Constraints on Cubic and $f(P)$ Gravity from the Cosmic Chronometers, BAO & CMB datasets : Use of Machine Learning Algorithms
Kinsuk Giri (NITTTR, Kolkata), Prabir Rudra (Asutosh College, Kolkata)

TL;DR
This paper constrains Einsteinian cubic and $f(P)$ gravity models using cosmic chronometers, BAO, and CMB data, employing machine learning algorithms like linear regression and neural networks to estimate the Hubble parameter and compare with observations.
Contribution
It introduces a novel combination of observational data analysis with machine learning techniques to constrain and estimate parameters in advanced gravity models.
Findings
Theoretical models fit observational data well.
Machine learning models accurately estimate $H(z)$.
Parameter bounds are effectively derived using MCMC.
Abstract
In this work, we perform observational data analysis on Einsteinian cubic gravity and gravity to constrain the parameter space of the theories. We use the 30-point cosmic chronometer data as the observational tool for our analysis along with the BAO and the CMB peak parameters. The statistic is used for the fitting analysis and it is minimized to obtain the best fit values for the free model parameters. We have used the Markov chain Monte Carlo algorithm to obtain bounds for the free parameters. To achieve this we used the publicly available CosmoMC code to put parameter bounds and subsequently generate contour plots for them with different confidence intervals. Besides finding the Hubble parameter in terms of the redshift theoretically from our gravity models, we have exercised correlation coefficients and two machine learning models, namely the linear…
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