Measurements of proton radiative capture cross sections relevant to the astrophysical rp- and gamma-processes

F.R. Chloupek; A.S. Murphy; R.N. Boyd; A.L. Cole; J. Gorres; R. T. Guray; G. Raimann; J.J. Zach; T. Rauscher; J.V. Schwarzenberg; P. Tischhauser; M. Wiescher

doi:10.1016/S0375-9474(99)00167-0

Measurements of proton radiative capture cross sections relevant to the astrophysical rp- and gamma-processes

F.R. Chloupek, A.S. Murphy, R.N. Boyd, A.L. Cole, J. Gorres, R. T. Guray, G. Raimann, J.J. Zach, T. Rauscher, J.V. Schwarzenberg, P. Tischhauser, M. Wiescher

Centre for Astrophysics Research (CAR)

Research output: Contribution to journal › Article › peer-review

48 Citations (Scopus)

Abstract

Measurements have been made of the Zr-96(p,gamma)Nb-97, Sn-112(p,gamma)Sb-113, and Sn-119(p,gamma) Sb-120 cross section excitation functions, Incident proton energies ranged from 2.8 MeV to 8.5 MeV. These reactions are relevant to several processes of stellar nucleosynthesis. The resulting astrophysical S-factors are compared to those from theoretical statistical model calculations using the SMOKER, and the more recent NON-SMOKER, codes to judge their applicability to these reactions. (C) 1999 Elsevier Science B.V. All rights reserved.

Original language	English
Pages (from-to)	391-405
Number of pages	15
Journal	Nuclear Physics A
Volume	652
Issue number	4
DOIs	https://doi.org/10.1016/S0375-9474(99)00167-0
Publication status	Published - 21 Jun 1999

Keywords

p-process
astrophysical S-factors
RATES
nuclear cross sections
NUCLEI
proton radiative capture reactions
P-PROCESS

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10.1016/S0375-9474(99)00167-0

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Chloupek, F. R., Murphy, A. S., Boyd, R. N., Cole, A. L., Gorres, J., Guray, R. T., Raimann, G., Zach, J. J., Rauscher, T., Schwarzenberg, J. V., Tischhauser, P., & Wiescher, M. (1999). Measurements of proton radiative capture cross sections relevant to the astrophysical rp- and gamma-processes. Nuclear Physics A, 652(4), 391-405. https://doi.org/10.1016/S0375-9474(99)00167-0

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title = "Measurements of proton radiative capture cross sections relevant to the astrophysical rp- and gamma-processes",

abstract = "Measurements have been made of the Zr-96(p,gamma)Nb-97, Sn-112(p,gamma)Sb-113, and Sn-119(p,gamma) Sb-120 cross section excitation functions, Incident proton energies ranged from 2.8 MeV to 8.5 MeV. These reactions are relevant to several processes of stellar nucleosynthesis. The resulting astrophysical S-factors are compared to those from theoretical statistical model calculations using the SMOKER, and the more recent NON-SMOKER, codes to judge their applicability to these reactions. (C) 1999 Elsevier Science B.V. All rights reserved.",

keywords = "p-process, astrophysical S-factors, RATES, nuclear cross sections, NUCLEI, proton radiative capture reactions, P-PROCESS",

author = "F.R. Chloupek and A.S. Murphy and R.N. Boyd and A.L. Cole and J. Gorres and Guray, {R. T.} and G. Raimann and J.J. Zach and T. Rauscher and J.V. Schwarzenberg and P. Tischhauser and M. Wiescher",

year = "1999",

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doi = "10.1016/S0375-9474(99)00167-0",

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pages = "391--405",

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TY - JOUR

T1 - Measurements of proton radiative capture cross sections relevant to the astrophysical rp- and gamma-processes

AU - Chloupek, F.R.

AU - Murphy, A.S.

AU - Boyd, R.N.

AU - Cole, A.L.

AU - Gorres, J.

AU - Guray, R. T.

AU - Raimann, G.

AU - Zach, J.J.

AU - Rauscher, T.

AU - Schwarzenberg, J.V.

AU - Tischhauser, P.

AU - Wiescher, M.

PY - 1999/6/21

Y1 - 1999/6/21

N2 - Measurements have been made of the Zr-96(p,gamma)Nb-97, Sn-112(p,gamma)Sb-113, and Sn-119(p,gamma) Sb-120 cross section excitation functions, Incident proton energies ranged from 2.8 MeV to 8.5 MeV. These reactions are relevant to several processes of stellar nucleosynthesis. The resulting astrophysical S-factors are compared to those from theoretical statistical model calculations using the SMOKER, and the more recent NON-SMOKER, codes to judge their applicability to these reactions. (C) 1999 Elsevier Science B.V. All rights reserved.

AB - Measurements have been made of the Zr-96(p,gamma)Nb-97, Sn-112(p,gamma)Sb-113, and Sn-119(p,gamma) Sb-120 cross section excitation functions, Incident proton energies ranged from 2.8 MeV to 8.5 MeV. These reactions are relevant to several processes of stellar nucleosynthesis. The resulting astrophysical S-factors are compared to those from theoretical statistical model calculations using the SMOKER, and the more recent NON-SMOKER, codes to judge their applicability to these reactions. (C) 1999 Elsevier Science B.V. All rights reserved.

KW - p-process

KW - astrophysical S-factors

KW - RATES

KW - nuclear cross sections

KW - NUCLEI

KW - proton radiative capture reactions

KW - P-PROCESS

U2 - 10.1016/S0375-9474(99)00167-0

DO - 10.1016/S0375-9474(99)00167-0

M3 - Article

SN - 0375-9474

VL - 652

SP - 391

EP - 405

JO - Nuclear Physics A

JF - Nuclear Physics A

IS - 4

ER -

Measurements of proton radiative capture cross sections relevant to the astrophysical rp- and gamma-processes

Abstract

Keywords

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