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Microwave Background Constraints on Decaying Defects

Embedded defects are predicted in a host of particle physics theories, in particular in the standard electroweak theory. They can be stabilized by interactions with the cosmological plasma, but will decay once the plasma falls out of equilibrium, emitting a substantial fraction of non-thermal photon...

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Detalles Bibliográficos
Autores principales: Brandenberger, Robert H., Carter, Brandon, Davis, Anne-Christine
Lenguaje:eng
Publicado: 2002
Materias:
Acceso en línea:https://dx.doi.org/10.1016/S0370-2693(02)01675-1
http://cds.cern.ch/record/538860
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author Brandenberger, Robert H.
Carter, Brandon
Davis, Anne-Christine
author_facet Brandenberger, Robert H.
Carter, Brandon
Davis, Anne-Christine
author_sort Brandenberger, Robert H.
collection CERN
description Embedded defects are predicted in a host of particle physics theories, in particular in the standard electroweak theory. They can be stabilized by interactions with the cosmological plasma, but will decay once the plasma falls out of equilibrium, emitting a substantial fraction of non-thermal photons. If the decay happens after a redshift of about $10^6$, these photons will give rise to spectral distortions of the Cosmic Microwave Background, which leads to strong constraints on the underlying particle physics theory. Such constraints apply to any model with decaying defects, and in particular to theories predicting decaying vortons, thereby leading to constraints stronger than the dark matter limit.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2002
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spelling cern-5388602023-03-14T20:19:35Zdoi:10.1016/S0370-2693(02)01675-1http://cds.cern.ch/record/538860engBrandenberger, Robert H.Carter, BrandonDavis, Anne-ChristineMicrowave Background Constraints on Decaying DefectsParticle Physics - PhenomenologyEmbedded defects are predicted in a host of particle physics theories, in particular in the standard electroweak theory. They can be stabilized by interactions with the cosmological plasma, but will decay once the plasma falls out of equilibrium, emitting a substantial fraction of non-thermal photons. If the decay happens after a redshift of about $10^6$, these photons will give rise to spectral distortions of the Cosmic Microwave Background, which leads to strong constraints on the underlying particle physics theory. Such constraints apply to any model with decaying defects, and in particular to theories predicting decaying vortons, thereby leading to constraints stronger than the dark matter limit.Embedded defects are predicted in a host of particle physics theories, in particular in the standard electroweak theory. They can be stabilized by interactions with the cosmological plasma, but will decay once the plasma falls out of equilibrium, emitting a substantial fraction of non-thermal photons. If the decay happens after a redshift of about $10^6$, these photons will give rise to spectral distortions of the Cosmic Microwave Background, which leads to strong constraints on the underlying particle physics theory. Such constraints apply to any model with decaying defects, and in particular to theories predicting decaying vortons, thereby leading to constraints stronger than the dark matter limit.Embedded defects are predicted in a host of particle physics theories, in particular, in the standard electroweak theory. They can be stabilized by interactions with the cosmological plasma, but will decay once the plasma falls out of equilibrium, emitting a substantial fraction of non-thermal photons. If the decay happens after a redshift of about 10 6 , these photons will give rise to spectral distortions of the Cosmic Microwave Background, which leads to strong constraints on the underlying particle physics theory. Such constraints apply to any model with decaying defects, and in particular to theories predicting decaying vortons, thereby leading to constraints stronger than the dark matter limit.hep-ph/0202168CERN-TH-2002-043oai:cds.cern.ch:5388602002-02-17
spellingShingle Particle Physics - Phenomenology
Brandenberger, Robert H.
Carter, Brandon
Davis, Anne-Christine
Microwave Background Constraints on Decaying Defects
title Microwave Background Constraints on Decaying Defects
title_full Microwave Background Constraints on Decaying Defects
title_fullStr Microwave Background Constraints on Decaying Defects
title_full_unstemmed Microwave Background Constraints on Decaying Defects
title_short Microwave Background Constraints on Decaying Defects
title_sort microwave background constraints on decaying defects
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1016/S0370-2693(02)01675-1
http://cds.cern.ch/record/538860
work_keys_str_mv AT brandenbergerroberth microwavebackgroundconstraintsondecayingdefects
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