UTK EOSs for Astrophysical SimulationsΒΆ

This C++ code constructs the equation of state of homogeneous nucleonic matter for use in simulations of core-collapse supernovae and neutron star mergers. This code was originally described in a paper on arxiv.org. The source code is available on github. The installation of Boost, GSL (versions 1.16 and later), HDF5 (versions 1.8.14 and later), and the most current version of O2scl is required.

More documentation will be added as time permits.