The Goldstone Awakens: Unimodular dark energy in scale-invariant R squared gravity
Mariaveronica De Angelis, Javier Rubio
astro-ph.CO, gr-qc, hep-th
Submitted: 2026-07-17
Comments: 32 pages, 8 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Naturalness and Dimensional Transmutation in Classically Scale-Invariant Gravity
- Conformal symmetry: towards the link between the Fermi and the Planck scales
- Gravity, Scale Invariance and the Hierarchy Problem
- Standard Model Meets Gravity: Electroweak Symmetry Breaking and Inflation
- One residue to rule them all: Electroweak symmetry breaking, inflation and field-space geometry
- The Standard Model Higgs boson as the inflaton
- Asymptotic safety of gravity and the Higgs boson mass
- Agravity
- On the robustness of the primordial power spectrum in renormalized Higgs inflation
- Scale-invariant alternatives to general relativity
- On the geometrical interpretation of scale-invariant models of inflation
- Emergent scale symmetry: Connecting inflation and dark energy
- Inflation and reheating in scale-invariant scalar-tensor gravity
- Inflation in a scale invariant universe
- Scale-invariant alternatives to general relativity. III. The inflation--dark-energy connection
- Higgs inflation
- Scale independent $R^2$ inflation
- Weyl $R^2$ inflation with an emergent Planck scale
- Nonminimal Coleman--Weinberg Inflation with an $R^2$ term
- Einstein-Cartan gravity, matter, and scale-invariant generalization
Related papers
- Angular clustering and bias of photometric quasars in the Kilo-Degree Survey Data Release 4
- A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
- Magnetic fields at the dawn of structure formation I. The CARLA J1510+5958 proto-cluster
- Dark Energy Survey Year 6 Results: Weak Lensing and Galaxy Clustering Cosmological Analysis Framework
- Exploring the Impact of Systematic Bias in Type Ia Supernova Cosmology Across Diverse Dark Energy Parametrizations
- Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation