Properties of high-density matter in neutron stars

dc.creatorWeber, Fridolin
dc.creatorContrera, Gustavo Aníbal
dc.creatorOrsaria, Milva Gabriela
dc.creatorSpinella, William
dc.creatorZubairi, Omair
dc.date2014
dc.date2020-05-29T22:34:51Z
dc.date.accessioned2023-07-14T20:05:43Z
dc.date.available2023-07-14T20:05:43Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/97138
dc.identifierhttps://ri.conicet.gov.ar/11336/80531
dc.identifierhttp://www.worldscientific.com/doi/abs/10.1142/S0217732314300225
dc.identifierissn:0217-7323
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7437881
dc.descriptionThis 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.descriptionInstituto de Física La Plata
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.format1-9
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 2.5 Argentina (CC BY-NC-SA 2.5)
dc.subjectAstronomía
dc.subjectFísica
dc.subjectCiencias Exactas
dc.subjectNeutron stars
dc.subjectStrange stars
dc.subjectSuperdense matter
dc.titleProperties of high-density matter in neutron stars
dc.typeArticulo
dc.typePreprint


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