Thermal properties of spacetime foam
Spacetime foam can be modeled in terms of nonlocal effective interactions in a classical nonfluctuating background. Then, the density matrix for the low-energy fields evolves, in the weak-coupling approximation, according to a master equation that contains a diffusion term. Furthermore, it is argued...
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| Format: | article |
| Publication Date: | 1998 |
| Country: | España |
| Institution: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repository: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/100756 |
| Online Access: | http://hdl.handle.net/10261/100756 |
| Access Level: | Open access |
| Keyword: | [PACS] Foundations, theory of measurement, miscellaneous theories [PACS] Spacetime topology, causal structure, spinor structure [PACS] Quantum aspects of black holes, evaporation, thermodynamics [PACS] Quantum gravity |
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Thermal properties of spacetime foamGaray, Luis Javier[PACS] Foundations, theory of measurement, miscellaneous theories[PACS] Spacetime topology, causal structure, spinor structure[PACS] Quantum aspects of black holes, evaporation, thermodynamics[PACS] Quantum gravitySpacetime foam can be modeled in terms of nonlocal effective interactions in a classical nonfluctuating background. Then, the density matrix for the low-energy fields evolves, in the weak-coupling approximation, according to a master equation that contains a diffusion term. Furthermore, it is argued that spacetime foam behaves as a quantum thermal field that, apart from inducing loss of coherence, gives rise to effects such as gravitational Lamb and Stark shifts as well as quantum damping in the evolution of the low-energy observables. These effects can be, at least in principle, experimentally tested. ©1998 The American Physical SocietyI was supported by funds provided by DGICYT and MEC (Spain) under Contract Adjunct to the Project No. PB94-0107.Peer ReviewedAmerican Physical Society2014201419982014info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501http://hdl.handle.net/10261/100756reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglésinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/1007562026-05-22T06:33:51Z |
| dc.title.none.fl_str_mv |
Thermal properties of spacetime foam |
| title |
Thermal properties of spacetime foam |
| spellingShingle |
Thermal properties of spacetime foam Garay, Luis Javier [PACS] Foundations, theory of measurement, miscellaneous theories [PACS] Spacetime topology, causal structure, spinor structure [PACS] Quantum aspects of black holes, evaporation, thermodynamics [PACS] Quantum gravity |
| title_short |
Thermal properties of spacetime foam |
| title_full |
Thermal properties of spacetime foam |
| title_fullStr |
Thermal properties of spacetime foam |
| title_full_unstemmed |
Thermal properties of spacetime foam |
| title_sort |
Thermal properties of spacetime foam |
| dc.creator.none.fl_str_mv |
Garay, Luis Javier |
| author |
Garay, Luis Javier |
| author_facet |
Garay, Luis Javier |
| author_role |
author |
| dc.subject.none.fl_str_mv |
[PACS] Foundations, theory of measurement, miscellaneous theories [PACS] Spacetime topology, causal structure, spinor structure [PACS] Quantum aspects of black holes, evaporation, thermodynamics [PACS] Quantum gravity |
| topic |
[PACS] Foundations, theory of measurement, miscellaneous theories [PACS] Spacetime topology, causal structure, spinor structure [PACS] Quantum aspects of black holes, evaporation, thermodynamics [PACS] Quantum gravity |
| description |
Spacetime foam can be modeled in terms of nonlocal effective interactions in a classical nonfluctuating background. Then, the density matrix for the low-energy fields evolves, in the weak-coupling approximation, according to a master equation that contains a diffusion term. Furthermore, it is argued that spacetime foam behaves as a quantum thermal field that, apart from inducing loss of coherence, gives rise to effects such as gravitational Lamb and Stark shifts as well as quantum damping in the evolution of the low-energy observables. These effects can be, at least in principle, experimentally tested. ©1998 The American Physical Society |
| publishDate |
1998 |
| dc.date.none.fl_str_mv |
1998 2014 2014 2014 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 |
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article |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/10261/100756 |
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http://hdl.handle.net/10261/100756 |
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Inglés |
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Inglés |
| dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess |
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openAccess |
| dc.publisher.none.fl_str_mv |
American Physical Society |
| publisher.none.fl_str_mv |
American Physical Society |
| dc.source.none.fl_str_mv |
reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC instname:Consejo Superior de Investigaciones Científicas (CSIC) |
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Consejo Superior de Investigaciones Científicas (CSIC) |
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DIGITAL.CSIC. Repositorio Institucional del CSIC |
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DIGITAL.CSIC. Repositorio Institucional del CSIC |
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1869420480027426816 |
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15.812429 |