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.
Finsler gravity action from variational completion
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
years
2026 3verdicts
UNVERDICTED 3roles
background 1polarities
background 1representative citing papers
The paper classifies Einstein-Kropina metrics satisfying the Pfeifer-Wohlfarth vacuum Finsler gravity equation, proving they are Berwald and Ricci-flat with vanishing cosmological constant in dimensions five and higher.
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.
citing papers explorer
-
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.
-
Einstein-Kropina Metrics and Their Application in Finsler Gravity
The paper classifies Einstein-Kropina metrics satisfying the Pfeifer-Wohlfarth vacuum Finsler gravity equation, proving they are Berwald and Ricci-flat with vanishing cosmological constant in dimensions five and higher.
-
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.