Rotational properties of strange-pulsar models

Details Rotational properties of strange-pulsar models Rotational properties of strange-pulsar models

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phrvd..44.1321b&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 44, Issue 4, 15 August 1991, pp.1321-1322

Physics

2

Scientific paper

We present a study of the rotational properties of strange pulsars:
strange-matter stars capable of supporting glitches. It is shown that
their differentiated internal structure implies a lower maximum
rotational frequency than that of homogeneous strange stars.
Nevertheless, they are able to fit the known pulsar properties.

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