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Combined experimental and computational study of the reactivity of the methanimine radical cation (H<sub>2</sub>CNH<SUP>•</SUP><SUP>+</SUP>) and its isomer aminomethylene (HCNH<sub>2</sub><SUP>•</SUP><SUP>+</SUP>) with propene (CH<sub>3</sub>CHCH<sub>2</sub>)

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61388955%3A_____%2F24%3A00598166" target="_blank" >RIV/61388955:_____/24:00598166 - isvavai.cz</a>

  • Result on the web

    <a href="https://hdl.handle.net/11104/0355902" target="_blank" >https://hdl.handle.net/11104/0355902</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1039/d4cp02002b" target="_blank" >10.1039/d4cp02002b</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Combined experimental and computational study of the reactivity of the methanimine radical cation (H<sub>2</sub>CNH<SUP>•</SUP><SUP>+</SUP>) and its isomer aminomethylene (HCNH<sub>2</sub><SUP>•</SUP><SUP>+</SUP>) with propene (CH<sub>3</sub>CHCH<sub>2</sub>)

  • Original language description

    The gas phase reactivity of the radical cation isomers H2CNH˙+ (methanimine) and HCNH2˙+ (aminomethylene) with propene (CH3CHCH2) has been investigated by measuring absolute reactive cross sections and product branching ratios, under single collision conditions, as a function of collision energy (in the range ∼0.07-11.80 eV) using guided ion beam mass spectrometry coupled with VUV photoionization for selective isomer generation. Experimental results have been merged with theoretical calculations to elucidate reaction pathways and structures of products. The H2CNH˙+ isomer is over a factor two more reactive than HCNH2˙+. A major channel from both isomers is production of protonated methanimine CH2NH2+via hydrogen-atom transfer reaction but, while H2CNH˙+ additionally gives charge and proton transfer products, the HCNH2˙+ isomer leads instead to protonated vinylimine CH2CHCHNH2+, produced alongside CH3˙ radicals. The reactions have astrochemical implications in the build up of chemical complexity in both the interstellar medium and the hydrocarbon-rich atmospheres of planets and satellites. © 2024 The Royal Society of Chemistry.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10403 - Physical chemistry

Result continuities

  • Project

    <a href="/en/project/LTC20062" target="_blank" >LTC20062: Reactivity of negative ions in the gas phase</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2024

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Physical Chemistry Chemical Physics

  • ISSN

    1463-9076

  • e-ISSN

    1463-9084

  • Volume of the periodical

    26

  • Issue of the periodical within the volume

    35

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    13

  • Pages from-to

    22990-23002

  • UT code for WoS article

    001296108800001

  • EID of the result in the Scopus database

    2-s2.0-85201871658