Dark matter effects in modified teleparallel gravity

被引:3
|
作者
Vilhena, S. G. [1 ,3 ]
Dutra, M. [1 ,2 ]
Lourenco, O. [1 ,2 ]
Pompeia, P. J. [1 ]
机构
[1] Inst Tecnol Aeronaut, Dept Fis, DCTA, BR-12228900 Sao Jose Dos Campos, SP, Brazil
[2] Univ Claude Bernard Lyon 1, Univ Lyon, CNRS, IP2I Lyon,IN2P3,UMR 5822, CNRS-IN2P3, IP2I Lyon, UMR 5822, F-69622 Villeurbanne, France
[3] Ctr Brasileiro Pesquisas Fis, Rua Dr Xavier Sigaud,150 URCA, BR-22290180 Rio De Janeiro, RJ, Brazil
基金
巴西圣保罗研究基金会;
关键词
MILLISECOND PULSAR; NEUTRON-STARS; MASS; GALAXIES; PHYSICS; RANGE;
D O I
10.1103/PhysRevD.108.104051
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This work investigates dark matter (DM) effects in compact objects in modified teleparallel gravity (MTG) in which a modification of teleparallel equivalent to general relativity is used. We applied a tetrad to the modified field equations where a set of relations is found. The conservation equation allows us to rewrite our Tolman-Oppenheimer-Volkoff equations with an effective gravitational coupling constant. As input to these new equations, we use a relativistic mean-field (RMF) model with dark matter content included, obtained from a Lagrangian density with both, hadronic and dark particle degrees of freedom, as well as the Higgs boson, used as a mediator in both sectors of the theory. Through numerical calculations, we analyze the mass-radius diagrams obtained from different parametrizations of the RMF-DM model, generated by assuming different values of the dark particle Fermi momentum and running the free parameter coming from the MTG. Our results show that it is possible for the system simultaneously support more DM content, and be compatible with recent astrophysical data provided by the LIGO and Virgo Collaborations, as well as by NASA's Neutron star Interior Composition Explorer (NICER).
引用
收藏
页数:9
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