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Title: γ spectroscopy of states in Cl 32 relevant for the S 31 ( p , γ ) Cl 32 reaction rate

Abstract

Background: The 31S(p,gamma) 32Cl reaction becomes important for sulfur production in novae if the P-31(p, alpha)Si-28 reaction rate is somewhat greater than currently accepted. The rate of the S-31(p,gamma) Cl-32 reaction is uncertain, primarily due to the properties of resonances at E-c.m. = 156 and 549 keV. Purpose: We precisely determined the excitation energies of states in Cl-32 through high-resolution. spectroscopy including the two states most important for the S-31(p,gamma) Cl-32 reaction at nova temperatures. Method: Excited states in Cl-32 were populated using the B-10(Mg-24, 2n) Cl-32 reaction with a Mg-24 beam from the ATLAS facility at Argonne National Laboratory. The reaction channel of interest was selected using recoils in the Fragment Mass Analyzer, and we determined precise level energies by detecting. rays with Gammasphere. Results: We also observed. rays from the decay of six excited states in Cl-32. The excitation energies for two unbound levels at E-x = 1738.1 (6) keV and 2130.5 (10) keV were determined and found to be in agreement with a previous high-precision measurement of the S-32(He-3, t) Cl-32 reaction [1]. Conclusions: An updated 31S(p,gamma) Cl-32 reaction rate is presented. With the excitation energies of important levels firmly established, the dominant uncertainty in the reactionmore » rate at nova temperatures is due to the strength of the resonance corresponding to the 2131-keV state in Cl-32.« less

Authors:
 [1];  [1];  [1];  [1];  [1];  [1];  [2];  [2];  [2];  [2];  [2];  [2];  [2]
  1. Louisiana State Univ., Baton Rouge, LA (United States). Dept. of Physics and Astronomy
  2. Argonne National Lab. (ANL), Argonne, IL (United States). Physics Division
Publication Date:
Research Org.:
Argonne National Lab. (ANL), Argonne, IL (United States)
Sponsoring Org.:
USDOE Office of Science (SC), Nuclear Physics (NP) (SC-26)
OSTI Identifier:
1392901
Alternate Identifier(s):
OSTI ID: 1378135
Grant/Contract Number:  
AC02-06CH11357; FG02-96ER40978
Resource Type:
Accepted Manuscript
Journal Name:
Physical Review C
Additional Journal Information:
Journal Volume: 96; Journal Issue: 3; Journal ID: ISSN 2469-9985
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
73 NUCLEAR PHYSICS AND RADIATION PHYSICS

Citation Formats

Afanasieva, L., Blackmon, J. C., Deibel, C. M., Lai, J., Linhardt, L. E., Rasco, B. C., Seweryniak, D., Alcorta, M., Carpenter, M. P., Clark, J. A., Hoffman, C. R., Janssens, R. V. F., and Zhu, S. γ spectroscopy of states in Cl32 relevant for the S31(p,γ)Cl32 reaction rate. United States: N. p., 2017. Web. doi:10.1103/PhysRevC.96.035801.
Afanasieva, L., Blackmon, J. C., Deibel, C. M., Lai, J., Linhardt, L. E., Rasco, B. C., Seweryniak, D., Alcorta, M., Carpenter, M. P., Clark, J. A., Hoffman, C. R., Janssens, R. V. F., & Zhu, S. γ spectroscopy of states in Cl32 relevant for the S31(p,γ)Cl32 reaction rate. United States. doi:10.1103/PhysRevC.96.035801.
Afanasieva, L., Blackmon, J. C., Deibel, C. M., Lai, J., Linhardt, L. E., Rasco, B. C., Seweryniak, D., Alcorta, M., Carpenter, M. P., Clark, J. A., Hoffman, C. R., Janssens, R. V. F., and Zhu, S. Fri . "γ spectroscopy of states in Cl32 relevant for the S31(p,γ)Cl32 reaction rate". United States. doi:10.1103/PhysRevC.96.035801. https://www.osti.gov/servlets/purl/1392901.
@article{osti_1392901,
title = {γ spectroscopy of states in Cl32 relevant for the S31(p,γ)Cl32 reaction rate},
author = {Afanasieva, L. and Blackmon, J. C. and Deibel, C. M. and Lai, J. and Linhardt, L. E. and Rasco, B. C. and Seweryniak, D. and Alcorta, M. and Carpenter, M. P. and Clark, J. A. and Hoffman, C. R. and Janssens, R. V. F. and Zhu, S.},
abstractNote = {Background: The 31S(p,gamma) 32Cl reaction becomes important for sulfur production in novae if the P-31(p, alpha)Si-28 reaction rate is somewhat greater than currently accepted. The rate of the S-31(p,gamma) Cl-32 reaction is uncertain, primarily due to the properties of resonances at E-c.m. = 156 and 549 keV. Purpose: We precisely determined the excitation energies of states in Cl-32 through high-resolution. spectroscopy including the two states most important for the S-31(p,gamma) Cl-32 reaction at nova temperatures. Method: Excited states in Cl-32 were populated using the B-10(Mg-24, 2n) Cl-32 reaction with a Mg-24 beam from the ATLAS facility at Argonne National Laboratory. The reaction channel of interest was selected using recoils in the Fragment Mass Analyzer, and we determined precise level energies by detecting. rays with Gammasphere. Results: We also observed. rays from the decay of six excited states in Cl-32. The excitation energies for two unbound levels at E-x = 1738.1 (6) keV and 2130.5 (10) keV were determined and found to be in agreement with a previous high-precision measurement of the S-32(He-3, t) Cl-32 reaction [1]. Conclusions: An updated 31S(p,gamma) Cl-32 reaction rate is presented. With the excitation energies of important levels firmly established, the dominant uncertainty in the reaction rate at nova temperatures is due to the strength of the resonance corresponding to the 2131-keV state in Cl-32.},
doi = {10.1103/PhysRevC.96.035801},
journal = {Physical Review C},
number = 3,
volume = 96,
place = {United States},
year = {2017},
month = {9}
}

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