2 papers
nucl-th2019
The APR equation of state for simulations of supernovae, neutron stars and binary mergers
A. S. Schneider, C. Constantinou, B. Muccioli +1
Differences in the equation of state (EOS) of dense matter translate into differences in astrophysical simulations and their multi-messenger signatures. Thus, extending the number…
nucl-th2015
Degenerate limit thermodynamics beyond leading order for models of dense matter
Constantinos Constantinou, Brian Muccioli, Madappa Prakash +1
Analytical formulas for next-to-leading order temperature corrections to the thermal state variables of interacting nucleons in bulk matter are derived in the degenerate limit. The…