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Cubic neutrons

dc.contributor.authorLlanes Estrada, Felipe José
dc.contributor.authorMoreno Navarro, Gaspar
dc.date.accessioned2023-06-20T03:33:59Z
dc.date.available2023-06-20T03:33:59Z
dc.date.issued2012-02-28
dc.description© World Scientific Publishing Company. F.J.L.E. thanks a Caja Madrid fellowship for advanced study and the hospitality of the theory group at TU-Munich and the Exzellenzcluster Origin and Structure of the Universe. This work has been supported by grants 227431 HadronPhysics2 (EU), Consolider-CSD2007-00042, AIC10-D 000582, FPA2008-00592, FIS2008-01323, and UCM-BSCH GR58/08 910309 (Spain).
dc.description.abstractThe neutron is largely spherical and incompressible in atomic nuclei. These two properties are however challenged in the extreme pressure environment of a neutron star. Our variational computation within the Cornell model of Coulomb gauge QCD shows that the neutron (and also the Delta(3/2) baryon) can adopt cubic symmetry at an energy cost of about 150 MeV. Balancing this with the free energy gained by tighter neutron packing, we expose the possible softening of the equation of state of neutron matter.
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipCaja Madrid fellowship
dc.description.sponsorshipEU
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/22115
dc.identifier.doi10.1142/S0217732312500332
dc.identifier.issn0217-7323
dc.identifier.officialurlhttp://dx.doi.org/10.1142/S0217732312500332
dc.identifier.relatedurlhttp://arxiv.org/abs/1108.1859
dc.identifier.relatedurlhttp://www.worldscientific.com
dc.identifier.urihttps://hdl.handle.net/20.500.14352/43893
dc.issue.number6
dc.journal.titleModern Physics Letters A
dc.language.isoeng
dc.publisherWorld Scientific Publ Co Pte Ltd
dc.relation.projectID227431-HadronPhysics2
dc.relation.projectIDConsolider-CSD2007-000/12
dc.relation.projectIDAIC10-D-000582
dc.relation.projectIDFPA2008-00592
dc.relation.projectIDFIS2008-01323
dc.relation.projectIDUCM-BSCH GR58/08 910309
dc.rights.accessRightsopen access
dc.subject.cdu53
dc.subject.keywordHadron Deformation
dc.subject.keywordNeutron Stars
dc.subject.keywordEquation of State of Neutron Matter.
dc.subject.ucmFísica (Física)
dc.subject.unesco22 Física
dc.titleCubic neutrons
dc.typejournal article
dc.volume.number27
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dspace.entity.typePublication
relation.isAuthorOfPublication6290fe55-04e6-4532-91e6-1df735bdbdca
relation.isAuthorOfPublication.latestForDiscovery6290fe55-04e6-4532-91e6-1df735bdbdca

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