Exploring Hu-Sawicki-like modified gravity with Genetic Algorithms
Chiara De Leo, Elisa Fazzari, Matteo Martinelli, Savvas Nesseris
astro-ph.CO, gr-qc
Submitted: 2026-07-14
Comments: Prepared for submission to PRD. 15 pages and 5 figures
Code: https://github.com/snesseris/Genetic-Algorithms
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars
- DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data
- DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest
- DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest
- Validation of the DESI DR2 Measurements of Baryon Acoustic Oscillations from Galaxies and Quasars
- Accelerating Universes with Scaling Dark Matter
- Exploring the Expansion History of the Universe
- Extended Dark Energy analysis using DESI DR2 BAO measurements
- Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements
- Robustness of dark energy phenomenology across different parameterizations
- To CPL, or not to CPL? What we have not learned about the dark energy equation of state
- Cosmographic Footprints of Dynamical Dark Energy
- Distinguishing Coupled Dark Energy Models with Neural Networks
- Nonparametric reconstructions of dynamical dark energy via flexknots
- Reconstructing the dark energy density in light of DESI BAO observations
- New Expansion Rate Anomalies at Characteristic Redshifts Geometrically Determined using DESI-DR2 BAO and DES-SN5YR Observations
- f(R) Theories Of Gravity
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