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

K. Langanke, G. Martı́nez-Pinedo

Open source

DOI: 10.1016/s0375-9474(00)00131-7
Published: 2000-06
Container: Nuclear Physics A
Publisher: Elsevier BV
Open access: unknown

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Cite this work

BibTeX

@article{allodium:10.1016/s0375-9474-00-00131-7,
  title = {Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range in supernovae environments},
  author = {K. Langanke and G. Martı́nez-Pinedo},
  year = {2000},
  journal = {Nuclear Physics A},
  doi = {10.1016/s0375-9474(00)00131-7},
  url = {https://doi.org/10.1016/s0375-9474(00)00131-7}
}

RIS

TY  - JOUR
TI  - Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range in supernovae environments
AU  - K. Langanke
AU  - G. Martı́nez-Pinedo
PY  - 2000
JO  - Nuclear Physics A
DO  - 10.1016/s0375-9474(00)00131-7
UR  - https://doi.org/10.1016/s0375-9474(00)00131-7
ER  -

APA

Langanke, K., & Martı́nez-Pinedo, G. (2000). Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range in supernovae environments. Nuclear Physics A. https://doi.org/10.1016/s0375-9474(00)00131-7

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crossref · retrieved 2026-11-10T12:55:14.998Z