Analysis reveals how mass and charge influence red and blue shifts of light from geodesic particles around Kerr-Newman black holes.
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 zr and blue zb shifts of light emitted by geodesic particles traveling in circular orbits around it for both cases: corotating and counterrotating directions. These shifts zr and zb cannot acquire arbitrary values; bounds of these shifts are found as functions of the parameters a and Q.
No takes yet. Share an insight, caveat, or question.
Becerril et al. (2025) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: