2019/05/10 by Roman Plyatsko, Plyatsko, Roman, Mykola Fenyk +1
Engineering · Physics and Astronomy · #F.2.2 #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Geophysics and Sensor Technology #High Energy Astrophysical Phenomena (astro-ph.HE) #High Energy Physics - Theory (hep-th) #Pulsars and Gravitational Waves Research #Relativity and Gravitational Theory
paper · pdf · doi:10.48550/arxiv.1905.04342
openalex publication_date 2019/05/10 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The Mathisson-Papapetrou equations are used for investigations of influence\nof the spin-gravity coupling on a highly relativistic spinning particle in\nSchwarzschild's field. It is established that interaction of the particle spin\nwith the gravitomagnetic components of the field, estimated in the proper frame\nof the particle, causes the large acceleration of the spinning particle\nrelative to geodesic free fall. As a result the accelerated charged spinning\nparticle can generate intensive electromagnetic radiation when its velocity is\nhighly relativistic. The significant contribution of the highly relativistic\nspin-gravity coupling to the energy of the spinning particle is analyzed.\n