Particles Production in Neutron Stars by Means of the Parametric Resonance Mechanism
arXiv:0811.0767
Abstract
Using 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.
7 pages,5 figures, revtex format