Nonlinear interglitch dynamics, the braking index of the Vela pulsar and the time to the next glitch
Onur Akbal, M. Ali Alpar, Sarah Buchner, David Pines

TL;DR
This paper models the inter-glitch timing of the Vela pulsar using a nonlinear vortex creep model, predicts the next glitch date, and discusses the impact of persistent shifts on glitch timing and braking index estimation.
Contribution
It introduces a modified inter-glitch timing model incorporating persistent shifts, improving predictions of glitch intervals and estimating the braking index for the Vela pulsar.
Findings
The braking index of Vela is estimated at 2.81 +/- 0.12.
The predicted next glitch date is around Dec. 22, 2017, with variations depending on persistent shifts.
The model's prediction was confirmed by an observed glitch 138 days after the forecast.
Abstract
The inter-glitch timing of the Vela pulsar is characterized by a constant second derivative of the rotation rate. This takes over after the post-glitch exponential relaxation, and is completed at about the time of the next glitch. The vortex creep model explains the second derivatives in terms of non-linear response to the glitch. We present inter-glitch timing fits to the present sample covering 16 large glitches, taking into account the possibility that in some glitches part of the step in spin-down rate may involve a "persistent shift", as observed in the Crab pulsar. Modifying the expression for the time between glitches with this hypothesis leads to better agreement with the observed inter-glitch time intervals. We extrapolate the inter-glitch model fits to obtain spin-down rates just prior to each glitch, and use these to calculate the braking index n = 2.81 +/- 0.12. The next…
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