Rotational properties of strange pulsar models.

Details Rotational properties of strange pulsar models. Rotational properties of strange pulsar models.

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phrvd..44..555b&link_type=abstract

Physical Review D, Vol. 44, No. 2, p. 555 - 556

Physics

Scientific paper

The authors 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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