Observational properties of Coherent Quantum Black Holes

Fuente: arXiv
Saved in:
Bibliographic Details
Main Authors: Urmanov, Abdybek, Chakrabarty, Hrishikesh, Malafarina, Daniele
Format: Preprint
Published: 2024
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866914829475774464
author Urmanov, Abdybek
Chakrabarty, Hrishikesh
Malafarina, Daniele
author_facet Urmanov, Abdybek
Chakrabarty, Hrishikesh
Malafarina, Daniele
contents We consider null and time-like geodesics around a spherically symmetric, non-rotating Coherent Quantum Black Hole (CQBH). The classical limit of the geometry of CQBH departs from that of the Schwarzschild spacetime at short scales and depends on one parameter $R_s$ which can be interpreted as the physical radius of the 'quantum' core. We study circular orbits, photon rings, and lensing effects and compare them with the Schwarzschild metric. Using the relativistic ray-tracing code GYOTO, we produce a simulation of the shadow and show that thin accretion disks around a CQBH possess unique ring structures that distinguish them from other theoretical models.
format Preprint
id arxiv_https___arxiv_org_abs_2406_04813
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Observational properties of Coherent Quantum Black Holes
Urmanov, Abdybek
Chakrabarty, Hrishikesh
Malafarina, Daniele
General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
We consider null and time-like geodesics around a spherically symmetric, non-rotating Coherent Quantum Black Hole (CQBH). The classical limit of the geometry of CQBH departs from that of the Schwarzschild spacetime at short scales and depends on one parameter $R_s$ which can be interpreted as the physical radius of the 'quantum' core. We study circular orbits, photon rings, and lensing effects and compare them with the Schwarzschild metric. Using the relativistic ray-tracing code GYOTO, we produce a simulation of the shadow and show that thin accretion disks around a CQBH possess unique ring structures that distinguish them from other theoretical models.
title Observational properties of Coherent Quantum Black Holes
topic General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2406.04813