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

Abstract

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, Ec.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.

Authors:
 [1];  [2];  [3];  [4];  [2];  [5];  [2];  [2];  [6];  [2];  [7]; ORCiD logo [1];  [8];  [2];  [1];  [5];  [5];  [9];  [7];  [5] more »;  [2];  [10] « less
+ Show Author Affiliations
  1. Colorado School of Mines, Golden, CO (United States)
  2. TRIUMF, Vancouver, BC (Canada)
  3. TRIUMF, Vancouver, BC (Canada); Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
  4. TRIUMF, Vancouver, BC (Canada); Univ. of York (United Kingdom)
  5. McMaster Univ., Hamilton, ON (Canada)
  6. Michigan State Univ., East Lansing, MI (United States)
  7. Ohio Univ., Athens, OH (United States)
  8. Univ. of Northern British Columbia, Prince George, BC (Canada)
  9. Univ. of Notre Dame, IN (United States)
  10. Univ. of Edinburgh, Scotland (United Kingdom)
Publication Date:
Research Org.:
Colorado School of Mines, Golden, CO (United States)
Sponsoring Org.:
USDOE Office of Science (SC); Natural Sciences and Engineering Research Council of Canada (NSERC); National Science Foundation (NSF)
Contributing Org.:
DRAGON Collaboration
OSTI Identifier:
1830733
Grant/Contract Number:  
FG02-93ER40789; SAPPJ-2019-00039; PHY-1565546; PHY-1401343; PHY-1419765
Resource Type:
Accepted Manuscript
Journal Name:
Physical Review C
Additional Journal Information:
Journal Volume: 103; Journal Issue: 5; Journal ID: ISSN 2469-9985
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
73 NUCLEAR PHYSICS AND RADIATION PHYSICS; nuclear astrophysics

Citation Formats

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., and Shotter, A. C. Proton capture on 34S in the astrophysical energy regime of O-Ne novae. United States: N. p., 2021. Web. doi:10.1103/physrevc.103.055801.
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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. Proton capture on 34S in the astrophysical energy regime of O-Ne novae. United States. https://doi.org/10.1103/physrevc.103.055801
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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., and Shotter, A. C. Thu . "Proton capture on 34S in the astrophysical energy regime of O-Ne novae". United States. https://doi.org/10.1103/physrevc.103.055801. https://www.osti.gov/servlets/purl/1830733.
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@article{osti_1830733,
title = {Proton capture on 34S in the astrophysical energy regime of O-Ne novae},
author = {Lovely, M. and Lennarz, A. and Connolly, D. and Williams, M. and Alcorta, M. and Chen, A. A. and Davids, B. and Esker, N. E. and Fry, C. and Gillespie, S. A. and Giri, R. and Greife, U. and Hussein, A. and Hutcheon, D. and Karpesky, J. and Kroll, L. and Liang, J. and O'Malley, P. D. and Paneru, S. and Psaltis, A. and Ruiz, C. and Shotter, A. C.},
abstractNote = {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, Ec.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.},
doi = {10.1103/physrevc.103.055801},
journal = {Physical Review C},
number = 5,
volume = 103,
place = {United States},
year = {Thu May 06 00:00:00 EDT 2021},
month = {Thu May 06 00:00:00 EDT 2021}
}
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