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Proton-capture reactions in thermonuclear supernovae and the p process

  • XIII Nuclei in the Cosmos, 7-11 July, 2014 Debrecen, Hungary. As an alternative production scenario to the so-called g process, the most abundant p nucleus 92Mo may be produced by a chain of proton-capture reactions in supernovae type Ia. The reactions 90Zr(p,g) and 91Nb(p,g) are the most important reactions in this chain. We have measured the first reaction using high-resolution in-beam g-spectroscopy at HORUS, Cologne, Germany, to contribute to the existing experimental data base. So far, we only investigated the high-energy part of the Gamow window and the analysis is still in progress. We plan to study the second reaction in standard kinematics at the FRANZ facility, Frankfurt, Germany. Current developments at FRANZ will be explained in detail.

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Author:Kerstin SonnabendGND, Ceyhun Arda, Anne EndresGND, Philipp ErbacherORCiDGND, Jan GloriusORCiDGND, Kathrin GöbelORCiDGND, Ole Djürko HinrichsGND, Markus ReichORCiDGND, Benedikt Thomas, Taniya Thomas
URN:urn:nbn:de:hebis:30:3-365850
URL:http://pos.sissa.it/archive/conferences/204/027/NIC%20XIII_027.pdf
ISSN:1824-8039
Parent Title (English):Proceedings of Science
Publisher:SISSA
Place of publication:Trieste
Document Type:Conference Proceeding
Language:English
Year of Completion:2014
Year of first Publication:2014
Publishing Institution:Universitätsbibliothek Johann Christian Senckenberg
Release Date:2015/05/28
Issue:(NIC XIII)027
Page Number:8
First Page:1
Last Page:8
Note:
(c) Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.
HeBIS-PPN:41756435X
Institutes:Physik / Physik
Dewey Decimal Classification:5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik
Sammlungen:Universitätspublikationen
Licence (German):License LogoCreative Commons - Namensnennung-Weitergabe unter gleichen Bedingungen