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Unconventional gas-phase preparation of the prototype polycyclic aromatic hydrocarbon naphthalene (C10H8) via the reaction of benzyl (C7H7) and propargyl (C3H3) radicals coupled with hydrogen-atom assisted isomerization

Journal Article · · Chemical Science
DOI:https://doi.org/10.1039/d3sc00911d· OSTI ID:1972235
 [1];  [1];  [2];  [2];  [3];  [4];  [5];  [5];  [6];  [6]
  1. University of Hawai'i at Mānoa, Honolulu, HI (United States)
  2. Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
  3. Lebedev Physical Institute, Samara (Russian Federation); Samara National Research University (Russian Federation)
  4. Samara National Research University (Russian Federation)
  5. Lebedev Physical Institute, Samara (Russian Federation)
  6. Florida International University, Miami, FL (United States)
Polycyclic aromatic hydrocarbons (PAHs) are ubiquitous in the interstellar medium and in meteorites such as Murchison and Allende and signify the missing link between resonantly stabilized free radicals and carbonaceous nanoparticles (soot particles, interstellar grains). However, the predicted lifetime of interstellar PAHs of some 108 years imply that PAHs should not exist in extraterrestrial environments suggesting that key mechanisms of their formation are elusive. Exploiting a microchemical reactor and coupling these data with computational fluid dynamics (CFD) simulations and kinetic modeling, we reveal through an isomer selective product detection that the reaction of the resonantly stabilized benzyl (C7H7) and the propargyl (C3H3) synthesizes the simplest representative of PAHs – the 10π Hückel aromatic naphthalene (C10H8) molecule – via the novel Propargyl Addition–BenzAnnulation (PABA) mechanism. The gas-phase preparation of naphthalene affords a versatile concept of the reaction of combustion and astronomically abundant propargyl radicals with aromatic radicals carrying the radical center at the methylene moiety (aromatic-CH2) as a previously passed over source of aromatics in high temperature environments thus bringing us closer to an understanding of the aromatic universe we live in.
Research Organization:
Florida International University (FIU), Miami, FL (United States); Florida International University, Miami, FL (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); University of Hawai'i at Mānoa, Honolulu, HI (United States)
Sponsoring Organization:
Ministry of Higher Education and Science of the Russian Federation; Ministry of Science and Higher Education of the Russian Federation; USDOE; USDOE Office of Science (SC), Basic Energy Sciences (BES); USDOE Office of Science (SC), Basic Energy Sciences (BES). Chemical Sciences, Geosciences & Biosciences Division (CSGB)
Grant/Contract Number:
AC02-05CH11231; FG02-03ER15411; FG02-04ER15570
OSTI ID:
1972235
Alternate ID(s):
OSTI ID: 2371718
OSTI ID: 1975327
OSTI ID: 2997069
Journal Information:
Chemical Science, Journal Name: Chemical Science Journal Issue: 20 Vol. 14; ISSN 2041-6520
Publisher:
Royal Society of ChemistryCopyright Statement
Country of Publication:
United States
Language:
English

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