Generalized Chaplygin gas and accelerating universe in gravity
arXiv:2206.10336 · doi:10.1016/j.dark.2022.101074
Abstract
The generalized Chaplygin gas (GCG), which has an unusual perfect fluid equation of state, is another promising candidate for dark energy. We investigate the GCG scenario coupled with a baryonic matter in a newly suggested gravity, an arbitrary function of non-metricity and the trace of energy-momentum tensor . We consider the functional form of as a linear combination of and an arbitrary function of , denoted by . Furthermore, we obtain two different functional forms of the model under high pressure and high-density scenarios of GCG. We also test each model with the recent Pantheon supernovae data set of 1048 data points, Hubble data set of 31 points, and baryon acoustic oscillations. The deceleration parameter is constructed using , predicting a transition from decelerated to accelerated phases of the universe expansion. Also, the equation of state parameter acquires a negative behavior depicting acceleration. Finally, we analyze the statefinder diagnostic to discriminate between the GCG and other dark energy models.
Physics of the Dark Universe published version
References in corpus (17)
- f(R,T) gravity
- Disappearing cosmological constant in f(R) gravity
- Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z2
- Cosmological Evolution of a Quintom Model of Dark Energy
- Hubble parameter measurement constraints on the redshift of the deceleration-acceleration transition, dynamical dark energy, and space curvature
- Large Scale Structure as a Probe of Gravitational Slip
- Correcting Type Ia Supernova Distances for Selection Biases and Contamination in Photometrically Identified Samples
- Modelling wormholes in gravity
- gravity models with observational constraints
- Three thermodynamically-based parametrizations of the deceleration parameter
- Cosmological Perturbation Theory in Gravity
- Fitting gravity models with a CDM limit using H(z) and Pantheon data
- Constraining effective equation of state in gravity
- Observational constraints on Myrzakulov gravity
- Viscous cosmology in the Weyl-type gravity
- Late time acceleration due to generic modification of gravity and Hubble tension
- Possible Resolution of the Hubble Tension with Weyl Invariant Gravity
Cited by in corpus (12)
- Phase structure of charged AdS black holes surrounded by exotic fluid with modified Chaplygin equation of state
- Reconstruction of Lagrangian for various cosmological scenario
- Non-exotic static spherically symmetric thin-shell wormhole solution in gravity
- Interaction of divergence-free deceleration parameter in Weyl-type gravity
- Dark energy constraint on equation of state parameter in the Weyl type gravity
- Effects of the matter Lagrangian degeneracy in gravity
- Statistical and Observation Comparison of Weyl-Type Models with the CDM Paradigm
- Parameterized Deceleration in Gravity: A Logarithmic Approach
- Revisiting kink-like parametrization and constraints using OHD/Pantheon+/BAO samples
- Testing Gauss-Bonnet Gravity with DESI BAO Data
- Observational Constraints on Chaplygin Gas Models in Non-Minimally Coupled Power Law Gravity with Quasars
- Physical Implications and Updated Observational Constraints of the PAge-like Unified Dark Fluid Model