R-modes in neutron stars: Theory and observations
arXiv:1509.04370 · doi:10.1142/S0218301315410074
Abstract
In this article I will review the theory behind the gravitational wave driven r-mode instability in rapidly rotating neutron stars and discuss which constraints can be derived from observations of spins and temperatures in Low Mass X-ray Binaries. I will discuss how a standard, `minimal' neutron star model is not consistent with the data, and discuss some of the additional physical mechanisms that could reconcile theory with observations. In particular I will focus on additional forms of damping due to exotic cores and on strong mutual friction due to superfluid vortices cutting through superconducting flux tubes, and examine the repercussions these effects could have on the saturation amplitude of the mode. Finally I will also discuss the possibility that oscillations due to r-modes may have been recently observed in the X-ray light curves of two Low Mass X-ray Binaries.
17 pages
References in corpus (18)
- Color superconductivity in dense quark matter
- Maximum elastic deformations of compact stars with exotic equations of state
- Detecting gravitational wave emission from the known accreting neutron stars
- Spin Evolution of Accreting Neutron Stars: Nonlinear Development of the R-mode Instability
- Detecting gravitational waves from mountains on neutron stars in the Advanced Detector Era
- Are neutron stars with crystalline colour superconducting cores interesting for the LIGO experiment?
- Implications of an r-mode in XTE J1751-305: Mass, radius and spin evolution
- Ekman layer damping of r-modes revisited
- Discovery of a Neutron Star Oscillation Mode During a Superburst
- Viscosity of neutron star matter and -modes in rotating pulsars
- Excitation of a nonradial mode in a millisecond X-ray pulsar XTE J1751-305
- On the oscillations of dissipative superfluid neutron stars
- Oscillations of Rapidly Rotating Superfluid Stars
- New possible class of neutron stars: hot and fast non-accreting rotators
- Non-radial oscillations of the magnetized rotating stars with purely toroidal magnetic fields
- Gravitational waves from rapidly rotating neutron stars
- Differential rotation and r-modes in magnetized neutron stars
- Probing dense matter in compact star cores with radio pulsar data
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- Measuring the neutron star equation of state using X-ray timing
- The Spin Distribution of Fast Spinning Neutron Stars in Low Mass X-Ray Binaries: Evidence for Two Sub-Populations
- Continuous gravitational waves from neutron stars: current status and prospects
- Search for gravitational waves from Scorpius X-1 in the first Advanced LIGO observing run with a hidden Markov model
- The Science of the Einstein Telescope
- Reaction rates and transport in neutron stars
- Superradiance in rotating stars and pulsar-timing constraints on dark photons
- Deep learning for clustering of continuous gravitational wave candidates
- Search for Continuous Gravitational Waves from Scorpius X-1 in LIGO O2 Data
- Are gravitational waves spinning down PSR J1023+0038?
- Chandra studies of the globular cluster 47 Tucanae: A deeper X-ray source catalogue, five new X-ray counterparts to millisecond radio pulsars, and new constraints to r-mode instability window
- Transport in strongly coupled quark matter
- Bulk viscosity in neutron stars with hyperon cores
- A universal formula for the relativistic correction to the mutual friction coupling time-scale in neutron stars
- Gravitational waves from mountains in newly born millisecond magnetars
- Ultra-compact X-ray binaries as dual-line gravitational-wave sources
- R-modes and neutron star recycling scenario
- Deep learning for clustering of continuous gravitational wave candidates II: identification of low-SNR candidates
- -mode Stability of GW190814's Secondary Component as a Supermassive and Superfast Pulsar
- Dissipative relativistic magnetohydrodynamics of a multicomponent mixture and its application to neutron stars
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- Results from an Einstein@Home search for continuous gravitational waves from G347.3 at low frequencies in LIGO O2 data
- Temperature-dependent r-modes in superfluid neutron stars stratified by muons
- Strengthening the bounds on the r-mode amplitude with X-ray observations of millisecond pulsars
- Observational signatures of neutron stars in low-mass X-ray binaries climbing a stability peak
- Role of nucleon-nucleon correlation in transport coefficients and gravitational-wave-driven -mode instability of neutron stars
- Optimizing the third generation of gravitational-wave observatories for Galactic astrophysics
- Multi-messenger Emission from Tidal Waves in Neutron Star Oceans
- Diffusion as a leading dissipative mechanism in superconducting neutron stars
- Eclipses of continuous gravitational waves as a probe of stellar structure
- Transport coefficients in neutron star cores in BHF approach. Comparison of different nucleon potentials
- Influence of the nuclear matter equation of state on the r-mode instability using the finite-range simple effective interaction
- Limits on Magnetic Field Amplification from the r-Mode Instability
- Resonance suppression of the r-mode instability in superfluid neutron stars: Accounting for muons and entrainment
- Instability windows of relativistic r-modes
- Astroseismology of neutron stars from gravitational waves in the limit of perfect measurement
- Stability of the neutron-proton-electron matter under strong magnetic fields: the covariant Vlasov approach
- Effect of Magnetic Fields on Urca Rates in Neutron Star Mergers
- Evolution of newborn rapidly rotating magnetars: effects of r-mode and fall-back accretion
- Search for continuous gravitational waves from HESS~J1427-608 with a hidden Markov model
- r-mode instability of neutron stars in low-mass X-ray binaries: effects of Fermi surface depletion and superfluidity of dense matter
- Radiation driven instability of rapidly rotating relativistic stars: criterion and evolution equations via multipolar expansion of gravitational waves
- Non-analytic behavior of the relativistic r-modes in slowly rotating neutron stars
- Long term evolution of CFS-unstable neutron stars and role of differential rotation on short time-scales
- Constraining the -mode oscillations frequency in Neutron Stars through Universal Relations in the realm of Energy-Momentum Squared Gravity
- Observability of HOFNARs with SRG/eROSITA
- Simulating bulk viscosity in neutron stars. I. Formalism
- Radial Oscillations of Viscous Neutron Stars: Zero Diffusion Case
- Of Mountains and Molehills : Gravitational Waves from Neutron Stars
- Results from an Einstein@Home search for continuous gravitational waves from Cassiopeia A and Vela Jr. using LIGO O2 data
- R-mode instability in compact stars
- Magnetic field amplification by the r-mode instability
- Observability of sharp phase transitions in neutron stars
- Instability windows of relativistic r-modes in stably stratified neutron stars with hyperonic cores
- Constraints from LIGO O3 data on gravitational-wave emission due to r-modes in the glitching pulsar PSR J0537-6910
- Multicomponent Superfluids and Superconductors in Dense Nuclear and Quark Matter
- Dissipative superfluid relativistic magnetohydrodynamics of a multicomponent fluid: the combined effect of particle diffusion and vortices
- Non-perturbative Aspects of Quantum Field Theories from Holography