Emergence of cosmic space and horizon thermodynamics in the context of the quantum-deformed entropy
Jianming Chen, Gerui Chen

TL;DR
This paper explores how q-deformed entropy influences the emergence of cosmic space and horizon thermodynamics, deriving modified Friedmann equations and linking entropy maximization with the law of emergence in the universe.
Contribution
It introduces a q-deformed entropy framework into cosmology, deriving corresponding Friedmann equations and connecting entropy maximization with the universe's emergence law.
Findings
Derived Friedmann equations from q-deformed entropy and thermodynamics.
Established the connection between the law of emergence and entropy maximization.
Showed consistency of the q-deformed entropy approach with cosmic evolution.
Abstract
According to the quantum deformation approach to quantum gravity, the thermodynamical entropy of a quantum-deformed (q-deformed) black hole with horizon area established by Jalalzadeh is expressed as , where is the q-deformation parameter, denotes the Planck length, and denotes the quantum-deformed cosmic apparent horizon distance. In this paper, assuming that the q-deformed entropy is associated with the apparent horizon of the Friedmann-Robertson-Walker (FRW) universe, we derive the Friedmann equation from the unified first law of thermodynamics, . And this one obtained is in line with the Friedmann equation derived from the law of emergence proposed by Padmanabhan. It clearly shows the connection between the law of…
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Taxonomy
TopicsCosmology and Gravitation Theories · Advanced Thermodynamics and Statistical Mechanics · Earth Systems and Cosmic Evolution
