Photoreactions in nuclear astrophysics

被引：0

作者：

Mohr, P ^{[1
]}

Babilon, M ^{[1
]}

Bayer, W ^{[1
]}

Galaviz, D ^{[1
]}

Hartmann, T ^{[1
]}

Hutter, C ^{[1
]}

Sonnabend, K ^{[1
]}

Vogt, K ^{[1
]}

Volz, S ^{[1
]}

Zilges, A ^{[1
]}

机构：

[1] Tech Univ Darmstadt, Inst Kernphys, D-64289 Darmstadt, Germany

来源：

PROCEEDINGS OF THE INTERNATIONAL SYMPOSIUM ON ELECTROMAGNETIC INTERACTIONS IN NUCLEAR AND HADRON PHYSICS | 2002年

关键词：

D O I：

暂无

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

Photon-induced reactions are the key reactions for the nucleosynthesis of neutron-deficient p-nuclei. We present a new technique which simulates a thermal photon bath at typical temperatures of several billion Kelvin during a supernova explosion. We are able to determine astrophysical reaction rates for the relevant photon-induced reactions. Additionally, we give some examples for the relevance of photon-induced reactions in the astrophysical s-process.

引用

页码：207 / 216

页数：10

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