activity
20042022
most citedModels of Pulsar Glitches

323 citations · 1.3k across the 21 of their papers we have counts for

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astro-ph.HE202211 cited

Continuous gravitational wave emission from neutron stars with pinned superfluids in the core

Brynmor Haskell, Marco Antonelli, Pierre Pizzochero

We investigate the effect of a pinned superfluid component on the gravitational wave emission of a rotating neutron star. Pinning of superfluid vortices to the flux-tubes in the ou…

astro-ph.HE202013 cited

Superfluid dynamics in neutron star crusts: the Iordanskii force and chemical gauge covariance

Lorenzo Gavassino, Marco Antonelli, Brynmor Haskell

We present a geometrical derivation of the relativistic dynamics of the superfluid inner crust of a neutron star. The resulting model is analogous to the Hall-Vinen-Bekarevich-Khal…

astro-ph.HE202010 cited

Statistical estimates of the pulsar glitch activity

Alessandro Montoli, Marco Antonelli, Brynmor Haskell +1

A common way to calculate the glitch activity of a pulsar is an ordinary linear regression of the observed cumulative glitch history. This method however is likely to underestimate…

astro-ph.HE202028 cited

Axisymmetric models for neutron star merger remnants with realistic thermal and rotational profiles

Giovanni Camelio, Tim Dietrich, Stephan Rosswog +1

Merging neutron stars are expected to produce hot, metastable remnants in rapid differential rotation, which subsequently cool and evolve into rigidly rotating neutron stars or col…

astro-ph.HE2020

Gravitational waves from mountains in newly born millisecond magnetars

Ankan Sur, Brynmor Haskell

In this paper we study the spin-evolution and gravitational-wave luminosity of a newly born millisecond magnetar, formed either after the collapse of a massive star or after the me…

astro-ph.HE202013 cited

Proper motion, spectra, and timing of PSR J1813-1749 using Chandra and NICER

Wynn C. G. Ho, Sebastien Guillot, P. M. Saz Parkinson +7

PSR J1813-1749 is one of the most energetic rotation-powered pulsars known, producing a pulsar wind nebula (PWN) and gamma-ray and TeV emission, but whose spin period is only measu…