Cross section measurements of the Pd-102(p, gamma)Ag-103 Sn-116(p, gamma)Sb-117, and Sn-112(alpha, gamma)Te-116 reactions relevant to the astrophysical rp- and gamma-processes

N. Ozkan; A.S.J. Murphy; R.N. Boyd; A.L. Cole; A. Famiano; R. T. Guray; M. Howard; L. Sahin; J.J. Zach; R. deHaan; J. Gorres; M. Wiescher; M.S. Islam; T. Rauscher

Cross section measurements of the Pd-102(p, gamma)Ag-103 Sn-116(p, gamma)Sb-117, and Sn-112(alpha, gamma)Te-116 reactions relevant to the astrophysical rp- and gamma-processes

N. Ozkan, A.S.J. Murphy, R.N. Boyd, A.L. Cole, A. Famiano, R. T. Guray, M. Howard, L. Sahin, J.J. Zach, R. deHaan, J. Gorres, M. Wiescher, M.S. Islam, T. Rauscher

Centre for Astrophysics Research (CAR)

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

63 Citations (Scopus)

Abstract

Total cross section measurements for the Pd-102(p, gamma)Ag-103 and Sn-116(p, gamma)Sb-117 reactions have been performed in the proton energy range 2.6 to 4.25 MeV, and for the Sn-112(alpha,gamma)T-116, reaction over the alpha beam energy range 7.0 to 10.5 MeV. An activation technique was used in which gamma rays from decays of the reaction products were detected off-line by two hyper-pure germanium detectors in a low background environment. Where possible, reaction rates are derived and the results compared to those of calculations generated by the NON-SMOKER and the MOST statistical model codes so as to judge their applicability for describing the cross sections needed for network calculations of nucleosynthesis in explosive astrophysical environments via the gamma- and rp-processes. (C) 2002 Elsevier Science B.V. All rights reserved.

Original language	English
Pages (from-to)	469-485
Number of pages	17
Journal	Nuclear Physics A
Volume	710
Issue number	3-4
Publication status	Published - 18 Nov 2002

Keywords

astrophysical S-factors
RATES
proton radiative
nuclear cross sections
gamma-process
capture reactions
rp-process
P-PROCESS

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Ozkan, N., Murphy, A. S. J., Boyd, R. N., Cole, A. L., Famiano, A., Guray, R. T., Howard, M., Sahin, L., Zach, J. J., deHaan, R., Gorres, J., Wiescher, M., Islam, M. S., & Rauscher, T. (2002). Cross section measurements of the Pd-102(p, gamma)Ag-103 Sn-116(p, gamma)Sb-117, and Sn-112(alpha, gamma)Te-116 reactions relevant to the astrophysical rp- and gamma-processes. Nuclear Physics A, 710(3-4), 469-485.

@article{315f3d602e4f4cc0b12adf7c0e31f4ff,

title = "Cross section measurements of the Pd-102(p, gamma)Ag-103 Sn-116(p, gamma)Sb-117, and Sn-112(alpha, gamma)Te-116 reactions relevant to the astrophysical rp- and gamma-processes",

abstract = "Total cross section measurements for the Pd-102(p, gamma)Ag-103 and Sn-116(p, gamma)Sb-117 reactions have been performed in the proton energy range 2.6 to 4.25 MeV, and for the Sn-112(alpha,gamma)T-116, reaction over the alpha beam energy range 7.0 to 10.5 MeV. An activation technique was used in which gamma rays from decays of the reaction products were detected off-line by two hyper-pure germanium detectors in a low background environment. Where possible, reaction rates are derived and the results compared to those of calculations generated by the NON-SMOKER and the MOST statistical model codes so as to judge their applicability for describing the cross sections needed for network calculations of nucleosynthesis in explosive astrophysical environments via the gamma- and rp-processes. (C) 2002 Elsevier Science B.V. All rights reserved.",

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

author = "N. Ozkan and A.S.J. Murphy and R.N. Boyd and A.L. Cole and A. Famiano and Guray, {R. T.} and M. Howard and L. Sahin and J.J. Zach and R. deHaan and J. Gorres and M. Wiescher and M.S. Islam and T. Rauscher",

note = "PII: S0375-9474(02)01134-X",

year = "2002",

month = nov,

day = "18",

language = "English",

volume = "710",

pages = "469--485",

journal = "Nuclear Physics A",

issn = "0375-9474",

publisher = "Elsevier",

number = "3-4",

}

Ozkan, N, Murphy, ASJ, Boyd, RN, Cole, AL, Famiano, A, Guray, RT, Howard, M, Sahin, L, Zach, JJ, deHaan, R, Gorres, J, Wiescher, M, Islam, MS & Rauscher, T 2002, 'Cross section measurements of the Pd-102(p, gamma)Ag-103 Sn-116(p, gamma)Sb-117, and Sn-112(alpha, gamma)Te-116 reactions relevant to the astrophysical rp- and gamma-processes', Nuclear Physics A, vol. 710, no. 3-4, pp. 469-485.

TY - JOUR

T1 - Cross section measurements of the Pd-102(p, gamma)Ag-103 Sn-116(p, gamma)Sb-117, and Sn-112(alpha, gamma)Te-116 reactions relevant to the astrophysical rp- and gamma-processes

AU - Ozkan, N.

AU - Murphy, A.S.J.

AU - Boyd, R.N.

AU - Cole, A.L.

AU - Famiano, A.

AU - Guray, R. T.

AU - Howard, M.

AU - Sahin, L.

AU - Zach, J.J.

AU - deHaan, R.

AU - Gorres, J.

AU - Wiescher, M.

AU - Islam, M.S.

AU - Rauscher, T.

N1 - PII: S0375-9474(02)01134-X

PY - 2002/11/18

Y1 - 2002/11/18

N2 - Total cross section measurements for the Pd-102(p, gamma)Ag-103 and Sn-116(p, gamma)Sb-117 reactions have been performed in the proton energy range 2.6 to 4.25 MeV, and for the Sn-112(alpha,gamma)T-116, reaction over the alpha beam energy range 7.0 to 10.5 MeV. An activation technique was used in which gamma rays from decays of the reaction products were detected off-line by two hyper-pure germanium detectors in a low background environment. Where possible, reaction rates are derived and the results compared to those of calculations generated by the NON-SMOKER and the MOST statistical model codes so as to judge their applicability for describing the cross sections needed for network calculations of nucleosynthesis in explosive astrophysical environments via the gamma- and rp-processes. (C) 2002 Elsevier Science B.V. All rights reserved.

AB - Total cross section measurements for the Pd-102(p, gamma)Ag-103 and Sn-116(p, gamma)Sb-117 reactions have been performed in the proton energy range 2.6 to 4.25 MeV, and for the Sn-112(alpha,gamma)T-116, reaction over the alpha beam energy range 7.0 to 10.5 MeV. An activation technique was used in which gamma rays from decays of the reaction products were detected off-line by two hyper-pure germanium detectors in a low background environment. Where possible, reaction rates are derived and the results compared to those of calculations generated by the NON-SMOKER and the MOST statistical model codes so as to judge their applicability for describing the cross sections needed for network calculations of nucleosynthesis in explosive astrophysical environments via the gamma- and rp-processes. (C) 2002 Elsevier Science B.V. All rights reserved.

KW - astrophysical S-factors

KW - RATES

KW - proton radiative

KW - nuclear cross sections

KW - gamma-process

KW - capture reactions

KW - rp-process

KW - P-PROCESS

M3 - Article

SN - 0375-9474

VL - 710

SP - 469

EP - 485

JO - Nuclear Physics A

JF - Nuclear Physics A

IS - 3-4

ER -

Cross section measurements of the Pd-102(p, gamma)Ag-103 Sn-116(p, gamma)Sb-117, and Sn-112(alpha, gamma)Te-116 reactions relevant to the astrophysical rp- and gamma-processes

Abstract

Keywords

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