[Users] non vacuum binary neutron star

[黃世杰]

If I want to simulate the situation of the binary neutron star with the gas
surrounding, and the gas can be in different density and different velocity
distribution, how could I do ?(Should I insert the thorns
"GRHydro_InitData"and "EOS_Polytrope" into the parameter file of binary
neutron stars--"NsNsToHMNS.par" ?)





Best,
Shih-Jie
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