New black hole solutions with a dynamical traceless nonmetricity tensor in Metric-Affine Gravity

被引:14
作者
Bahamonde, Sebastian [1 ,2 ]
Chevrier, Johann [3 ]
Valcarcel, Jorge Gigante [2 ]
机构
[1] Tokyo Inst Technol, Dept Phys, 1-12-1 Ookayama,Meguro Ku, Tokyo 1528551, Japan
[2] Univ Tartu, Inst Phys, Lab Theoret Phys, W Ostwaldi 1, EE-50411 Tartu, Estonia
[3] Ecole Normale Super Paris Saclay, Dept Enseignement & Rech Phys, Ave Sci 4, F-91190 Gif Sur Yvette, France
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2023年 / 02期
关键词
astrophysical black holes; Exact solutions; black holes and black hole thermodynamics in GR and beyond; modified gravity; stars; POINCARE GAUGE-THEORY; GENERAL-RELATIVITY; VACUUM SOLUTION; FIELD; TORSION; IDENTITIES; SPIN;
D O I
10.1088/1475-7516/2023/02/018
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In the framework of Metric-Affine Gravity, the existing correspondence between the Einstein tensor and the energy-momentum tensor of matter provided by General Relativity is extended towards a post-Riemannian description in terms of the torsion and nonmetricity fields, which are sourced by the spin, dilation and shear currents of matter. In this work, we focus on the dynamical role of the traceless part of the nonmetricity tensor and its intrinsic connection with shears, defining a model which encloses a new black hole solution endowed with shear charges. We show that the extension in the presence of dynamical torsion and Weyl vector leads to the broadest family of static and spherically symmetric black hole solutions with spin, dilation and shear charges in Metric-Affine Gravity so far.
引用
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页数:27
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