31 citations · 95 across the 4 of their papers we have counts for
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The effect of non-linear mutual friction on pulsar glitch sizes and rise times
Thomas Celora, Vadym Khomenko, Marco Antonelli +1
Observations of pulsar glitches have the potential to provide constraints on the dynamics of the high density interior of neutron stars. However, to do so, realistic glitch models…
Hydrodynamical instabilities in superfluid neutron stars with background flows between the components
Vadym Khomenko, Marco Antonelli, Brynmor Haskell
The interiors of mature neutron stars are expected to be superfluid. Superfluidity of matter on the microscopic scale can have a number of large scale, potentially observable conse…
Core and crust contributions in pulsar glitches: constraints from the slow rise of the largest glitch observed in the Crab pulsar
Brynmor Haskell, Vadym Khomenko, Marco Antonelli +1
Pulsar glitches are attributed to the sudden re-coupling of very weakly coupled large scale superfluid components in the neutron star interior. This process leads to rapid exchange…
Modelling pulsar glitches: the hydrodynamics of superfluid vortex avalanches in neutron stars
Vadym Khomenko, Brynmor Haskell
The dynamics of quantised vorticity in neutron star interiors is at the heart of most pulsar glitch models. However, the large number of vortices (up to ) involved…