A Skyrme parametrization from subnuclear to neutron star densities
Identifieur interne : 000145 ( France/Analysis ); précédent : 000144; suivant : 000146A Skyrme parametrization from subnuclear to neutron star densities
Auteurs : E. Chabanat [France] ; P. Bonche [France] ; P. Haensel [Pologne] ; J. Meyer [France] ; R. Schaeffer [France]Source :
- Nuclear Physics, Section A [ 0375-9474 ] ; 1997.
Abstract
Skyrme effective forces are revisited to improve their behavior with respect to the isospin degree of freedom from the stability line to the most exotic nuclei that coming experimental facilities will produce. To achieve the best possible calculation of nuclear properties up to the neutron drip line, it is proposed to fit the neutron matter equation of state of the UV14+UVII theoretical model up to high densities to avoid any collapses or unphysical features of the resulting equation of state in the Skyrme framework. This last and very severe constraint on these interactions allows a prospective study of both neutron rich nuclei and neutron star matter.
Url:
DOI: 10.1016/S0375-9474(97)00596-4
Affiliations:
Links toward previous steps (curation, corpus...)
- to stream Main, to step Corpus: 001020
- to stream Main, to step Curation: 001020
- to stream Main, to step Exploration: 000545
- to stream France, to step Extraction: 000145
Links to Exploration step
ISTEX:9248180B5C7CB00F05BF7AFBBBB0CBABD44CA5D1Le document en format XML
<record><TEI wicri:istexFullTextTei="biblStruct"><teiHeader><fileDesc><titleStmt><title>A Skyrme parametrization from subnuclear to neutron star densities</title><author><name sortKey="Chabanat, E" sort="Chabanat, E" uniqKey="Chabanat E" first="E." last="Chabanat">E. Chabanat</name></author><author><name sortKey="Bonche, P" sort="Bonche, P" uniqKey="Bonche P" first="P." last="Bonche">P. Bonche</name></author><author><name sortKey="Haensel, P" sort="Haensel, P" uniqKey="Haensel P" first="P." last="Haensel">P. Haensel</name></author><author><name sortKey="Meyer, J" sort="Meyer, J" uniqKey="Meyer J" first="J." last="Meyer">J. Meyer</name></author><author><name sortKey="Schaeffer, R" sort="Schaeffer, R" uniqKey="Schaeffer R" first="R." last="Schaeffer">R. Schaeffer</name></author></titleStmt><publicationStmt><idno type="wicri:source">ISTEX</idno><idno type="RBID">ISTEX:9248180B5C7CB00F05BF7AFBBBB0CBABD44CA5D1</idno><date when="1997" year="1997">1997</date><idno type="doi">10.1016/S0375-9474(97)00596-4</idno><idno type="url">https://api.istex.fr/document/9248180B5C7CB00F05BF7AFBBBB0CBABD44CA5D1/fulltext/pdf</idno><idno type="wicri:Area/Main/Corpus">001020</idno><idno type="wicri:explorRef" wicri:stream="Main" wicri:step="Corpus" wicri:corpus="ISTEX">001020</idno><idno type="wicri:Area/Main/Curation">001020</idno><idno type="wicri:Area/Main/Exploration">000545</idno><idno type="wicri:explorRef" wicri:stream="Main" wicri:step="Exploration">000545</idno><idno type="wicri:Area/France/Extraction">000145</idno></publicationStmt><sourceDesc><biblStruct><analytic><title level="a">A Skyrme parametrization from subnuclear to neutron star densities</title><author><name sortKey="Chabanat, E" sort="Chabanat, E" uniqKey="Chabanat E" first="E." last="Chabanat">E. Chabanat</name><affiliation wicri:level="3"><country xml:lang="fr">France</country><wicri:regionArea>Institut de Physique Nucléaire de Lyon, CNRS-IN2P3 / Université Claude Bernard Lyon 1, 43, Bd. du 11.11.18, 69622 Villeurbanne Cedex</wicri:regionArea><placeName><region type="region" nuts="2">Auvergne-Rhône-Alpes</region><region type="old region" nuts="2">Rhône-Alpes</region><settlement type="city">Villeurbanne</settlement></placeName></affiliation></author><author><name sortKey="Bonche, P" sort="Bonche, P" uniqKey="Bonche P" first="P." last="Bonche">P. Bonche</name><affiliation wicri:level="3"><country xml:lang="fr">France</country><wicri:regionArea>Service de Physique Théorique, CEA Saclay, 91191 Gif sur Yvette Cedex</wicri:regionArea><placeName><region type="region" nuts="2">Île-de-France</region><settlement type="city">Gif sur Yvette</settlement></placeName></affiliation></author><author><name sortKey="Haensel, P" sort="Haensel, P" uniqKey="Haensel P" first="P." last="Haensel">P. Haensel</name><affiliation wicri:level="1"><country xml:lang="fr">Pologne</country><wicri:regionArea>N. Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, PL-00-716 Warszawa</wicri:regionArea><wicri:noRegion>PL-00-716 Warszawa</wicri:noRegion></affiliation></author><author><name sortKey="Meyer, J" sort="Meyer, J" uniqKey="Meyer J" first="J." last="Meyer">J. Meyer</name><affiliation wicri:level="3"><country xml:lang="fr">France</country><wicri:regionArea>Institut de Physique Nucléaire de Lyon, CNRS-IN2P3 / Université Claude Bernard Lyon 1, 43, Bd. du 11.11.18, 69622 Villeurbanne Cedex</wicri:regionArea><placeName><region type="region" nuts="2">Auvergne-Rhône-Alpes</region><region type="old region" nuts="2">Rhône-Alpes</region><settlement type="city">Villeurbanne</settlement></placeName></affiliation><affiliation wicri:level="1"><country wicri:rule="url">France</country></affiliation></author><author><name sortKey="Schaeffer, R" sort="Schaeffer, R" uniqKey="Schaeffer R" first="R." last="Schaeffer">R. Schaeffer</name><affiliation wicri:level="3"><country xml:lang="fr">France</country><wicri:regionArea>Service de Physique Théorique, CEA Saclay, 91191 Gif sur Yvette Cedex</wicri:regionArea><placeName><region type="region" nuts="2">Île-de-France</region><settlement type="city">Gif sur Yvette</settlement></placeName></affiliation></author></analytic><monogr></monogr><series><title level="j">Nuclear Physics, Section A</title><title level="j" type="abbrev">NUPHA</title><idno type="ISSN">0375-9474</idno><imprint><publisher>ELSEVIER</publisher><date type="published" when="1997">1997</date><biblScope unit="volume">627</biblScope><biblScope unit="issue">4</biblScope><biblScope unit="page" from="710">710</biblScope><biblScope unit="page" to="746">746</biblScope></imprint><idno type="ISSN">0375-9474</idno></series><idno type="istex">9248180B5C7CB00F05BF7AFBBBB0CBABD44CA5D1</idno><idno type="DOI">10.1016/S0375-9474(97)00596-4</idno><idno type="PII">S0375-9474(97)00596-4</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0375-9474</idno></seriesStmt></fileDesc><profileDesc><textClass></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">Skyrme effective forces are revisited to improve their behavior with respect to the isospin degree of freedom from the stability line to the most exotic nuclei that coming experimental facilities will produce. To achieve the best possible calculation of nuclear properties up to the neutron drip line, it is proposed to fit the neutron matter equation of state of the UV14+UVII theoretical model up to high densities to avoid any collapses or unphysical features of the resulting equation of state in the Skyrme framework. This last and very severe constraint on these interactions allows a prospective study of both neutron rich nuclei and neutron star matter.</div></front></TEI><affiliations><list><country><li>France</li><li>Pologne</li></country><region><li>Auvergne-Rhône-Alpes</li><li>Rhône-Alpes</li><li>Île-de-France</li></region><settlement><li>Gif sur Yvette</li><li>Villeurbanne</li></settlement></list><tree><country name="France"><region name="Auvergne-Rhône-Alpes"><name sortKey="Chabanat, E" sort="Chabanat, E" uniqKey="Chabanat E" first="E." last="Chabanat">E. Chabanat</name></region><name sortKey="Bonche, P" sort="Bonche, P" uniqKey="Bonche P" first="P." last="Bonche">P. Bonche</name><name sortKey="Meyer, J" sort="Meyer, J" uniqKey="Meyer J" first="J." last="Meyer">J. Meyer</name><name sortKey="Meyer, J" sort="Meyer, J" uniqKey="Meyer J" first="J." last="Meyer">J. Meyer</name><name sortKey="Schaeffer, R" sort="Schaeffer, R" uniqKey="Schaeffer R" first="R." last="Schaeffer">R. Schaeffer</name></country><country name="Pologne"><noRegion><name sortKey="Haensel, P" sort="Haensel, P" uniqKey="Haensel P" first="P." last="Haensel">P. Haensel</name></noRegion></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
EXPLOR_STEP=$WICRI_ROOT/Wicri/France/explor/AussoisV1/Data/France/Analysis
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 000145 | SxmlIndent | more
Ou
HfdSelect -h $EXPLOR_AREA/Data/France/Analysis/biblio.hfd -nk 000145 | SxmlIndent | more
Pour mettre un lien sur cette page dans le réseau Wicri
{{Explor lien
|wiki= Wicri/France
|area= AussoisV1
|flux= France
|étape= Analysis
|type= RBID
|clé= ISTEX:9248180B5C7CB00F05BF7AFBBBB0CBABD44CA5D1
|texte= A Skyrme parametrization from subnuclear to neutron star densities
}}
| This area was generated with Dilib version V0.6.29. |  |