A density-responsive scalar-field framework for singularity regularization and dynamical dark energy
arXiv:2506.12464 · doi:10.1088/1361-6382/ae1ac1
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 scale without fine-tuning. The model makes distinctive, testable predictions: and , where the positive distinguishes it from CDM and standard quintessence models. Despite the novel interaction terms, the fifth forces are suppressed by , yielding factors below in laboratory environments, and ensuring compatibility with all precision gravity tests. This framework demonstrates how a single quantum field theory mechanism can simultaneously address UV singularities and IR dark energy, providing concrete predictions for future Stage-IV cosmological surveys.
arXiv commentRevised per referee reports; resubmitted to Classical and Quantum Gravity. Title and Abstract updated, Structure clarified and updated; updated figures; expanded appendices
References in corpus (39)
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- The Hierarchy Problem and New Dimensions at a Millimeter
- Dynamics of dark energy
- The Confrontation between General Relativity and Experiment
- Cosmological Constant - the Weight of the Vacuum
- Quasilocal Energy and Conserved Charges Derived from the Gravitational Action
- Chameleon Fields: Awaiting Surprises for Tests of Gravity in Space
- Exponential potentials and cosmological scaling solutions
- Formation and evaporation of non-singular black holes
- Science Case for the Einstein Telescope
- Loop Quantum Cosmology: A Status Report
- Dark Matter Self-interactions and Small Scale Structure
- Cluster Abundance Constraints on Quintessence Models
- Science with the space-based interferometer eLISA. II: Gravitational waves from cosmological phase transitions
- Cosmological Backgrounds of Gravitational Waves
- Quantum Gravity and Extra Dimensions at High-Energy Colliders
- Cosmic Growth History and Expansion History
- Precise Relic WIMP Abundance and its Impact on Searches for Dark Matter Annihilation
- Symmetron Fields: Screening Long-Range Forces Through Local Symmetry Restoration
- Cosmological Relaxation of the Electroweak Scale
- Renormalization group improved black hole spacetimes
- Discovering the QCD Axion with Black Holes and Gravitational Waves
- Dark Matter Halos as Particle Colliders: A Unified Solution to Small-Scale Structure Puzzles from Dwarfs to Clusters
- The non-gravitational interactions of dark matter in colliding galaxy clusters
- Detecting Dark Energy in Orbit -- the Cosmological Chameleon
- The Relation between Physical and Gravitational Geometry
- Gravitational wave searches for ultralight bosons with LIGO and LISA
- Cosmological constant and vacuum energy: old and new ideas
- Inflation and quintessence with nonminimal coupling
- Information Loss
- ETHOS - An Effective Theory of Structure Formation: Dark matter physics as a possible explanation of the small-scale CDM problems
- Gravitational waves from first-order cosmological phase transitions: lifetime of the sound wave source
- Sequestering the Standard Model Vacuum Energy
- Is there a supernova bound on axions?
- Regular black holes with stable cores
- Constraints on Relaxion Windows
- Cosmic Censorship in Quantum Einstein Gravity
- Asymptotic Safety: Swampland or Wonderland?
- Microscopic origin of Einstein's field equations and the raison d'être for a positive cosmological constant