Astrophysical S-factors and reaction rates of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn

Ye Skakun; T. Rauscher

doi:10.1051/ndata:07216

Astrophysical S-factors and reaction rates of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn

Ye Skakun, T. Rauscher

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

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Abstract

Astrophysical S-factors and reaction rates were derived from available cross sections of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn isotopes at incident proton energies up to 9 MeV. The statistical theory predictions of the observable quantities are similar to 2 times smaller at near threshold energies and have better agreement at higher energies.

Original language	English
Title of host publication	Int Conf on Nuclear Data for Science and Technology
Editors	O. Bersillon, F. Gunsing, E. Bauge, R. Jacqmin, S. Leray
Place of Publication	CEDEX A
Publisher	EDP Sciences
Pages	1325-1327
Number of pages	3
Volume	2
ISBN (Print)	978-2-7598-0091-9
DOIs	https://doi.org/10.1051/ndata:07216
Publication status	Published - 2008
Event	International Conference on Nuclear Data for Science and Technology - Nice, France Duration: 22 Apr 2007 → 27 Apr 2007

Conference

Conference	International Conference on Nuclear Data for Science and Technology
Country/Territory	France
City	Nice
Period	22/04/07 → 27/04/07

Keywords

ISOTOPES

Access to Document

10.1051/ndata:07216

Ndata07216Final published version, 122 KB

Cite this

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title = "Astrophysical S-factors and reaction rates of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn",

abstract = "Astrophysical S-factors and reaction rates were derived from available cross sections of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn isotopes at incident proton energies up to 9 MeV. The statistical theory predictions of the observable quantities are similar to 2 times smaller at near threshold energies and have better agreement at higher energies.",

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Skakun, Y & Rauscher, T 2008, Astrophysical S-factors and reaction rates of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn. in O Bersillon, F Gunsing, E Bauge, R Jacqmin & S Leray (eds), Int Conf on Nuclear Data for Science and Technology. vol. 2, EDP Sciences, CEDEX A, pp. 1325-1327, International Conference on Nuclear Data for Science and Technology, Nice, France, 22/04/07. https://doi.org/10.1051/ndata:07216

Astrophysical S-factors and reaction rates of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn. / Skakun, Ye; Rauscher, T.
Int Conf on Nuclear Data for Science and Technology. ed. / O. Bersillon; F. Gunsing; E. Bauge; R. Jacqmin; S. Leray. Vol. 2 CEDEX A: EDP Sciences, 2008. p. 1325-1327.

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - Astrophysical S-factors and reaction rates of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn

AU - Skakun, Ye

AU - Rauscher, T.

PY - 2008

Y1 - 2008

N2 - Astrophysical S-factors and reaction rates were derived from available cross sections of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn isotopes at incident proton energies up to 9 MeV. The statistical theory predictions of the observable quantities are similar to 2 times smaller at near threshold energies and have better agreement at higher energies.

AB - Astrophysical S-factors and reaction rates were derived from available cross sections of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn isotopes at incident proton energies up to 9 MeV. The statistical theory predictions of the observable quantities are similar to 2 times smaller at near threshold energies and have better agreement at higher energies.

KW - ISOTOPES

U2 - 10.1051/ndata:07216

DO - 10.1051/ndata:07216

M3 - Conference contribution

SN - 978-2-7598-0091-9

VL - 2

SP - 1325

EP - 1327

BT - Int Conf on Nuclear Data for Science and Technology

A2 - Bersillon, O.

A2 - Gunsing, F.

A2 - Bauge, E.

A2 - Jacqmin, R.

A2 - Leray, S.

PB - EDP Sciences

CY - CEDEX A

T2 - International Conference on Nuclear Data for Science and Technology

Y2 - 22 April 2007 through 27 April 2007

ER -

Astrophysical S-factors and reaction rates of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn

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