A non-local origin for massive gravity and late-time acceleration
Susobhan Mandal, S. Shankaranarayanan

TL;DR
This paper proposes a non-local gravity model that naturally produces a massive graviton and explains late-time cosmic acceleration, while remaining free of ghosts and consistent with observations.
Contribution
It introduces a novel non-local gravity action that yields a stable de Sitter universe and a ghost-free massive graviton, offering an alternative to scalar-tensor dark energy models.
Findings
The model has a stable de Sitter attractor.
All perturbations are ghost-free and stable.
Predicts distinct gravitational wave polarization signatures.
Abstract
The accelerated expansion of the universe poses a significant challenge to General Relativity. Non-local modifications to gravity have emerged as a compelling class of theories to address this dark energy puzzle. Building upon earlier proposals, we investigate a specific non-local modified gravity action incorporating terms like , , and demonstrate that it provides a dynamical origin for a massive graviton by reducing to the standard and extended Fierz-Pauli action at the linearized level. A fixed-point analysis of the background cosmology reveals a stable de Sitter attractor, ensuring the model naturally drives accelerated expansion. Crucially, we investigate the cosmological perturbations and show that the theory's six propagating degrees of freedom are free from ghost instabilities. We…
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Taxonomy
TopicsCosmology and Gravitation Theories · Pulsars and Gravitational Waves Research · Black Holes and Theoretical Physics
