High frequency QPOs: nonlinear oscillations in strong gravity
arXiv:astro-ph/0510725 · doi:10.1002/asna.200510420
Abstract
Some of the more promising ideas about the origin of the high frequency variability (kHz QPOs) in the observed X-ray emissions of low-mass X-ray binaries are contrasted with less promising ones.
References in corpus (10)
- A precise determination of angular momentum in the black hole candidate GRO J1655-40
- Evidence for Harmonic Relationships in the High Frequency QPOs of XTE J1550-564 and GRO J1655-40
- Non-linear resonance in nearly geodesic motion in low-mass X-ray binaries
- Relativistic Diskoseismology
- Evidence for a 2:3 resonance in Sco X-1 kHz QPOs
- Non-linear resonance in the accretion disk of a millisecond pulsar
- Resonance in Forced Oscillations of an Accretion Disk and Kilohertz Quasi Periodic Oscillations
- Twin peaks kHz QPOs: mathematics of the 3:2 orbital resonance
- On the high coherence of kilo-Hz Quasi-Periodic Oscillations
- General-relativistic constraints on the equation of state of dense matter implied by kilohertz quasi-periodic oscillations in neutron-star X-ray binaries
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- Constraining Black Holes with Light Boson Hair and Boson Stars using Epicyclic Frequencies and QPOs
- Frequency Correlations of QPOs Based on a Disk Oscillation Model in Warped Disks
- Quasi-periodic oscillations from relativistic hydrodynamical slender tori
- Epicyclic frequencies for rotating strange quark stars: the importance of stellar oblateness
- Relativistic, Viscous, Radiation Hydrodynamic Simulations of Geometrically Thin Disks. II. Disk Variability
- Breathing Oscillations in a Global Simulation of a Thin Accretion Disk
- Oscillations of radiation pressure supported tori near black holes
- Correlations between the frequencies of twin kHz QPOs and spins of neutron stars in LMXBs
- Radial modes of levitating atmospheres around Eddington-luminosity neutron stars
- Quasi-periodic oscillations of perturbed tori
- Persistent Patterns in Accretion Disks
- Unusual behavior of epicyclic frequencies around rapidly rotating compact stars