Three families of non-Ricci-flat, asymptotically flat, SO(3)-symmetric Berwald vacuum solutions are derived as the first non-trivial exact solutions in Finsler gravity.
Finsler spacetime geometry in Physics
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Finsler gravity vacuum equation reduces to vanishing Finsler Ricci curvature when some power F^n is regular with non-degenerate metric on light cones and Landsberg term vanishes, enabling solutions for homogeneous isotropic Landsberg spacetimes.
Quantum deformation of projective phase-space geometry induces a conformally deformed FLRW metric whose time-dependent corrections modify inflationary background equations, slow-roll parameters, and perturbations in a covariant manner.
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Spherically symmetric, asymptotically flat Berwald vacuum solutions in Finsler gravity
Three families of non-Ricci-flat, asymptotically flat, SO(3)-symmetric Berwald vacuum solutions are derived as the first non-trivial exact solutions in Finsler gravity.
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Reduction of the Finsler gravity vacuum equation and dynamics for the cosmological Landsberg spacetimes
Finsler gravity vacuum equation reduces to vanishing Finsler Ricci curvature when some power F^n is regular with non-degenerate metric on light cones and Landsberg term vanishes, enabling solutions for homogeneous isotropic Landsberg spacetimes.
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Quantum-Deformed Phase-Space Geometry and Emergent Inflation in Effective Four-Dimensional Spacetime
Quantum deformation of projective phase-space geometry induces a conformally deformed FLRW metric whose time-dependent corrections modify inflationary background equations, slow-roll parameters, and perturbations in a covariant manner.