Brany Liouville Inflation

We present a specific model for cosmological inflation driven by the Liouville field in a non-critical supersymmetric string framework, in which the departure from criticality is due to open strings stretched between the two moving Type-II 5-branes. We use WMAP and other data on fluctuations in the...

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Detalles Bibliográficos
Autores principales: Ellis, John R., Mavromatos, N.E., Nanopoulos, Dimitri V., Sakharov, A.
Lenguaje:eng
Publicado: 2004
Materias:
General Relativity and Cosmology
Acceso en línea:https://dx.doi.org/10.1088/1367-2630/6/1/171
http://cds.cern.ch/record/779897
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author Ellis, John R.
Mavromatos, N.E.
Nanopoulos, Dimitri V.
Sakharov, A.
author_facet Ellis, John R.
Mavromatos, N.E.
Nanopoulos, Dimitri V.
Sakharov, A.
author_sort Ellis, John R.
collection CERN
description We present a specific model for cosmological inflation driven by the Liouville field in a non-critical supersymmetric string framework, in which the departure from criticality is due to open strings stretched between the two moving Type-II 5-branes. We use WMAP and other data on fluctuations in the cosmic microwave background to fix parameters of the model, such as the relative separation and velocity of the 5-branes, respecting also the constraints imposed by data on light propagation from distant gamma-ray bursters. The model also suggests a small, relaxing component in the present vacuum energy that may accommodate the breaking of supersymmetry.
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spelling cern-7798972023-03-14T19:12:25Zdoi:10.1088/1367-2630/6/1/171http://cds.cern.ch/record/779897engEllis, John R.Mavromatos, N.E.Nanopoulos, Dimitri V.Sakharov, A.Brany Liouville InflationGeneral Relativity and CosmologyWe present a specific model for cosmological inflation driven by the Liouville field in a non-critical supersymmetric string framework, in which the departure from criticality is due to open strings stretched between the two moving Type-II 5-branes. We use WMAP and other data on fluctuations in the cosmic microwave background to fix parameters of the model, such as the relative separation and velocity of the 5-branes, respecting also the constraints imposed by data on light propagation from distant gamma-ray bursters. The model also suggests a small, relaxing component in the present vacuum energy that may accommodate the breaking of supersymmetry.We present a specific model for cosmological inflation driven by the Liouville field in a non-critical supersymmetric string framework, in which the departure from criticality is due to open strings stretched between the two moving Type-II 5-branes. We use WMAP and other data on fluctuations in the cosmic microwave background to fix parameters of the model, such as the relative separation and velocity of the 5-branes, respecting also the constraints imposed by data on light propagation from distant gamma-ray bursters. The model also suggests a small, relaxing component in the present vacuum energy that may accommodate the breaking of supersymmetry.gr-qc/0407089CERN-PH-TH-2004-134ACT-05-04MIFP-04-14CERN-PH-TH-2004-134ACT-5MIFP-2004-14oai:cds.cern.ch:7798972004-07-23
spellingShingle General Relativity and Cosmology
Ellis, John R.
Mavromatos, N.E.
Nanopoulos, Dimitri V.
Sakharov, A.
Brany Liouville Inflation
title Brany Liouville Inflation
title_full Brany Liouville Inflation
title_fullStr Brany Liouville Inflation
title_full_unstemmed Brany Liouville Inflation
title_short Brany Liouville Inflation
title_sort brany liouville inflation
topic General Relativity and Cosmology
url https://dx.doi.org/10.1088/1367-2630/6/1/171
http://cds.cern.ch/record/779897
work_keys_str_mv AT ellisjohnr branyliouvilleinflation
AT mavromatosne branyliouvilleinflation
AT nanopoulosdimitriv branyliouvilleinflation
AT sakharova branyliouvilleinflation

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