Post-Newtonian effective theory breaks down in generic many-body relativistic dynamics despite small local potentials and velocities, due to sensitivity from absent conserved charges and non-integrability, supplying a criterion for reliable weak-field mass inference relevant to the dark matter
Title resolution pending
8 Pith papers cite this work. Polarity classification is still indexing.
8
Pith papers citing it
citation-role summary
background 3
citation-polarity summary
fields
gr-qc 8years
2026 8roles
background 3polarities
background 3representative citing papers
Bounded tidal fields imply a rigorous limit on accumulated geodesic deviation set by τ* = λ_max^{-1/2} and a critical wavenumber k* ~ τ*^{-1} for perturbation transfer with exponential suppression at high k.
Derives perihelion shift equations for S2 star in generalized Schwarzschild-Dehnen BH-DM spacetime and constrains gamma, rho_s, rs via MCMC on Do et al. and Gillessen et al. datasets.
An RG-improved Schwarzschild-like black hole yields a multipole-independent SCC ratio at the 6% level, a bell-shaped Hawking temperature, and remains the most Schwarzschild-like among regular black hole models while shadow-degenerate with Hayward and Bonanno-Reuter at the 1% level.
An exact black hole solution in Born-Infeld-f(R) gravity shows thermodynamic quantities that deviate from Schwarzschild-AdS predictions.
Skyrmion black holes show modified photon spheres, shadows, and sparser Hawking radiation due to the Skyrme coupling strength and background parameters.
Gravitational lensing is recast as an optical phenomenon governed by effective refractive index, yielding closed-form deflection angles and Einstein radii for modified gravity models including deep-MOND, Yukawa, and power-law f(R).
citing papers explorer
-
When Weak Fields Arent Weak: Post-Newtonian effective theory and the Dark Matter Puzzle
Post-Newtonian effective theory breaks down in generic many-body relativistic dynamics despite small local potentials and velocities, due to sensitivity from absent conserved charges and non-integrability, supplying a criterion for reliable weak-field mass inference relevant to the dark matter
-
Tidal Deformation Bounds and Perturbation Transfer in Bounded Curvature Spacetimes
Bounded tidal fields imply a rigorous limit on accumulated geodesic deviation set by τ* = λ_max^{-1/2} and a critical wavenumber k* ~ τ*^{-1} for perturbation transfer with exponential suppression at high k.
-
Constraints on Schwarzschild Black Hole in a Generalized Dehnen-Type $(1,4,\gamma)$ Dark Matter Halo via the S2 Star Orbit around Sgr A$^\star$
Derives perihelion shift equations for S2 star in generalized Schwarzschild-Dehnen BH-DM spacetime and constrains gamma, rho_s, rs via MCMC on Do et al. and Gillessen et al. datasets.
-
Renormalization-group improved Schwarzschild black hole: shadow, ringdown, and strong cosmic censorship
An RG-improved Schwarzschild-like black hole yields a multipole-independent SCC ratio at the 6% level, a bell-shaped Hawking temperature, and remains the most Schwarzschild-like among regular black hole models while shadow-degenerate with Hayward and Bonanno-Reuter at the 1% level.
-
Born-Infeld-f(R) black holes
An exact black hole solution in Born-Infeld-f(R) gravity shows thermodynamic quantities that deviate from Schwarzschild-AdS predictions.
-
Shadow, Sparsity of Radiation and Energy Emission Rate in Skyrmion Black Holes
Skyrmion black holes show modified photon spheres, shadows, and sparser Hawking radiation due to the Skyrme coupling strength and background parameters.
-
Gravitational Lensing as an Optical Framework for Modified Gravity Theories
Gravitational lensing is recast as an optical phenomenon governed by effective refractive index, yielding closed-form deflection angles and Einstein radii for modified gravity models including deep-MOND, Yukawa, and power-law f(R).
- Astrophysical Objects in Modified Theories of Gravity