A model of eternal accelerated expansion without particle horizon
Zi-Liang Wang, Jian-Bo Deng

TL;DR
This paper presents a cosmological model based on the emergence of space that naturally avoids the horizon and flatness problems, addressing early universe inflation issues without requiring traditional inflationary mechanisms.
Contribution
It introduces a novel emergent space model that resolves horizon and flatness problems without early universe inflation.
Findings
Model avoids horizon and flatness problems
Vacuum energy evaluated from Hubble constant and universe age
Addresses early universe inflation issues
Abstract
In our previous paper \cite{8}, we proposed a cosmological model from the emergence of space, which possesses a significant character of evaluating the vacuum energy from the Hubble constant and the age of universe. And one problem of this model is that there is no inflation in the early universe. In this paper, we aim at resolving this problem which leads us to a rather surprising conclusion that our cosmological model can avoid the horizon and flatness problems.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Computational Physics and Python Applications
