Mathematical Model for Glitches in Pulsars

Details Mathematical Model for Glitches in Pulsars Mathematical Model for Glitches in Pulsars

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010wscm.conf..297m&link_type=abstract

WAVES AND STABILITY IN CONTINUOUS MEDIA . Proceedings of the 15th Conference on WASCOM 2009 . Held 28 June-1 July 2009 in Palerm

Mathematics

Neutron Star, Superfluidity

Scientific paper

The aim of this work is to propose a simple mathematical model which is
able to capture the peculiar behaviour of the rotating neutron star:
glitches. This is made by using the knowledge on helium superfluid and
particularly on rotating superfluid helium, which has interested many
researchers over the years.

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