Vortex pinning and dynamics in the neutron star crust
arXiv:1606.04847 · doi:10.1103/PhysRevLett.117.232701
Abstract
The nature of the interaction between superfluid vortices and the neutron star crust, conjectured by Anderson and Itoh in 1975 to be at the heart vortex creep and the cause of glitches, has been a long-standing question in astrophysics. Using a qualitatively new approach, we follow the dynamics as superfluid vortices move in response to the presence of "nuclei" (nuclear defects in the crust). The resulting motion is perpendicular to the force, similar to the motion of a spinning top when pushed. We show that nuclei repel vortices in the neutron star crust, and characterize the force as a function of the vortex-nucleus separation.
supplemental materials included
References in corpus (11)
- Models of Pulsar Glitches
- Local Density Functional Theory for Superfluid Fermionic Systems: The Unitary Gas
- Screening Effects in Superfluid Nuclear and Neutron Matter within Brueckner Theory
- A Unitary Fermi Supersolid: The Larkin-Ovchinnikov Phase
- Linear Algebraic Calculation of Green's function for Large-Scale Electronic Structure Theory
- Large Amplitude Dynamics of the Pairing Correlations in a Unitary Fermi Gas
- Quantum calculation of vortices in the inner crust of neutron stars
- Vortex-nucleus interaction in the inner crust of neutron stars
- Dynamics of Quantum Vorticity in a Random Potential
- Life Cycle of Superfluid Vortices and Quantum Turbulence in the Unitary Fermi Gas
- Relativistic Coulomb excitation within Time Dependent Superfluid Local Density Approximation
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- Heavy-ions collisions and fission dynamics with the time-dependent Hartree-Fock theory and its extensions
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- TDHF Theory and Its Extensions for the Multinucleon Transfer Reaction: a Mini Review
- Superfluidity and Superconductivity in Neutron Stars
- Novel Role of Superfluidity in Low-Energy Nuclear Reactions
- Glitch rises as a test for rapid superfluid coupling in neutron stars
- Constraints on pulsar masses from the maximum observed glitch
- Time-Dependent Density Functional Theory for Fermionic Superfluids: from Cold Atomic Gases, to Nuclei and Neutron Stars Crust
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- Avalanches and Criticality in Driven Magnetic Skyrmions
- Superfluid vortex-mediated mutual friction in non-homogeneous neutron star interiors
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- Towards Quantum Turbulence in Cold Atomic Fermionic Superfluids
- Insights into the physics of neutron star interiors from pulsar glitches
- Time-dependent extension of the self-consistent band theory for neutron star matter: Anti-entrainment effects in the slab phase
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- Shear Banding, Intermittency, Jamming and Dynamic Phases for Skyrmions in Inhomogeneous Pinning Arrays
- Nuclear Quantum Many-Body Dynamics: From Collective Vibrations to Heavy-Ion Collisions (2nd edition)
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- The proto-neutron star inner crust in the liquid phase
- Effects of pairing gap and band gap on superfluid density in the inner crust of neutron stars
- Entrainment effects in neutron-proton mixtures within the nuclear-energy density functional theory. II. Finite temperatures and arbitrary currents
- Superfluid extension of the self-consistent time-dependent band theory for neutron star matter: Anti-entrainment versus superfluid effects in the slab phase
- Gapless neutron superfluidity can explain the late time cooling of transiently accreting neutron stars
- Equation of state of superfluid neutron matter with low-momentum interactions
- Modelling of vorticity, sound and their interaction in two-dimensional superfluids
- Quantum vortices in fermionic superfluids: from ultracold atoms to neutron stars
- Microscopic calculation of the pinning energy of a vortex in the inner crust of a neutron star
- Measuring the vortex-nucleus pinning force from pulsar glitch rates
- Solitonic excitations in collisions of superfluid nuclei: a qualitatively new phenomenon distinct from the Josephson effect
- Time-dependent nuclear energy-density functional theory toolkit for neutron star crust: Dynamics of a nucleus in a neutron superfluid
- Probing neutron star interiors with pulsar glitches
- Sensitivity to the initial conditions of the Time-Dependent Density Functional Theory
- Persistent gravitational radiation from glitching pulsars. II. Updated scaling with vortex number
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- Gapless neutron superfluidity in the crust of the accreting neutron stars KS 1731-260 and MXB 1659-29
- Comparative study of the requantization of the time-dependent mean field for the dynamics of nuclear pairing
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- Dynamic Phases and Reentrant Hall Effect for Vortices and Skyrmions on Periodic Pinning Arrays
- On the pulsar spin frequency derivatives and the glitch activity
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- Multicomponent Superfluids and Superconductors in Dense Nuclear and Quark Matter
- The LISE package: solvers for static and time-dependent superfluid local density approximation equations in three dimensions
- Microscopic Calculations of Vortex-Nucleus Interaction in the Neutron Star Crust
- Phase transitions in the inner crust of neutron stars within the superfluid band theory: Competition between pairing and spin polarization under finite temperature and magnetic field