Spinning particle orbits around a black hole in an expanding background. (1st April 2019)

• Record Type: Journal Article
• Authors: Antoniou, I; Papadopoulos, D; Perivolaropoulos, L
• Is Part Of: Classical and quantum gravity. Volume 36:Number 8(2019:Apr.)
• Publication Date: 2019-04-01
• Subjects: geodesics -- spinning particle orbits -- spin–orbit coupling -- black hole spacetime with expansion; Quantum gravity -- Periodicals; Gravitation -- Periodicals; Relativity (Physics) -- Periodicals; Space and time -- Periodicals; Periodicals; 521.1
• DOI: 10.1088/1361-6382/ab0fc1
• Languages: English
• ISSNs: 0264-9381

Abstract

Abstract: We investigate analytically and numerically the orbits of spinning particles around black holes in the post Newtonian limit and in the presence of cosmic expansion. We show that orbits that are circular in the absence of spin, get deformed when the orbiting particle has spin. We show that the origin of this deformation is twofold: (a) the background expansion rate which induces an attractive (repulsive) interaction due to the cosmic background fluid when the expansion is decelerating (accelerating) and (b) a spin–orbit interaction which can be attractive or repulsive depending on the relative orientation between spin and orbital angular momentum and on the expansion rate.