Second Order Kerr-Newman Time Delay
arXiv:2007.10566 · doi:10.1103/PhysRevD.93.023005
Abstract
The explicit form for the post-Newtonian gravitational time delay of light signals propagating on the equatorial plane of a Kerr-Newman black hole is derived. Based on the null geodesic in Kerr-Newman spacetime, we adopt the iterative method to calculate the time delay. Our result reduces to the previous formulation for Kerr black hole if we drop off the contribution from the electrical charge. Our time-delay formula for the Reissner-Nordström geometry is different from the previous publication [Phys. Rev. D 69, 023002 (2004)], in which the largest second-order contribution to the time delay is missing.
References in corpus (21)
- GAIA: Composition, Formation and Evolution of the Galaxy
- Reissner-Nordstrom black hole lensing
- Formalism for Testing Theories of Gravity Using Lensing by Compact Objects. I: Static, Spherically Symmetric Case
- Lorentz Covariant Theory of Light Propagation in Gravitational Fields of Arbitrary-Moving Bodies
- Time Delay in Black Hole Gravitational Lensing as a Distance Estimator
- Detecting dark matter substructure spectroscopically in strong gravitational lenses
- Gravitational lensing and frame dragging of light in the Kerr-Newman and the Kerr-Newman-(anti) de Sitter black hole spacetimes
- Weak field limit of Reissner-Nordstrom black hole lensing
- Gravitomagnetism in the Kerr-Newman-Taub-NUT spacetime
- High precision astrometry mission for the detection and characterization of nearby habitable planetary systems with the Nearby Earth Astrometric Telescope (NEAT)
- Deflection of light and particles by moving gravitational lenses
- Magnification relations for Kerr lensing and testing Cosmic Censorship
- The Dark Matter Halos of Moderate Luminosity X-ray AGN as Determined from Weak Gravitational Lensing and Host Stellar Masses
- Constraining the Redshift z=6 Quasar Luminosity Function Using Gravitational Lensing
- Time Delay between Relativistic Images as a probe of Cosmic Censorship
- A Morse-theoretical analysis of gravitational lensing by a Kerr-Newman black hole
- Pulse Arrival-Times from Binary Pulsars with Rotating Black Hole Companions
- Sub-Microarcsecond Astrometry with SIM-Lite: A Testbed-based Performance Assessment
- Light defection due to a charged, rotating body
- New method for determining the light travel time in static, spherically symmetric spacetimes. Calculation of the terms of order
- An inquiry into the nature of the gamma-ray source 3EG J1828+0142
Cited by in corpus (7)
- Weak and strong deflection gravitational lensings by a charged Horndeski black hole
- The Klein-Gordon-Fock equation in the curved spacetime of the Kerr-Newman (anti) de Sitter black hole
- Second-order time delay by a radially moving Kerr-Newman black hole
- Constraining the spacetime spin using time delay in stationary axisymmetric spacetimes
- Kerr-Newman black hole lensing of relativistic massive particles in the weak field limit
- Light propagation in 2PN approximation in the field of one moving monopole II. Boundary value problem
- Is it possible to distinguish between different black hole solutions using the Shapiro time delay?