Urca processes in dense matter and neutron star cooling

Urca-processes were introduced into astrophysics by Gamow and Schoenberg in 1941. Neutrino cooling resulting from urca-processes plays an important role at the latest stages of evolution of massive stars. Recent work on neutrino emissivity of dense matter shows that neutrino cooling via urca-process...

Full description

Saved in:
Bibliographic Details
Published in:Space science reviews 1995-11, Vol.74 (3-4), p.427-436
Main Author: Haensel, Pawe?
Format: Article
Language:English
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c303t-75336a60726474902fc9732c09e661d57a9de6102f847400ddfdce07861fbbc53
cites cdi_FETCH-LOGICAL-c303t-75336a60726474902fc9732c09e661d57a9de6102f847400ddfdce07861fbbc53
container_end_page 436
container_issue 3-4
container_start_page 427
container_title Space science reviews
container_volume 74
creator Haensel, Pawe?
description Urca-processes were introduced into astrophysics by Gamow and Schoenberg in 1941. Neutrino cooling resulting from urca-processes plays an important role at the latest stages of evolution of massive stars. Recent work on neutrino emissivity of dense matter shows that neutrino cooling via urca-processes could determine the thermal evolution of young neutron stars, and that it depends dramatically on the composition of the neutron star core. In particular, if a neutron star contains a central core in which the 'direct urca-process' is operative, the cooling timescale shortens by many orders of magnitude. (Author)
doi_str_mv 10.1007/BF00751429
format article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_25949945</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>25949945</sourcerecordid><originalsourceid>FETCH-LOGICAL-c303t-75336a60726474902fc9732c09e661d57a9de6102f847400ddfdce07861fbbc53</originalsourceid><addsrcrecordid>eNpFkEFLxDAQhYMoWFcv_oKcPAjVSdImzVEXV4UFL-65ZJOpVNp0zbQH_70tu-DlPZj3Mcw8xm4FPAgA8_i8mbUUhbRnLBOlkbnVRp6zDEBVuVZQXbIrom-ABTcZM7vkHT-kwSMREm8jDxgJee_GERN3MfCI05iGyGl0ifth6Nr4dc0uGtcR3px8xXabl8_1W779eH1fP21zr0CNuSmV0k6DkbowhQXZeGuU9GBRaxFK42xALeZ5NecAITTBI5hKi2a_96Vasbvj3vnEnwlprPuWPHadizhMVMvSFtYWC3h_BH0aiBI29SG1vUu_tYB6ebb-70b9Ae5SVLE</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>25949945</pqid></control><display><type>article</type><title>Urca processes in dense matter and neutron star cooling</title><source>Springer Archives (Through 1996)</source><creator>Haensel, Pawe?</creator><creatorcontrib>Haensel, Pawe?</creatorcontrib><description>Urca-processes were introduced into astrophysics by Gamow and Schoenberg in 1941. Neutrino cooling resulting from urca-processes plays an important role at the latest stages of evolution of massive stars. Recent work on neutrino emissivity of dense matter shows that neutrino cooling via urca-processes could determine the thermal evolution of young neutron stars, and that it depends dramatically on the composition of the neutron star core. In particular, if a neutron star contains a central core in which the 'direct urca-process' is operative, the cooling timescale shortens by many orders of magnitude. (Author)</description><identifier>ISSN: 0038-6308</identifier><identifier>EISSN: 1572-9672</identifier><identifier>DOI: 10.1007/BF00751429</identifier><language>eng</language><ispartof>Space science reviews, 1995-11, Vol.74 (3-4), p.427-436</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c303t-75336a60726474902fc9732c09e661d57a9de6102f847400ddfdce07861fbbc53</citedby><cites>FETCH-LOGICAL-c303t-75336a60726474902fc9732c09e661d57a9de6102f847400ddfdce07861fbbc53</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>315,786,790,27957,27958</link.rule.ids></links><search><creatorcontrib>Haensel, Pawe?</creatorcontrib><title>Urca processes in dense matter and neutron star cooling</title><title>Space science reviews</title><description>Urca-processes were introduced into astrophysics by Gamow and Schoenberg in 1941. Neutrino cooling resulting from urca-processes plays an important role at the latest stages of evolution of massive stars. Recent work on neutrino emissivity of dense matter shows that neutrino cooling via urca-processes could determine the thermal evolution of young neutron stars, and that it depends dramatically on the composition of the neutron star core. In particular, if a neutron star contains a central core in which the 'direct urca-process' is operative, the cooling timescale shortens by many orders of magnitude. (Author)</description><issn>0038-6308</issn><issn>1572-9672</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1995</creationdate><recordtype>article</recordtype><recordid>eNpFkEFLxDAQhYMoWFcv_oKcPAjVSdImzVEXV4UFL-65ZJOpVNp0zbQH_70tu-DlPZj3Mcw8xm4FPAgA8_i8mbUUhbRnLBOlkbnVRp6zDEBVuVZQXbIrom-ABTcZM7vkHT-kwSMREm8jDxgJee_GERN3MfCI05iGyGl0ifth6Nr4dc0uGtcR3px8xXabl8_1W779eH1fP21zr0CNuSmV0k6DkbowhQXZeGuU9GBRaxFK42xALeZ5NecAITTBI5hKi2a_96Vasbvj3vnEnwlprPuWPHadizhMVMvSFtYWC3h_BH0aiBI29SG1vUu_tYB6ebb-70b9Ae5SVLE</recordid><startdate>199511</startdate><enddate>199511</enddate><creator>Haensel, Pawe?</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>199511</creationdate><title>Urca processes in dense matter and neutron star cooling</title><author>Haensel, Pawe?</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c303t-75336a60726474902fc9732c09e661d57a9de6102f847400ddfdce07861fbbc53</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1995</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Haensel, Pawe?</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Space science reviews</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Haensel, Pawe?</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Urca processes in dense matter and neutron star cooling</atitle><jtitle>Space science reviews</jtitle><date>1995-11</date><risdate>1995</risdate><volume>74</volume><issue>3-4</issue><spage>427</spage><epage>436</epage><pages>427-436</pages><issn>0038-6308</issn><eissn>1572-9672</eissn><notes>SourceType-Scholarly Journals-2</notes><notes>ObjectType-Feature-2</notes><notes>ObjectType-Conference Paper-1</notes><notes>content type line 23</notes><notes>SourceType-Conference Papers &amp; Proceedings-1</notes><notes>ObjectType-Article-3</notes><abstract>Urca-processes were introduced into astrophysics by Gamow and Schoenberg in 1941. Neutrino cooling resulting from urca-processes plays an important role at the latest stages of evolution of massive stars. Recent work on neutrino emissivity of dense matter shows that neutrino cooling via urca-processes could determine the thermal evolution of young neutron stars, and that it depends dramatically on the composition of the neutron star core. In particular, if a neutron star contains a central core in which the 'direct urca-process' is operative, the cooling timescale shortens by many orders of magnitude. (Author)</abstract><doi>10.1007/BF00751429</doi><tpages>10</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0038-6308
ispartof Space science reviews, 1995-11, Vol.74 (3-4), p.427-436
issn 0038-6308
1572-9672
language eng
recordid cdi_proquest_miscellaneous_25949945
source Springer Archives (Through 1996)
title Urca processes in dense matter and neutron star cooling
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-09-22T01%3A53%3A25IST&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=Urca%20processes%20in%20dense%20matter%20and%20neutron%20star%20cooling&rft.jtitle=Space%20science%20reviews&rft.au=Haensel,%20Pawe?&rft.date=1995-11&rft.volume=74&rft.issue=3-4&rft.spage=427&rft.epage=436&rft.pages=427-436&rft.issn=0038-6308&rft.eissn=1572-9672&rft_id=info:doi/10.1007/BF00751429&rft_dat=%3Cproquest_cross%3E25949945%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c303t-75336a60726474902fc9732c09e661d57a9de6102f847400ddfdce07861fbbc53%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=25949945&rft_id=info:pmid/&rfr_iscdi=true