Precision Detection of the Cosmic Neutrino Background

In the standard big bang cosmology the canonical value for the ratio of relic neutrinos to cosmic microwave background (CMB) photons is 9/11. Within the framework of the standard model of particle physics there are small corrections, in sum about 1{percent} , due to slight heating of neutrinos by el...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	Physical Review Letters 1999-05, Vol.82 (20), p.3952-3955
Hauptverfasser:	Lopez, Robert E., Dodelson, Scott, Heckler, Andrew, Turner, Michael S.
Format:	Artikel
Sprache:	eng
Schlagworte:	BACKGROUND RADIATION COSMIC NEUTRINOS COSMIC RADIATION COSMOLOGY ELECTRON-POSITRON INTERACTIONS PHYSICS QUANTUM ELECTRODYNAMICS STANDARD MODEL
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

container_end_page	3955
container_issue	20
container_start_page	3952
container_title	Physical Review Letters
container_volume	82
creator	Lopez, Robert E. Dodelson, Scott Heckler, Andrew Turner, Michael S.
description	In the standard big bang cosmology the canonical value for the ratio of relic neutrinos to cosmic microwave background (CMB) photons is 9/11. Within the framework of the standard model of particle physics there are small corrections, in sum about 1{percent} , due to slight heating of neutrinos by electron-positron annihilations and finite-temperature QED effects. We show that this leads to changes in the predicted CMB anisotropies that will bias determination of the other cosmological parameters if not correctly taken into account. These changes might be detected by future satellite experiments. {copyright} {ital 1999} {ital The American Physical Society}
doi_str_mv	10.1103/PhysRevLett.82.3952
format	Article
fullrecord	<record><control><sourceid>crossref_osti_</sourceid><recordid>TN_cdi_crossref_primary_10_1103_PhysRevLett_82_3952</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>10_1103_PhysRevLett_82_3952</sourcerecordid><originalsourceid>FETCH-LOGICAL-c384t-31adaf6edd6bf412c3d4dca1d8b816f4b5ef0fa0a231a54ba2221c68607368fc3</originalsourceid><addsrcrecordid>eNpNkMtKAzEYhYMoWKtP4GZ8gKn_n2Qy6VLrFQYtouuQycVG7USSVOjbO6UuXJ2z-DgcPkLOEWaIwC6Xq21-cT-dK2Um6YzNG3pAJgjtvG4R-SGZADCs5wDtMTnJ-QMAkAo5Ic0yORNyiEN144ozZdeir8rKVYuY18FUT25TUhhida3N53uKm8GekiOvv7I7-8spebu7fV081N3z_ePiqqsNk7zUDLXVXjhrRe85UsMst0ajlb1E4XnfOA9eg6Yj2fBeU0rRCCmgZUJ6w6bkYr8bcwkqmzA-XJk4DONRxThyaEaG7RmTYs7JefWdwlqnrUJQOzvqnx0lqdrZYb_hp1uF</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Precision Detection of the Cosmic Neutrino Background</title><source>American Physical Society Journals</source><creator>Lopez, Robert E. ; Dodelson, Scott ; Heckler, Andrew ; Turner, Michael S.</creator><creatorcontrib>Lopez, Robert E. ; Dodelson, Scott ; Heckler, Andrew ; Turner, Michael S.</creatorcontrib><description>In the standard big bang cosmology the canonical value for the ratio of relic neutrinos to cosmic microwave background (CMB) photons is 9/11. Within the framework of the standard model of particle physics there are small corrections, in sum about 1{percent} , due to slight heating of neutrinos by electron-positron annihilations and finite-temperature QED effects. We show that this leads to changes in the predicted CMB anisotropies that will bias determination of the other cosmological parameters if not correctly taken into account. These changes might be detected by future satellite experiments. {copyright} {ital 1999} {ital The American Physical Society}</description><identifier>ISSN: 0031-9007</identifier><identifier>EISSN: 1079-7114</identifier><identifier>DOI: 10.1103/PhysRevLett.82.3952</identifier><language>eng</language><publisher>United States</publisher><subject>BACKGROUND RADIATION ; COSMIC NEUTRINOS ; COSMIC RADIATION ; COSMOLOGY ; ELECTRON-POSITRON INTERACTIONS ; PHYSICS ; QUANTUM ELECTRODYNAMICS ; STANDARD MODEL</subject><ispartof>Physical Review Letters, 1999-05, Vol.82 (20), p.3952-3955</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c384t-31adaf6edd6bf412c3d4dca1d8b816f4b5ef0fa0a231a54ba2221c68607368fc3</citedby><cites>FETCH-LOGICAL-c384t-31adaf6edd6bf412c3d4dca1d8b816f4b5ef0fa0a231a54ba2221c68607368fc3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,777,781,882,2863,2864,27905,27906</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/341405$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Lopez, Robert E.</creatorcontrib><creatorcontrib>Dodelson, Scott</creatorcontrib><creatorcontrib>Heckler, Andrew</creatorcontrib><creatorcontrib>Turner, Michael S.</creatorcontrib><title>Precision Detection of the Cosmic Neutrino Background</title><title>Physical Review Letters</title><description>In the standard big bang cosmology the canonical value for the ratio of relic neutrinos to cosmic microwave background (CMB) photons is 9/11. Within the framework of the standard model of particle physics there are small corrections, in sum about 1{percent} , due to slight heating of neutrinos by electron-positron annihilations and finite-temperature QED effects. We show that this leads to changes in the predicted CMB anisotropies that will bias determination of the other cosmological parameters if not correctly taken into account. These changes might be detected by future satellite experiments. {copyright} {ital 1999} {ital The American Physical Society}</description><subject>BACKGROUND RADIATION</subject><subject>COSMIC NEUTRINOS</subject><subject>COSMIC RADIATION</subject><subject>COSMOLOGY</subject><subject>ELECTRON-POSITRON INTERACTIONS</subject><subject>PHYSICS</subject><subject>QUANTUM ELECTRODYNAMICS</subject><subject>STANDARD MODEL</subject><issn>0031-9007</issn><issn>1079-7114</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1999</creationdate><recordtype>article</recordtype><recordid>eNpNkMtKAzEYhYMoWKtP4GZ8gKn_n2Qy6VLrFQYtouuQycVG7USSVOjbO6UuXJ2z-DgcPkLOEWaIwC6Xq21-cT-dK2Um6YzNG3pAJgjtvG4R-SGZADCs5wDtMTnJ-QMAkAo5Ic0yORNyiEN144ozZdeir8rKVYuY18FUT25TUhhida3N53uKm8GekiOvv7I7-8spebu7fV081N3z_ePiqqsNk7zUDLXVXjhrRe85UsMst0ajlb1E4XnfOA9eg6Yj2fBeU0rRCCmgZUJ6w6bkYr8bcwkqmzA-XJk4DONRxThyaEaG7RmTYs7JefWdwlqnrUJQOzvqnx0lqdrZYb_hp1uF</recordid><startdate>19990517</startdate><enddate>19990517</enddate><creator>Lopez, Robert E.</creator><creator>Dodelson, Scott</creator><creator>Heckler, Andrew</creator><creator>Turner, Michael S.</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope></search><sort><creationdate>19990517</creationdate><title>Precision Detection of the Cosmic Neutrino Background</title><author>Lopez, Robert E. ; Dodelson, Scott ; Heckler, Andrew ; Turner, Michael S.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c384t-31adaf6edd6bf412c3d4dca1d8b816f4b5ef0fa0a231a54ba2221c68607368fc3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1999</creationdate><topic>BACKGROUND RADIATION</topic><topic>COSMIC NEUTRINOS</topic><topic>COSMIC RADIATION</topic><topic>COSMOLOGY</topic><topic>ELECTRON-POSITRON INTERACTIONS</topic><topic>PHYSICS</topic><topic>QUANTUM ELECTRODYNAMICS</topic><topic>STANDARD MODEL</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Lopez, Robert E.</creatorcontrib><creatorcontrib>Dodelson, Scott</creatorcontrib><creatorcontrib>Heckler, Andrew</creatorcontrib><creatorcontrib>Turner, Michael S.</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Physical Review Letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Lopez, Robert E.</au><au>Dodelson, Scott</au><au>Heckler, Andrew</au><au>Turner, Michael S.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Precision Detection of the Cosmic Neutrino Background</atitle><jtitle>Physical Review Letters</jtitle><date>1999-05-17</date><risdate>1999</risdate><volume>82</volume><issue>20</issue><spage>3952</spage><epage>3955</epage><pages>3952-3955</pages><issn>0031-9007</issn><eissn>1079-7114</eissn><abstract>In the standard big bang cosmology the canonical value for the ratio of relic neutrinos to cosmic microwave background (CMB) photons is 9/11. Within the framework of the standard model of particle physics there are small corrections, in sum about 1{percent} , due to slight heating of neutrinos by electron-positron annihilations and finite-temperature QED effects. We show that this leads to changes in the predicted CMB anisotropies that will bias determination of the other cosmological parameters if not correctly taken into account. These changes might be detected by future satellite experiments. {copyright} {ital 1999} {ital The American Physical Society}</abstract><cop>United States</cop><doi>10.1103/PhysRevLett.82.3952</doi><tpages>4</tpages><oa>free_for_read</oa></addata></record>
fulltext	fulltext
identifier	ISSN: 0031-9007
ispartof	Physical Review Letters, 1999-05, Vol.82 (20), p.3952-3955
issn	0031-9007 1079-7114
language	eng
recordid	cdi_crossref_primary_10_1103_PhysRevLett_82_3952
source	American Physical Society Journals
subjects	BACKGROUND RADIATION COSMIC NEUTRINOS COSMIC RADIATION COSMOLOGY ELECTRON-POSITRON INTERACTIONS PHYSICS QUANTUM ELECTRODYNAMICS STANDARD MODEL
title	Precision Detection of the Cosmic Neutrino Background
url	https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-19T19%3A56%3A47IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-crossref_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Precision%20Detection%20of%20the%20Cosmic%20Neutrino%20Background&rft.jtitle=Physical%20Review%20Letters&rft.au=Lopez,%20Robert%20E.&rft.date=1999-05-17&rft.volume=82&rft.issue=20&rft.spage=3952&rft.epage=3955&rft.pages=3952-3955&rft.issn=0031-9007&rft.eissn=1079-7114&rft_id=info:doi/10.1103/PhysRevLett.82.3952&rft_dat=%3Ccrossref_osti_%3E10_1103_PhysRevLett_82_3952%3C/crossref_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true