Beyond the Formulations of the Fluctuation Dissipation Theorem Given by Callen and Welton (1951) and Expanded by Kubo (1966)

被引:4
作者
Reggiani, Lino [1 ]
Alfinito, Eleonora [2 ]
机构
[1] Univ Salento, Dipartimento Matemat & Fis Ennio de Giorgi, Lecce, Italy
[2] Univ Salento, Dipartimento Ingn Innovaz, Lecce, Italy
关键词
fluctuation dissipation theorem; Casimir effect; noise; vacuum fluctuations; zero-point energy; Stefan-Boltzmann law;
D O I
10.3389/fphy.2020.00238
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The quantum formula of the fluctuation dissipation theorem (FDT) was given by Callen and Welton in 1951 [1] for the case of conductors, and then expanded by Kubo in 1966 [2,3]. The drawback of these quantum relations concerns with the appearance of a zero-point contribution,h omega/2 withhthe reduced Planck constant and omega the angular frequency of the considered photon, which implies a divergence of the fluctuation spectrum at increasing frequencies. This divergence is responsible for a vacuum-catastrophe, to keep the analogy with the well-known ultraviolet catastrophe of the classical black-body radiation spectrum. As a consequence, the quantum formulation of the FDT as given by Callen-Welton and Kubo introduces a Field Grand Challenge associated with the existence or less of a vacuum-fluctuations catastrophe for the energy-density spectrum. Here we propose a solution to this challenge by taking into account of the Casimir energy that, in turns, is found to be responsible for a quantum correction of the Stefan-Boltzmann law.
引用
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页数:4
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