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Nuclear physics of the outer layers of accreting neutron stars
Now 50 years since the existence of the neutron star crust was proposed, we review the
current understanding of the nuclear physics of the outer layers of accreting neutron stars …
current understanding of the nuclear physics of the outer layers of accreting neutron stars …
[HTML][HTML] Stellar weak-interaction rates for rp-process waiting-point nuclei from projected shell model
ZR Chen, LJ Wang - Physics Letters B, 2024 - Elsevier
We propose a projected shell model (PSM) for description of stellar weak-interaction rates
between even-even and odd-odd nuclei with extended configuration space where up to six …
between even-even and odd-odd nuclei with extended configuration space where up to six …
Sensitivity studies on the excited states of nuclei in beta decays in the r-process of neutron star mergers
R Lau - Journal of Physics G: Nuclear and Particle Physics, 2020 - iopscience.iop.org
Sensitivity studies conducted in this paper aim to examine the influence of uncertainties in
beta decay rates on simulations of rapid neutron capture (r-process) nucleosynthesis …
beta decay rates on simulations of rapid neutron capture (r-process) nucleosynthesis …
Sensitivity studies on the thermal beta+ decay and thermal neutrino decay rates in the one-zone X-ray burst model
R Lau - Monthly Notices of the Royal Astronomical Society, 2020 - academic.oup.com
We investigated how the thermal beta+ decay rates and their corresponding neutrino energy
loss rates affect the properties of X-ray bursts. Previous studies carried out showed how the …
loss rates affect the properties of X-ray bursts. Previous studies carried out showed how the …
Sensitivity studies on the thermal beta+decay and thermal neutrino loss rates in the multizone X-ray burst model mesa
R Lau - Monthly Notices of the Royal Astronomical Society, 2022 - academic.oup.com
Recently, it has been discovered that the beta+ decay rates and neutrino loss rates of 64Ga
and 68Se greatly affect the light curves and final abundances of X-ray bursts in a one-zone …
and 68Se greatly affect the light curves and final abundances of X-ray bursts in a one-zone …