Indirect study of the stellar reaction rate through reaction measurements
Abstract
The 34Ar(α,p) 37K reaction is believed to be one of the last in a sequence of (α,p) and (p,γ) reactions within the Tz = -1 , sd-shell nuclei, known as the αp-process. This process is expected to influence the shape and rise times of luminosity curves coming from type I x-ray bursts (XRBs). With very little experimental information known on many of the reactions within the αp-process, stellar rates are calculated using a statistical model, such as Hauser-Feshbach. Questions on the applicability of a Hauser-Feshbach model for the 34Ar (α,p) 37K reaction arise due to level density considerations in the compound nucleus, 38Ca . We have performed high energy-resolution forward-angle 40Ca (p,t) 38Ca measurements with the K = 600 spectrograph at iThemba LABS in order to identify levels above the α-threshold in 38Ca . States identified in this work were then used to determine the 34Ar (α,p) 37K reaction rate based on a narrow-resonance formalism. Comparisons are made to two standard Hauser-Feshbach model predicted rates at XRB temperatures.
- Authors:
-
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- Univ. of Notre Dame, IN (United States). Dept. of Physics and the Joint Inst. for Nuclear Astrophysics; Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Tohoku Univ., Sendai (Japan). Research Center for Electron Photon Science
- Univ. of Notre Dame, IN (United States). Dept. of Physics and the Joint Inst. for Nuclear Astrophysics
- iThemba Lab. for Accelerator Sciences, Somerset West, Western Cape (South Africa)
- Univ. of Witwatersrand, Johannesburg (South Africa). School of Physics
- Univ.of Cape Town, Rondebosch, Western Cape (South Africa). Physics Dept.
- Univ. of Stellenbosch, Matieland, Western Cape (South Africa)
- iThemba Lab. for Accelerator Sciences, Somerset West, Western Cape (South Africa); Univ. of Stellenbosch, Matieland, Western Cape (South Africa)
- iThemba Lab. for Accelerator Sciences, Somerset West, Western Cape (South Africa); Univ. of Stellenbosch, Matieland, Western Cape (South Africa); Katholieke Univ. Leuven, Leuven (Belgium). Inst. for voor Kern- en Stralingsfysica,
- Univ. of Notre Dame, IN (United States). Dept. of Physics and the Joint Inst. for Nuclear Astrophysics; Argonne National Lab. (ANL), Argonne, IL (United States)
- Florida State Univ., Tallahassee, FL (United States). Dept. of Physics
- Publication Date:
- Research Org.:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC). Nuclear Physics (NP) (SC-26); USDOE
- OSTI Identifier:
- 1392814
- Alternate Identifier(s):
- OSTI ID: 1356447
- Report Number(s):
- LA-UR-17-25567
Journal ID: ISSN 2469-9985; PRVCAN
- Grant/Contract Number:
- AC52-06NA25396; SC0009883
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review C
- Additional Journal Information:
- Journal Volume: 95; Journal Issue: 5; Journal ID: ISSN 2469-9985
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Atomic and Nuclear Physics; Astronomy and Astrophysics
Citation Formats
Long, Alexander Makenzie, Adachi, T., Beard, M., Berg, G. P. A., Buthelezi, Z., Carter, J., Couder, M., deBoer, R. J., Fearick, R. W., Förtsch, S. V., Görres, J., Mira, J. P., Murray, S. H. T., Neveling, R., Papka, P., Smit, F. D., Sideras-Haddad, E., Swartz, J. A., Talwar, R., Usman, I. T., Wiescher, M., Van Zyl, J. J., and Volya, A. Indirect study of the stellar Ar34(α,p)K37 reaction rate through Ca40(p,t)Ca38 reaction measurements. United States: N. p., 2017.
Web. doi:10.1103/PhysRevC.95.055803.
Long, Alexander Makenzie, Adachi, T., Beard, M., Berg, G. P. A., Buthelezi, Z., Carter, J., Couder, M., deBoer, R. J., Fearick, R. W., Förtsch, S. V., Görres, J., Mira, J. P., Murray, S. H. T., Neveling, R., Papka, P., Smit, F. D., Sideras-Haddad, E., Swartz, J. A., Talwar, R., Usman, I. T., Wiescher, M., Van Zyl, J. J., & Volya, A. Indirect study of the stellar Ar34(α,p)K37 reaction rate through Ca40(p,t)Ca38 reaction measurements. United States. https://doi.org/10.1103/PhysRevC.95.055803
Long, Alexander Makenzie, Adachi, T., Beard, M., Berg, G. P. A., Buthelezi, Z., Carter, J., Couder, M., deBoer, R. J., Fearick, R. W., Förtsch, S. V., Görres, J., Mira, J. P., Murray, S. H. T., Neveling, R., Papka, P., Smit, F. D., Sideras-Haddad, E., Swartz, J. A., Talwar, R., Usman, I. T., Wiescher, M., Van Zyl, J. J., and Volya, A. Wed .
"Indirect study of the stellar Ar34(α,p)K37 reaction rate through Ca40(p,t)Ca38 reaction measurements". United States. https://doi.org/10.1103/PhysRevC.95.055803. https://www.osti.gov/servlets/purl/1392814.
@article{osti_1392814,
title = {Indirect study of the stellar Ar34(α,p)K37 reaction rate through Ca40(p,t)Ca38 reaction measurements},
author = {Long, Alexander Makenzie and Adachi, T. and Beard, M. and Berg, G. P. A. and Buthelezi, Z. and Carter, J. and Couder, M. and deBoer, R. J. and Fearick, R. W. and Förtsch, S. V. and Görres, J. and Mira, J. P. and Murray, S. H. T. and Neveling, R. and Papka, P. and Smit, F. D. and Sideras-Haddad, E. and Swartz, J. A. and Talwar, R. and Usman, I. T. and Wiescher, M. and Van Zyl, J. J. and Volya, A.},
abstractNote = {The 34Ar(α,p) 37K reaction is believed to be one of the last in a sequence of (α,p) and (p,γ) reactions within the Tz = -1 , sd-shell nuclei, known as the αp-process. This process is expected to influence the shape and rise times of luminosity curves coming from type I x-ray bursts (XRBs). With very little experimental information known on many of the reactions within the αp-process, stellar rates are calculated using a statistical model, such as Hauser-Feshbach. Questions on the applicability of a Hauser-Feshbach model for the 34Ar (α,p) 37K reaction arise due to level density considerations in the compound nucleus, 38Ca . We have performed high energy-resolution forward-angle 40Ca (p,t) 38Ca measurements with the K = 600 spectrograph at iThemba LABS in order to identify levels above the α-threshold in 38Ca . States identified in this work were then used to determine the 34Ar (α,p) 37K reaction rate based on a narrow-resonance formalism. Comparisons are made to two standard Hauser-Feshbach model predicted rates at XRB temperatures.},
doi = {10.1103/PhysRevC.95.055803},
journal = {Physical Review C},
number = 5,
volume = 95,
place = {United States},
year = {Wed May 10 00:00:00 EDT 2017},
month = {Wed May 10 00:00:00 EDT 2017}
}
Web of Science
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