Particles Production in Neutron Stars by Means of the Parametric Resonance Mechanism

Simple item page
dc.creatorCampos, S. D.
dc.date2008-11-05
dc.date.accessioned2026-07-07T10:15:44Z
dc.date.available2026-07-07T10:15:44Z
dc.descriptionUsing a Lagrangean toy model the coupling of a negative pion superconducting field and the electromagnetic field of the star is analyzed. A numerical study of particles produced in the neutron star medium by means of the well-known parametric resonance phenomenon is performed.
dc.description7 pages,5 figures, revtex format
dc.identifierhttps://arxiv.org/abs/0811.0767
dc.identifierhttp://arxiv.org/abs/0811.0767
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/173269
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleParticles Production in Neutron Stars by Means of the Parametric Resonance Mechanism
dc.typetext

Files

Collections

arXiv