dc.creatorAguirre, Ricardo Miguel
dc.creatorBauer, Eduardo
dc.date2015-08
dc.date2020-06-25T16:49:17Z
dc.date.accessioned2023-07-14T19:51:54Z
dc.date.available2023-07-14T19:51:54Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/99156
dc.identifierhttps://ri.conicet.gov.ar/11336/50038
dc.identifierissn:0954-3899
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7436986
dc.descriptionThe equation of state of nuclear matter is strongly affected by the presence of a magnetic field. Here we study the equilibrium configuration of asymmetric nuclear matter for a wide range of densities, isospin composition, temperatures and magnetic fields. Special attention is paid to the low density and low temperature domain, where a thermodynamical instability exists. Neglecting fluctuations of the Coulomb force, a coexistence of phases is found under such conditions, even for extreme magnetic intensities. We describe the nuclear interaction by using the non-relativistic Skyrme potential model within a Hartree-Fock approach. We found that the coexistence of phases modifies the equilibrium configuration, masking most of the manifestations of the spin polarized matter. However, the compressibility and the magnetic susceptibility show clear signals of this fact. Thermal effects are significative for both quantities, mainly out of the coexistence region.
dc.descriptionInstituto de Física La Plata
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.format105101-105120
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectFísica
dc.subjectAsymmetric matter
dc.subjectNeutron matter
dc.subjectNuclear forces
dc.subjectNuclear matter aspects of neutron stars
dc.titleCoexistence of phases in asymmetric nuclear matter under strong magnetic fields
dc.typeArticulo
dc.typePreprint


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