Can a late-time cosmological model based on baby universe absorption explain the z-variation of w?

Fuente: arXiv
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Autori principali: Ambjorn, Jan, Watabiki, Yoshiyuki
Natura: Preprint
Pubblicazione: 2026
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author Ambjorn, Jan
Watabiki, Yoshiyuki
author_facet Ambjorn, Jan
Watabiki, Yoshiyuki
contents We point out that a simple late-time cosmological model where our Universe can absorb "baby universes" explains the exponential expansion of our universe without the need of a cosmological constant and leads to a z-dependence of the parameter w(z) in the equation of state. In this model w(z) is less than -1 for z sufficiently large.
format Preprint
id arxiv_https___arxiv_org_abs_2605_15045
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Can a late-time cosmological model based on baby universe absorption explain the z-variation of w?
Ambjorn, Jan
Watabiki, Yoshiyuki
General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
High Energy Physics - Theory
We point out that a simple late-time cosmological model where our Universe can absorb "baby universes" explains the exponential expansion of our universe without the need of a cosmological constant and leads to a z-dependence of the parameter w(z) in the equation of state. In this model w(z) is less than -1 for z sufficiently large.
title Can a late-time cosmological model based on baby universe absorption explain the z-variation of w?
topic General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
High Energy Physics - Theory
url https://arxiv.org/abs/2605.15045