Bulletin of the Astronomical Society of India
Sushan Konar1 and Mihir Arjunwadkar2*
1NCRA-TIFR, University of Pune Campus, Pune, India
2Centre for Modeling and Simulation, University of Pune, Pune, India
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We present statistical evidence suggesting more than one population in the energy distributon of pulsar glitches, which implies the presence of dierent mechanisms accessing dierent energy ranges responsible for glitches.