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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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Lenguaje: | eng |
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2022
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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. |
id | cern-2845031 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2022 |
record_format | invenio |
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 |
work_keys_str_mv | AT pradlerjosef istherearadioexcessfromthedecouplingofprerecombinationbremsstrahlung |