Electron capture in highly evolved stars

Details Electron capture in highly evolved stars Electron capture in highly evolved stars

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pthph..54.1339e&link_type=abstract

Progress of Theoretical Physics, vol. 54, Nov. 1975, p. 1339-1355. Research supported by the Ministry of Education and Universi

Physics

17

Electron Capture, Stellar Evolution, Beta Particles, Electron Transitions, Energy Dissipation, Reaction Kinetics, Tables (Data)

Scientific paper

Electron-capture rates in highly evolved stars are calculated within the framework of a beta-decay theory for about 130 nuclei near the beta stability line (Z values between 9 and 30; A values between 20 and 60). Special individual transitions whose contributions are important at relatively low densities and low temperatures are also examined separately. The numerical results for the electron capture rates are approximated by simple empirical formulas convenient for practical use.

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