N=82Shell Quenching of the Classicalr-Process “Waiting-Point” NucleusCd130-Reference-Cited by-同舟云学术

N=82Shell Quenching of the Classicalr-Process “Waiting-Point” NucleusCd130

Published:2003-10-16 Issue:16 Volume:91 Page:
ISSN:0031-9007
Container-title:Physical Review Letters
language:en
Short-container-title:Phys. Rev. Lett.

Author:

Dillmann I.,Kratz K.-L.,Wöhr A.,Arndt O.,Brown B. A.,Hoff P.,Hjorth-Jensen M.,Köster U.,Ostrowski A. N.,Pfeiffer B.,Seweryniak D.,Shergur J.,Walters W. B.

Publisher

American Physical Society (APS)

Subject

General Physics and Astronomy

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevLett.91.162503/fulltext

Reference27 articles.

1. Synthesis of the Elements in Stars

2. The chemistry of creation of the heavy elements

3. The beta-decay half-life of 48 130 Cd82 and its importance for astrophysicalr-process scenarios

4. Constraints on r-process conditions from beta-decay properties far off stability and r-abundances

5. Nuclear structure studies for the astrophysical r-process

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