Multi-resonance orbital model of high-frequency quasi-periodic oscillations: possible high-precision determination of black hole and neutron star spin

2013/02/01 by Zdenek Stuchlik, Z. Stuchlík, Andrea Kotrlova +3 · 1 citation
Physics and Astronomy · #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Black hole (networking) #Dimensionless quantity #Neutron star #Pulsars and Gravitational Waves Research #Resonance (particle physics) #Rotating black hole #Spin (aerodynamics) #Spin-flip #Stellar black hole #astro-ph.HE

paper · pdf · doi:10.1051/0004-6361/201219724

published as Astronomy and Astrophysics, Volume 552, id.A10, 2013 · 43 pages, 10 figures

openalex publication_date 2013/02/01 · arxiv created 2013/05/15 · arxiv updated 2013/05/16 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. Using known frequencies of the twin-peak high-frequency quasiperiodic oscillations (HF QPOs) and known mass of the central black hole, the black-hole dimensionless spin a can be determined by assuming a concrete version of the resonance model. However, a wide range of observationally limited values of the black hole mass implies low precision of the spin estimates.

Citations

• Modelling the behaviour of accretion flows in X-ray binaries
• The distribution of kHz QPO frequencies in bright low mass X-ray binaries
• Evidence for a 2:3 resonance in Sco X-1 kHz QPOs
• Measuring mass and angular momentum of black holes with high-frequency quasi-periodic oscillations
• Epicyclic Oscillations of Fluid Bodies: Newtonian Nonslender Torus
• Periapsis and gravitomagnetic precessions of stellar orbits in Kerr and Kerr–de Sitter black hole spacetimes
• Gravitational lensing by naked singularities
• Oscillations of vertically integrated relativistic tori - I. Axisymmetric modes in a Schwarzschild space-time
• The Importance of Discovering a 3�2 Twin-Peak Quasi-periodic Oscillation in an Ultraluminous X-Ray Source, or How to Solve the Puzzle of Intermediate-Mass Black Holes
• Oscillations of tori in the pseudo-Newtonian potential
• The MHD Alfven wave oscillation model of kHz Quasi Periodic Oscillations of Accreting X-ray binaries
• The high-frequency QPOs in GRS 1915+105
• Orbital resonances in discs around braneworld Kerr black holes
• Angular Momentum Transport in Accretion Disks and Its Implications for Spin Estimates in Black Hole Binaries
• Measuring neutron star mass and radius with three mass-radius relations
• Searching for the trigger of the active galactic nucleus quasi-periodic oscillation: 8 years of RE J1034+396
• Relativistic images in Randall-Sundrum II braneworld lensing
• The correlations between the twin kHz quasi-periodic oscillation frequencies of low-mass X-ray binaries
• X-ray flares reveal mass and angular momentum of the Galactic Center black hole
• On the kHz QPO frequency correlations in bright neutron star X-ray binaries
• On the distribution of frequency ratios of kHz quasi-periodic oscillations
• Confronting the models of 3:2 quasiperiodic oscillations with the rapid spin of the microquasar GRS 1915+105
• X-Ray Properties of Black-Hole Binaries

Cited by

• Multi-resonance orbital model applied to high-frequency quasi-periodic oscillations observed in Sgr A*