Gravitational Deflection of Massive Particles by a Schwarzschild Black Hole in Radiation Gauge
arXiv:1906.06470 · doi:10.1088/0253-6102/71/10/1219
Abstract
The exact metric of a Schwarzschild black hole in the true radiation gauge was recently reported. In this work, we base on this gravity and calculate the gravitational deflection of relativistic massive particles up to the fourth post-Minkowskian order. It is found that the result is consistent with the previous formulations for both the case of dropping the fourth-order contribution and the case of light deflection. Our result might be helpful for future high-accuracy observations.
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- Exploring light deflection and black hole shadows in Rastall theory with plasma effects
- Extending Gibbons-Werner method to bound orbits of massive particles
- Kerr-Newman black hole lensing of relativistic massive particles in the weak field limit
- Deflection of charged signals in a dipole magnetic field in Schwarzschild background using Gauss-Bonnet theorem
- A comparison between the deflection angles of massive and massless particles in the Shchwarzschild space-time and their consequences on black hole shadows
- Particle dynamics in spherically symmetric electro-vacuum instantons
- Strong field gravitational lensing of particles by a black-bounce-Schwarzschild black hole