Negativity of the Casimir Self-Entropy in Spherical Geometries

被引:4
|
作者
Li, Yang [1 ]
Milton, Kimball A. [2 ]
Parashar, Prachi [3 ]
Hong, Lujun [4 ]
机构
[1] Nanchang Univ, Dept Phys, Nanchang 330031, Jiangxi, Peoples R China
[2] Univ Oklahoma, Homer L Dodge Dept Phys & Astron, Norman, OK 73019 USA
[3] John A Logan Coll, Carterville, IL 62918 USA
[4] Nanchang Univ, Inst Space Sci & Technol, Nanchang 330031, Jiangxi, Peoples R China
基金
美国国家科学基金会;
关键词
Casimir free energy; entropy; Abel– Plana formula;
D O I
10.3390/e23020214
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
It has been recognized for some time that, even for perfect conductors, the interaction Casimir entropy, due to quantum/thermal fluctuations, can be negative. This result was not considered problematic because it was thought that the self-entropies of the bodies would cancel this negative interaction entropy, yielding a total entropy that was positive. In fact, this cancellation seems not to occur. The positive self-entropy of a perfectly conducting sphere does indeed just cancel the negative interaction entropy of a system consisting of a perfectly conducting sphere and plate, but a model with weaker coupling in general possesses a regime where negative self-entropy appears. The physical meaning of this surprising result remains obscure. In this paper, we re-examine these issues, using improved physical and mathematical techniques, partly based on the Abel-Plana formula, and present numerical results for arbitrary temperatures and couplings, which exhibit the same remarkable features.
引用
收藏
页码:1 / 11
页数:11
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