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arXiv 0905.1446hep-th
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杨氏量子化时空代数中的全息关系和$D_0$膜气体系统中的面积熵关系

Holographic Relation in Yang's Quantized Space-Time Algebra and Area-Entropy Relation in $D_0$ Brane Gas System

Sho Tanaka

摘要:

在前文中,我们导出了洛伦兹协变杨氏量子化时空代数(YSTA)中的一种运动学全息关系(KHR)。它本质上反映了YSTA的非对易几何及其表示的基本性质,即与普通格点空间相比,空间自由度在运动学上有一定的减少。在此基础上,我们利用M理论的思想,导出了简单$D_0$膜气体系统在YSTA作用下的面积熵关系.进一步阐明了它与Schwarzschild黑洞的Bekenstein-Hawking面积熵关系的内在联系。

英文摘要:

In the preceding paper, we derived a kind of kinematical holographic relation (KHR) in the Lorentz-covariant Yang's quantized space-time algebra (YSTA). It essentially reflects the fundamental nature of the noncommutative geometry of YSTA and its representation, that is, a definite kinematical reduction of spatial degrees of freedom in comparison with the ordinary lattice space. On the basis of the relation and its extension to various spatial dimensions, we derive a new area-entropy relation in a simple $D_0$ brane gas system subject to YSTA, following the idea of M-theory. Furthermore, we make clear its inner relation with the Bekenstein-Hawking area-entropy relation in connection with Schwarzschild black hole.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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