Correspondence between two gravitational lens equations in a static and spherically symmetric spacetime
arXiv:2407.02046 · doi:10.1103/PhysRevD.111.044014
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.
7 pages, 9 figures, appendix added for a proof of the unphysical branch, published in PRD
References in corpus (24)
- First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- The Confrontation between General Relativity and Experiment
- First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
- First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole
- First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole
- First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring
- First M87 Event Horizon Telescope Results. II. Array and Instrumentation
- First M87 Event Horizon Telescope Results. III. Data Processing and Calibration
- Gravitational lensing in the strong field limit
- First Sagittarius A* Event Horizon Telescope Results. VI: Testing the Black Hole Metric
- Calculating black hole shadows: Review of analytical studies
- First Sagittarius A* Event Horizon Telescope Results. V. Testing Astrophysical Models of the Galactic Center Black Hole
- An Update on Monitoring Stellar Orbits in the Galactic Center
- First Sagittarius A* Event Horizon Telescope Results. III: Imaging of the Galactic Center Supermassive Black Hole
- First Sagittarius A* Event Horizon Telescope Results. II. EHT and Multi-wavelength Observations, Data Processing, and Calibration
- First Sagittarius A* Event Horizon Telescope Results. IV. Variability, Morphology, and Black Hole Mass
- Applications of the Gauss-Bonnet theorem to gravitational lensing
- Gravitational bending angle of light for finite distance and the Gauss-Bonnet theorem
- On the exact gravitational lens equation in spherically symmetric and static spacetimes
- Finite-distance corrections to the gravitational bending angle of light in the strong deflection limit
- A comparison of approximate gravitational lens equations and a proposal for an improved new one
- Distortions of images of Schwarzschild lensing
- Conservation of distortion of gravitationally lensed images
- Gravitational lens without asymptotic flatness: Its application to the Weyl gravity
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- Phenomenology of Schwarzschild-like Black Holes with a Generalized Compton Wavelength