Vortex structure of neutron stars with triplet neutron superfluidity
作者： K. M. Shahabasyan , M. K. Shahabasyan
DOI: 10.1007/S10511-011-9193-6
关键词: Cooper pair 、 Proton 、 Astrophysics 、 Neutron 、 r-process 、 Neutron star 、 Superfluidity 、 Physics 、 Vortex 、 Superconductivity
摘要: The vortex structure of the “npe” phase neutron stars with a 3P2 superfluid condensate Cooper pairs is discussed. It shown that, as star rotates, filaments described by unitary ordering parameter develop in phase. entrainment superconducting protons rotating neutrons examined. effect leads to appearance clusters proton vortices around each and generates magnetic field on order 1012 G. combine quark semi-superfluid at boundary “CFL” phases. At “Aen” phases, they 1S0 filaments. In this way, unified formed. existence its collective elastic oscillations explain observed angular rotation velocity pulsars.
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