Stellar equilibrium configurations of compact stars in f ( R , T ) theory of gravity

In this article we study the hydrostatic equilibrium configuration of neutron stars and strange stars, whose fluid pressure is computed from the equations of state p =ωρ{sup 5/3} and p =0.28(ρ−4B), respectively, with ω and B being constants and ρ the energy density of the fluid. We start by deriving...

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Veröffentlicht in:	Journal of cosmology and astroparticle physics 2016-06, Vol.2016 (6), p.5-5
Hauptverfasser:	Moraes, P.H.R.S., Arbañil, José D.V., Malheiro, M.
Format:	Artikel
Sprache:	eng
Schlagworte:	ASTROPHYSICS, COSMOLOGY AND ASTRONOMY CONFIGURATION ENERGY DENSITY ENERGY-MOMENTUM TENSOR EQUATIONS OF STATE EQUILIBRIUM GENERAL RELATIVITY THEORY GRAVITATION HYDROSTATICS MASS NEUTRON STARS PHYSICAL PROPERTIES PULSARS QUANTUM GRAVITY STARS
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