Observational Hubble parameter data constraints on the interactive model of $f(T)$ gravity with particle creation
S. Ganjizadeh, Alireza Amani, and M. A. Ramzanpour

TL;DR
This paper explores how particle creation within an $f(T)$ gravity framework influences cosmological evolution, using observational Hubble data to constrain the model and analyze the universe's accelerated expansion and stability.
Contribution
It establishes a novel equivalence between particle creation effects and $f(T)$ gravity's modified continuity equation, linking particle number dynamics with cosmological parameters.
Findings
Reconstructed particle number as a function of redshift.
Constrained $f(T)$ gravity model using observational Hubble data.
Analyzed stability of the model across different cosmic eras.
Abstract
In this paper, we consider an open system from the thermodynamic perspective for an adiabatic FRW universe model in which particle creation occurs within the system. In that case, the modified continuity equation is obtained and then we correspond it to the continuity equation of gravity. So, we take gravity with the viscous fluid in flat-FRW metric, in which is the torsion scalar. We consider the contents of the universe to be dark matter and dark energy and consider an interaction term between them. The interesting point of this study is that we make equivalent the modified continuity equation resulting from the particle creation with the matter continuity equation resulting from gravity. The result of this evaluation creates a relationship between the number of particles and the scale factor. In what follows, we write the corresponding cosmological parameters…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Geophysics and Gravity Measurements
