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astro-ph2000
Evolution from Canonical to Millisecond Pulsar through the X-ray Accretion Stage
Norman K. Glendenning, Fridolin Weber
We model the evolution of canonical pulsars from the death line to millisecond pulsars through the X-ray neutron star stage of accretion from a low-mass companion. We trace this ev…
astro-ph2000★ 40 cited
Strangeness in Neutron Stars
Fridolin Weber
It is generally agreed on that the tremendous densities reached in the centers of neutron stars provide a high-pressure environment in which numerous novel particles processes are…