Falsifiable anthropic model from the string landscape

arXiv:2607.24100 · astro-ph.CO, gr-qc, hep-ph, hep-th · Submitted 2026-07-27 · Read on arXiv

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

Submitted: 2026-07-27

Updated: 2026-09-25

Comments: 3 figures, 1 table

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

Terminology

• Fine-Tuning — 8× in this paper · explained in 5 episodes
• Consistency — 7× in this paper · explained in 3 episodes
• Accuracy — 4× in this paper · explained in 1 episode
• Quintessence — 2× in this paper · explained in 2 episodes
• Abundance — 1× in this paper · explained in 1 episode
• Akaike Information Criterion — 1× in this paper
• Core — 1× in this paper · explained in 2 episodes
• Dark Energy Spectroscopic Instrument — 1× in this paper
• Gravitational Lensing — 1× in this paper · explained in 2 episodes

Sources

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• Planck 2018 results. VI. Cosmological parameters
• de Sitter Vacua in String Theory
• Quintessence, Cosmic Coincidence, and the Cosmological Constant
• String Axiverse
• Unification of Inflation with Dark Energy in $f(R)$ Gravity and Axion Dark Matter
• What if string theory has no de Sitter vacua?
• Why $w \ne -1$? Anthropic Selection in a $\Lambda$ + Axion Dark Energy Model
• Dynamical dark energy from an ultralight axion
• Why anthropic reasoning cannot predict Lambda
• Testing anthropic reasoning for the cosmological constant with a realistic galaxy formation model
• The impact of the cosmological constant on past and future star formation
• The Lifespan of our Universe
• The cosmological constant and the time of its dominance
• Testing anthropic predictions for Lambda and the CMB temperature
• Predictions from Star Formation in the Multiverse
• Galaxy Formation Efficiency and the Multiverse Explanation of the Cosmological Constant with EAGLE Simulations
• The impact of dark energy on galaxy formation. What does the future of our Universe hold?
• The fate of baryons in counterfactual universes

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