Hawking radiation in moving plasmas
L.C. Garcia de Andrade

TL;DR
This paper demonstrates the emergence of Hawking radiation and bi-metricity in non-relativistic moving magnetohydrodynamics (MHD) plasmas, revealing effective black hole horizons in a plasma medium with two distinct Riemannian metrics.
Contribution
It introduces a novel analysis of Hawking radiation in MHD plasmas with two effective metrics, one flat and one with a horizon, expanding analog gravity models to plasma physics.
Findings
Identification of two effective metrics in MHD plasma
Hawking radiation associated with the horizon metric
Analogy to optical black holes in moving dielectrics
Abstract
Bi-metricity and Hawking radiation are exhibit in non-relativistic moving magnetohydrodynamics (MHD) plasma medium generating two Riemannian effective spacetimes. The first metric is a flat metric although the speed of "light" is given by a time dependent signal where no Hawking radiation or effective black holes are displayed. This metric comes from a wave equation which the scalar function comes from the scalar potential of the background velocity of the fluid and depends on the perturbation of the magnetic background field. The second metric is an effective spacetime metric which comes from the perturbation of the background MHD fluid. This Riemann metric exhibits a horizon and Hawking radiation which can be expressed in terms of the background constant magnetic field. The effective velocity is given Alfven wave velocity of plasma physics. The effective black hole found here is…
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Taxonomy
TopicsCosmology and Gravitation Theories · Advanced Differential Geometry Research · Relativity and Gravitational Theory
