detalle del documento
IDENTIFICACIÓN
oai:arXiv.org:2409.20335
Tema
General Relativity and Quantum Cos... Astrophysics - High Energy Astroph...Autor
Pugliese, D. Quevedo, H.Categoría
ciencias: astrofísica
Año
2024
fecha de cotización
2/10/2024
Palabras clave
particular orbits physics related replicas shadow hole blackResumen
Recently, new exploratory channels have opened up for the physics of highly compact objects, such as gravitational waves and black hole shadows.
Moreover, more precise analysis and observations are now possible in the physics of accretion around compact objects.
These advancements provide in particular an unprecedented insight into the physics near the horizons of a black hole.
In this work we focus on the shadow boundary of a Kerr black hole, introducing observables related to special null orbits, called horizons replicas, solutions of the shadow edge equations which are related to particular photon orbits, defined by constraints on their impact parameter, carrying information about the angular momentum of the central spinning object.
These orbits are related to particular regions on the shadow boundary and might be used to determine the spin of the black hole.
The results provide the conditions by which horizon replicas are imprinted in the black hole shadow profile, in dependence on the black hole dimensionless spin and observational angle, providing eventually new templates for the future observations.
;Comment: 24 pages, 12 figures.
To appear in NPB
Pugliese, D.,Quevedo, H., 2024, Horizon replicas in black hole shadows
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