The nuclear equation of state (EOS) is at the center of numerous theoretical and
experimental efforts in nuclear physics. With advances in microscopic theories for nuclear …

The discovery of neutrinoless β β decay could soon be within reach. This hypothetical
ultrarare nuclear decay offers a privileged portal to physics beyond the standard model of …

In recent years our understanding of the dense matter equation of state (EOS) of neutron
stars has significantly improved by analyzing multimessenger data from radio/X-ray pulsars …

The production of about half of the heavy elements found in nature is assigned to a specific
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …

The nuclear matrix elements that govern the rate of neutrinoless double beta decay must be
accurately calculated if experiments are to reach their full potential. Theorists have been …

We introduce a new framework for quantifying correlated uncertainties of the infinite-matter
equation of state derived from chiral effective field theory (χ EFT). Bayesian machine …

The dense matter equation of state (EOS) determines neutron star (NS) structure but can be
calculated reliably only up to one to two times the nuclear saturation density, using accurate …

Both the mass and radius of the millisecond pulsar PSR J0030+ 0451 have been inferred
via pulse-profile modeling of X-ray data obtained by NASA's Neutron Star Interior …

Abstract The Neutron Star Interior Composition Explorer collaboration recently published a
joint estimate of the mass and the radius of PSR J0030+ 0451, derived via X-ray pulse …

The correlation of the tidal polarizabilities Λ 1-Λ 2 for GW170817 is predicted by combining
dense-matter equations of state (EOSs) that satisfy nuclear physics constraints with the chirp …