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Gravitational Deflection of Massive Particles by a Schwarzschild Black Hole in Radiation Gauge

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arxiv 1906.06470 v1 pith:DIEZDV2J submitted 2019-06-15 gr-qc astro-ph.HE

Zonghai Li , Xia Zhou , Weijun Li , Guansheng He This is my paper
classification gr-qcastro-ph.HE
keywords deflectionblackcasegaugegravitationalholemassiveparticles
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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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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Deflection angle of charged massive particles in slowly rotating Kerr-Newman space-times via Gauss-Bonnet theorem and Hamilton-Jacobi method

    gr-qc 2019-06 unverdicted novelty 6.0 of 10

    Deflection angle of charged massive particles in slowly rotating Kerr-Newman spacetimes derived via Gauss-Bonnet theorem (via plasma correspondence) and Hamilton-Jacobi method, depending on M, a, Q, P, q, v.

  2. Strong field gravitational lensing of particles by a black-bounce-Schwarzschild black hole

    gr-qc 2026-02 accept novelty 5.0 of 10

    For a black-bounce-Schwarzschild black hole, the paper derives the strong-deflection lensing observables for massive particles and quantifies how they differ from photon lensing.

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