Thermal friction as a solution to the Hubble tension

A new component added to the standard model of cosmology that behaves like a cosmological constant at early times and then dilutes away as radiation or faster can resolve the Hubble tension. We show that a rolling axion coupled to a non-Abelian gauge group exhibits the behavior of such an extra comp...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Physical review. D 2020-04, Vol.101 (8), Article 083537
Hauptverfasser: Berghaus, Kim V., Karwal, Tanvi
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue 8
container_start_page
container_title Physical review. D
container_volume 101
creator Berghaus, Kim V.
Karwal, Tanvi
description A new component added to the standard model of cosmology that behaves like a cosmological constant at early times and then dilutes away as radiation or faster can resolve the Hubble tension. We show that a rolling axion coupled to a non-Abelian gauge group exhibits the behavior of such an extra component at the background level and can present a natural particle-physics model solution to the Hubble tension. We compare the contribution of this bottom-up model to the phenomenological fluid approximation and determine that CMB observables sensitive only to the background evolution of the Universe are expected to be similar in both cases, strengthening the case for this model to provide a viable solution to the Hubble tension.
doi_str_mv 10.1103/PhysRevD.101.083537
format Article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_2401234927</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2401234927</sourcerecordid><originalsourceid>FETCH-LOGICAL-c343t-fb023d585f7aa9f183925b830ac937a4eaa5c82494d6aea721aca8da0caa2cfc3</originalsourceid><addsrcrecordid>eNo9kF9LwzAUxYMoOOY-gS8BnztvctOleZT5Z8JAkfkcbrOEdXTtTFph395q1ad77uFwDvwYuxYwFwLw9nV3Sm_-834uQMyhwBz1GZtIpSEDkOb8Xwu4ZLOU9jDIBRgtxISpzc7HA9U8xMp1VdtwSpx4auv-5-ta3u08X_VlWXve-SYN7hW7CFQnP_u9U_b--LBZrrL1y9Pz8m6dOVTYZaEEidu8yIMmMkEUaGReFgjkDGpSnih3hVRGbRfkSUtBjootgSOSLjicspux9xjbj96nzu7bPjbDpJUKhERlpB5SOKZcbFOKPthjrA4UT1aA_SZk_wgNhrAjIfwCqvBaeA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2401234927</pqid></control><display><type>article</type><title>Thermal friction as a solution to the Hubble tension</title><source>American Physical Society Journals</source><creator>Berghaus, Kim V. ; Karwal, Tanvi</creator><creatorcontrib>Berghaus, Kim V. ; Karwal, Tanvi</creatorcontrib><description>A new component added to the standard model of cosmology that behaves like a cosmological constant at early times and then dilutes away as radiation or faster can resolve the Hubble tension. We show that a rolling axion coupled to a non-Abelian gauge group exhibits the behavior of such an extra component at the background level and can present a natural particle-physics model solution to the Hubble tension. We compare the contribution of this bottom-up model to the phenomenological fluid approximation and determine that CMB observables sensitive only to the background evolution of the Universe are expected to be similar in both cases, strengthening the case for this model to provide a viable solution to the Hubble tension.</description><identifier>ISSN: 2470-0010</identifier><identifier>EISSN: 2470-0029</identifier><identifier>DOI: 10.1103/PhysRevD.101.083537</identifier><language>eng</language><publisher>College Park: American Physical Society</publisher><subject>Astronomical models ; Cosmic microwave background ; Cosmological constant ; Cosmology</subject><ispartof>Physical review. D, 2020-04, Vol.101 (8), Article 083537</ispartof><rights>Copyright American Physical Society Apr 15, 2020</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c343t-fb023d585f7aa9f183925b830ac937a4eaa5c82494d6aea721aca8da0caa2cfc3</citedby><cites>FETCH-LOGICAL-c343t-fb023d585f7aa9f183925b830ac937a4eaa5c82494d6aea721aca8da0caa2cfc3</cites><orcidid>0000-0002-1384-9949 ; 0000-0003-2294-8188</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,2863,2864,27901,27902</link.rule.ids></links><search><creatorcontrib>Berghaus, Kim V.</creatorcontrib><creatorcontrib>Karwal, Tanvi</creatorcontrib><title>Thermal friction as a solution to the Hubble tension</title><title>Physical review. D</title><description>A new component added to the standard model of cosmology that behaves like a cosmological constant at early times and then dilutes away as radiation or faster can resolve the Hubble tension. We show that a rolling axion coupled to a non-Abelian gauge group exhibits the behavior of such an extra component at the background level and can present a natural particle-physics model solution to the Hubble tension. We compare the contribution of this bottom-up model to the phenomenological fluid approximation and determine that CMB observables sensitive only to the background evolution of the Universe are expected to be similar in both cases, strengthening the case for this model to provide a viable solution to the Hubble tension.</description><subject>Astronomical models</subject><subject>Cosmic microwave background</subject><subject>Cosmological constant</subject><subject>Cosmology</subject><issn>2470-0010</issn><issn>2470-0029</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNo9kF9LwzAUxYMoOOY-gS8BnztvctOleZT5Z8JAkfkcbrOEdXTtTFph395q1ad77uFwDvwYuxYwFwLw9nV3Sm_-834uQMyhwBz1GZtIpSEDkOb8Xwu4ZLOU9jDIBRgtxISpzc7HA9U8xMp1VdtwSpx4auv-5-ta3u08X_VlWXve-SYN7hW7CFQnP_u9U_b--LBZrrL1y9Pz8m6dOVTYZaEEidu8yIMmMkEUaGReFgjkDGpSnih3hVRGbRfkSUtBjootgSOSLjicspux9xjbj96nzu7bPjbDpJUKhERlpB5SOKZcbFOKPthjrA4UT1aA_SZk_wgNhrAjIfwCqvBaeA</recordid><startdate>20200427</startdate><enddate>20200427</enddate><creator>Berghaus, Kim V.</creator><creator>Karwal, Tanvi</creator><general>American Physical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-1384-9949</orcidid><orcidid>https://orcid.org/0000-0003-2294-8188</orcidid></search><sort><creationdate>20200427</creationdate><title>Thermal friction as a solution to the Hubble tension</title><author>Berghaus, Kim V. ; Karwal, Tanvi</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c343t-fb023d585f7aa9f183925b830ac937a4eaa5c82494d6aea721aca8da0caa2cfc3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Astronomical models</topic><topic>Cosmic microwave background</topic><topic>Cosmological constant</topic><topic>Cosmology</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Berghaus, Kim V.</creatorcontrib><creatorcontrib>Karwal, Tanvi</creatorcontrib><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Physical review. D</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Berghaus, Kim V.</au><au>Karwal, Tanvi</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Thermal friction as a solution to the Hubble tension</atitle><jtitle>Physical review. D</jtitle><date>2020-04-27</date><risdate>2020</risdate><volume>101</volume><issue>8</issue><artnum>083537</artnum><issn>2470-0010</issn><eissn>2470-0029</eissn><abstract>A new component added to the standard model of cosmology that behaves like a cosmological constant at early times and then dilutes away as radiation or faster can resolve the Hubble tension. We show that a rolling axion coupled to a non-Abelian gauge group exhibits the behavior of such an extra component at the background level and can present a natural particle-physics model solution to the Hubble tension. We compare the contribution of this bottom-up model to the phenomenological fluid approximation and determine that CMB observables sensitive only to the background evolution of the Universe are expected to be similar in both cases, strengthening the case for this model to provide a viable solution to the Hubble tension.</abstract><cop>College Park</cop><pub>American Physical Society</pub><doi>10.1103/PhysRevD.101.083537</doi><orcidid>https://orcid.org/0000-0002-1384-9949</orcidid><orcidid>https://orcid.org/0000-0003-2294-8188</orcidid></addata></record>
fulltext fulltext
identifier ISSN: 2470-0010
ispartof Physical review. D, 2020-04, Vol.101 (8), Article 083537
issn 2470-0010
2470-0029
language eng
recordid cdi_proquest_journals_2401234927
source American Physical Society Journals
subjects Astronomical models
Cosmic microwave background
Cosmological constant
Cosmology
title Thermal friction as a solution to the Hubble tension
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-21T19%3A50%3A41IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Thermal%20friction%20as%20a%20solution%20to%20the%20Hubble%20tension&rft.jtitle=Physical%20review.%20D&rft.au=Berghaus,%20Kim%20V.&rft.date=2020-04-27&rft.volume=101&rft.issue=8&rft.artnum=083537&rft.issn=2470-0010&rft.eissn=2470-0029&rft_id=info:doi/10.1103/PhysRevD.101.083537&rft_dat=%3Cproquest_cross%3E2401234927%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2401234927&rft_id=info:pmid/&rfr_iscdi=true