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- W2951424910 abstract "Abstract The glitch size, Δ ν / ν , inter-glitch time interval, t i , and frequency of glitches in pulsars are key parameters in discussing glitch phenomena. In this paper, the glitch sizes and inter-glitch time intervals are statistically analyzed in a sample of 168 pulsars with a total of 483 glitches. The glitches are broadly divided into two groups. Those with Δ ν / ν < 10 −7 are regarded as small size glitches, while those with Δ ν / ν ≥ 10 −7 are considered as relatively large size glitches. In the ensemble of glitches, the distribution of Δ ν / ν is seen to be bimodal as usual. The distribution of inter-glitch time intervals is unimodal and the inter-glitch time intervals between small and large size glitches are not significantly different from each other. This observation shows that inter-glitch time intervals are size independent. In addition, the distribution of the ratio Δ ν / ν : t i in both small and large size glitches has the same pattern. This observation suggests that a parameter which depends on time, which could be the spin-down rate of a pulsar, plays a similar role in the processes that regulate both small and large size glitches. Equally, this could be an indication that a single physical mechanism, which could produce varying glitch sizes at similar time-intervals, could be responsible for both classes of glitch sizes." @default.
- W2951424910 created "2019-06-27" @default.
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- W2951424910 date "2019-06-01" @default.
- W2951424910 modified "2023-09-26" @default.
- W2951424910 title "On the distributions of pulsar glitch sizes and the inter-glitch time intervals" @default.
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- W2951424910 doi "https://doi.org/10.1088/1674-4527/19/6/89" @default.
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