Thermodynamics of the Variable Modified Chaplygin gas
D. Panigrahi, S. Chatterjee

TL;DR
This paper investigates a new thermodynamically stable variant of the Chaplygin gas model, called Variable Modified Chaplygin Gas (VMCG), which can describe the universe's accelerated expansion and transition from big bang to big rip.
Contribution
It introduces a novel VMCG model with a parameter n that influences stability, showing it aligns with observations and obeys thermodynamic laws, unlike previous models.
Findings
VMCG can describe current accelerated expansion.
Parameter n must be negative for stability.
Model supports a smooth transition from big bang to big rip.
Abstract
A cosmological model with a new variant of Chaplygin gas obeying an equation of state(EoS), where is investigated in the context of its thermodynamical behaviour. Here and are constants and is the scale factor. We show that the equation of state of this `Variable Modified Chaplygin gas' (VMCG) can describe the current accelerated expansion of the universe. Following standard thermodynamical criteria we mainly discuss the classical thermodynamical stability of the model and find that the new parameter, introduced in VMCG plays a crucial role in determining the stability considerations and should always be \emph{negative.} We further observe that although the earlier model of Lu explains many of the current observational findings of different probes it fails the desirable tests of thermodynamical stability. We also…
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