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Gravitational Deflection of Massive Particles by a Schwarzschild Black Hole in Radiation Gauge
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Gravitational Deflection of Massive Particles by a Schwarzschild Black Hole in Radiation Gauge
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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.
Forward citations
Cited by 1 Pith paper
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Deflection angle of charged massive particles in slowly rotating Kerr-Newman space-times via Gauss-Bonnet theorem and Hamilton-Jacobi method
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.
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