dorsal/arxiv
View SchemaH-theorem for classical matter around a black hole
| Authors | Piero Nicolini, Massimo Tessarotto |
|---|---|
| Categories | |
| ArXiv ID | physics/0506130 |
| URL | https://arxiv.org/abs/physics/0506130 |
| DOI | 10.1063/1.2198469 |
| Journal | Phys.Plasmas 13:052901,2006 |
Abstract
We propose a classical solution for the kinetic description of matter falling into a black hole, which permits to evaluate both the kinetic entropy and the entropy production rate of classical infalling matter at the event horizon. The formulation is based on a relativistic kinetic description for classical particles in the presence of an event horizon. An H-theorem is established which holds for arbitrary models of black holes and is valid also in the presence of contracting event horizons.
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"abstract": "We propose a classical solution for the kinetic description of matter falling\ninto a black hole, which permits to evaluate both the kinetic entropy and the\nentropy production rate of classical infalling matter at the event horizon. The\nformulation is based on a relativistic kinetic description for classical\nparticles in the presence of an event horizon. An H-theorem is established\nwhich holds for arbitrary models of black holes and is valid also in the\npresence of contracting event horizons.",
"arxiv_id": "physics/0506130",
"authors": [
"Piero Nicolini",
"Massimo Tessarotto"
],
"categories": [
"physics.class-ph"
],
"doi": "10.1063/1.2198469",
"journal_ref": "Phys.Plasmas 13:052901,2006",
"title": "H-theorem for classical matter around a black hole",
"url": "https://arxiv.org/abs/physics/0506130"
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