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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...
Autores principales: | , , |
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Lenguaje: | eng |
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2002
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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. |
id | cern-538860 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2002 |
record_format | invenio |
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 AT carterbrandon microwavebackgroundconstraintsondecayingdefects AT davisannechristine microwavebackgroundconstraintsondecayingdefects |