Preprint Article Version 1 Preserved in Portico This version is not peer-reviewed

Entangled Particles Spinning on the Black Hole Horizon

Version 1 : Received: 18 December 2020 / Approved: 21 December 2020 / Online: 21 December 2020 (11:15:07 CET)

How to cite: Bousder, M. Entangled Particles Spinning on the Black Hole Horizon. Preprints 2020, 2020120508 (doi: 10.20944/preprints202012.0508.v1). Bousder, M. Entangled Particles Spinning on the Black Hole Horizon. Preprints 2020, 2020120508 (doi: 10.20944/preprints202012.0508.v1).

Abstract

In this paper, we present a technique to unify the Reissner–Nordstr¨om metric and the Kerr–Newman metric. We construct a specifific model and calculate the entanglement entropy of black horizon. We are interested in the entangled particle and antiparticle spinning on the black hole horizon. The two Reissner-Nordstr¨om horizons r±, are the results of the rotation of several entangled particle-antiparticle on the real horizon. The energy absorbed by a black hole is transformed into a kinetic energy of the entangled particle-antiparticles. This study provides a new type of black hole metric. We show that the rotation of an entangled system of a particle and an antiparticle can create a extremal black hole. We also explore some of the implications of this point of view for the black hole entanglement.

Subject Areas

black hole;, entanglement; entropy; entagled particle

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