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arxiv: 1210.0680 · v2 · pith:PDSXHTGAnew · submitted 2012-10-02 · ⚛️ nucl-th · astro-ph.SR· nucl-ex

β-decay half-lives of neutron-rich nuclei and matter flow in the r-process

classification ⚛️ nucl-th astro-ph.SRnucl-ex
keywords betadecayhalf-livesneutron-richnucleielementsflowleqslant
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The $\beta$-decay half-lives of neutron-rich nuclei with $20 \leqslant Z \leqslant 50$ are systematically investigated using the newly developed fully self-consistent proton-neutron quasiparticle random phase approximation (QRPA), based on the spherical relativistic Hartree-Fock-Bogoliubov (RHFB) framework. Available data are reproduced by including an isospin-dependent proton-neutron pairing interaction in the isoscalar channel of the RHFB+QRPA model. With the calculated $\beta$-decay half-lives of neutron-rich nuclei a remarkable speeding up of $r$-matter flow is predicted. This leads to enhanced $r$-process abundances of elements with $A \gtrsim 140$, an important result for the understanding of the origin of heavy elements in the universe.

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