SdS black holes support only a finite number of bound-state resonance levels with closed-form energies, while asymptotically flat Schwarzschild black holes have infinitely many that delocalize without bound.
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The paper analyzes total gravitational energy and its flux in asymptotic regions of radiative spacetimes to provide a theoretical basis for assessing gravitational radiation's contribution to cosmological acceleration.
An f(R,T) gravity model in anisotropic spacetime is reconstructed via a variable deceleration parameter and tightly constrained by Hubble and Pantheon+ data, reproducing the deceleration-to-acceleration transition and approaching de Sitter expansion.
citing papers explorer
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Bound-State Resonances of Schwarzschild-de Sitter Black Holes: Analytic Treatment
SdS black holes support only a finite number of bound-state resonance levels with closed-form energies, while asymptotically flat Schwarzschild black holes have infinitely many that delocalize without bound.
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The Role of Gravitational Energy Flux in Cosmic Acceleration
The paper analyzes total gravitational energy and its flux in asymptotic regions of radiative spacetimes to provide a theoretical basis for assessing gravitational radiation's contribution to cosmological acceleration.
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Anisotropic Cosmology with interacting Dark Energy in f(R,T) Gravity: A Data-Constrained & independent Approach
An f(R,T) gravity model in anisotropic spacetime is reconstructed via a variable deceleration parameter and tightly constrained by Hubble and Pantheon+ data, reproducing the deceleration-to-acceleration transition and approaching de Sitter expansion.