The Klein first integrals in an equilibrium system with electromagnetic, weak, strong and gravitational interactions

摘要

The isothermal Tolman condition and the constancy of the Klein potentialsoriginally expressed for the sole gravitational interaction in a single fluidare here generalized to the case of a three quantum fermion fluid duly takinginto account the strong, electromagnetic, weak and gravitational interactions.The set of constitutive equations including the Einstein-Maxwell-Thomas-Fermiequations as well as the ones corresponding to the strong interactiondescription are here presented in the most general relativistic isothermalcase. This treatment represents an essential step to correctly formulate aself-consistent relativistic field theoretical approach of neutron stars.