REVIEW 2 cited by
Correspondence between two gravitational lens equations in a static and spherically symmetric spacetime
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
Signed reviews
read the original abstract
Virbhadra and Ellis have proposed a very accurate equation (referred to as VE equation) for the gravitational lens in a static and spherically symmetric spacetime [Phys. Rev. D 62,084003 (2000)], whereas an improved equation (referred to as OB equation) has been derived by Bozza [Phys. Rev. D 78, 103005 (2008)] based on a relation found by Ohanian [Am. J. Phys. 55, 428 (1987)]. The OB equation was rediscovered later by Takizawa, Ono and Asada [Phys. Rev. D, 102, 064060 (2020)]. VE and OB equations seem to be very different from each other. The present paper shows that there exists an unphysical branch in the VE equation. Consequently, the VE equation can be improved by removing the unphysical branch. The improved version of the VE equation is found to be the same as the OB equation when a suitable transformation is made between the deflection angles defined differently in the two formulations. An explicit expression of the transformation is found. We also argue possible numerical differences when the transformation between the deflection angles is ignored.
Forward citations
Cited by 2 Pith papers
-
Periodic orbits and gravitational waveforms in quantum-corrected black hole spacetimes
For one effective quantum gravity black hole model (BH-I), the quantum parameter shifts periodic orbits and delays gravitational wave phase, while for the other model (BH-II) the effect is negligible, making BH-I pote...
-
Phenomenology of Schwarzschild-like Black Holes with a Generalized Compton Wavelength
A generalized Compton wavelength deformation of Schwarzschild spacetime yields EHT and solar system bounds on the deformation parameter epsilon, currently consistent with general relativity.
Discussion (0). Continue with ORCID to comment.