Separation of variables in Hamilton-Jacobi and Klein-Gordon-Fock equations for a charged test particle in the Stackel spaces of type (1.1)
arXiv:2012.02548 · doi:10.1142/S0219887821500365
Abstract
All equivalence classes for electromagnetic potentials and space-time metrics of Stackel spaces, provided that Hamilton-Jacobi equation and Klein-Gordon-Fock equation for a charged test particle can be integrated by the method of complete separation of variables are found. The separation is carried out using the complete sets of mutually-commuting integrals of motion of type (1.1). Whereby in a privileged coordinate system the given equations turn into parabolic type equations. Hence, these metrics can be used as models for describing plane gravitational waves.
arXiv commentThe article will be published in IJGMMP
References in corpus (14)
- Charged particle in higher dimensional weakly charged rotating black hole spacetime
- Aspects of Axion Gravity
- The evolution of gravitons in accelerating cosmologies: the case of extended gravity
- On stability of exponential cosmological solutions with non-static volume factor in the Einstein-Gauss-Bonnet model
- Gravity with an Axion-like Particle: Dynamics, Gravity Waves, Late and Early-time Phenomenology
- On the propagation of gravitational waves in strong magnetic fields
- Separability in Riemannian Manifolds
- Pure radiation in space-time models that admit integration of the eikonal equation by the separation of variables method
- Separation of variables in Hamilton-Jacobi equation for a charged test particle in the Stackel spaces of type (2.0)
- Shapovalov wave-like spacetimes
- The space-time models with dust matter that admit separation of variables in Hamilton-Jacobi equations of a test particle
- Separation of variables in Hamilton-Jacobi equation for a charged test particle in the Stackel spaces of type (2.1)
- The extended Einstein-Maxwell-aether-axion model: Exact solutions for axionically controlled pp-wave aether modes
- Stable exponential cosmological solutions with zero variation of G in the Einstein-Gauss-Bonnet model with a Lambda-term
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- Solutions of Maxwell equations for admissible electromagnetic fields, in spaces with simply transitive four-parameter groups of motions
- Gravitational wave of the Bianchi VII universe: particle trajectories, geodesic deviation and tidal accelerations
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