2014/04/29 by Hai Lin, K. Saifullah, Shing-Tung Yau
Physics and Astronomy · #Acceleration #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Black hole (networking) #Event horizon #Field (mathematics) #Horizon #Magnetic field #Particle acceleration #Relativity and Gravitational Theory #gr-qc #hep-th
paper · pdf · doi:10.1142/s0217732315500443
18 pages
arxiv created 2014/04/29 · openalex publication_date 2015/01/28 · openalex created_date 2016/06/24 · arxiv updated 2017/12/21 · openalex updated_date 2026/08/05
We consider spin-[Formula: see text] particles on the background of general accelerating black holes and the C-metric. The Rarita–Schwinger equations of spin-[Formula: see text] particles are analyzed on these backgrounds. The emission and absorption probabilities of these particles on these spacetimes are calculated. These backgrounds which we analyze contain both black hole horizon and acceleration horizon, and have general electric and magnetic charges, rotation, and acceleration parameter. Other physical quantities of the spin-[Formula: see text] field near the acceleration horizon are also computed.