Hawking radiation in moving plasmas
| dc.creator | de Andrade, L. C. Garcia | |
| dc.date | 2005-09-07 | |
| dc.date.accessioned | 2026-07-07T03:29:55Z | |
| dc.date.available | 2026-07-07T03:29:55Z | |
| dc.description | 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 analogous to the optical black hole in moving dielectrics found by De Lorenci et al [Phys. Rev. D (2003)] where bi-metricity and Hawking radiation in terms of the electric field are found. | |
| dc.description | Latex file | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0509027 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0509027 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/35373 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Hawking radiation in moving plasmas | |
| dc.type | text |