Orbital motion near Sagittarius A*-Constraints from polarimetric ALMA observations
We report on the polarized light curves of the Galactic Center supermassive black hole
Sagittarius A*, obtained at millimeter wavelength with the Atacama Large Millimeter …
Sagittarius A*, obtained at millimeter wavelength with the Atacama Large Millimeter …
[PDF][PDF] Fundamental physics opportunities with the next-generation event horizon telescope
D Ayzenberg, L Blackburn, R Brito… - arXiv preprint arXiv …, 2023 - researchgate.net
Abstract The Event Horizon Telescope (EHT) Collaboration recently published the first
images of the supermassive black holes in the cores of the Messier 87 and Milky Way …
images of the supermassive black holes in the cores of the Messier 87 and Milky Way …
The shape of the black hole photon ring: A precise test of strong-field general relativity
SE Gralla, A Lupsasca, DP Marrone - Physical Review D, 2020 - APS
We propose a new test of strong-field general relativity (GR) based on the universal
interferometric signature of the black hole photon ring. The photon ring is a narrow ring …
interferometric signature of the black hole photon ring. The photon ring is a narrow ring …
Observing the inner shadow of a black hole: a direct view of the event horizon
Simulated images of a black hole surrounded by optically thin emission typically display two
main features: a central brightness depression and a narrow" photon ring" consisting of …
main features: a central brightness depression and a narrow" photon ring" consisting of …
Lensing by Kerr black holes
SE Gralla, A Lupsasca - Physical Review D, 2020 - APS
Interpreting horizon-scale observations of astrophysical black holes demands a general
understanding of null geodesics in the Kerr spacetime. These may be divided into two …
understanding of null geodesics in the Kerr spacetime. These may be divided into two …
Images and photon ring signatures of thick disks around black holes
FH Vincent, SE Gralla, A Lupsasca… - Astronomy & …, 2022 - aanda.org
Context. High-frequency very-long-baseline interferometry (VLBI) observations can now
resolve the event-horizon-scale emission from sources in the immediate vicinity of nearby …
resolve the event-horizon-scale emission from sources in the immediate vicinity of nearby …
[HTML][HTML] Polarimetric signatures of hot spots in black hole accretion flows
J Vos, MA Mościbrodzka, M Wielgus - Astronomy & Astrophysics, 2022 - aanda.org
Context. The flaring events observed in the Sagittarius A* supermassive black hole system
can be attributed to the nonhomogeneous nature of the near-horizon accretion flow. Bright …
can be attributed to the nonhomogeneous nature of the near-horizon accretion flow. Bright …
Verification of radiative transfer schemes for the EHT
The Event Horizon Telescope (EHT) is a millimeterwavelength, Earth-sized very long
baseline interferometry experiment that has recently imaged the shadow of the black hole …
baseline interferometry experiment that has recently imaged the shadow of the black hole …
Photon ring astrometry for superradiant clouds
Gravitational atoms produced from the superradiant extraction of rotational energy of
spinning black holes can reach energy densities significantly higher than that of dark matter …
spinning black holes can reach energy densities significantly higher than that of dark matter …
Adaptive analytical ray tracing of black hole photon rings
Recent interferometric observations by the Event Horizon Telescope have resolved the
horizon-scale emission from sources in the vicinity of nearby supermassive black holes …
horizon-scale emission from sources in the vicinity of nearby supermassive black holes …