TY - JOUR
T1 - H2 roaming chemistry and the formation of H3+ from organic molecules in strong laser fields
AU - Ekanayake, Nagitha
AU - Severt, Travis
AU - Nairat, Muath
AU - Weingartz, Nicholas P.
AU - Farris, Benjamin M.
AU - Kaderiya, Balram
AU - Feizollah, Peyman
AU - Jochim, Bethany
AU - Ziaee, Farzaneh
AU - Borne, Kurtis
AU - Raju P, Kanaka
AU - Carnes, Kevin D.
AU - Rolles, Daniel
AU - Rudenko, Artem
AU - Levine, Benjamin G.
AU - Jackson, James E.
AU - Ben-Itzhak, Itzik
AU - Dantus, Marcos
N1 - Publisher Copyright:
© 2018, The Author(s).
PY - 2018/12/1
Y1 - 2018/12/1
N2 - Roaming mechanisms, involving the brief generation of a neutral atom or molecule that stays in the vicinity before reacting with the remaining atoms of the precursor, are providing valuable insights into previously unexplained chemical reactions. Here, the mechanistic details and femtosecond time-resolved dynamics of H3+ formation from a series of alcohols with varying primary carbon chain lengths are obtained through a combination of strong-field laser excitation studies and ab initio molecular dynamics calculations. For small alcohols, four distinct pathways involving hydrogen migration and H2 roaming prior to H3+ formation are uncovered. Despite the increased number of hydrogens and possible combinations leading to H3+ formation, the yield decreases as the carbon chain length increases. The fundamental mechanistic findings presented here explore the formation of H3+, the most important ion in interstellar chemistry, through H2 roaming occurring in ionic species.
AB - Roaming mechanisms, involving the brief generation of a neutral atom or molecule that stays in the vicinity before reacting with the remaining atoms of the precursor, are providing valuable insights into previously unexplained chemical reactions. Here, the mechanistic details and femtosecond time-resolved dynamics of H3+ formation from a series of alcohols with varying primary carbon chain lengths are obtained through a combination of strong-field laser excitation studies and ab initio molecular dynamics calculations. For small alcohols, four distinct pathways involving hydrogen migration and H2 roaming prior to H3+ formation are uncovered. Despite the increased number of hydrogens and possible combinations leading to H3+ formation, the yield decreases as the carbon chain length increases. The fundamental mechanistic findings presented here explore the formation of H3+, the most important ion in interstellar chemistry, through H2 roaming occurring in ionic species.
UR - https://www.scopus.com/pages/publications/85057969718
U2 - 10.1038/s41467-018-07577-0
DO - 10.1038/s41467-018-07577-0
M3 - Article
C2 - 30518927
AN - SCOPUS:85057969718
SN - 2041-1723
VL - 9
JO - Nature Communications
JF - Nature Communications
IS - 1
M1 - 5186
ER -