Gravitational Magnus effect
arXiv:1805.01097 · doi:10.1103/PhysRevD.98.024026
Abstract
It is well known that a spinning body moving in a fluid suffers a force orthogonal to its velocity and rotation axis --- it is called the Magnus effect. Recent simulations of spinning black holes and (indirect) theoretical predictions, suggest that a somewhat analogous effect may occur for purely gravitational phenomena. The magnitude and precise direction of this "gravitational Magnus effect" is still the subject of debate. Starting from the rigorous equations of motion for spinning bodies in General Relativity (Mathisson-Papapetrou equations), we show that indeed such an effect takes place and is a fundamental part of the spin-curvature force. The effect arises whenever there is a current of mass/energy, non-parallel to a body's spin. We compute the effect explicitly for some astrophysical systems of interest: a galactic dark matter halo, a black hole accretion disk, and the Friedmann-Lemaître-Robertson-Walker (FLRW) spacetime. It is seen to lead to secular orbital precessions potentially observable by future astrometric experiments and gravitational-wave detectors. Finally, we consider also the reciprocal problem: the "force" exerted by the body on the surrounding matter, and show that (from this perspective) the effect is due to the body's gravitomagnetic field. We compute it rigorously, showing the matching with its reciprocal, and clarifying common misconceptions in the literature regarding the action-reaction law in post-Newtonian gravity.
arXiv comment28 pages, 9 figures. References added, matches the final published version
References in corpus (49)
- Quintessence, Cosmic Coincidence, and the Cosmological Constant
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
- The Structure of Dark Matter Haloes in Dwarf Galaxies
- Gravitational-wave sensitivity curves
- The international pulsar timing array project: using pulsars as a gravitational wave detector
- Can dark energy evolve to the Phantom?
- Can environmental effects spoil precision gravitational-wave astrophysics?
- The Stellar Cusp Around the Supermassive Black Hole in the Galactic Center
- The Local Dark Matter Density
- Towards models of gravitational waveforms from generic binaries II: Modelling precession effects with a single effective precession parameter
- Estimating spinning binary parameters and testing alternative theories of gravity with LISA
- The NANOGrav Nine-year Data Set: Limits on the Isotropic Stochastic Gravitational Wave Background
- Higher-order spin effects in the dynamics of compact binaries I. Equations of motion
- Third-Epoch Magellanic Cloud Proper Motions II: The Large Magellanic Cloud Rotation Field in Three Dimensions
- Gravito-electromagnetism
- Validating the effective-one-body model of spinning, precessing binary black holes against numerical relativity
- LISA observations of rapidly spinning massive black hole binary systems
- Measuring coalescing massive binary black holes with gravitational waves: The impact of spin-induced precession
- Time-Dependent Models for Dark Matter at the Galactic Center
- SFI++ II: A New I-band Tully-Fisher Catalog, Derivation of Peculiar Velocities and Dataset Properties
- Non-axisymmetric relativistic Bondi-Hoyle accretion onto a Kerr black hole
- Level sets of the lapse function in static GR
- A gravito-electromagnetic analogy based on tidal tensors
- Spinning particles in general relativity: Momentum-velocity relation for the Mathisson-Pirani spin condition
- Localizing coalescing massive black hole binaries with gravitational waves
- Center of mass, spin supplementary conditions, and the momentum of spinning particles
- Free motion around black holes with discs or rings: between integrability and chaos - I
- Einstein's 1917 Static Model of the Universe: A Centennial Review
- Estimating the sensitivity of pulsar timing arrays
- Bobbing and Kicks in Electromagnetism and Gravity
- Free motion around black holes with discs or rings: between integrability and chaos -- IV
- Spacetime dynamics of spinning particles - exact electromagnetic analogies
- The Chaplygin gas as a model for dark energy
- Binary pulsars as dark-matter probes
- Relativistic Static Thin Disks: The Counter-Rotating Model
- Modelling gravitational waves from precessing black-hole binaries: Progress, challenges and prospects
- Post-Newtonian Approximation in Maxwell-Like Form
- Momentum Flow in Black Hole Binaries: I. Post-Newtonian Analysis of the Inspiral and Spin-Induced Bobbing
- Analytical Potential-Density Pairs for Flat Rings and Toroidal Structures
- Precessing supermassive black hole binaries and dark energy measurements with LISA
- Gravitomagnetic dynamical friction
- Electromagnetic duality in general relativity
- The Coriolis field
- General-relativistic versus Newtonian: geometric dragging and dynamic anti-dragging in stationary disks in the first post-Newtonian approximation
- Black holes and fundamental fields: hair, kicks and a gravitational "Magnus" effect
- Perturbation of a Schwarzschild black hole due to a rotating thin disc
- Exact potential-density pairs for flattened dark haloes
- Schwarzschild black hole encircled by a rotating thin disc: Properties of perturbative solution
- Gyroscope deviation from geodesic motion: quasiresonant oscillations on a circular orbit
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- Mass and spin coevolution of black holes inspiralling through dark matter
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