Neutron star calculations with the phenomenological three-nucleon force
In this work, we have studied the effect of three-nucleon interaction on the neutron stars structure. In our calculations, we have considered the neutron star matter as a beta-stable nuclear matter. We have put the results concerning the TBF effect in perspective against two-body results and other c...
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| Veröffentlicht in: | European physical journal plus 2024-07, Vol.139 (7), p.620, Article 620 |
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| creator | Moeini, H. Bordbar, G. H. |
| description | In this work, we have studied the effect of three-nucleon interaction on the neutron stars structure. In our calculations, we have considered the neutron star matter as a beta-stable nuclear matter. We have put the results concerning the TBF effect in perspective against two-body results and other calculations of three-nucleon interactions, using the Urbana
v
14
potential and the parabolic approximation of the nuclear matter energy for approximating the problem of asymmetric nuclear matter. As such, solving the Tolman–Oppenheimer–Volkoff equation, we have estimated bulk properties of neutron stars and investigated how the present calculations would agree with the expected dynamical stability condition. |
| doi_str_mv | 10.1140/epjp/s13360-024-05416-4 |
| format | Article |
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v
14
potential and the parabolic approximation of the nuclear matter energy for approximating the problem of asymmetric nuclear matter. As such, solving the Tolman–Oppenheimer–Volkoff equation, we have estimated bulk properties of neutron stars and investigated how the present calculations would agree with the expected dynamical stability condition.</description><identifier>ISSN: 2190-5444</identifier><identifier>EISSN: 2190-5444</identifier><identifier>DOI: 10.1140/epjp/s13360-024-05416-4</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>Applied and Technical Physics ; Approximation ; Atomic ; Complex Systems ; Condensed Matter Physics ; Energy ; Equilibrium ; Gravity ; Mathematical and Computational Physics ; Molecular ; Neutron stars ; Neutrons ; Nuclear matter ; Nucleons ; Optical and Plasma Physics ; Physics ; Physics and Astronomy ; Regular Article ; Symmetry ; Theoretical ; Theory of relativity</subject><ispartof>European physical journal plus, 2024-07, Vol.139 (7), p.620, Article 620</ispartof><rights>The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2024. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c210t-dea57572a7a0d760e1c52fc0f979ee6a90176fbb03c210185ceb57677d2dd5823</cites><orcidid>0000-0002-3938-5820</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1140/epjp/s13360-024-05416-4$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1140/epjp/s13360-024-05416-4$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>315,781,785,27929,27930,41493,42562,51324</link.rule.ids></links><search><creatorcontrib>Moeini, H.</creatorcontrib><creatorcontrib>Bordbar, G. H.</creatorcontrib><title>Neutron star calculations with the phenomenological three-nucleon force</title><title>European physical journal plus</title><addtitle>Eur. Phys. J. Plus</addtitle><description>In this work, we have studied the effect of three-nucleon interaction on the neutron stars structure. In our calculations, we have considered the neutron star matter as a beta-stable nuclear matter. We have put the results concerning the TBF effect in perspective against two-body results and other calculations of three-nucleon interactions, using the Urbana
v
14
potential and the parabolic approximation of the nuclear matter energy for approximating the problem of asymmetric nuclear matter. As such, solving the Tolman–Oppenheimer–Volkoff equation, we have estimated bulk properties of neutron stars and investigated how the present calculations would agree with the expected dynamical stability condition.</description><subject>Applied and Technical Physics</subject><subject>Approximation</subject><subject>Atomic</subject><subject>Complex Systems</subject><subject>Condensed Matter Physics</subject><subject>Energy</subject><subject>Equilibrium</subject><subject>Gravity</subject><subject>Mathematical and Computational Physics</subject><subject>Molecular</subject><subject>Neutron stars</subject><subject>Neutrons</subject><subject>Nuclear matter</subject><subject>Nucleons</subject><subject>Optical and Plasma Physics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Regular Article</subject><subject>Symmetry</subject><subject>Theoretical</subject><subject>Theory of relativity</subject><issn>2190-5444</issn><issn>2190-5444</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><recordid>eNqFkNFKwzAUhoMoOOaewYLXcSdp0rSXMnQKQ2_0OqTp6dbRNTVpEd_e1Ap6ZyDkcPi_P_ARcs3gljEBa-yP_TqwNM2AAhcUpGAZFWdkwVkBVAohzv_Ml2QVwhHiEQUThViQ7TOOg3ddEgbjE2taO7ZmaFwXko9mOCTDAZP-gJ07xdu6fRMjcekRaTfaFiNZO2_xilzUpg24-nmX5O3h_nXzSHcv26fN3Y5azmCgFRqppOJGGahUBsis5LWFulAFYmYKYCqryxLSKc9yabGUKlOq4lUlc54uyc3c23v3PmIY9NGNvotf6hRyJkGkQsSUmlPWuxA81rr3zcn4T81AT-L0JE7P4nQUp7_F6YnMZzJEotuj_-3_D_0Cr_h0zg</recordid><startdate>20240716</startdate><enddate>20240716</enddate><creator>Moeini, H.</creator><creator>Bordbar, G. H.</creator><general>Springer Berlin Heidelberg</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><orcidid>https://orcid.org/0000-0002-3938-5820</orcidid></search><sort><creationdate>20240716</creationdate><title>Neutron star calculations with the phenomenological three-nucleon force</title><author>Moeini, H. ; Bordbar, G. H.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c210t-dea57572a7a0d760e1c52fc0f979ee6a90176fbb03c210185ceb57677d2dd5823</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Applied and Technical Physics</topic><topic>Approximation</topic><topic>Atomic</topic><topic>Complex Systems</topic><topic>Condensed Matter Physics</topic><topic>Energy</topic><topic>Equilibrium</topic><topic>Gravity</topic><topic>Mathematical and Computational Physics</topic><topic>Molecular</topic><topic>Neutron stars</topic><topic>Neutrons</topic><topic>Nuclear matter</topic><topic>Nucleons</topic><topic>Optical and Plasma Physics</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Regular Article</topic><topic>Symmetry</topic><topic>Theoretical</topic><topic>Theory of relativity</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Moeini, H.</creatorcontrib><creatorcontrib>Bordbar, G. H.</creatorcontrib><collection>CrossRef</collection><jtitle>European physical journal plus</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Moeini, H.</au><au>Bordbar, G. H.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Neutron star calculations with the phenomenological three-nucleon force</atitle><jtitle>European physical journal plus</jtitle><stitle>Eur. Phys. J. Plus</stitle><date>2024-07-16</date><risdate>2024</risdate><volume>139</volume><issue>7</issue><spage>620</spage><pages>620-</pages><artnum>620</artnum><issn>2190-5444</issn><eissn>2190-5444</eissn><abstract>In this work, we have studied the effect of three-nucleon interaction on the neutron stars structure. In our calculations, we have considered the neutron star matter as a beta-stable nuclear matter. We have put the results concerning the TBF effect in perspective against two-body results and other calculations of three-nucleon interactions, using the Urbana
v
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| fulltext | fulltext |
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| language | eng |
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| source | SpringerNature Journals |
| subjects | Applied and Technical Physics Approximation Atomic Complex Systems Condensed Matter Physics Energy Equilibrium Gravity Mathematical and Computational Physics Molecular Neutron stars Neutrons Nuclear matter Nucleons Optical and Plasma Physics Physics Physics and Astronomy Regular Article Symmetry Theoretical Theory of relativity |
| title | Neutron star calculations with the phenomenological three-nucleon force |
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