Where Does Black Hole Entropy Lie? Some Remarks on Area-Entropy Law, Holographic Principle and Noncommutative Space-Time
Sho Tanaka

TL;DR
This paper explores how noncommutative space-time frameworks, like Yang's quantized space-time, provide a foundational basis for the area-entropy law of black holes and the holographic principle, linking geometry with quantum gravity.
Contribution
It introduces a Kinematical Holographic Relation in noncommutative space-time that explains the area-entropy law and connects black hole thermodynamics with quantum geometry.
Findings
KHR establishes a proportional relation between degrees of freedom and boundary area.
Supports a new area-entropy law based on noncommutative geometry.
Links black hole thermodynamics with noncommutative space-time concepts.
Abstract
In confrontation with serious and fundamental problems towards ultimate theory of quantum gravity and physics of Planck scale, we emphasize the importance of underlying noncommutative space-time such as Snyder's or Yang's Lorentz-covariant quantized space-time. The background of Bekenstein-Hawking's Area-entropy law and Holographic principle is now substantially understood in terms of {\it Kinematical} Holographic Relation [KHR], which holds in Yang's quantized space-time as the result of the kinematical reduction of spatial degrees of freedom caused by its own nature of noncommutative geometry. [KHR] implies a definite proportional relation, , between the number of spatial degrees of freedom inside of any dimensional spherical volume with radius and its boundary area It yields a…
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