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No-Hair Theorem in the Wake of Event Horizon Telescope

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TLDR
In this paper, the authors used the EHT image of shadow attributed to the M87* supermassive black hole (SMBH) to assess the validity of fundamental physics in the strong-field regime.
Abstract
Thanks to the release of the extraordinary EHT image of shadow attributed to the M87* supermassive black hole (SMBH), we have a novel window to assess the validity of fundamental physics in the strong-field regime. Motivated by this, we consider Johannsen \& Psaltis metric parameterized by mass, spin, and an additional dimensionless hair parameter $\epsilon$ which in the high rotation regimes is able to provide a suitable framework for the test of the no-hair theorem (NHT) using the EHT data. Incorporating the $\epsilon$ into the standard Kerr spacetime enrich it in the sense that, depending on setting the positive and negative values for that, we deal with alternative compact objects: deformed Kerr naked singularity and Kerr BH solutions, respectively. Shadows associated with these two possible solutions indicate that the deformation parameter $\epsilon$ affects the geometry shape of standard shadow such that it become more oblate and prolate with $\epsilon 0$, respectively. By scanning the window associated with three shadow observables: oblateness, deviation from circularity, and shadow diameter, we perform a numerical analysis within the range $a_*=0.9\mp0.1$ of the dimensionless rotation parameter, to find the constraints on the hair parameter $\epsilon$ in both possible solutions. For both possible signs of $\epsilon$, we extract a variety of upper bounds that are in interplay with $a_*$. Our analysis suggests that as the rotation parameter approaches the extreme limit, although the allowable range of both hair parameters becomes narrower, the hairy Kerr BH solution is a more promising candidate to play a role of the alternative compact object instead of standard Kerr BH. The lack of tension between hairy Kerr BH with the current observation of the EHT shadow of the M87* SMBH carries this message that the possibility of NHT violation is not excluded.

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Citations
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Journal ArticleDOI

Superradiance evolution of black hole shadows revisited

TL;DR: In this article , the superradiance-induced BH shadow evolution was studied in the presence of two ultralight bosons, whose combined effect could help reduce the shadow evolution time scale.
Journal ArticleDOI

Superradiant evolution of the shadow and photon ring of Sgr <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi mathvariant="normal">A</mml:mi></mml:mrow><mml:mrow><mml:mo>⋆</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math>

TL;DR: In this paper , the shadow drift and the variation in the azimuthal angle lapse associated to the photon ring autocorrelation were studied for the supermassive object Sgr A$^\star.
Journal ArticleDOI

Testing dynamical torsion effects on the charged black hole’s shadow, deflection angle and greybody with M87* and Sgr. A* from EHT

Reggie C. Pantig, +1 more
- 05 Jun 2022 - 
TL;DR: In this article , the authors used Reissner-Nordstrom de Sitter and anti-de Sitter solutions to analyze the weak deflection angles of massive and null particles in finite distance regime.
Journal ArticleDOI

Shadow, lensing, quasinormal modes, greybody bounds and neutrino propagation by dyonic ModMax black holes

TL;DR: In this article , the effect of the ModMax parameters on the shadow cast, weak field gravitational lensing, and neutrino propagation in the vicinity of a dyonic ModMax black hole was investigated.
Journal ArticleDOI

Strong gravitational lensing and shadow constraint from M87* of slowly rotating Kerr-like black hole

Xiaomei Kuang, +1 more
- 23 May 2022 - 
TL;DR: In this paper , the authors apply the Einstein bumblebee gravity with Lorentz violation (LV) to the study of strong gravitational lensing effect and the black hole shadow of slowly rotating Kerr-like black hole.
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