Can a regular black hole be observationally distinguished from singular black holes as spinning lens partner in PSR-BH binaries?

To answer the question posed in the title, we consider a novel diagnostic, viz., the difference in the time of arrival (TOA) at the observer of two light rays that simultaneously emanate from a source behind a spinning lens and pass by either side of the lens to reach the observer. This is completel...

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Veröffentlicht in:	Journal of astrophysics and astronomy 2021-10, Vol.42 (2), Article 79
Hauptverfasser:	Tuleganova, G. Y., Karimov, R. K. H., Izmailov, R. N., Nandi, K. K.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Astrophysics and Astroparticles Black holes Gyromagnetic ratio Lenses Observations and Techniques Physics Physics and Astronomy Pulsars Time lag
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