323 citations · 3.6k across the 75 of their papers we have counts for
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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…
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…
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…
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…
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…
Return of the Big Glitcher: NICER timing and glitches of PSR J0537-6910
Wynn C. G. Ho, Cristobal M. Espinoza, Zaven Arzoumanian +7
PSR J0537-6910, also known as the Big Glitcher, is the most prolific glitching pulsar known, and its spin-induced pulsations are only detectable in X-ray. We present results from a…