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Core-collapse supernova equations of state based on neutron star observations
Andrew W. Steiner, Matthias Hempel, Tobias Fischer
Many of the currently available equations of state for core-collapse supernova simulations give large neutron star radii and do not provide large enough neutron star masses, both o…
The Neutron Star Mass-Radius Relation and the Equation of State of Dense Matter
Andrew W. Steiner, James M. Lattimer, Edward F. Brown
The equation of state (EOS) of dense matter has been a long-sought goal of nuclear physics. Equations of state generate unique mass versus radius (M-R) relations for neutron stars,…
Constraints on the symmetry energy and neutron skins from experiments and theory
M. B. Tsang, J. R. Stone, F. Camera +16
The symmetry energy contribution to the nuclear Equation of State (EoS) impacts various phenomena in nuclear astrophysics, nuclear structure, and nuclear reactions. Its determinati…
Deep Crustal Heating in a Multicomponent Accreted Neutron Star Crust
Andrew W. Steiner
A quasi-statistical equilibrium model is constructed to simulate the multicomponent composition of the crust of an accreting neutron star. The ashes of rp-process nucleosynthesis a…