Proton capture on 34S in the astrophysical energy regime of O-Ne novae

Lovely, M.; Lennarz, A.; Connolly, D.; Williams, M.; Alcorta, M.; Chen, A. A.; Davids, B.; Esker, N. E.; Fry, C.; Gillespie, S. A.; Giri, R.; Greife, U.; Hussein, A.; Hutcheon, D.; Karpesky, J.; Kroll, L.; Liang, J.; O'Malley, P. D.; Paneru, S.; Psaltis, A.; Ruiz, C.; Shotter, A. C.

doi:10.1103/physrevc.103.055801

Proton capture on ³⁴S in the astrophysical energy regime of O-Ne novae

Journal Article · Thu May 06 00:00:00 EDT 2021 · Physical Review C

DOI:https://doi.org/10.1103/physrevc.103.055801· OSTI ID:1830733

Lovely, M. ^[1]; Lennarz, A. ^[2]; Connolly, D. ^[3]; Williams, M. ^[4]; Alcorta, M. ^[2]; Chen, A. A. ^[5]; Davids, B. ^[2]; Esker, N. E. ^[2]; Fry, C. ^[6]; Gillespie, S. A. ^[2]; Giri, R. ^[7]; ^[8]; Hussein, A. ^[9]; Hutcheon, D. ^[2]; Karpesky, J. ^[8]; Kroll, L. ^[5]; Liang, J. ^[5]; O'Malley, P. D. ^[10]; Paneru, S. ^[7]; Psaltis, A. ^[5] more »

Colorado School of Mines, Golden, CO (United States); Colorado School of Mines
TRIUMF, Vancouver, BC (Canada)
TRIUMF, Vancouver, BC (Canada); Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
TRIUMF, Vancouver, BC (Canada); Univ. of York (United Kingdom)
McMaster Univ., Hamilton, ON (Canada)
Michigan State Univ., East Lansing, MI (United States)
Ohio Univ., Athens, OH (United States)
Colorado School of Mines, Golden, CO (United States)
Univ. of Northern British Columbia, Prince George, BC (Canada)
Univ. of Notre Dame, IN (United States)
Univ. of Edinburgh, Scotland (United Kingdom)

Nuclear reaction sensitivity studies have shown that the final isotopic abundance of O-Ne nova nucleosynthesis is dependent on the ³⁴S(p,γ)³⁵Cl reaction at astrophysical energies corresponding to peak nova burning temperatures of 0.1–0.4 GK. Isotopic ratios of the S, Cl, and Ar products are all used in various methods of cosmochemical analysis of presolar meteoritic grains. Due to the lack of direct experimental data, the ³⁴S+p reaction rate has been estimated using statistical modeling or information from indirect nucleon transfer experiments. In order to provide direct reaction information, here the resonance strengths of several low energy resonances, E_c.m. = 272–495 keV, in the ³⁴S(p,γ)³⁵Cl reaction were measured for the first time in inverse kinematics using the DRAGON recoil separator located at TRIUMF, Canada’s Particle Accelerator Centre in Vancouver.

View Accepted Manuscript (DOE)

Research Organization:: Colorado School of Mines, Golden, CO (United States)

Sponsoring Organization:: National Science Foundation (NSF); Natural Sciences and Engineering Research Council of Canada (NSERC); USDOE Office of Science (SC)

Contributing Organization:: DRAGON Collaboration

Grant/Contract Number:: FG02-93ER40789

OSTI ID:: 1830733

Journal Information:: Physical Review C, Journal Name: Physical Review C Journal Issue: 5 Vol. 103; ISSN 2469-9985

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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