Testing general relativity with the event horizon telescope

DOI10.1007/s10714-019-2611-5zbMath1434.83074arXiv1806.09740OpenAlexW2810784386MaRDI QIDQ2281392

Dimitrios Psaltis

Publication date: 19 December 2019

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1806.09740

zbMATH Keywords

black holesM87Milky Waygravitational physicsaccretion physics

Mathematics Subject Classification ID

Black holes (83C57) Observational and experimental questions in relativity and gravitational theory (83B05) Galactic and stellar structure (85A15) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (16)

Testing no-hair theorem by quasi-periodic oscillations: the quadrupole of GRO J1655–40 ⋮ Magnetically charged black holes from non-linear electrodynamics and the Event Horizon Telescope ⋮ Shadows and optical appearance of black bounces illuminated by a thin accretion disk ⋮ Rotating black holes in 4D Einstein-Gauss-Bonnet gravity and its shadow ⋮ Black hole solutions in scalar-tensor symmetric teleparallel gravity ⋮ Gravity at the tip of the throat ⋮ Shadows and photon rings of regular black holes and geonic horizonless compact objects ⋮ Non-commutative inspired black holes in Euler-Heisenberg non-linear electrodynamics ⋮ Generalized no-hair theorems without horizons ⋮ Spontaneous scalarisation of charged black holes: coupling dependence and dynamical features ⋮ Infinitely degenerate exact Ricci-flat solutions in f(R) gravity ⋮ EHT tests of the strong-field regime of general relativity ⋮ Topical collection: testing the Kerr spacetime with gravitational-wave and electromagnetic observations ⋮ Calculating black hole shadows: review of analytical studies ⋮ Analytical study of gravitational lensing in Kerr-Newman black-bounce spacetime ⋮ Double shadows of reflection-asymmetric wormholes supported by positive energy thin-shells

Cites Work

• Unnamed Item
• Black holes: complementarity or firewalls?
• Probes and tests of strong-field gravity with observations in the electromagnetic spectrum
• Spherical photon orbits around a Kerr black hole
• Shadows of Kerr black holes with and without scalar hair
• Possible imprints of cosmic strings in the shadows of galactic black holes
• Shape and position of the shadow in the δ = 2 Tomimatsu–Sato spacetime
• Testing the black hole no-hair theorem at the galactic center: perturbing effects of stars in the surrounding cluster
• Publisher’s Note: Kerr Black Holes Are Not Unique to General Relativity [Phys. Rev. Lett.100, 091101 (2008)]
• The apparent shape of a rotating charged black hole, closed photon orbits and the bifurcation set A ₄
• STU black holes and SgrA^⋆
• Shadow casted by a Konoplya-Zhidenko rotating non-Kerr black hole
• Observing the shadow of modified gravity black hole
• The confrontation between general relativity and experiment

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