Periodicity, Thermal Effects, and Vacuum Force: Rotation in Random Classical Zero-Point Radiation
Yefim Semenovitch Levin

TL;DR
This paper demonstrates that a detector rotating in a classical zero-point field experiences thermal effects similar to a temperature proportional to its angular velocity, and introduces a vacuum force that influences the rotation, with implications for confinement and asymptotic freedom.
Contribution
It reveals thermal effects and vacuum forces for rotating detectors in classical zero-point fields, linking rotation, thermal spectra, and vacuum forces to phenomena like confinement.
Findings
Rotating detectors observe a thermal spectrum proportional to rotation speed.
Vacuum force on the detector depends on radius and diverges at a critical radius.
The vacuum force behavior suggests a connection to confinement and asymptotic freedom.
Abstract
We show that for a detector rotating in a random classical zero-point electromagnetic or massless scalar field at T=0 thermal effects exist. The rotating reference system is constructed as an infinite set of Frenet-Seret tetrads defined so that the detector is at rest in a tetrad at each proper time. Correlation functions, more exactly their frequency spectrum, contain the Planck thermal factor, and the energy density the rotating detector observes is proportional to the sum of energy densities of Planck's spectrum at the temperature T_rot = \hbar \Omega / (2 \pi k_B) and zero-point radiation. The proportionality factor is (2/3)(4\gamma^2 - 1) for an electromagnetic field and (2/9)(4\gamma^2 - 1) for a massless scalar field, where \gamma = (1 - (\Omega r/c)^2)^(-1/2), and r is a detector rotation radius. The origin of these thermal effects is the periodicity of the correlation functions…
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Taxonomy
TopicsQuantum Electrodynamics and Casimir Effect · Cosmology and Gravitation Theories · Advanced Thermodynamics and Statistical Mechanics
