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dc.contributor.author
Weber, Fridolin
dc.contributor.author
Contrera, Gustavo Aníbal Gabriel
dc.contributor.author
Orsaria, Milva Gabriela
dc.contributor.author
Spinella, William
dc.contributor.author
Zubairi, Omair
dc.date.available
2019-07-29T22:06:19Z
dc.date.issued
2014-07
dc.identifier.citation
Weber, Fridolin; Contrera, Gustavo Aníbal Gabriel; Orsaria, Milva Gabriela; Spinella, William; Zubairi, Omair; Properties of high-density matter in neutron stars; World Scientific; Modern Physics Letters A: Particles and Fields; Gravitation; Cosmology and Nuclear Physics; 29; 23; 7-2014; 1430022-1430034
dc.identifier.issn
0217-7323
dc.identifier.uri
http://hdl.handle.net/11336/80531
dc.description.abstract
This short review aims at giving a brief overview of various states of matter that have been suggested to exist in the ultra-dense centers of neutron stars. Particular emphasis is put on the role of quark deconfinement in neutron stars and on the possible existence of compact stars made of absolutely stable strange quark matter (strange stars). Astrophysical phenomena, which distinguish neutron stars from quark stars, are discussed and the question of whether or not quark deconfinement may occur in neutron stars is investigated. Combined with observed astrophysical data, such studies are invaluable to delineate the complex structure of compressed baryonic matter and to put firm constraints on the largely unknown equation of state of such matter.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
World Scientific
dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
Neutron Stars
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Strange Stars
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Superdense Matter
dc.subject.classification
Astronomía
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Ciencias Físicas
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CIENCIAS NATURALES Y EXACTAS
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Física de Partículas y Campos
dc.subject.classification
Ciencias Físicas
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CIENCIAS NATURALES Y EXACTAS
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Física Nuclear
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Ciencias Físicas
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS
dc.title
Properties of high-density matter in neutron stars
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2019-06-19T16:53:38Z
dc.journal.volume
29
dc.journal.number
23
dc.journal.pagination
1430022-1430034
dc.journal.pais
Singapur
dc.description.fil
Fil: Weber, Fridolin. San Diego State University; Estados Unidos. University of California; Estados Unidos
dc.description.fil
Fil: Contrera, Gustavo Aníbal Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Área Física Teórica; Argentina. San Diego State University; Estados Unidos
dc.description.fil
Fil: Orsaria, Milva Gabriela. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Área Física Teórica; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina. San Diego State University; Estados Unidos
dc.description.fil
Fil: Spinella, William. San Diego State University. Computational Sciences Research Center; Estados Unidos
dc.description.fil
Fil: Zubairi, Omair. San Diego State University. Computational Sciences Research Center; Estados Unidos
dc.journal.title
Modern Physics Letters A: Particles and Fields; Gravitation; Cosmology and Nuclear Physics
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/http://www.worldscientific.com/doi/abs/10.1142/S0217732314300225
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1142/S0217732314300225
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1408.0079


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