Abstract: bamr is an MPI implementation of a Bayesian analysis of neutron star mass and radius data that determines the mass versus radius curve and the equation of state of dense matter. Written in C++, bamr provides some EOS models. This code requires O2scl (ascl:1408.019) be installed before compilation.
Credit: Steiner, Andrew W.
Site: https://isospin.roam.utk.edu/static/cod ... index.html
Preferred citation method: http://adsabs.harvard.edu/abs/2014ascl.soft08020S