Event horizon silhouette: implications to supermassive black holes M87* and SgrA*
arXiv:1903.09594 · doi:10.1007/s10714-019-2564-8
Abstract
We demonstrate that a dark silhouette of the black hole illuminated by a thin accretion disk and seen by a distant observer is, in fact, a silhouette of the event horizon hemisphere. The boundary of this silhouette is a contour of the event horizon equatorial circle if a thin accretion disk is placed in the black hole equatorial plane. A luminous matter plunging into black hole from different directions provides the observational opportunity for recovering a total silhouette of the invisible event horizon globe. The event horizon silhouette is projected on the celestial sphere within a position of the black hole shadow. A relative position of brightest point in the accretion disk with respect to the position of event horizon silhouette in the image of black hole in the galaxy M87, observed by the Event Horizon Telescope, corresponds to a rather high value of the black hole spin, .
arXiv comment17 pages, 12 figures, references added, accepted to Gen. Rel. Gravit
References in corpus (26)
- Monitoring stellar orbits around the Massive Black Hole in the Galactic Center
- High Resolution Linear Polarimetric Imaging for the Event Horizon Telescope
- The Shortest Known Period Star Orbiting our Galaxy's Supermassive Black Hole
- Resolved Magnetic-Field Structure and Variability Near the Event Horizon of Sagittarius A*
- The old nuclear star cluster in the Milky Way: dynamics, mass, statistical parallax, and black hole mass
- Testing General Relativity with the Shadow Size of Sgr A*
- BlackHoleCam: fundamental physics of the Galactic center
- Sgr A* and General Relativity
- The Milky Way's Supermassive Black Hole: How good a case is it? A Challenge for Astrophysics & Philosophy of Science
- Millimeter Flares and VLBI Visibilities from Relativistic Simulations of Magnetized Accretion onto the Galactic Center Black Hole
- Gravitational Lensing by Spinning Black Holes in Astrophysics, and in the Movie Interstellar
- Line Emission from an Accretion Disk around a Rotating Black Hole: Toward a Measurement of Frame Dragging
- Modeling Seven Years of Event Horizon Telescope Observations with Radiatively Inefficient Accretion Flow Models
- Testing General Relativity with Accretion-Flow Imaging of Sgr A*
- A geometric crescent model for black hole images
- Imaging an Event Horizon: Mitigation of Source Variability of Sagittarius A*
- Physical laboratory at the center of the Galaxy
- Test of Einstein equivalence principle near the Galactic center supermassive black hole
- Constraining the distribution of dark matter at the Galactic centre using the high-resolution Event Horizon Telescope
- Spin and mass of the nearest supermassive black hole
- Quantifying Intrinsic Variability of Sagittarius A* using Closure Phase Measurements of the Event Horizon Telescope
- Bayesian techniques for comparing time-dependent GRMHD simulations to variable Event Horizon Telescope observations
- Testing General Relativity with the Black Hole Shadow Size and Asymmetry of Sagittarius A*: Limitations from Interstellar Scattering
- Seeing the unseeable
- To see invisible: image of the event horizon within the black hole shadow
- Tests of gravity theories with Galactic Center observations
Cited by in corpus (15)
- Shadow, lensing, quasinormal modes, greybody bounds and neutrino propagation by dyonic ModMax black holes
- Black hole shadow as a standard ruler in cosmology
- First analytical calculation of black hole shadow in McVittie metric
- Observational signature of a near-extremal Kerr-Sen black hole in the heterotic string theory
- Silhouettes of invisible black holes
- The brightest point in accretion disk and black hole spin: implication to the image of black hole M87*
- Spin oscillations of neutrinos scattered off a rotating black hole
- Modeling the motion of a bright spot in jets from black holes M87* and SgrA*
- Testing the Black Hole No-hair Theorem with Galactic Center Stellar Orbits
- Spins of supermassive black holes M87* and SgrA* revealed from the size of dark spots in Event Horizon Telescope Images
- Black Hole Shadow Observations with Space-Ground Interferometers
- Physical origin of the dark spot at the image of supermassive black hole SgrA* revealed by the EHT collaboration
- Visible shapes of black holes M87* and SgrA*
- Images of black holes viewed by distant observer
- Generalized Einstein-Rosen bridge inside black holes