50 citations · 197 across the 11 of their papers we have counts for
12 papers
Interior Magnetic Fields in Magnetars and Radio Pulsars
Raj Kishor Joshi, Brynmor Haskell, William Cook +1
Magnetic fields are fundamental for neutron star physics and play a central role in powering the extreme phenomenology of magnetars, including Soft Gamma Repeaters and Anomalous X-…
Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO
Avishek Basu, Vanessa Graber, Marcus E. Lower +19
Matter inside neutron stars is compressed to densities several times greater than nuclear saturation density, while maintaining low temperatures and large asymmetries between neutr…
Superfluid He aerogel experiments as a laboratory neutron star analogue
Samuli Autti, Vanessa Graber, Brynmor Haskell
Neutron stars make a unique astrophysical test bench for our understanding of quantum physics at kilometre scales. The rotation of a neutron star features glitches, sudden spin-ups…
Magnetic field dynamics in isolated neutron stars with an external dipole field
Aurora Capobianco, William Cook, Sebastiano Bernuzzi +2
Neutron stars can harbor extremely strong magnetic fields, yet the structure and stability of their magnetic field configuration remain poorly understood. Observations of pulsars i…
Probing neutron star interiors and the properties of cold ultra-dense matter with the SKAO
Avishek Basu, Vanessa Graber, Marcus E. Lower +19
Matter inside neutron stars is compressed to densities several times greater than nuclear saturation density, while maintaining low temperatures and large asymmetries between neutr…
Gravitational pulsars: correlations between the electromagnetic and the continuous gravitational wave signal
Marco Antonelli, Avishek Basu, Brynmor Haskell
Neutron stars emitting continuous gravitational waves may be regarded as gravitational pulsars, in the sense that it could be possible to track the evolution of their rotational pe…
Glitching pulsars as gravitational wave sources
Brynmor Haskell, David Ian Jones
Spinning neutron stars, when observed as pulsars, are seen to undergo occasional spin-up events known as glitches. Despite several decades of study, the physical mechanisms respons…
Symmetric-hyperbolic quasi-hydrodynamics
Lorenzo Gavassino, Marco Antonelli, Brynmor Haskell
We set up a general framework for systematically building and classifying, in the linear regime, causal and stable dissipative hydrodynamic theories that, alongside with the usual…
The dynamics of dissipative multi-fluid neutron star cores
B. Haskell, N. Andersson, G. L. Comer
We present a Newtonian multi-fluid formalism for superfluid neutron star cores, focussing on the additional dissipative terms that arise when one takes into account the individual…
Spin equilibrium with or without gravitational wave emission: the case of XTE J1814-338 and SAX J1808.4-3658
Brynmor Haskell, Alessandro Patruno
In this letter we present a new analysis of the torques acting on the accreting millisecond X-ray pulsars SAX J1808.4-365 and XTE J1814-338, and show how our results can be used to…
Lagrangian perturbation theory for a superfluid immersed in an elastic neutron star crust
N. Andersson, B. Haskell, L. Samuelsson
The inner crust of mature neutron stars, where an elastic lattice of neutron-rich nuclei coexists with a neutron superfluid, impacts on a range of astrophysical phenomena. The pres…
Implications of burst oscillations from the slowly rotating accreting pulsar IGR 17480-2446 in the globular cluster Terzan 5
Y. Cavecchi, A. Patruno, B. Haskell +6
The recently-discovered accreting X-ray pulsar IGR J17480--2446 spins at a frequency of ~11 Hz. We show that Type I X-ray bursts from this source display oscillations at the same f…