Inertial mass from Unruh temperatures
It has been proposed that inertia can be explained as follows: when objects accelerate in one direction a Rindler horizon forms in the other direction, suppressing Unruh radiation on that side, and producing a net Unruh radiation pressure that always opposes the acceleration, just like inertia. So f...
| Authors: | , |
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| Format: | article |
| Status: | Versión aceptada para publicación |
| Publication Date: | 2016 |
| Country: | España |
| Institution: | Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya) |
| Repository: | Recercat. Dipósit de la Recerca de Catalunya |
| OAI Identifier: | oai:recercat.cat:10459.1/58386 |
| Online Access: | https://doi.org/10.1142/S0217732316501078 http://hdl.handle.net/10459.1/58386 |
| Access Level: | Open access |
| Keyword: | Cosmology Unruh radiation Hubble-scale Casimir effect Inertial mass |
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Inertial mass from Unruh temperaturesGiné, JaumeMcCulloch, M. E.CosmologyUnruh radiationHubble-scale Casimir effectInertial massIt has been proposed that inertia can be explained as follows: when objects accelerate in one direction a Rindler horizon forms in the other direction, suppressing Unruh radiation on that side, and producing a net Unruh radiation pressure that always opposes the acceleration, just like inertia. So far this model has predicted masses over twice those expected. In this paper an error in this model is corrected so that its prediction improves to within 29\% of the expected Planck mass. It is also shown that inertial mass may be understood qualitatively by applying Carnot's principle and entropy to Unruh temperatures, so that the work needed for inertia comes from the difference in the Unruh temperatures seen by the accelerated object and the cosmos. This implies that highly-accelerated systems may emit heat in a new way.The first author is partially supported by a MINECO/ FEDER grant number MTM2014-53703-P and an AGAUR (Generalitat de Catalunya) grant number 2014SGR 1204.World Scientific Publishing2016info:eu-repo/semantics/articleinfo:eu-repo/semantics/acceptedVersionapplication/pdfhttps://doi.org/10.1142/S0217732316501078http://hdl.handle.net/10459.1/58386reponame:Recercat. Dipósit de la Recerca de Catalunyainstname:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)InglésMINECO/PN2013-2016/MTM2014-53703-PVersió postprint del document publicat a https://doi.org/10.1142/S0217732316501078Modern Physics Letters A, 2016, vol. 31, num. 17, p. 1650107-1650107(c) World Scientific Publishing, 2016info:eu-repo/semantics/openAccessoai:recercat.cat:10459.1/583862026-05-29T05:05:01Z |
| dc.title.none.fl_str_mv |
Inertial mass from Unruh temperatures |
| title |
Inertial mass from Unruh temperatures |
| spellingShingle |
Inertial mass from Unruh temperatures Giné, Jaume Cosmology Unruh radiation Hubble-scale Casimir effect Inertial mass |
| title_short |
Inertial mass from Unruh temperatures |
| title_full |
Inertial mass from Unruh temperatures |
| title_fullStr |
Inertial mass from Unruh temperatures |
| title_full_unstemmed |
Inertial mass from Unruh temperatures |
| title_sort |
Inertial mass from Unruh temperatures |
| dc.creator.none.fl_str_mv |
Giné, Jaume McCulloch, M. E. |
| author |
Giné, Jaume |
| author_facet |
Giné, Jaume McCulloch, M. E. |
| author_role |
author |
| author2 |
McCulloch, M. E. |
| author2_role |
author |
| dc.subject.none.fl_str_mv |
Cosmology Unruh radiation Hubble-scale Casimir effect Inertial mass |
| topic |
Cosmology Unruh radiation Hubble-scale Casimir effect Inertial mass |
| description |
It has been proposed that inertia can be explained as follows: when objects accelerate in one direction a Rindler horizon forms in the other direction, suppressing Unruh radiation on that side, and producing a net Unruh radiation pressure that always opposes the acceleration, just like inertia. So far this model has predicted masses over twice those expected. In this paper an error in this model is corrected so that its prediction improves to within 29\% of the expected Planck mass. It is also shown that inertial mass may be understood qualitatively by applying Carnot's principle and entropy to Unruh temperatures, so that the work needed for inertia comes from the difference in the Unruh temperatures seen by the accelerated object and the cosmos. This implies that highly-accelerated systems may emit heat in a new way. |
| publishDate |
2016 |
| dc.date.none.fl_str_mv |
2016 |
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info:eu-repo/semantics/article info:eu-repo/semantics/acceptedVersion |
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article |
| status_str |
acceptedVersion |
| dc.identifier.none.fl_str_mv |
https://doi.org/10.1142/S0217732316501078 http://hdl.handle.net/10459.1/58386 |
| url |
https://doi.org/10.1142/S0217732316501078 http://hdl.handle.net/10459.1/58386 |
| dc.language.none.fl_str_mv |
Inglés |
| language_invalid_str_mv |
Inglés |
| dc.relation.none.fl_str_mv |
MINECO/PN2013-2016/MTM2014-53703-P Versió postprint del document publicat a https://doi.org/10.1142/S0217732316501078 Modern Physics Letters A, 2016, vol. 31, num. 17, p. 1650107-1650107 |
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(c) World Scientific Publishing, 2016 info:eu-repo/semantics/openAccess |
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(c) World Scientific Publishing, 2016 |
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openAccess |
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application/pdf |
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World Scientific Publishing |
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World Scientific Publishing |
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reponame:Recercat. Dipósit de la Recerca de Catalunya instname:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya) |
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Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya) |
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Recercat. Dipósit de la Recerca de Catalunya |
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Recercat. Dipósit de la Recerca de Catalunya |
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