A density-responsive scalar-field framework for singularity regularization and dynamical dark energy
Martin Drobczyk

TL;DR
This paper introduces a covariant scalar-field model that regularizes space-time singularities at high densities and explains dark energy at low densities, making testable cosmological predictions.
Contribution
It presents a unified scalar-field framework that links singularity regularization with dynamical dark energy without fine-tuning, and predicts distinctive cosmological parameters.
Findings
Provides a Planck-scale upper bound on energy density to regularize singularities
Predicts dark energy equation of state parameters: w0 ≈ -0.99, wa ≈ +0.03
Suppresses fifth forces below 10^{-58} in laboratory tests
Abstract
We present a covariant scalar-field framework that unifies the space-time singularity regularization with dynamical dark energy. The theory extends general relativity by introducing a scalar field whose potential couples to the Lorentz-invariant quantity , ensuring manifest covariance. The resulting density-responsive scalar energy exhibits dual behavior: (i) in high-density regimes, it saturates at , providing a Planck-scale upper bound on the total energy density that regularizes classical singularities; (ii) in low-density regimes, it approaches a constant , driving cosmic acceleration as dynamical dark energy. A natural renormalization group evolution with an anomalous dimension connects the Planck scale to the meV dark energy…
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Taxonomy
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Astronomy and Astrophysical Research
