Dynamical Dark Energy Emerges from Massive Gravity
Juri Smirnov

TL;DR
This paper shows that massive gravity can produce a dynamic dark energy component with distinctive evolution, fitting current data better than the standard model and predicting testable deviations at high redshift.
Contribution
It introduces a self-consistent massive gravity model that naturally explains phantom dark energy and a small cosmological constant, with specific observational predictions.
Findings
Favored over ΛCDM by current datasets
Predicts a graviton mass around 4.0×10^{-33} eV
Suggests deviations in the equation of state at z~3
Abstract
In this work, we demonstrate that a dynamical dark energy component predicted by massive gravity gives rise to a distinctive evolution of the equation of state. This scenario is favoured over the standard CDM model when confronted with the latest combined datasets from the Dark Energy Spectroscopic Instrument (DESI), the cosmic microwave background (CMB), and supernova observations. The model stands out as a rare example of a healthy, self-consistent theory that accommodates phantom dark energy while maintaining a technically natural, small asymptotic cosmological constant. Our analysis indicates a preferred graviton mass of approximately , suggesting the emergence of a new cosmological length scale. This leads to a maximal deviation of the equation of state around , a prediction that will be robustly tested by upcoming, deeper surveys…
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Taxonomy
TopicsCosmology and Gravitation Theories · Pulsars and Gravitational Waves Research · Particle physics theoretical and experimental studies
