A molecular beam and computational study on the barrierless gas phase formation of (iso)quinoline in low temperature extraterrestrial environments

Author:

Zhao Long1,Prendergast Matthew1,Kaiser Ralf I.1ORCID,Xu Bo2,Lu Wenchao2ORCID,Ahmed Musahid2ORCID,Hasan Howlader A.3ORCID,Wnuk Stanislaw F.3ORCID,Korotchenko Alexander S.4,Evseev Mikhail M.4,Bashkirov Eugene K.4,Azyazov Valeriy N.45,Mebel Alexander M.3ORCID

Affiliation:

1. Department of Chemistry, University of Hawaii at Manoa, Honolulu, HI 96822, USA

2. Chemical Sciences Division, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA

3. Department of Chemistry and Biochemistry, Florida International University, Miami, FL 33199, USA

4. Samara National Research University, Samara 443086, Russian Federation

5. Lebedev Physical Institute, Samara 443011, Russian Federation

Abstract

Quinoline and isoquinoline can be formed through molecular mass growth processes in low-temperature environments.

Funder

U.S. Department of Energy

University of Hawai'i

Ministry of Education and Science of the Russian Federation

Publisher

Royal Society of Chemistry (RSC)

Subject

Physical and Theoretical Chemistry,General Physics and Astronomy

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