Salvato in:
Dettagli Bibliografici
Autori principali: Faria, F. F., Silva, G. S.
Natura: Preprint
Pubblicazione: 2025
Soggetti:
Accesso online:https://arxiv.org/abs/2508.09244
Tags: Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!
_version_ 1866917237545238528
author Faria, F. F.
Silva, G. S.
author_facet Faria, F. F.
Silva, G. S.
contents We study the evolution of matter density perturbations in the framework of massive conformal gravity (MCG). Starting from the conservation of the energy-momentum tensor, we find the continuity and Euler equations for the conformal perfect fluid that fills the MCG universe. We then obtain the perturbed MCG cosmological equations, from which we derive the equation that determines the linear growth of matter fluctuations in the MCG universe. The resulting growth equation shows that MCG enhances cosmic structure formation at high redshifts and suppresses it at low redshifts when compared to the $Λ$CDM cosmological model.
format Preprint
id arxiv_https___arxiv_org_abs_2508_09244
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Cosmic structure formation in massive conformal gravity
Faria, F. F.
Silva, G. S.
General Relativity and Quantum Cosmology
We study the evolution of matter density perturbations in the framework of massive conformal gravity (MCG). Starting from the conservation of the energy-momentum tensor, we find the continuity and Euler equations for the conformal perfect fluid that fills the MCG universe. We then obtain the perturbed MCG cosmological equations, from which we derive the equation that determines the linear growth of matter fluctuations in the MCG universe. The resulting growth equation shows that MCG enhances cosmic structure formation at high redshifts and suppresses it at low redshifts when compared to the $Λ$CDM cosmological model.
title Cosmic structure formation in massive conformal gravity
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2508.09244