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Main Authors: Costa, Emanuel Wallison de Oliveira, Jalalzadeh, Raheleh, Júnior, Pedro Felix da Silva, Rasouli, Seyed Meraj Mousavi, Jalalzadeh, Shahram
Format: Preprint
Published: 2023
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Online Access:https://arxiv.org/abs/2310.09464
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author Costa, Emanuel Wallison de Oliveira
Jalalzadeh, Raheleh
Júnior, Pedro Felix da Silva
Rasouli, Seyed Meraj Mousavi
Jalalzadeh, Shahram
author_facet Costa, Emanuel Wallison de Oliveira
Jalalzadeh, Raheleh
Júnior, Pedro Felix da Silva
Rasouli, Seyed Meraj Mousavi
Jalalzadeh, Shahram
contents Our proposed cosmological framework, which is based on fractional quantum cosmology, aims to address the issue of synchronicity in the age of the universe. To achieve this, we have developed a new fractional $Λ$CDM cosmological model. We obtained the necessary formalism by obtaining the fractional Hamiltonian constraint in a general minisuperspace. This formalism has allowed us to derive the fractional Friedmann and Raychaudhuri equations for a homogeneous and isotropic cosmology. Unlike the traditional de Sitter phase, our model exhibits a power-law accelerated expansion in the late-time universe, when vacuum energy becomes dominant. By fitting the model's parameters to cosmological observations, we determined that the fractional parameter of Lévy equals $α=1.986$. Additionally, we have calculated the age of the universe to be 13.8196 Gyr. Furthermore, we have found that the ratio of the age to Hubble time from the present epoch to the distant future is finite and confined within the interval $0.9858\leq Ht<95.238$.
format Preprint
id arxiv_https___arxiv_org_abs_2310_09464
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Estimated Age of the Universe in Fractional Cosmology
Costa, Emanuel Wallison de Oliveira
Jalalzadeh, Raheleh
Júnior, Pedro Felix da Silva
Rasouli, Seyed Meraj Mousavi
Jalalzadeh, Shahram
General Relativity and Quantum Cosmology
Our proposed cosmological framework, which is based on fractional quantum cosmology, aims to address the issue of synchronicity in the age of the universe. To achieve this, we have developed a new fractional $Λ$CDM cosmological model. We obtained the necessary formalism by obtaining the fractional Hamiltonian constraint in a general minisuperspace. This formalism has allowed us to derive the fractional Friedmann and Raychaudhuri equations for a homogeneous and isotropic cosmology. Unlike the traditional de Sitter phase, our model exhibits a power-law accelerated expansion in the late-time universe, when vacuum energy becomes dominant. By fitting the model's parameters to cosmological observations, we determined that the fractional parameter of Lévy equals $α=1.986$. Additionally, we have calculated the age of the universe to be 13.8196 Gyr. Furthermore, we have found that the ratio of the age to Hubble time from the present epoch to the distant future is finite and confined within the interval $0.9858\leq Ht<95.238$.
title Estimated Age of the Universe in Fractional Cosmology
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2310.09464