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A Note on the Swampland Distance Conjecture
We discuss the Swampland Distance Conjecture in the framework of black hole thermodynamics. In particular, we consider black holes in de Sitter space and we show that the Swampland Distance Conjecture is a consequence of the fact that apparent horizons are always inside cosmic event horizons wheneve...
Autores principales: | , |
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Lenguaje: | eng |
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2019
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Acceso en línea: | https://dx.doi.org/10.1002/prop.201900099 http://cds.cern.ch/record/2703565 |
_version_ | 1780964638028988416 |
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author | Kehagias, A. Riotto, A. |
author_facet | Kehagias, A. Riotto, A. |
author_sort | Kehagias, A. |
collection | CERN |
description | We discuss the Swampland Distance Conjecture in the framework of black hole thermodynamics. In particular, we consider black holes in de Sitter space and we show that the Swampland Distance Conjecture is a consequence of the fact that apparent horizons are always inside cosmic event horizons whenever they exist in the case of fast‐roll inflation. In addition, we show that the Bekenstein and the Hubble entropy bounds for the entropy in a region of spacetime lead similarly to the same conjecture. |
id | cern-2703565 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2019 |
record_format | invenio |
spelling | cern-27035652023-10-04T06:05:39Zdoi:10.1002/prop.201900099http://cds.cern.ch/record/2703565engKehagias, A.Riotto, A.A Note on the Swampland Distance Conjecturehep-phParticle Physics - Phenomenologygr-qcGeneral Relativity and Cosmologyastro-ph.COAstrophysics and Astronomyhep-thParticle Physics - TheoryWe discuss the Swampland Distance Conjecture in the framework of black hole thermodynamics. In particular, we consider black holes in de Sitter space and we show that the Swampland Distance Conjecture is a consequence of the fact that apparent horizons are always inside cosmic event horizons whenever they exist in the case of fast‐roll inflation. In addition, we show that the Bekenstein and the Hubble entropy bounds for the entropy in a region of spacetime lead similarly to the same conjecture.We discuss the Swampland Distance Conjecture in the framework of black hole thermodynamics. In particular, we consider black holes in de Sitter space and we show that the Swampland Distance Conjecture is a consequence of the fact that apparent horizons are always inside cosmic event horizons whenever they exist in the case of fast-roll inflation. In addition, we show that the Bekenstein and the Hubble entropy bounds for the entropy in a region of spacetime lead similarly to the same conjecture.arXiv:1911.09050oai:cds.cern.ch:27035652019-11-20 |
spellingShingle | hep-ph Particle Physics - Phenomenology gr-qc General Relativity and Cosmology astro-ph.CO Astrophysics and Astronomy hep-th Particle Physics - Theory Kehagias, A. Riotto, A. A Note on the Swampland Distance Conjecture |
title | A Note on the Swampland Distance Conjecture |
title_full | A Note on the Swampland Distance Conjecture |
title_fullStr | A Note on the Swampland Distance Conjecture |
title_full_unstemmed | A Note on the Swampland Distance Conjecture |
title_short | A Note on the Swampland Distance Conjecture |
title_sort | note on the swampland distance conjecture |
topic | hep-ph Particle Physics - Phenomenology gr-qc General Relativity and Cosmology astro-ph.CO Astrophysics and Astronomy hep-th Particle Physics - Theory |
url | https://dx.doi.org/10.1002/prop.201900099 http://cds.cern.ch/record/2703565 |
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