Non-equilibrium Landauer transport model for Hawking radiation from a black hole
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Franco Nori | - |
dc.contributor.author | Paul Nation | - |
dc.date.accessioned | 2021-09-03T09:51:27Z | - |
dc.date.available | 2021-09-03T09:51:27Z | - |
dc.date.created | 2021-06-21 | - |
dc.date.issued | 2012-03 | - |
dc.identifier.issn | 13672630 | - |
dc.identifier.uri | https://scholar.korea.ac.kr/handle/2021.sw.korea/84554 | - |
dc.description.abstract | We propose that the Hawking radiation energy and entropy flow rates from a black hole can be viewed as a one-dimensional (1D), non-equilibrium Landauer transport process. Support for this viewpoint comes from previous calculations invoking conformal symmetry in the near-horizon region, which give radiation rates that are identical to those of a single 1D quantum channel connected to a thermal reservoir at the Hawking temperature. The Landauer approach shows in a direct way the particle statistics independence of the energy and entropy fluxes of a black hole radiating into vacuum, as well as one near thermal equilibrium with its environment. As an application of the Landauer approach, we show that Hawking radiation gives a net entropy production that is 50% larger than that obtained assuming standard 3D emission into vacuum. | - |
dc.language | English | - |
dc.language.iso | en | - |
dc.publisher | IOP PUBLISHING LTD | - |
dc.title | Non-equilibrium Landauer transport model for Hawking radiation from a black hole | - |
dc.type | Article | - |
dc.contributor.affiliatedAuthor | Franco Nori | - |
dc.contributor.affiliatedAuthor | Paul Nation | - |
dc.identifier.bibliographicCitation | NEW JOURNAL OF PHYSICS, v.14 | - |
dc.relation.isPartOf | NEW JOURNAL OF PHYSICS | - |
dc.citation.title | NEW JOURNAL OF PHYSICS | - |
dc.citation.volume | 14 | - |
dc.type.rims | ART | - |
dc.description.journalClass | 1 | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |
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