Equation of State
The beta-equilibrated nuclear EoS’ input files are required. It must contain the following columns, presented in order:
Variable |
Unit |
|---|---|
Temperature (T) |
MeV |
Baryon chemical potential (\(\mu_B\)) |
MeV |
Strange chemical potential (\(\mu_S\)) |
MeV |
Electric charge chemical potential (\(\mu_Q\)) |
MeV |
Baryon density (\(n_B\)) |
fm-3 |
Strange density (\(n_S\)) |
fm-3 |
Electric charge density (\(n_Q\)) |
fm-3 |
Energy density (\(\varepsilon\)) |
MeV/fm3 |
Pressure (\(P\)) |
MeV/fm3 |
Entropy density (\(s\)) |
1/fm3 |
The grid nuclear EoS’ and the Lepton EoS input files are required only for the Gibbs phase transition. The grids follow the same format as the beta-equilibrated nuclear EoS, and the lepton EoS file must contain the following columns:
Variable |
Unit |
|---|---|
Temperature (T) |
MeV |
Electron chemical potential (\(\mu_e\)) |
MeV |
Neutrino chemical potential (\(\mu_\nu\)) |
MeV |
Lepton density (\(n_L\)) |
fm-3 |
Electric charge density (\(n_Q\)) |
fm-3 |
Energy density (\(\varepsilon\)) |
MeV/fm3 |
Pressure (\(P\)) |
MeV/fm3 |
Entropy density (\(s\)) |
1/fm3 |