work is a combined experimental and computational study of a series of anions reacting with H atoms by associative detachment (A-- + H -> AH + e --). The anions include deprotonated nitriles (CH2CN--, CH3CHCN--, and (CH3)2CCN--), acetaldehyde (HC(O)CH2 --), acetone (CH3C(O)CH2 --), ethyl acetate (CH3CH2OC(O)CH2 --), methanol (CH3O--), and acetic acid (CH3CO2 --). Experimental measurements of the reaction rate constants were made with the flowing afterglow-selected ion flow tube technique. Ab initio theoretical calculations were carried out to explore the reaction mechanism and investigate the factors influencing reaction efficiencies, which are largely proportional to reaction exothermicities. Other factors influencing reaction efficiencies include the charge density on the reactive site of the anion, the characteristics of the potential energy surfaces along the approach of the reactants, and angular momentum conservation of the anion-H atom collision. |
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Hydrogen atoms are the most abundant atomic species in the ISM, and the chemistry of H atoms with anions may contribute to molecular synthesis in interstellar clouds. This work is a combined experimental and computational study of a series of anions reacting with H atoms by associative detachment (A-- + H -> AH + e --). The anions include deprotonated nitriles (CH2CN--, CH3CHCN--, and (CH3)2CCN--), acetaldehyde (HC(O)CH2 --), acetone (CH3C(O)CH2 --), ethyl acetate (CH3CH2OC(O)CH2 --), methanol (CH3O--), and acetic acid (CH3CO2 --). Experimental measurements of the reaction rate constants were made with the flowing afterglow-selected ion flow tube technique. Ab initio theoretical calculations were carried out to explore the reaction mechanism and investigate the factors influencing reaction efficiencies, which are largely proportional to reaction exothermicities. Other factors influencing reaction efficiencies include the charge density on the reactive site of the anion, the characteristics of the potential energy surfaces along the approach of the reactants, and angular momentum conservation of the anion-H atom collision.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1088/0004-637X/723/2/1325</identifier><identifier>CODEN: ASJOAB</identifier><language>eng</language><publisher>Bristol: IOP Publishing</publisher><subject>ACETALDEHYDE ; ACETATES ; ACETIC ACID ; ACETONE ; AFTERGLOW ; ALCOHOLS ; ALDEHYDES ; ANGULAR MOMENTUM ; ANIONS ; Astronomy ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; ATOM COLLISIONS ; CARBOXYLIC ACID SALTS ; CARBOXYLIC ACIDS ; CHARGE DENSITY ; CHARGED PARTICLES ; COLLISIONS ; Earth, ocean, space ; ELEMENTS ; ENERGY ; Exact sciences and technology ; HYDROGEN ; HYDROXY COMPOUNDS ; INTERSTELLAR GRAINS ; IONS ; KETONES ; KINETICS ; METHANOL ; MONOCARBOXYLIC ACIDS ; NITRILES ; NONMETALS ; ORGANIC ACIDS ; ORGANIC COMPOUNDS ; ORGANIC NITROGEN COMPOUNDS ; PARTICLES ; POTENTIAL ENERGY ; REACTION KINETICS</subject><ispartof>The Astrophysical journal, 2010-11, Vol.723 (2), p.1325-1330</ispartof><rights>2015 INIST-CNRS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a486t-78b10633b5b64156f191b950137426f0d63c9a9d5f3cd2bed8fda7b49d3186fc3</citedby><cites>FETCH-LOGICAL-a486t-78b10633b5b64156f191b950137426f0d63c9a9d5f3cd2bed8fda7b49d3186fc3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,27924,27925</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=23424440$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/21471257$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Yang, Zhibo</creatorcontrib><creatorcontrib>Eichelberger, Brian</creatorcontrib><creatorcontrib>Carpenter, Marshall Y</creatorcontrib><creatorcontrib>Martinez, Oscar</creatorcontrib><creatorcontrib>Snow, Theodore P</creatorcontrib><creatorcontrib>Bierbaum, Veronica M</creatorcontrib><title>Experimental and Theoretical Studies of Reactions Between H Atoms and Carbanions of Interstellar Relevance</title><title>The Astrophysical journal</title><description>The recent detection of molecular anions in the interstellar medium (ISM) has highlighted the need for laboratory studies of negative ion chemistry. Hydrogen atoms are the most abundant atomic species in the ISM, and the chemistry of H atoms with anions may contribute to molecular synthesis in interstellar clouds. This work is a combined experimental and computational study of a series of anions reacting with H atoms by associative detachment (A-- + H -> AH + e --). The anions include deprotonated nitriles (CH2CN--, CH3CHCN--, and (CH3)2CCN--), acetaldehyde (HC(O)CH2 --), acetone (CH3C(O)CH2 --), ethyl acetate (CH3CH2OC(O)CH2 --), methanol (CH3O--), and acetic acid (CH3CO2 --). Experimental measurements of the reaction rate constants were made with the flowing afterglow-selected ion flow tube technique. Ab initio theoretical calculations were carried out to explore the reaction mechanism and investigate the factors influencing reaction efficiencies, which are largely proportional to reaction exothermicities. Other factors influencing reaction efficiencies include the charge density on the reactive site of the anion, the characteristics of the potential energy surfaces along the approach of the reactants, and angular momentum conservation of the anion-H atom collision.</description><subject>ACETALDEHYDE</subject><subject>ACETATES</subject><subject>ACETIC ACID</subject><subject>ACETONE</subject><subject>AFTERGLOW</subject><subject>ALCOHOLS</subject><subject>ALDEHYDES</subject><subject>ANGULAR MOMENTUM</subject><subject>ANIONS</subject><subject>Astronomy</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>ATOM COLLISIONS</subject><subject>CARBOXYLIC ACID SALTS</subject><subject>CARBOXYLIC ACIDS</subject><subject>CHARGE DENSITY</subject><subject>CHARGED PARTICLES</subject><subject>COLLISIONS</subject><subject>Earth, ocean, space</subject><subject>ELEMENTS</subject><subject>ENERGY</subject><subject>Exact sciences and technology</subject><subject>HYDROGEN</subject><subject>HYDROXY COMPOUNDS</subject><subject>INTERSTELLAR GRAINS</subject><subject>IONS</subject><subject>KETONES</subject><subject>KINETICS</subject><subject>METHANOL</subject><subject>MONOCARBOXYLIC ACIDS</subject><subject>NITRILES</subject><subject>NONMETALS</subject><subject>ORGANIC ACIDS</subject><subject>ORGANIC COMPOUNDS</subject><subject>ORGANIC NITROGEN COMPOUNDS</subject><subject>PARTICLES</subject><subject>POTENTIAL ENERGY</subject><subject>REACTION KINETICS</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNp9kF1rFTEQhhex4LH1H3ixIOJFWTefm-xlPVRbKAhawbuQTSY0ZU-yJjla_73ZnnJuFK-GYZ53Znia5jVG7zGSskcIsW6g4nsvCO1Jjynhz5oN5lR2jHLxvNkckRfNy5zv15aM46a5v3xYIPkdhKLnVgfb3t5BTFC8qf3Xsrcechtd-wW0KT6G3H6A8gsgtFftRYm7_Bja6jTp8Diu7HUokHKBedapBmf4qYOBs-bE6TnDq6d62nz7eHm7vepuPn-63l7cdJrJoXRCThgNlE58Ghjmg8MjnkaOMBWMDA7ZgZpRj5Y7aiyZwEpntZjYaCmWgzP0tHlz2Btz8SobX8DcmRgCmKIIZgITLir17kAtKf7YQy5q57NZXw4Q91mNBAkpJOOVZAfSpJhzAqeWKkyn3wojtfpXq021ylXVvyJq9V9jb58O6FxdulQd-HzMEsoIYwxV7vzA-bgcp__aqBbrKt3_Tf_3jz9lRKDp</recordid><startdate>20101110</startdate><enddate>20101110</enddate><creator>Yang, Zhibo</creator><creator>Eichelberger, Brian</creator><creator>Carpenter, Marshall Y</creator><creator>Martinez, Oscar</creator><creator>Snow, Theodore P</creator><creator>Bierbaum, Veronica M</creator><general>IOP Publishing</general><general>IOP</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>OTOTI</scope></search><sort><creationdate>20101110</creationdate><title>Experimental and Theoretical Studies of Reactions Between H Atoms and Carbanions of Interstellar Relevance</title><author>Yang, Zhibo ; Eichelberger, Brian ; Carpenter, Marshall Y ; Martinez, Oscar ; Snow, Theodore P ; Bierbaum, Veronica M</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a486t-78b10633b5b64156f191b950137426f0d63c9a9d5f3cd2bed8fda7b49d3186fc3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>ACETALDEHYDE</topic><topic>ACETATES</topic><topic>ACETIC ACID</topic><topic>ACETONE</topic><topic>AFTERGLOW</topic><topic>ALCOHOLS</topic><topic>ALDEHYDES</topic><topic>ANGULAR MOMENTUM</topic><topic>ANIONS</topic><topic>Astronomy</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>ATOM COLLISIONS</topic><topic>CARBOXYLIC ACID SALTS</topic><topic>CARBOXYLIC ACIDS</topic><topic>CHARGE DENSITY</topic><topic>CHARGED PARTICLES</topic><topic>COLLISIONS</topic><topic>Earth, ocean, space</topic><topic>ELEMENTS</topic><topic>ENERGY</topic><topic>Exact sciences and technology</topic><topic>HYDROGEN</topic><topic>HYDROXY COMPOUNDS</topic><topic>INTERSTELLAR GRAINS</topic><topic>IONS</topic><topic>KETONES</topic><topic>KINETICS</topic><topic>METHANOL</topic><topic>MONOCARBOXYLIC ACIDS</topic><topic>NITRILES</topic><topic>NONMETALS</topic><topic>ORGANIC ACIDS</topic><topic>ORGANIC COMPOUNDS</topic><topic>ORGANIC NITROGEN COMPOUNDS</topic><topic>PARTICLES</topic><topic>POTENTIAL ENERGY</topic><topic>REACTION KINETICS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Yang, Zhibo</creatorcontrib><creatorcontrib>Eichelberger, Brian</creatorcontrib><creatorcontrib>Carpenter, Marshall Y</creatorcontrib><creatorcontrib>Martinez, Oscar</creatorcontrib><creatorcontrib>Snow, Theodore P</creatorcontrib><creatorcontrib>Bierbaum, Veronica M</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Yang, Zhibo</au><au>Eichelberger, Brian</au><au>Carpenter, Marshall Y</au><au>Martinez, Oscar</au><au>Snow, Theodore P</au><au>Bierbaum, Veronica M</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Experimental and Theoretical Studies of Reactions Between H Atoms and Carbanions of Interstellar Relevance</atitle><jtitle>The Astrophysical journal</jtitle><date>2010-11-10</date><risdate>2010</risdate><volume>723</volume><issue>2</issue><spage>1325</spage><epage>1330</epage><pages>1325-1330</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><coden>ASJOAB</coden><abstract>The recent detection of molecular anions in the interstellar medium (ISM) has highlighted the need for laboratory studies of negative ion chemistry. Hydrogen atoms are the most abundant atomic species in the ISM, and the chemistry of H atoms with anions may contribute to molecular synthesis in interstellar clouds. This work is a combined experimental and computational study of a series of anions reacting with H atoms by associative detachment (A-- + H -> AH + e --). The anions include deprotonated nitriles (CH2CN--, CH3CHCN--, and (CH3)2CCN--), acetaldehyde (HC(O)CH2 --), acetone (CH3C(O)CH2 --), ethyl acetate (CH3CH2OC(O)CH2 --), methanol (CH3O--), and acetic acid (CH3CO2 --). Experimental measurements of the reaction rate constants were made with the flowing afterglow-selected ion flow tube technique. Ab initio theoretical calculations were carried out to explore the reaction mechanism and investigate the factors influencing reaction efficiencies, which are largely proportional to reaction exothermicities. Other factors influencing reaction efficiencies include the charge density on the reactive site of the anion, the characteristics of the potential energy surfaces along the approach of the reactants, and angular momentum conservation of the anion-H atom collision.</abstract><cop>Bristol</cop><pub>IOP Publishing</pub><doi>10.1088/0004-637X/723/2/1325</doi><tpages>6</tpages><oa>free_for_read</oa></addata></record> |
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subjects | ACETALDEHYDE ACETATES ACETIC ACID ACETONE AFTERGLOW ALCOHOLS ALDEHYDES ANGULAR MOMENTUM ANIONS Astronomy ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ATOM COLLISIONS CARBOXYLIC ACID SALTS CARBOXYLIC ACIDS CHARGE DENSITY CHARGED PARTICLES COLLISIONS Earth, ocean, space ELEMENTS ENERGY Exact sciences and technology HYDROGEN HYDROXY COMPOUNDS INTERSTELLAR GRAINS IONS KETONES KINETICS METHANOL MONOCARBOXYLIC ACIDS NITRILES NONMETALS ORGANIC ACIDS ORGANIC COMPOUNDS ORGANIC NITROGEN COMPOUNDS PARTICLES POTENTIAL ENERGY REACTION KINETICS |
title | Experimental and Theoretical Studies of Reactions Between H Atoms and Carbanions of Interstellar Relevance |
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