Zobrazeno 1 - 5
of 5
pro vyhledávání: '"César V. Flores"'
Autor:
Clésio E. Mota, Luis C. N. Santos, Franciele M. da Silva, César V. Flores, Iarley P. Lobo, Valdir B. Bezerra
Publikováno v:
Universe, Vol 9, Iss 6, p 260 (2023)
In this work, we investigate the existence of neutron stars (NS) in the framework of f(T,T) gravity, where T is the torsion tensor and T is the trace of the energy–momentum tensor. The hydrostatic equilibrium equations are obtained, however, with p
Externí odkaz:
https://doaj.org/article/f7cb54f76ae6460ebe8c12f064c5650d
Autor:
Bezerra, Clésio E. Mota, Luis C. N. Santos, Franciele M. da Silva, César V. Flores, Iarley P. Lobo, Valdir B.
Publikováno v:
Universe; Volume 9; Issue 6; Pages: 260
In this work, we investigate the existence of neutron stars (NS) in the framework of f(T,T) gravity, where T is the torsion tensor and T is the trace of the energy–momentum tensor. The hydrostatic equilibrium equations are obtained, however, with p
Autor:
Clésio E Mota, Luis C N Santos, Franciele M da Silva, César V Flores, Tiago J N da Silva, Débora P Menezes
Publikováno v:
Classical and Quantum Gravity. 39:085008
In this work, we investigate anisotropic effects on the equations of state (EoS) used to describe neutron and quark stars in the framework of Rastall–Rainbow gravity. All our calculations are computed using two different EoS to describe the matter
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 82, Iss 6, Pp 1-13 (2022)
Abstract In this work, we have made a systematic study of how the gravitational wave frequency of the fundamental mode from compact stars is affected by anisotropic effects using realistic equations of state. Our study is an extension of the seminal
Externí odkaz:
https://doaj.org/article/94845c689faf4fc6a261bfb43725fad7
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 80, Iss 12, Pp 1-15 (2020)
Abstract Motivated by the recent gravitational wave detection by the LIGO–VIRGO observatories, we study the Love number and dimensionless tidal polarizability of highly magnetized stars. We also investigate the fundamental quasi-normal mode of neut
Externí odkaz:
https://doaj.org/article/6e8dc4c83f074c119a3221c13890def0