LOW TEMPERATURE FORMATION of NITROGEN-SUBSTITUTED POLYCYCLIC AROMATIC HYDROCARBONS (PANHs) - BARRIERLESS ROUTES to DIHYDRO(iso)QUINOLINES

  • Dorian S.N. Parker
  • , Tao Yang
  • , Beni B. Dangi
  • , Ralf I. Kaiser
  • , Partha P. Bera
  • , Timothy J. Lee

Research output: Contribution to journalArticlepeer-review

33 Scopus citations

Abstract

Meteorites contain bio-relevant molecules such as vitamins and nucleobases, which consist of aromatic structures with embedded nitrogen atoms. Questions remain over the chemical mechanisms responsible for the formation of nitrogen-substituted polycyclic aromatic hydrocarbons (PANHs) in extraterrestrial environments. By exploiting single collision conditions, we show that a radical mediated bimolecular collision between pyridyl radicals and 1,3-butadiene in the gas phase forms nitrogen-substituted polycyclic aromatic hydrocarbons (PANHs) 1,4-dihydroquinoline and to a minor amount 1,4-dihydroisoquinoline. The reaction proceeds through the formation of a van der Waals complex, which circumnavigates the entrance barrier implying it can operate at very low kinetic energy and therefore at low temperatures of 10 K as present in cold molecular clouds such as TMC-1. The discovery of facile de facto barrierless exoergic reaction mechanisms leading to PANH formation could play an important role in providing a population of aromatic structures upon which further photo-processing of ice condensates could occur to form nucleobases.

Original languageEnglish
Article number115
JournalAstrophysical Journal
Volume815
Issue number2
DOIs
StatePublished - 20 Dec 2015
Externally publishedYes

Keywords

  • ISM: molecules
  • astrobiology
  • astrochemistry
  • molecular processes

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