A solid unification of the dark sector
Jose Beltrán Jiménez, María Pérez Garrote, Florencia A. Teppa Pannia, Shinji Tsujikawa
astro-ph.CO, gr-qc
Submitted: 2026-06-25
Comments: 27 pages, 5 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
- Planck 2018 results. VI. Cosmological parameters
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- Measuring the matter density using baryon oscillations in the SDSS
- Detailed Mass Map of CL0024+1654 from Strong Lensing
- A direct empirical proof of the existence of dark matter
- Particle Dark Matter: Evidence, Candidates and Constraints
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- The Case for a Positive Cosmological Lambda-term
- The Cosmological Constant
- Cosmological Constant - the Weight of the Vacuum
- The Cosmological Constant and Dark Energy
- Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)
- Tensions between the Early and the Late Universe
- In the Realm of the Hubble tension $-$ a Review of Solutions
- A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
- Measurements of the Hubble Constant: Tensions in Perspective
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
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