Spin-up of Solitary Pulsars: Signal of Deconfinement

Details Spin-up of Solitary Pulsars: Signal of Deconfinement Spin-up of Solitary Pulsars: Signal of Deconfinement

1998-03-06

arxiv.org/abs/astro-ph/9803070v1

Astronomy and Astrophysics

Astrophysics

7 pages, 4 figures, Latex (To be published in Proceedings of `Neutron Stars and Pulsars' November 1997, Tokyo by Universal Aca

Scientific paper

A phase transition in the nature of matter in the core of a neutron star,
such as quark deconfinement or Bose condensation, can cause the spontaneous
spin-up of a solitary millisecond pulsar. The spin-up epoch for our model lasts
for $2\times 10^7$ years or 1/50 of the spin-down time.

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