New calculations of gross β-decay properties for astrophysical applications: Speeding-up the classical r process

Peter Möller, Bernd Pfeiffer, and Karl-Ludwig Kratz
Phys. Rev. C 67, 055802 – Published 19 May 2003
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Abstract

Recent compilations of experimental gross β-decay properties, i.e., half-lives (T1/2) and neutron-emission probabilities (Pn), are compared to improved global macroscopic-microscopic model predictions. The model combines calculations within the quasiparticle (QP) random-phase approximation for the Gamow-Teller (GT) part with an empirical spreading of the QP strength and the gross theory for the first-forbidden part of β decay. Nuclear masses are either taken from the 1995 data compilation of Audi et al., when available, otherwise from the finite-range droplet model. Especially for spherical and neutron-(sub-)magic isotopes a considerable improvement compared to our earlier predictions for pure GT decay (ADNDT, 1997) is observed. T1/2 and Pn values up to the neutron drip line have been used in r-process calculations within the classical “waiting-point” approximation. With the new nuclear-physics input, a considerable speeding-up of the r-matter flow is observed, in particular at those r-abundance peaks which are related to magic neutron-shell closures.

  • Received 30 May 2002

DOI:https://doi.org/10.1103/PhysRevC.67.055802

©2003 American Physical Society

Authors & Affiliations

Peter Möller

  • Theoretical Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545

Bernd Pfeiffer and Karl-Ludwig Kratz

  • Institut für Kernchemie, Universität Mainz, Germany

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Vol. 67, Iss. 5 — May 2003

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