Equation of State ===================== The EoS input file **is required** if the options **use_beta_equilibrium** or **use_charge_neutrality** are enabled. It must contain the following columns, presented in order: +----------------------------------------------------+------------------+ | **Variable** | **Unit** | +====================================================+==================+ | Temperature (T) | MeV | +----------------------------------------------------+------------------+ | Baryon chemical potential (:math:`\mu_B`) | MeV | +----------------------------------------------------+------------------+ | Strange chemical potential (:math:`\mu_S`) | MeV | +----------------------------------------------------+------------------+ | Electric charge chemical potential (:math:`\mu_Q`) | MeV | +----------------------------------------------------+------------------+ | Baryon density (:math:`n_B`) | fm\ :sup:`-3` | +----------------------------------------------------+------------------+ | Strange density (:math:`n_S`) | fm\ :sup:`-3` | +----------------------------------------------------+------------------+ | Electric charge density (:math:`n_Q`) | fm\ :sup:`-3` | +----------------------------------------------------+------------------+ | Energy density (:math:`\varepsilon`) | MeV/fm\ :sup:`3` | +----------------------------------------------------+------------------+ | Pressure (:math:`P`) | MeV/fm\ :sup:`3` | +----------------------------------------------------+------------------+ | Entropy density (:math:`s`) | 1/fm\ :sup:`3` | +----------------------------------------------------+------------------+ If your model distinguishes between the 'physical' baryon density (:math:`n_B= \partial P/\partial \mu_B`) and the total baryon density resulting sum of particle densities (:math:`n_B^{particles}= \sum_i B_i n_i`), please pass the physical baryon density in the fifth EoS file, and append the particle baryon density in the last (11th) column, in fm\ :sup:`-3`. This happens, for example, in models with a potential that is an explicit functions of :math:`\mu_B`. This is crucial if neutrinos are used, as the code will calculate the lepton fraction from the particle baryon density (:math:`Y_L= n_L / n_B^{particles}`), if provided.