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Is there a Radio Excess from the Decoupling of Pre-recombination Bremsstrahlung?

Recently it has been suggested that thermal bremsstrahlung emission, when it decouples prior to recombination, creates an excess over the Planck cosmic microwave background spectrum at sub-GHz frequencies. Remarkable by itself, this would also explain a long-standing unexplained deficit in the predi...

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Autor principal: Pradler, Josef
Lenguaje:eng
Publicado: 2022
Materias:
Acceso en línea:https://dx.doi.org/10.3847/2515-5172/acab64
http://cds.cern.ch/record/2845031
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author Pradler, Josef
author_facet Pradler, Josef
author_sort Pradler, Josef
collection CERN
description Recently it has been suggested that thermal bremsstrahlung emission, when it decouples prior to recombination, creates an excess over the Planck cosmic microwave background spectrum at sub-GHz frequencies. Remarkable by itself, this would also explain a long-standing unexplained deficit in the predictions of the extragalactic radio background. In this brief note, I reiterate that no such non-thermal component can arise by itself when matter and radiation remain kinetically coupled.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2022
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spelling cern-28450312023-01-31T09:41:36Zdoi:10.3847/2515-5172/acab64http://cds.cern.ch/record/2845031engPradler, JosefIs there a Radio Excess from the Decoupling of Pre-recombination Bremsstrahlung?hep-phastro-ph.COParticle Physics - PhenomenologyAstrophysics and AstronomyRecently it has been suggested that thermal bremsstrahlung emission, when it decouples prior to recombination, creates an excess over the Planck cosmic microwave background spectrum at sub-GHz frequencies. Remarkable by itself, this would also explain a long-standing unexplained deficit in the predictions of the extragalactic radio background. In this brief note, I reiterate that no such non-thermal component can arise by itself when matter and radiation remain kinetically coupled.Recently it has been suggested that thermal bremsstrahlung emission, when it decouples prior to recombination, creates an excess over the Planck cosmic microwave background spectrum at sub-GHz frequencies. Remarkable by itself, this would also explain a long-standing unexplained deficit in the predictions of the extragalactic radio background. In this brief note we reiterate that no such non-thermal component can arise by itself when matter and radiation remain kinetically coupled.arXiv:2205.07474oai:cds.cern.ch:28450312022-05-16
spellingShingle hep-ph
astro-ph.CO
Particle Physics - Phenomenology
Astrophysics and Astronomy
Pradler, Josef
Is there a Radio Excess from the Decoupling of Pre-recombination Bremsstrahlung?
title Is there a Radio Excess from the Decoupling of Pre-recombination Bremsstrahlung?
title_full Is there a Radio Excess from the Decoupling of Pre-recombination Bremsstrahlung?
title_fullStr Is there a Radio Excess from the Decoupling of Pre-recombination Bremsstrahlung?
title_full_unstemmed Is there a Radio Excess from the Decoupling of Pre-recombination Bremsstrahlung?
title_short Is there a Radio Excess from the Decoupling of Pre-recombination Bremsstrahlung?
title_sort is there a radio excess from the decoupling of pre-recombination bremsstrahlung?
topic hep-ph
astro-ph.CO
Particle Physics - Phenomenology
Astrophysics and Astronomy
url https://dx.doi.org/10.3847/2515-5172/acab64
http://cds.cern.ch/record/2845031
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