A Higher Dimensional Cosmological Model for the Search of Dark Energy Source
Pheiroijam Suranjoy Singh, Kangujam Priyokumar Singh

TL;DR
This paper proposes a 5D cosmological model within Lyra geometry that describes an oscillating, isotropic universe dominated by dark energy, with expansion rates consistent with Planck 2018 observations.
Contribution
It introduces a higher-dimensional (5D) cosmological model in Lyra geometry that predicts an oscillating universe with super-exponential expansion and aligns with current Hubble parameter measurements.
Findings
Universe modeled as oscillating with big bang and crunch cycles
Hubble parameter closely matches Planck 2018 data
Universe undergoes super-exponential expansion
Abstract
With due consideration of reasonable cosmological assumptions within the limit of the present cosmological scenario, we have analysed a spherically symmetric metric in 5D setting within the framework of Lyra manifold. The model universe is predicted to be a DE model, dominated by vacuum energy. The model represents an oscillating model, each cycle evolving with a big bang and ending at a big crunch, undergoing a series of bounces. The universe is isotropic and undergoes super-exponential expansion. The value of Hubble's parameter is measured to be which is very close to , the value estimated by the latest Planck 2018 result. A detailed discussion on the cosmological parameters obtained is also presented with graphs.
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