In this paper, we have studied the stability of neutron stars in the background of Palatini f(R, T) gravity. In this context, the static spherically symmetric geometry is considered which is assumed to be coupled with an isotropic matter configurations. The evolution of the system is considered with the help of Tolman–Oppenheimer–Volkoff equations and conformal transformations. We found the stable configurations of the spherical stars with some constraints.
机构:
Univ Fed Santa Catarina, CFM, Dept Fis, CP 476, BR-88040900 Florianopolis, SC, BrazilUniv Fed Santa Catarina, CFM, Dept Fis, CP 476, BR-88040900 Florianopolis, SC, Brazil
Mota, Clesio E.
Pretel, Juan M. Z.
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Ctr Brasileiro Pesquisas Fis, Rua Dr Xavier Sigaud,150 URCA, BR-22290180 Rio De Janeiro, RJ, BrazilUniv Fed Santa Catarina, CFM, Dept Fis, CP 476, BR-88040900 Florianopolis, SC, Brazil
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Univ Lisbon, Inst Super Tecn, CENTRA, Ave Rovisco Pais 1, Lisbon, PortugalUniv Lisbon, Inst Super Tecn, CENTRA, Ave Rovisco Pais 1, Lisbon, Portugal