How to identify a Strange Star

Details How to identify a Strange Star How to identify a Strange Star

1998-06-02

arxiv.org/abs/astro-ph/9806032v1

Phys.Rev.Lett. 81 (1998) 3311-3314

Astronomy and Astrophysics

Astrophysics

4 pages, 1 figure

Scientific paper

10.1103/PhysRevLett.81.3311

Contrary to young neutron stars, young strange stars are not subject to the
r-mode instability which slows rapidly rotating, hot neutron stars to rotation
periods near 10 ms via gravitational wave emission. Young millisecond pulsars
are therefore likely to be strange stars rather than neutron stars, or at least
to contain significant quantities of quark matter in the interior.

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