Nalazite se na CroRIS probnoj okolini. Ovdje evidentirani podaci neće biti pohranjeni u Informacijskom sustavu znanosti RH. Ako je ovo greška, CroRIS produkcijskoj okolini moguće je pristupi putem poveznice www.croris.hr
izvor podataka: crosbi

Spherically symmetric vacuum in covariant F(T) gravity theory (CROSBI ID 234231)

Prilog u časopisu | izvorni znanstveni rad | međunarodna recenzija

DeBenedictis, Andrew ; Ilijić, Saša Spherically symmetric vacuum in covariant F(T) gravity theory // Physical review. D, 94 (2016), 124025-1-124025-9. doi: 10.1103/PhysRevD.94.124025

Podaci o odgovornosti

DeBenedictis, Andrew ; Ilijić, Saša

engleski

Spherically symmetric vacuum in covariant F(T) gravity theory

Recently, a fully covariant version of the theory of F(T) torsion gravity has been introduced by M. Kršśák and E. Saridakis [Classical Quantum Gravity 33, 115009 (2016)]. In covariant F(T) gravity, the Schwarzschild solution is not a vacuum solution for F(T)≠T, and therefore determining the spherically symmetric vacuum is an important open problem. Within the covariant framework, we perturbatively solve the spherically symmetric vacuum gravitational equations around the Schwarzschild solution for the scenario with F(T)=T+(α/2)T2, representing the dominant terms in theories governed by Lagrangians analytic in the torsion scalar. From this, we compute the perihelion shift correction to solar system planetary orbits as well as perturbative gravitational effects near neutron stars. This allows us to set an upper bound on the magnitude of the coupling constant, α, which governs deviations from general relativity. We find the bound on this nonlinear torsion coupling constant by specifically considering the uncertainty in the perihelion shift of Mercury. We also analyze a bound from a similar comparison with the periastron orbit of the binary pulsar PSR J0045-7319 as an independent check for consistency. Setting bounds on the dominant nonlinear coupling is important in determining if other effects in the Solar System or greater universe could be attributable to nonlinear torsion.

Modified gravity theory ; F(T) gravity

nije evidentirano

nije evidentirano

nije evidentirano

nije evidentirano

nije evidentirano

nije evidentirano

Podaci o izdanju

94

2016.

124025-1-124025-9

objavljeno

2470-0010

2470-0029

10.1103/PhysRevD.94.124025

Povezanost rada

Fizika

Poveznice
Indeksiranost