REVIEW 6 cited by
Why the DESI Results Should Not Be A Surprise
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
The recent DESI results provide increasing evidence that the density of dark energy is time-dependent. I will recall why, from the point of view of fundamental theory,, this result should not be surprising.
Forward citations
Cited by 6 Pith papers
-
Weinberg's theorem, phantom crossing and screening
Graviton-loop-induced screening forces single-field dilaton and chameleon dark energy models to keep their equation of state near -1, making observable phantom crossing impossible in this class.
-
Evolving Dark Sector and the Dark Dimension Scenario
A two-parameter fading dark sector model, with exponential dark energy potential and exponential dark matter mass, matches DESI DR2 plus supernova data and naturally yields apparent w<-1 phantom behavior.
-
Constraints on Barrow and Tsallis Holographic Dark Energy from DESI DR2 BAO data
Barrow and Tsallis holographic dark energy models fit DESI DR2 data but are disfavored by information criteria versus LambdaCDM and do not ease the Hubble tension.
-
Holographic dark energy in a coasting cosmology
The authors construct a Tsallis-entropy holographic dark energy model that enforces a coasting expansion, fit it to SNIa, BAO and CC data, and report AIC/BIC/KIC improvements over LambdaCDM.
-
Constraint on Symmetric Teleparallel Gravity with Different Dark energy Parametrizations from DESI DR2 BAO Data
MCMC fits of CPL and BA dark energy parametrizations in power-law f(Q) gravity to DESI DR2 and prior BAO H(z) data find statistically competitive or better fits than Lambda-CDM.
-
DESI results and Dark Energy from QCD topological sectors
A QCD-vacuum dark-energy model with ρ_DE ∝ H can mimic DESI's evolving w(z), but its key z≥0 predictions rely on an uncomputed activation function.
Discussion (0). Sign in to comment.