2012/10/31 by Zhong-Ming Niu, Z. M. Niu, Y. F. Niu +10 · 1 citation
Physics and Astronomy · #Astronomical and nuclear sciences #Atomic physics #Double beta decay #Isoscalar #Neutrino #Neutron #Nuclear matter #Nuclear physics #Nuclear physics research studies #Nuclear reaction #Nucleon #Nucleosynthesis #Pairing #Particle physics #Physics #Proton #Quantum Chromodynamics and Particle Interactions #Quantum mechanics #Quasiparticle #Random phase approximation #astro-ph.SR #nucl-ex #nucl-th #r-process
paper · pdf · doi:10.1016/j.physletb.2013.04.048
published as Phys. Lett. B 723, 172-176 (2013) · 14 pages, 4 figures
openalex publication_date 2013/04/27 · arxiv created 2013/05/24 · arxiv updated 2013/05/27 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
The β-decay half-lives of neutron-rich nuclei with 20≤Z≤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 β-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≳140, an important result for the understanding of the origin of heavy elements in the universe.