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Vacuum Energy, Cosmological Supersymmetry Breaking and Inflation from Colliding Brane Worlds

In the context of colliding brane worlds I discuss a toy cosmological model, developed in collaboration with E. Gravanis, which arguably produces inflation and a relaxing to zero cosmological ``constant'' hierarchically small as compared to the supersymmetry breaking (TeV) scale. Supersymm...

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Autor principal: Mavromatos, Nikolaos E
Lenguaje:eng
Publicado: 2002
Materias:
Acceso en línea:http://cds.cern.ch/record/583868
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author Mavromatos, Nikolaos E
author_facet Mavromatos, Nikolaos E
author_sort Mavromatos, Nikolaos E
collection CERN
description In the context of colliding brane worlds I discuss a toy cosmological model, developed in collaboration with E. Gravanis, which arguably produces inflation and a relaxing to zero cosmological ``constant'' hierarchically small as compared to the supersymmetry breaking (TeV) scale. Supersymmetry breaking is induced by compactification of the brane worlds on magnetized tori. The crucial ingredient is the non-criticality (non conformality) of string theory on the observable brane world induced at the collision, which is thus viewed as a cause for departure from equilibrium in this system. The hierarchical smallness of the present-era vacuum energy, as compared to the SUSY breaking scale, is thus attributed to relaxation.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2002
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spelling cern-5838682019-09-30T06:29:59Zhttp://cds.cern.ch/record/583868engMavromatos, Nikolaos EVacuum Energy, Cosmological Supersymmetry Breaking and Inflation from Colliding Brane WorldsParticle Physics - TheoryIn the context of colliding brane worlds I discuss a toy cosmological model, developed in collaboration with E. Gravanis, which arguably produces inflation and a relaxing to zero cosmological ``constant'' hierarchically small as compared to the supersymmetry breaking (TeV) scale. Supersymmetry breaking is induced by compactification of the brane worlds on magnetized tori. The crucial ingredient is the non-criticality (non conformality) of string theory on the observable brane world induced at the collision, which is thus viewed as a cause for departure from equilibrium in this system. The hierarchical smallness of the present-era vacuum energy, as compared to the SUSY breaking scale, is thus attributed to relaxation.hep-th/0210008oai:cds.cern.ch:5838682002-10-01
spellingShingle Particle Physics - Theory
Mavromatos, Nikolaos E
Vacuum Energy, Cosmological Supersymmetry Breaking and Inflation from Colliding Brane Worlds
title Vacuum Energy, Cosmological Supersymmetry Breaking and Inflation from Colliding Brane Worlds
title_full Vacuum Energy, Cosmological Supersymmetry Breaking and Inflation from Colliding Brane Worlds
title_fullStr Vacuum Energy, Cosmological Supersymmetry Breaking and Inflation from Colliding Brane Worlds
title_full_unstemmed Vacuum Energy, Cosmological Supersymmetry Breaking and Inflation from Colliding Brane Worlds
title_short Vacuum Energy, Cosmological Supersymmetry Breaking and Inflation from Colliding Brane Worlds
title_sort vacuum energy, cosmological supersymmetry breaking and inflation from colliding brane worlds
topic Particle Physics - Theory
url http://cds.cern.ch/record/583868
work_keys_str_mv AT mavromatosnikolaose vacuumenergycosmologicalsupersymmetrybreakingandinflationfromcollidingbraneworlds