Quintessential Implications of the presence of AdS in the Dark Energy sector
arXiv:2501.18335 · doi:10.1103/fzg5-k6h9
Abstract
We explore the implications for an Anti-de Sitter (AdS) vacuum, equivalently a negative cosmological constant (nCC), in the dark energy (DE) sector using current cosmological observations. Our joint analysis uses DESI BAO, DESY5 supernovae, and P-ACT CMB (ACT-DR6 + Planck) measurements. We also use the KiDS weak-lensing measurement to cross-check consistency with the inferred value of . Within the Chevallier--Polarski--Linder parametrization for the evolving component of the DE, the inclusion of an AdS term provides a theoretically motivated mechanism that opens up a finite non-phantom region in the CPL parameter space while remaining compatible with current observations. A negative cosmological constant also implies a finite cosmic lifetime, thereby linking observational DE phenomenology to broader questions in quantum gravity and string theory.
6 pages, 7 sets of figures. Accepted in Phys. Rev. D
References in corpus (45)
- 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
- In the Realm of the Hubble tension a Review of Solutions
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
- The Pantheon+ Analysis: Cosmological Constraints
- Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
- Challenges for CDM: An update
- KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics
- KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints
- Reconstructing Dark Energy
- Cobaya: Code for Bayesian Analysis of hierarchical physical models
- A population of red candidate massive galaxies ~600 Myr after the Big Bang
- Cosmology Intertwined II: The Hubble Constant Tension
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Cosmology Intertwined III: and
- Stress Testing CDM with High-redshift Galaxy Candidates
- DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars
- DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest
- Cosmological parameters derived from the final (PR4) Planck data release
- LiteBIRD: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization
- Assessing observational constraints on dark energy
- Interpreting DESI's evidence for evolving dark energy
- Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data
- Scant evidence for thawing quintessence
- Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension
- Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat CDM cosmological parameterization result
- Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?
- Underdetermination of dark energy
- Negative cosmological constant in the dark sector?
- Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements
- Matching current observational constraints with nonminimally coupled dark energy
- A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data
- Do cosmological observations allow a negative ?
- Omnipotent dark energy: A phenomenological answer to the Hubble tension
- DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
- Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
- On the Null Energy Condition and Cosmology
- Model-independent cosmological inference post DESI DR1 BAO measurements
- Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant
- Consistency tests between SDSS and DESI BAO measurements
- New Expansion Rate Anomalies at Characteristic Redshifts Geometrically Determined using DESI-DR2 BAO and DES-SN5YR Observations
- Scalar-Tensor Gravity and DESI 2024 BAO data
- Post-reionization HI 21-cm signal: A probe of negative cosmological constant
- Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity
- Probing galaxy evolution through HI 21-cm emission and absorption: current status and prospects with the Square Kilometre Array
- Model-Agnostic Cosmological Inference with SDSS-IV eBOSS: Simultaneous Probing for Background and Perturbed Universe
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- Revisiting CPL with sign-switching density: To cross or not to cross the NECB
- Can an Anti-de Sitter Vacuum in the Dark Energy Sector Explain JWST High-Redshift Galaxy and Reionization Observations?
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