Search Results - "Haskell, B"

The Spin Distribution of Fast-spinning Neutron Stars in Low-mass X-Ray Binaries: Evidence for Two Subpopulations by Patruno, A., Haskell, B., Andersson, N.

“…We study the current sample of rapidly rotating neutron stars in both accreting and non-accreting binaries in order to determine whether the spin distribution…”
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Superfluid vortex-mediated mutual friction in non-homogeneous neutron star interiors by Antonelli, M, Haskell, B

“…ABSTRACT Understanding the average motion of a multitude of superfluid vortices in the interior of a neutron star is a key ingredient for most theories of…”
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Are Gravitational Waves Spinning Down PSR J1023+0038? by Haskell, B, Patruno, A

“…The pulsar J1023+0038 rotates with a frequency ν≈592  Hz and has been observed to transition between a radio state, during which it is visible as a millisecond…”
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Thermodynamic Stability Implies Causality by Gavassino, L, Antonelli, M, Haskell, B

“…The stability conditions of a relativistic hydrodynamic theory can be derived directly from the requirement that the entropy should be maximized in…”
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Asymmetric accretion and thermal ‘mountains’ in magnetized neutron star crusts by Singh, N, Haskell, B, Mukherjee, D, Bulik, T

“…ABSTRACT Accreting neutron stars (NSs) are one of the main targets for continuous gravitational wave searches, as asymmetric accretion may lead to quadrupolar…”
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Turbulent, pinned superfluids in neutron stars and pulsar glitch recoveries by Haskell, B, Antonopoulou, D, Barenghi, C

“…ABSTRACT Pulsar glitches offer an insight into the dynamics of superfluids in the high-density interior of a neutron star. To model these phenomena, however,…”
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On the universality of I-Love-Q relations in magnetized neutron stars by Haskell, B., Ciolfi, R., Pannarale, F., Rezzolla, L.

“…Recently, general relations among the quadrupole moment (Q), the moment of inertia (I) and the tidal deformability (Love number) of a neutron star were shown…”
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Crust or core? Insights from the slow rise of large glitches in the Crab pulsar by Haskell, B, Khomenko, V, Antonelli, M, Antonopoulou, D

“…ABSTRACT Pulsar glitches are attributed to the sudden recoupling of weakly coupled superfluid components in the neutron star interior. The transfer of angular…”
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Stochastic Approximation for Risk-Aware Markov Decision Processes by Huang, Wenjie, Haskell, William B.

“…We develop a stochastic approximation-type algorithm to solve finite state/action, infinite-horizon, risk-aware Markov decision processes. Our algorithm has…”
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A universal formula for the relativistic correction to the mutual friction coupling time-scale in neutron stars by Gavassino, L, Antonelli, M, Pizzochero, P M, Haskell, B

“…ABSTRACT Vortex-mediated mutual friction governs the coupling between the superfluid and normal components in neutron star interiors. By, for example,…”
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Detecting gravitational waves from mountains on neutron stars in the advanced detector era by Haskell, B., Priymak, M., Patruno, A., Oppenoorth, M., Melatos, A., Lasky, P. D.

“…Rapidly rotating neutron stars (NSs) in low-mass X-ray binaries (LMXBs) are thought to be interesting sources of gravitational waves (GWs) for current and next…”
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Magnetic fields in late-stage proto-neutron stars by Lander, S K, Haensel, P, Haskell, B, Zdunik, J L, Fortin, M

“…ABSTRACT We explore the thermal and magnetic field structure of a late-stage proto-neutron star (proto-NS). We find the dominant contribution to the entropy in…”
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Pinned vortex hopping in a neutron star crust by Haskell, B., Melatos, A.

“…The motion of superfluid vortices in a neutron star crust is at the heart of most theories of pulsar glitches. Pinning of vortices to ions can decouple the…”
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Simulating pulsar glitches: an N-body solver for superfluid vortex motion in two dimensions by Howitt, G, Melatos, A, Haskell, B

“…ABSTRACT A rotating superfluid forms an array of quantized vortex lines that determine its angular velocity. The spasmodic evolution of the array under the…”
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Mesoscopic pinning forces in neutron star crusts by Seveso, S, Pizzochero, P M, Grill, F, Haskell, B

“…The crust of a neutron star is thought to be comprised of a lattice of nuclei immersed in a sea of free electrons and neutrons. As the neutrons are superfluid,…”
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The Enigmatic Spin Evolution of PSR J0537-6910: r-modes, Gravitational Waves, and the Case for Continued Timing by Andersson, N., Antonopoulou, D., Espinoza, C. M., Haskell, B., Ho, W. C. G.

“…We discuss the unique spin evolution of the young X-ray pulsar PSR J0537-6910, a system in which the regular spin down is interrupted by glitches every few…”
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Observational constraints on neutron star crust–core coupling during glitches by Newton, W. G., Berger, S., Haskell, B.

“…We demonstrate that observations of glitches in the Vela pulsar can be used to investigate the strength of the crust–core coupling in a neutron star and…”
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Modelling magnetically deformed neutron stars by Haskell, B., Samuelsson, L., Glampedakis, K., Andersson, N.

“…Rotating deformed neutron stars are important potential sources for ground-based gravitational wave interferometers such as LIGO, GEO600 and VIRGO. One…”
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The effect of non-linear mutual friction on pulsar glitch sizes and rise times by Celora, T, Khomenko, V, Antonelli, M, Haskell, B

“…ABSTRACT Observations of pulsar glitches have the potential to provide constraints on the dynamics of the high density interior of neutron stars. However, to…”
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A new mechanism for saturating unstable r modes in neutron stars by Haskell, B., Glampedakis, K., Andersson, N.

“…We consider a new mechanism for damping the oscillations of a mature neutron star. The new dissipation channel arises if superfluid vortices are forced to cut…”
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