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Recent work, however, suggests that a starquake would not release sufficient energy for a neutron star glitch; it has been suggested that glitches may instead be caused by transitions of vortices in the theoretical superfluid core of the neutron star from one metastable energy state to a lower one, thereby releasing energy that appears as an increase in the rotation rate.<ref>{{cite web |url=http://physicsworld.com/cws/article/print/1756 |date=1 January 1998 |title=Pulsars, glitches and superfluids |publisher=Physicsworld.com |first=M. Ali |last=Alpar |access-date=12 January 2009 |archive-date=6 December 2008 |archive-url=https://web.archive.org/web/20081206090618/http://physicsworld.com/cws/article/print/1756 |url-status=live }}</ref>
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==Population and distances==
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