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Compact Stars and Magnetized CFL Matter

2011-12Journal article Open access
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dc.contributor.authorPerez Martinez, Aurora
dc.contributor.authorFelipe, Ricardo Gonzalez
dc.contributor.authorManreza Paret, Darye
dc.date.accessioned2012-09-10T15:47:54Z
dc.date.available2012-09-10T15:47:54Z
dc.date.issued2011-12
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. 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 color flavor locked matter is more stable and could become the ground state inside neutron stars. The anisotropy of the pressures is discussed. The mass-radius relation for such stars is also studied.por
dc.identifier.citationPerez Martinez Aurora, Felipe Ricardo Gonzalez, Manreza Paret Darye.Compact Stars and Magnetized CFL Matter. nternational Journal of Modern Physics E-Nuclear Physics. 2011: 20, 84-92.por
dc.identifier.issn0218-3013
dc.identifier.urihttp://hdl.handle.net/10400.21/1754
dc.language.isoengpor
dc.peerreviewedyespor
dc.publisherAddress Publisherpor
dc.subjectMIT Bag Modelpor
dc.subjectStrong Magnetic Fieldpor
dc.subjectNeutron Starspor
dc.subjectColor-Flavor Lockingpor
dc.subjectHigh-Density QCDpor
dc.subjectQuark Matterpor
dc.subjectSymmetry-Breakingpor
dc.subjectNeutron-Starpor
dc.subjectSuperconductivitypor
dc.subjectPulsarpor
dc.subjectField Ipor
dc.subjectGappor
dc.titleCompact Stars and Magnetized CFL Matterpor
dc.typejournal article
dspace.entity.typePublication
oaire.citation.conferencePlaceSingaporepor
oaire.citation.endPage92por
oaire.citation.startPage84por
oaire.citation.titleInternational Journal of Modern Physics E-Nuclear Physicspor
oaire.citation.volume20por
rcaap.rightsrestrictedAccesspor
rcaap.typearticlepor

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