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Comment on "More Axions from Strings''
We comment on a claim that axion strings show a long-term logarithmic increase in the number of Hubble lengths per Hubble volume [arXiv:2007.04990], thereby violating the standard "scaling" expectation of an O(1) constant. We demonstrate that the string density data presented in [arXiv:200...
Autores principales: | , , , |
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Lenguaje: | eng |
Publicado: |
2021
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Acceso en línea: | http://cds.cern.ch/record/2781793 |
_version_ | 1780971959156211712 |
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author | Hindmarsh, Mark Lizarraga, Joanes Lopez-Eiguren, Asier Urrestilla, Jon |
author_facet | Hindmarsh, Mark Lizarraga, Joanes Lopez-Eiguren, Asier Urrestilla, Jon |
author_sort | Hindmarsh, Mark |
collection | CERN |
description | We comment on a claim that axion strings show a long-term logarithmic increase in the number of Hubble lengths per Hubble volume [arXiv:2007.04990], thereby violating the standard "scaling" expectation of an O(1) constant. We demonstrate that the string density data presented in [arXiv:2007.04990] are consistent with standard scaling, at a string density consistent with that obtained by us [arXiv:1908.03522, arXiv:2102.07723] and other groups. A transient slow growth in Hubble lengths per Hubble volume towards its constant scaling value is explained by standard network modelling [arXiv:2102.07723]. |
id | cern-2781793 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2021 |
record_format | invenio |
spelling | cern-27817932021-12-17T09:00:16Zhttp://cds.cern.ch/record/2781793engHindmarsh, MarkLizarraga, JoanesLopez-Eiguren, AsierUrrestilla, JonComment on "More Axions from Strings''hep-phParticle Physics - Phenomenologyastro-ph.COAstrophysics and AstronomyWe comment on a claim that axion strings show a long-term logarithmic increase in the number of Hubble lengths per Hubble volume [arXiv:2007.04990], thereby violating the standard "scaling" expectation of an O(1) constant. We demonstrate that the string density data presented in [arXiv:2007.04990] are consistent with standard scaling, at a string density consistent with that obtained by us [arXiv:1908.03522, arXiv:2102.07723] and other groups. A transient slow growth in Hubble lengths per Hubble volume towards its constant scaling value is explained by standard network modelling [arXiv:2102.07723].arXiv:2109.09679oai:cds.cern.ch:27817932021-09-20 |
spellingShingle | hep-ph Particle Physics - Phenomenology astro-ph.CO Astrophysics and Astronomy Hindmarsh, Mark Lizarraga, Joanes Lopez-Eiguren, Asier Urrestilla, Jon Comment on "More Axions from Strings'' |
title | Comment on "More Axions from Strings'' |
title_full | Comment on "More Axions from Strings'' |
title_fullStr | Comment on "More Axions from Strings'' |
title_full_unstemmed | Comment on "More Axions from Strings'' |
title_short | Comment on "More Axions from Strings'' |
title_sort | comment on "more axions from strings'' |
topic | hep-ph Particle Physics - Phenomenology astro-ph.CO Astrophysics and Astronomy |
url | http://cds.cern.ch/record/2781793 |
work_keys_str_mv | AT hindmarshmark commentonmoreaxionsfromstrings AT lizarragajoanes commentonmoreaxionsfromstrings AT lopezeigurenasier commentonmoreaxionsfromstrings AT urrestillajon commentonmoreaxionsfromstrings |