Synchrotron Radiation From Weakly Magnetized Schwarzschild Black Hole
arXiv:1509.02535 · doi:10.1103/PhysRevD.92.124066
Abstract
We consider a synchrotron radiation from a charged particle moving in a bound orbit around a weakly magnetized Schwarzschild black hole (a static black hole immersed into a constant uniform magnetic field) in its equatorial plane, perpendicular to the magnetic field. In particular, we study the case when the Lorentz force acting on the charged particle is directed outward from the black hole. The particle is initially moving in a nongeodesic bound orbit which due to synchrotron radiation decays to a nongeodesic circular orbit. We study this transition and calculate the radiated power and energy loss of the particle.
7 pages, 4 figures
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- On the Non-Minimal Coupling of Magnetic Fields with Gravity in Schwarzschild Spacetime
- Structure of test magnetic fields and charged particle motion around the Hayward spacetime
- Can synchrotron radiation reveal the presence of {\it dark sector} around black hole?