Utilize este identificador para referenciar este registo: http://hdl.handle.net/10400.21/2210
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dc.contributor.authorFelipe, Ricardo Gonzalez-
dc.contributor.authorManreza Paret, D.-
dc.contributor.authorPerez Martinez, A.-
dc.date.accessioned2013-02-15T16:03:44Z-
dc.date.available2013-02-15T16:03:44Z-
dc.date.issued2011-01-
dc.identifier.citationFELIPE, R. Gonzalez; MANREZA PARET, D.; PEREZ MARTINEZ, A. - Magnetized color flavor locked state and compact stars. European Physical Journal A. ISSN 1434-6001. Vol. 47, n.º 1 (2011).por
dc.identifier.issn1434-6001-
dc.identifier.urihttp://hdl.handle.net/10400.21/2210-
dc.description.abstractThe stability of the color flavor locked phase in the presence of a strong magnetic field is investigated within the phenomenological MIT bag model, taking into account the variation of the strange quark mass, the baryon density, the magnetic field, as well as the bag and gap parameters. It is found that the minimum value of the energy per baryon in a color flavor locked state at vanishing pressure is lower than the corresponding one for unpaired magnetized strange quark matter and, as the magnetic field increases, the energy per baryon decreases. This implies that magnetized colorflavor locked matter is more stable and could become the ground state inside neutron stars. The mass-radius relation for such stars is also studied.por
dc.language.isoengpor
dc.publisherSpringerpor
dc.relation.ispartofseries;1-
dc.rightsrestrictedAccesspor
dc.subjectHigh-Density QCDpor
dc.subjectNeutron-Starpor
dc.subjectQuark Matterpor
dc.subjectSymmetry-Breakingpor
dc.subjectSuperconductivitypor
dc.subjectLockingpor
dc.subjectPulsarpor
dc.subjectFieldpor
dc.subjectGappor
dc.titleMagnetized color flavor locked state and compact starspor
dc.typearticlepor
dc.peerreviewedyespor
degois.publication.issue1por
degois.publication.locationNew Yorkpor
degois.publication.titleEuropean Physical Journal Apor
degois.publication.volume47por
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