Why zero-point quantum noise cannot be detected at thermal equilibrium: Casimir force and zero-point contribution in the fluctuation-dissipation theorem
Lino Reggiani, Eleonora Alfinito

TL;DR
This paper argues that zero-point quantum noise cannot be detected at thermal equilibrium because the Casimir force is balanced by the system's mechanical reaction, aligning observed noise spectra with classical predictions rather than quantum vacuum fluctuations.
Contribution
It demonstrates that at thermal equilibrium, zero-point fluctuations are effectively unobservable due to mechanical balancing, challenging the necessity of quantum noise in fluctuation-dissipation theorem.
Findings
Zero-point spectrum is unobservable at thermal equilibrium.
Casimir force is balanced by mechanical reaction, preventing detection of quantum noise.
Experimental validation aligns with the classical Planck spectrum, not quantum vacuum fluctuations.
Abstract
The role played by zero-point contribution, also called quantum noise or vacuum fluctuations, in the quantum expression of the fluctuation-dissipation theorem (FDT) is a long-standing open problem widely discussed by the physicist community since its announcement by Callen and Welton pioneer paper of 1951 [1]. From one hand, it has the drawbacks of: (i) the expectation value of its energy is infinite, (ii) it produces an ultraviolet catastrophe of the noise power spectral density and, (iii) it lacks of an experimental validation under thermal equilibrium conditions. From another hand, by imposing appropriate boundary conditions and eliminating divergences by regulation techniques, vacuum fluctuations are the source of an attractive force between opposite conducting plates, firstly predicted by Casimir in 1948 [2] and later validated experimentally with increasing accuracy. As a…
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Taxonomy
TopicsQuantum Electrodynamics and Casimir Effect · Advanced Thermodynamics and Statistical Mechanics · Cosmology and Gravitation Theories
