Electron Capture Rates on Nuclei and Implications for Stellar Core Collapse-Reference-Cited by-同舟云学术

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Electron Capture Rates on Nuclei and Implications for Stellar Core Collapse

Published:2003-06-19 Issue:24 Volume:90 Page:
ISSN:0031-9007
Container-title:Physical Review Letters
language:en
Short-container-title:Phys. Rev. Lett.

Author:

Langanke K.,Martínez-Pinedo G.,Sampaio J. M.,Dean D. J.,Hix W. R.,Messer O. E. B.,Mezzacappa A.,Liebendörfer M.,Janka H.-Th.,Rampp M.

Publisher

American Physical Society (APS)

Subject

General Physics and Astronomy

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevLett.90.241102/fulltext

Reference27 articles.

1. Stellar weak-interaction rates for sd-shell nuclei. I - Nuclear matrix element systematics with application to Al-26 and selected nuclei of importance to the supernova problem

2. Stellar weak interaction rates for intermediate mass nuclei. III - Rate tables for the free nucleons and nuclei with A = 21 to A = 60

3. Stellar weak interaction rates for intermediate-mass nuclei. II - A = 21 to A = 60

4. Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range in supernovae environments

5. RATE TABLES FOR THE WEAK PROCESSES OF pf-SHELL NUCLEI IN STELLAR ENVIRONMENTS

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