Possible Signatures of Quark-Hadron Phase Transitions inside Neutron Stars

Details Possible Signatures of Quark-Hadron Phase Transitions inside Neutron Stars Possible Signatures of Quark-Hadron Phase Transitions inside Neutron Stars

2001-06-09

arxiv.org/abs/astro-ph/0106169v1

Astronomy and Astrophysics

Astrophysics

7 pages, in "From Particles to the Universe", Proceedings of the Fifteenth Lake Louise Winter Institute Lake Louise, Alberta,

Scientific paper

The spin-down power of an isolated neutron star can drive its central density
increase and overall structural changes, and trigger a quark-hadron phase
transition. A series of observational signatures may be seen as a result of the
phase transition, including pulsar spin-down and glitch behaviors, Soft Gamma
Repeaters or Gamma-Ray Bursts.

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