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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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Lenguaje: | eng |
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2002
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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. |
id | cern-583868 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2002 |
record_format | invenio |
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 |