REVIEW 3 cited by
Unification of Dark Matter and Dark Energy: the Inhomogeneous Chaplygin Gas
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
Unification of Dark Matter and Dark Energy: the Inhomogeneous Chaplygin Gas
read the original abstract
We extend the world model of Kamenshchik et al. to large perturbations by formulating a Zeldovich-like approximation. We sketch how this model unifies dark matter with dark energy in a geometric setting reminiscent of M-theory.
Forward citations
Cited by 3 Pith papers
-
A solid unification of the dark sector
A generalized Chaplygin-type solid unifies dark matter and dark energy via an early pressureless phase transitioning to a late solid phase that supports acceleration and produces distinct low-redshift perturbation signatures.
-
Entropic Chaplygin-Gas cosmology and late-universe tension diagnostics
An entropic Chaplygin-gas dark sector can shift fitted H0 values, but the shift and any tension relief depend on supernova calibration and vanish with DES-Dovekie data.
-
Resolving the Planck-DESI tension by nonminimally coupled quintessence
Non-minimally coupled quintessence resolves the Planck-DESI Ω_m tension at >3σ while the effective equation of state stays above w=-1 and other tensions on neutrino mass and growth rate are relieved.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.