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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...

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Detalles Bibliográficos
Autores principales: Kehagias, A., Riotto, A.
Lenguaje:eng
Publicado: 2019
Materias:
Acceso en línea:https://dx.doi.org/10.1002/prop.201900099
http://cds.cern.ch/record/2703565
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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.
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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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