On the relation of the mass, spin and charge parameters with the red and blue shifts of photons emitted by particles orbiting a Kerr–Newman black hole

Abstract We found the mass M and rotation a parameters of the Kerr–Newman black hole in terms of the charge Q parameter as well as the red z r and blue z b shifts of light emitted by geodesic particles traveling in circular orbits around it for both cases: corotating and counterrotating directions. These shifts z r and z b cannot acquire arbitrary values; bounds of these shifts are found as functions of the parameters a and Q .

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Publication Details

Journal
Classical and Quantum Gravity
Published
2025-09-30
DOI
https://doi.org/10.1088/1361-6382/ae0ddb
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
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article

On the relation of the mass, spin and charge parameters with the red and blue shifts of photons emitted by particles orbiting a Kerr–Newman black hole

Ricardo Becerril, José Manuel Dávila, Susana Valdez-Alvarado, Roberto Esaú Ortega-Miranda
Classical and Quantum Gravity
Astrophysical Phenomena and Observations
article

On the relation of the mass, spin and charge parameters with the red and blue shifts of photons emitted by particles orbiting a Kerr–Newman black hole

Ricardo Becerril, José Manuel Dávila, Susana Valdez-Alvarado, Roberto Esaú Ortega-Miranda
article en

Abstract

Abstract We found the mass M and rotation a parameters of the Kerr–Newman black hole in terms of the charge Q parameter as well as the red z r and blue z b shifts of light emitted by geodesic particles traveling in circular orbits around it for both cases: corotating and counterrotating directions. These shifts z r and z b cannot acquire arbitrary values; bounds of these shifts are found as functions of the parameters a and Q .

Classical and Quantum GravityVol. 42(20)
Universidad Michoacana de San Nicolás de Hidalgo (MX), Universidad Autónoma del Estado de México (MX)
Openalex Percentile: Top 81%
Astrophysical Phenomena and Observations
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