Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A$^*$. (arXiv:2205.07787v1 [gr-qc])
<a href="http://arxiv.org/find/gr-qc/1/au:+Vagnozzi_S/0/1/0/all/0/1">Sunny Vagnozzi</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Roy_R/0/1/0/all/0/1">Rittick Roy</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Tsai_Y/0/1/0/all/0/1">Yu-Dai Tsai</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Visinelli_L/0/1/0/all/0/1">Luca Visinelli</a>

Horizon-scale images of black holes (BHs) and their shadows have opened an
unprecedented window onto tests of gravity and fundamental physics in the
strong-field regime, allowing us to test whether the Kerr metric provides a
good description of the space-time in the vicinity of the event horizons of
supermassive BHs. We consider a wide range of well-motivated deviations from
classical General Relativity solutions, and constrain them using the Event
Horizon Telescope (EHT) observations of Sagittarius A$^*$ (SgrA$^*$),
connecting the size of the bright ring of emission to that of the underlying BH
shadow and exploiting high-precision measurements of SgrA$^*$’s
mass-to-distance ratio. The scenarios we consider, and whose fundamental
parameters we constrain, include various regular BH models, string- and
non-linear electrodynamics-inspired space-times, scalar field-driven violations
of the no-hair theorem, alternative theories of gravity, new ingredients such
as the generalized uncertainty principle and Barrow entropy, and BH mimickers
including examples of wormholes and naked singularities. We demonstrate that
SgrA$^*$’s image places particularly stringent constraints on models predicting
a shadow size which is larger than that of a Schwarzschild BH of a given mass:
for instance, in the case of Barrow entropy we derive constraints which are
significantly tighter than the cosmological ones. Our results are among the
first tests of fundamental physics from the shadow of SgrA$^*$ and, while the
latter appears to be in excellent agreement with the predictions of General
Relativity, we have shown that various well-motivated alternative scenarios
(including BH mimickers) are far from being ruled out at present.

Horizon-scale images of black holes (BHs) and their shadows have opened an
unprecedented window onto tests of gravity and fundamental physics in the
strong-field regime, allowing us to test whether the Kerr metric provides a
good description of the space-time in the vicinity of the event horizons of
supermassive BHs. We consider a wide range of well-motivated deviations from
classical General Relativity solutions, and constrain them using the Event
Horizon Telescope (EHT) observations of Sagittarius A$^*$ (SgrA$^*$),
connecting the size of the bright ring of emission to that of the underlying BH
shadow and exploiting high-precision measurements of SgrA$^*$’s
mass-to-distance ratio. The scenarios we consider, and whose fundamental
parameters we constrain, include various regular BH models, string- and
non-linear electrodynamics-inspired space-times, scalar field-driven violations
of the no-hair theorem, alternative theories of gravity, new ingredients such
as the generalized uncertainty principle and Barrow entropy, and BH mimickers
including examples of wormholes and naked singularities. We demonstrate that
SgrA$^*$’s image places particularly stringent constraints on models predicting
a shadow size which is larger than that of a Schwarzschild BH of a given mass:
for instance, in the case of Barrow entropy we derive constraints which are
significantly tighter than the cosmological ones. Our results are among the
first tests of fundamental physics from the shadow of SgrA$^*$ and, while the
latter appears to be in excellent agreement with the predictions of General
Relativity, we have shown that various well-motivated alternative scenarios
(including BH mimickers) are far from being ruled out at present.

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