Scaling law for pulsar glitches.

Details Scaling law for pulsar glitches. Scaling law for pulsar glitches.

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993el.....23..185m&link_type=abstract

Europhys. Lett., Vol. 23, No. 3, p. 185 - 189

Mathematics

Probability

9

Scientific paper

If one assumes that the change of frequency in pulsar macro-glitches is due to the change in the moment of inertia of the rotating neutron star, then, using the available data, the authors extract a scaling law for the probability P(E) of a glitch of energy E: P(E) ≅ E-α with α ≍ 1.14. They make some comments on the physics of the observation.

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