Particle Creation and Variable Generalized Chaplygin Gas in $\mathcal{F}(\mathcal{R},Σ,\mathcal{T})$ Gravity

Fuente: arXiv
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Auteurs principaux: Myrzakulov, N., Shekh, S. H., Pradhan, Anirudh, Zeyauddin, M.
Format: Preprint
Publié: 2026
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author Myrzakulov, N.
Shekh, S. H.
Pradhan, Anirudh
Zeyauddin, M.
author_facet Myrzakulov, N.
Shekh, S. H.
Pradhan, Anirudh
Zeyauddin, M.
contents In this work, we investigate the cosmological dynamics of a spatially flat Friedmann--Lemaître--Robertson--Walker Universe in the framework of generalized \( \mathcal{F}(\mathcal{R},Σ,\mathcal{T}) \) gravity by incorporating gravitationally induced particle creation together with the variable generalized Chaplygin gas scenario. The modified gravitational action depends explicitly on the Ricci scalar \( \mathcal{R} \), the matter-coupling scalar \( Σ\), and the trace of the energy--momentum tensor \( \mathcal{T} \), which collectively generate significant corrections to the standard cosmological evolution. The particle creation mechanism is introduced through an open thermodynamic description of the Universe. In addition, the dark sector is modeled using the variable generalized Chaplygin gas formalism. To examine the observational consistency of the model, the free parameters are constrained using the Pantheon\(^+\) Type Ia Supernova compilation together with the combined observational Hubble and Pantheon\(^+\) datasets through a statistical \(χ^2\)-analysis. The cosmological behavior of the model is further explored through the evolution of the cosmological parameters. Furthermore, the thermodynamic properties of the model are investigated using the apparent horizon formalism. The obtained results demonstrate that the entropy evolution remains physically consistent throughout the cosmic evolution. Hence, the present \( \mathcal{F}(\mathcal{R},Σ,\mathcal{T}) \) gravity framework with particle creation provides a viable geometrical description of the late-time accelerated Universe and remains compatible with recent cosmological observations.
format Preprint
id arxiv_https___arxiv_org_abs_2605_14541
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Particle Creation and Variable Generalized Chaplygin Gas in $\mathcal{F}(\mathcal{R},Σ,\mathcal{T})$ Gravity
Myrzakulov, N.
Shekh, S. H.
Pradhan, Anirudh
Zeyauddin, M.
General Relativity and Quantum Cosmology
In this work, we investigate the cosmological dynamics of a spatially flat Friedmann--Lemaître--Robertson--Walker Universe in the framework of generalized \( \mathcal{F}(\mathcal{R},Σ,\mathcal{T}) \) gravity by incorporating gravitationally induced particle creation together with the variable generalized Chaplygin gas scenario. The modified gravitational action depends explicitly on the Ricci scalar \( \mathcal{R} \), the matter-coupling scalar \( Σ\), and the trace of the energy--momentum tensor \( \mathcal{T} \), which collectively generate significant corrections to the standard cosmological evolution. The particle creation mechanism is introduced through an open thermodynamic description of the Universe. In addition, the dark sector is modeled using the variable generalized Chaplygin gas formalism. To examine the observational consistency of the model, the free parameters are constrained using the Pantheon\(^+\) Type Ia Supernova compilation together with the combined observational Hubble and Pantheon\(^+\) datasets through a statistical \(χ^2\)-analysis. The cosmological behavior of the model is further explored through the evolution of the cosmological parameters. Furthermore, the thermodynamic properties of the model are investigated using the apparent horizon formalism. The obtained results demonstrate that the entropy evolution remains physically consistent throughout the cosmic evolution. Hence, the present \( \mathcal{F}(\mathcal{R},Σ,\mathcal{T}) \) gravity framework with particle creation provides a viable geometrical description of the late-time accelerated Universe and remains compatible with recent cosmological observations.
title Particle Creation and Variable Generalized Chaplygin Gas in $\mathcal{F}(\mathcal{R},Σ,\mathcal{T})$ Gravity
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2605.14541