Cosmology with the matter component decaying faster than radiation

Fuente: arXiv
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Autori principali: Kuzmichev, V. E., Kuzmichev, V. V.
Natura: Preprint
Pubblicazione: 2024
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author Kuzmichev, V. E.
Kuzmichev, V. V.
author_facet Kuzmichev, V. E.
Kuzmichev, V. V.
contents The impact of a fast decaying component of mass-energy, that decreases faster than radiation with the increase of the scale factor, on the evolution of the universe is studied using a hydrodynamic approach. Proceeding from the Hamiltonian formalism, the hydrodynamic-like equations for the velocity and acceleration of the expansion of the universe as a function of conformal time are obtained. The influence of a fast decaying component on the dynamics of the expansion of the universe is determined by the sign of its contribution to the total energy density of the system. The effects of this component are illustrated by figures.
format Preprint
id arxiv_https___arxiv_org_abs_2412_06455
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Cosmology with the matter component decaying faster than radiation
Kuzmichev, V. E.
Kuzmichev, V. V.
General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
The impact of a fast decaying component of mass-energy, that decreases faster than radiation with the increase of the scale factor, on the evolution of the universe is studied using a hydrodynamic approach. Proceeding from the Hamiltonian formalism, the hydrodynamic-like equations for the velocity and acceleration of the expansion of the universe as a function of conformal time are obtained. The influence of a fast decaying component on the dynamics of the expansion of the universe is determined by the sign of its contribution to the total energy density of the system. The effects of this component are illustrated by figures.
title Cosmology with the matter component decaying faster than radiation
topic General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2412.06455