REVIEW 1 cited by
Accelerated cosmic expansion, mass creation, and the QCD axion
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
Accelerated cosmic expansion, mass creation, and the QCD axion
read the original abstract
We propose a mechanism in which the current acceleration of cosmic expansion is driven by continuous creation of energy density $\rho_b$ for a certain field $\varphi_b$. We accordingly modify Einstein equation, derive modified Friedmann equations and analyze the regimes in which cosmic acceleration occurs. The creation process requires $\rho_b\neq 0$ as initial condition, which we enforce by identifying $\varphi_b$ with the axion of a hidden gauge group that confined in recent cosmological times, leading to a level crossing between $\varphi_b$ and the QCD axion, which is assumed to comprise dark matter. The conversion of a small fraction of QCD axions into $\varphi_b$ shortly before matter-dark energy equality generates the initial $\rho_b$ needed to trigger the creation process and offers a solution to the coincidence puzzle.
Forward citations
Cited by 1 Pith paper
-
Cosmology of axion dark energy in supersymmetric models and constraints on high scale parameters
A two-cosine axion dark energy potential fits CMB+BAO+supernova data better than the standard one-cosine potential, while preferring a sub-Planckian decay constant and a feeble dark-matter coupling.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.