Superfluidity in beta-stable neutron star matter
Phys.Rev.Lett.77:1428-1431,1996 In this work we present results for pairing gaps in $\beta$--stable neutron star matter with electrons and muons using a relativistic Dirac--Brueckner--Hartree--Fock approach, starting with modern meson--exchange models for the nucleon--nucleon interaction. Results ar...
Gespeichert in:
| Hauptverfasser: | , , , |
|---|---|
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext bestellen |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | |
|---|---|
| container_issue | |
| container_start_page | |
| container_title | |
| container_volume | |
| creator | Elgaroey, Oe Engvik, L Hjorth-Jensen, M Osnes, E |
| description | Phys.Rev.Lett.77:1428-1431,1996 In this work we present results for pairing gaps in $\beta$--stable neutron
star matter with electrons and muons using a relativistic
Dirac--Brueckner--Hartree--Fock approach, starting with modern meson--exchange
models for the nucleon--nucleon interaction. Results are given for
superconducting $^1S_0$ protons and $^3P_2$ and $^1D_2$ neutron superfluids. A
comparison is made with recent non--relativistic calculations and the
implications for neutron star cooling are discussed. |
| doi_str_mv | 10.48550/arxiv.nucl-th/9604041 |
| format | Article |
| fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_nucl_th_9604041</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>nucl_th_9604041</sourcerecordid><originalsourceid>FETCH-arxiv_primary_nucl_th_96040413</originalsourceid><addsrcrecordid>eNpjYJAzNNAzsTA1NdBPLKrILNPLK03O0S3J0Lc0MzAxMDHkZDAILi1ILUrLKc1MySypVMjMU0hKLUnULS5JTMpJVchLLS0pys9TAHKLFHITS0pSi3gYWNMSc4pTeaE0N4OKm2uIs4cu2IL4gqLM3MSiyniQRfElGfFQi4yJVAYAVqg4tw</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Superfluidity in beta-stable neutron star matter</title><source>arXiv.org</source><creator>Elgaroey, Oe ; Engvik, L ; Hjorth-Jensen, M ; Osnes, E</creator><creatorcontrib>Elgaroey, Oe ; Engvik, L ; Hjorth-Jensen, M ; Osnes, E</creatorcontrib><description>Phys.Rev.Lett.77:1428-1431,1996 In this work we present results for pairing gaps in $\beta$--stable neutron
star matter with electrons and muons using a relativistic
Dirac--Brueckner--Hartree--Fock approach, starting with modern meson--exchange
models for the nucleon--nucleon interaction. Results are given for
superconducting $^1S_0$ protons and $^3P_2$ and $^1D_2$ neutron superfluids. A
comparison is made with recent non--relativistic calculations and the
implications for neutron star cooling are discussed.</description><identifier>DOI: 10.48550/arxiv.nucl-th/9604041</identifier><language>eng</language><subject>Physics - Nuclear Theory</subject><creationdate>1996-04</creationdate><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/nucl-th/9604041$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.nucl-th/9604041$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1103/PhysRevLett.77.1428$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Elgaroey, Oe</creatorcontrib><creatorcontrib>Engvik, L</creatorcontrib><creatorcontrib>Hjorth-Jensen, M</creatorcontrib><creatorcontrib>Osnes, E</creatorcontrib><title>Superfluidity in beta-stable neutron star matter</title><description>Phys.Rev.Lett.77:1428-1431,1996 In this work we present results for pairing gaps in $\beta$--stable neutron
star matter with electrons and muons using a relativistic
Dirac--Brueckner--Hartree--Fock approach, starting with modern meson--exchange
models for the nucleon--nucleon interaction. Results are given for
superconducting $^1S_0$ protons and $^3P_2$ and $^1D_2$ neutron superfluids. A
comparison is made with recent non--relativistic calculations and the
implications for neutron star cooling are discussed.</description><subject>Physics - Nuclear Theory</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1996</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNpjYJAzNNAzsTA1NdBPLKrILNPLK03O0S3J0Lc0MzAxMDHkZDAILi1ILUrLKc1MySypVMjMU0hKLUnULS5JTMpJVchLLS0pys9TAHKLFHITS0pSi3gYWNMSc4pTeaE0N4OKm2uIs4cu2IL4gqLM3MSiyniQRfElGfFQi4yJVAYAVqg4tw</recordid><startdate>19960425</startdate><enddate>19960425</enddate><creator>Elgaroey, Oe</creator><creator>Engvik, L</creator><creator>Hjorth-Jensen, M</creator><creator>Osnes, E</creator><scope>GOX</scope></search><sort><creationdate>19960425</creationdate><title>Superfluidity in beta-stable neutron star matter</title><author>Elgaroey, Oe ; Engvik, L ; Hjorth-Jensen, M ; Osnes, E</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-arxiv_primary_nucl_th_96040413</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1996</creationdate><topic>Physics - Nuclear Theory</topic><toplevel>online_resources</toplevel><creatorcontrib>Elgaroey, Oe</creatorcontrib><creatorcontrib>Engvik, L</creatorcontrib><creatorcontrib>Hjorth-Jensen, M</creatorcontrib><creatorcontrib>Osnes, E</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Elgaroey, Oe</au><au>Engvik, L</au><au>Hjorth-Jensen, M</au><au>Osnes, E</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Superfluidity in beta-stable neutron star matter</atitle><date>1996-04-25</date><risdate>1996</risdate><abstract>Phys.Rev.Lett.77:1428-1431,1996 In this work we present results for pairing gaps in $\beta$--stable neutron
star matter with electrons and muons using a relativistic
Dirac--Brueckner--Hartree--Fock approach, starting with modern meson--exchange
models for the nucleon--nucleon interaction. Results are given for
superconducting $^1S_0$ protons and $^3P_2$ and $^1D_2$ neutron superfluids. A
comparison is made with recent non--relativistic calculations and the
implications for neutron star cooling are discussed.</abstract><doi>10.48550/arxiv.nucl-th/9604041</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | DOI: 10.48550/arxiv.nucl-th/9604041 |
| ispartof | |
| issn | |
| language | eng |
| recordid | cdi_arxiv_primary_nucl_th_9604041 |
| source | arXiv.org |
| subjects | Physics - Nuclear Theory |
| title | Superfluidity in beta-stable neutron star matter |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-11T04%3A30%3A35IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-arxiv_GOX&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Superfluidity%20in%20beta-stable%20neutron%20star%20matter&rft.au=Elgaroey,%20Oe&rft.date=1996-04-25&rft_id=info:doi/10.48550/arxiv.nucl-th/9604041&rft_dat=%3Carxiv_GOX%3Enucl_th_9604041%3C/arxiv_GOX%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 |