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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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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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.