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2013, Volume 1
Statistical Study of Glitch Behaviours of Glitching Pulsars
Information
) in simple power laws. Similarly, variation of glitch activity with the characteristic age (τ) traces a curve that peaks at τ = 104 yr and decays with age for older pulsars with τ ≥ 104yr. The angular momentum transfer resulting to glitches appears to be maximum at youthful age (≈ 104-106yr) of pulsars when certain rotational properties as well as temperature of the star best supports vortex pinning and unpinning of the superfluid of the star interior.