Implications of the statistical bootstrap model for cosmology and galaxy formation

The statistical bootstrap model suggests that the hadron level density is sigma (m) approximately Cm/sup -3/ exp(m/T/sub h/). With a spectrum of this type, massive hadron resonances will predominate in the early stages of the big bang. and the universe will evolve out of equilibrium. The decay chain...

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Detalles Bibliográficos
Autores principales: Carlitz, R, Frautschi, S, Nahm, W
Lenguaje:eng
Publicado: 1973
Materias:
Astrophysics and Astronomy
Acceso en línea:http://cds.cern.ch/record/880678
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author Carlitz, R
Frautschi, S
Nahm, W
author_facet Carlitz, R
Frautschi, S
Nahm, W
author_sort Carlitz, R
collection CERN
description The statistical bootstrap model suggests that the hadron level density is sigma (m) approximately Cm/sup -3/ exp(m/T/sub h/). With a spectrum of this type, massive hadron resonances will predominate in the early stages of the big bang. and the universe will evolve out of equilibrium. The decay chains of these resonances may be so lengthy that the hadron era is prolonged far past its conventional end. The subsequent radiation era will be considerably foreshortened. and will have major consequences. (38 refs).
id cern-880678
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1973
record_format invenio
spelling cern-8806782019-09-30T06:29:59Zhttp://cds.cern.ch/record/880678engCarlitz, RFrautschi, SNahm, WImplications of the statistical bootstrap model for cosmology and galaxy formationAstrophysics and AstronomyThe statistical bootstrap model suggests that the hadron level density is sigma (m) approximately Cm/sup -3/ exp(m/T/sub h/). With a spectrum of this type, massive hadron resonances will predominate in the early stages of the big bang. and the universe will evolve out of equilibrium. The decay chains of these resonances may be so lengthy that the hadron era is prolonged far past its conventional end. The subsequent radiation era will be considerably foreshortened. and will have major consequences. (38 refs).oai:cds.cern.ch:8806781973
spellingShingle Astrophysics and Astronomy
Carlitz, R
Frautschi, S
Nahm, W
Implications of the statistical bootstrap model for cosmology and galaxy formation
title Implications of the statistical bootstrap model for cosmology and galaxy formation
title_full Implications of the statistical bootstrap model for cosmology and galaxy formation
title_fullStr Implications of the statistical bootstrap model for cosmology and galaxy formation
title_full_unstemmed Implications of the statistical bootstrap model for cosmology and galaxy formation
title_short Implications of the statistical bootstrap model for cosmology and galaxy formation
title_sort implications of the statistical bootstrap model for cosmology and galaxy formation
topic Astrophysics and Astronomy
url http://cds.cern.ch/record/880678
work_keys_str_mv AT carlitzr implicationsofthestatisticalbootstrapmodelforcosmologyandgalaxyformation
AT frautschis implicationsofthestatisticalbootstrapmodelforcosmologyandgalaxyformation
AT nahmw implicationsofthestatisticalbootstrapmodelforcosmologyandgalaxyformation

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