The isothermal Tolman condition and the constancy of the Klein potentials originally expressed for the sole gravitational interaction in a single fluid are here generalized to the case of a three quantum fermion fluid duly taking into account the strong, electromagnetic, weak and gravitational interactions. The set of constitutive equations including the Einstein-Maxwell-Thomas-Fermi equations as well as the ones corresponding to the strong interaction description are here presented in the most general relativistic isothermal case. This treatment represents an essential step to correctly formulate a self-consistent relativistic field theoretical approach of neutron stars. (C) 2011 Elsevier B.V. All rights reserved.
The Klein first integrals in an equilibrium system with electromagnetic, weak, strong and gravitational interactions / A., Rueda Jorge; Ruffini, Remo; S. S., Xue. - In: NUCLEAR PHYSICS. A. - ISSN 0375-9474. - 872:1(2011), pp. 286-295. [10.1016/j.nuclphysa.2011.09.005]
The Klein first integrals in an equilibrium system with electromagnetic, weak, strong and gravitational interactions
RUFFINI, Remo;
2011
Abstract
The isothermal Tolman condition and the constancy of the Klein potentials originally expressed for the sole gravitational interaction in a single fluid are here generalized to the case of a three quantum fermion fluid duly taking into account the strong, electromagnetic, weak and gravitational interactions. The set of constitutive equations including the Einstein-Maxwell-Thomas-Fermi equations as well as the ones corresponding to the strong interaction description are here presented in the most general relativistic isothermal case. This treatment represents an essential step to correctly formulate a self-consistent relativistic field theoretical approach of neutron stars. (C) 2011 Elsevier B.V. All rights reserved.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
