Collider Probes of Dark Energy Microphysics

arXiv:2606.27441 · hep-ph, astro-ph.CO, gr-qc, hep-ex · Submitted 2026-06-25 · Read on arXiv

Chaitanya Bashyam, Alfredo Gurrola, Andres Florez, Cristian Rodriguez

hep-ph, astro-ph.CO, gr-qc, hep-ex

Submitted: 2026-06-25

Comments: 36 pages (26 pages of main text), 3 figures

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Quintessence — 18× in this paper · explained in 2 episodes
• Benchmark — 5× in this paper · explained in 2 episodes
• Standard Model — 5× in this paper
• Consistency — 4× in this paper · explained in 3 episodes
• Acoustic Metric — 1× in this paper · explained in 1 episode
• Clustering — 1× in this paper · explained in 2 episodes
• Decoupling — 1× in this paper · explained in 2 episodes
• Effective Field Theory (EFT) — 1× in this paper · explained in 2 episodes
• N-body simulations — 1× in this paper · explained in 2 episodes
• Phase Transitions — 1× in this paper · explained in 2 episodes
• Quantization — 1× in this paper · explained in 12 episodes
• Reheating — 1× in this paper · explained in 2 episodes
• Symmetry Breaking — 1× in this paper · explained in 3 episodes

Sources

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Observational Constraints on Dynamical Dark Energy Models
• Dark Energy: a Brief Review
• Dark Energy
• Dark Energy: A Short Review
• Dark energy two decades after: Observables, probes, consistency tests
• The Effective Field Theory of Inflation
• Recovering P(X) from a canonical complex field
• On the Bondi accretion of a self-interacting complex scalar field
• Direct detection of dark energy: the XENON1T excess and future prospects
• Dark energy in light of the early JWST observations: case for a negative cosmological constant?
• Soundness of Dark Energy properties
• Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
• Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• How much has DESI dark energy evolved since DR1?
• A new generic evolution for $k$-essence dark energy with $w \approx -1$
• Slow-roll k-essence
• Tracking quintessence and k-essence in a general cosmological background
• Effective Field Theory of Dark Energy: a Review

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