Breaking black-hole uniqueness at supermassive scales

被引:2
作者
Eichhorn, Astrid [1 ,2 ]
Fernandes, Pedro G. S. [1 ,2 ]
Held, Aaron [3 ]
Silva, Hector O. [4 ,5 ,6 ]
机构
[1] Univ Southern Denmark, CP3 Origins, Campusvej 55, DK-5230 Odense M, Denmark
[2] Heidelberg Univ, Inst Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany
[3] Univ Paris Cite, Univ PSL, Sorbonne Univ,Inst Phys Theor Philippe Meyer, Lab Phys,Ecole normale Super ENS, F-75005 Paris, France
[4] Univ Illinois, Dept Phys, Urbana, IL 61801 USA
[5] Univ Illinois, Illinois Ctr Adv Studies Universe, Urbana, IL 61801 USA
[6] Max Planck Inst Grav Phys Albert Einstein Inst, D-14476 Potsdam, Germany
关键词
black hole; scalarization; supermassive; modified gravity; black hole uniqueness; hairy black hole; TELESCOPE RESULTS. VI; FIELD; EQUATION; PHYSICS; MATTER; SPACE; STATE; MASS;
D O I
10.1088/1361-6382/add3b6
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In general relativity (GR), all asymptotically flat, stationary and axisymmetric vacuum black holes are described by the Kerr solution. Beyond GR, there is a prevailing expectation that deviations from the Kerr solution increase with the horizon curvature. We challenge this expectation by showing that, in a scalar-Gauss-Bonnet theory, black holes scalarize in a finite, adjustable window of black-hole masses, bounded from above and below. In this theory, there is an interplay between curvature scales and compactness, which we expect to protect neutron stars and other less compact objects from scalarization. In addition, this theory is the first to avoid the catastrophic instability of early-Universe cosmology that affects previous scalarization models. In this theory, black-hole uniqueness can be broken at supermassive black-hole scales, while stellar-mass black holes remain well-described by the general relativistic solution. To probe this scenario, observations targeting supermassive black holes are necessary.
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页数:12
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