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Title: Gamow-Teller strength distributions at finite temperatures and electron capture in stellar environments

Journal Article · · Physical Review. C, Nuclear Physics
;  [1];  [2];  [2];  [2];  [3]
  1. Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, RU-141980 Dubna (Russian Federation)
  2. Institut fuer Kernphysik, Technische Universitaet Darmstadt, D-64289 Darmstadt (Germany)
  3. GSI Helmholtzzentrum fuer Schwerionenforschung, Planckstr. 1, D-64291 Darmstadt (Germany)

We propose a new method to calculate stellar weak-interaction rates. It is based on the thermofield dynamics formalism and allows calculation of the weak-interaction response of nuclei at finite temperatures. The thermal evolution of the GT{sub +} distributions is presented for the sample nuclei {sup 54,56}Fe and {sup 76,78,80}Ge. For Ge we also calculate the strength distribution of first-forbidden transitions. We show that thermal effects shift the GT{sub +} centroid to lower excitation energies and make possible negative- and low-energy transitions. In our model we demonstrate that the unblocking effect for GT{sub +} transitions in neutron-rich nuclei is sensitive to increasing temperature. The results are used to calculate electron capture rates and are compared to those obtained from the shell model.

OSTI ID:
21388864
Journal Information:
Physical Review. C, Nuclear Physics, Vol. 81, Issue 1; Other Information: DOI: 10.1103/PhysRevC.81.015804; (c) 2010 The American Physical Society; ISSN 0556-2813
Country of Publication:
United States
Language:
English