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Spectator stresses and CMB observables

The large-scale curvature perturbations induced by spectator anisotropic stresses are analyzed across the matter-radiation transition. It is assumed that the anisotropic stress is associated with a plasma component whose energy density is subdominant both today and prior to photon decoupling. The en...

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Autor principal: Giovannini, Massimo
Lenguaje:eng
Publicado: 2009
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.81.127302
http://cds.cern.ch/record/1230430
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author Giovannini, Massimo
author_facet Giovannini, Massimo
author_sort Giovannini, Massimo
collection CERN
description The large-scale curvature perturbations induced by spectator anisotropic stresses are analyzed across the matter-radiation transition. It is assumed that the anisotropic stress is associated with a plasma component whose energy density is subdominant both today and prior to photon decoupling. The enforcement of the momentum constraint and the interplay with the neutrino anisotropic stress determine the regular initial conditions of the Einstein-Boltzmann hierarchy. The Cosmic Microwave Background observables have shapes and phases which differ both from the ones of the conventional adiabatic mode as well as from their non-adiabatic counterparts.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2009
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spelling cern-12304302023-03-12T05:20:19Zdoi:10.1103/PhysRevD.81.127302http://cds.cern.ch/record/1230430engGiovannini, MassimoSpectator stresses and CMB observablesAstrophysics and AstronomyThe large-scale curvature perturbations induced by spectator anisotropic stresses are analyzed across the matter-radiation transition. It is assumed that the anisotropic stress is associated with a plasma component whose energy density is subdominant both today and prior to photon decoupling. The enforcement of the momentum constraint and the interplay with the neutrino anisotropic stress determine the regular initial conditions of the Einstein-Boltzmann hierarchy. The Cosmic Microwave Background observables have shapes and phases which differ both from the ones of the conventional adiabatic mode as well as from their non-adiabatic counterparts.The large-scale curvature perturbations induced by spectator anisotropic stresses are analyzed across the matter-radiation transition. It is assumed that the anisotropic stress is associated with a plasma component whose energy density is subdominant both today and prior to photon decoupling. The enforcement of the momentum constraint and the interplay with the neutrino anisotropic stress determine the regular initial conditions of the Einstein-Boltzmann hierarchy. The Cosmic Microwave Background observables have shapes and phases which differ both from the ones of the conventional adiabatic mode as well as from their non-adiabatic counterparts.arXiv:0912.4427CERN-PH-TH-2009-261CERN-PH-TH-2009-261oai:cds.cern.ch:12304302009-12-23
spellingShingle Astrophysics and Astronomy
Giovannini, Massimo
Spectator stresses and CMB observables
title Spectator stresses and CMB observables
title_full Spectator stresses and CMB observables
title_fullStr Spectator stresses and CMB observables
title_full_unstemmed Spectator stresses and CMB observables
title_short Spectator stresses and CMB observables
title_sort spectator stresses and cmb observables
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1103/PhysRevD.81.127302
http://cds.cern.ch/record/1230430
work_keys_str_mv AT giovanninimassimo spectatorstressesandcmbobservables