This is the TOV solver used in quickStar, for tabulated¹ (EoS/) or polytropic equations of state. The bindings used to expose the TOV class to JavaScript are located in src/bindings.cpp. The Tolman–Oppenheimer–Volkoff (TOV) system of ODEs is solved by implementing a C++11 version of LSODA², which has been slightly modified to fit the TOV class. Additionaly, some modules from the BOOST³ C++ library are used to interpolate the tabulated equations of state, and also to find the central pressure in polytropic equations of state.

Compile, using the provided makefile.

The executable inputs are specified using the following flags:

• -m EoS model ('p' for polytrope, 't' for tabulated)
• -f EoS name (EoS file name, if EoS is tabulated).
• -g Gamma (polytropic parameter, if EoS is polytropic)
• -k Kappa (polytropic parameter, if EoS is polytropic)
• -e central energy density (central energy density in CGS/10^15).
• -p print option:
  • 0: Prints gravitational mass M and radius R.
  • 1: Prints (0) along with the distance, metric, energy density and pressure profiles.

For example,

./TOV -m t -f ppsly4.cold.rns1.1.txt -e 2.5

./TOV -m p -g 2.0 -k 100.0 -e 2.5