Fixed energy solutions to the Euler-Lagrange equations of an indefinite Lagrangian with affine Noether charge
arXiv:2307.07883 · doi:10.1007/s10231-024-01424-4
Abstract
We consider an autonomous, indefinite Lagrangian admitting an infinitesimal symmetry whose associated Noether charge is linear in each tangent space. Our focus lies in investigating solutions to the Euler-Lagrange equations having fixed energy and that connect a given point to a flow line of the infinitesimal generator . By utilizing the invariance of the Lagrangian under the flow of , we simplify the problem into a two-point boundary problem. Consequently, we derive an equation that involves the differential of the ``arrival time'', seen as a functional on the infinite dimensional manifold of connecting paths satisfying the semi-holonomic constraint defined by the Noether charge. When the Lagrangian is positively homogeneous of degree two in the velocities, the resulting equation establishes a variational principle that extends the Fermat's principle in a stationary spacetime. Furthermore, we also analyze the scenario where the Noether charge is affine.
36 pages; fully revised version: we show that the Lagrangians considered include a class of Lorentz-Finsler metrics which do not reduce to Lorentzian metrics; we added a new appendix where we deal with pseudocoercivity in connection with global hyperbolicity. To appear on Ann. Mat. Pura App
References in corpus (13)
- Applications of the Gauss-Bonnet theorem to gravitational lensing
- General Very Special Relativity is Finsler Geometry
- Planck-scale modified dispersion relations and Finsler geometry
- Riemann-Finsler geometry and Lorentz-violating kinematics
- The General Very Special Relativity in Finsler Cosmology
- Stationary Metrics and Optical Zermelo-Randers-Finsler Geometry
- Bipartite Riemann-Finsler geometry and Lorentz violation
- Light cones in Finsler spacetime
- On the analyticity of static solutions of a field equation in Finsler gravity
- Finsler Spinoptics
- Affine sphere relativity
- Fermat's principle in black-hole spacetimes
- A variational setting for an indefinite Lagrangian with an affine Noether charge