Rapidly rotating compact stars in Rastall’s gravity
Franciele M. da SilvaDepartamento de Física, CFM—Universidade Federal de Santa Catarina; C.P. 476, CEP 88.040-900, Florianópolis, SC, BrazilL C N SantosDepartamento de Física, CCEN—Universidade Federal da Paraíba; C.P. 5008, CEP 58.051-970, João Pessoa, PB, BrazilC C BarrosDepartamento de Física, CFM—Universidade Federal de Santa Catarina; C.P. 476, CEP 88.040-900, Florianópolis, SC, Brazil
2021en
ABI
Аннотация
Abstract In this work we study rapidly rotating stars by considering the Rastall theory of gravity. We obtain and solve the equations by numerical methods for two usual parametrization of polytropic stars. Then the mass–radius relations, moments of inertia and other results of interest are obtained and compared with the ones for non-rotating stars.
Ҳали таржима қилинмаган
Идентификаторлар
Иқтибослар ва манбалар
3 та иқтибос0 та фойдаланилган манба