Symmetries and Thermal Radiation: A Classical Derivation of the Planck Spectrum
Timothy H. Boyer

TL;DR
This paper presents a classical, relativistic derivation of the Planck spectrum for thermal radiation based on wave fluctuations and zero-point radiation, emphasizing the importance of Lorentz invariance.
Contribution
It offers a novel classical derivation of the Planck spectrum using relativistic wave theory and zero-point fluctuations, contrasting with nonrelativistic approaches.
Findings
Classical zero-point radiation exists only in relativistic theories.
The derivation relies on frame-independent thermal fluctuations.
A Lorentz-covariant classical theory can reproduce the Planck spectrum.
Abstract
A derivation of the Planck spectrum for thermal radiation is given based upon wave fluctuations within relativistic classical physics. The derivation depends crucially on thermal fluctuations existing above the fundamental inertial-frame-independent fluctuations of classical zero-point radiation. Such frame-independent zero-point fluctuations exist only in a relativistic wave theory and cannot exist in a nonrelativistic wave theory. Thus such a classical derivation of the Planck spectrum exists in a Lorentz-covariant classical theory, such as classical electrodynamics, but not in a Galilean-covariant theory where all waves are based upon material media. Classical zero-point radiation provides a purely classical alternative to quanta in the analysis of the Planck spectrum.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAdvanced Thermodynamics and Statistical Mechanics · Quantum Mechanics and Applications · Advanced Mathematical Theories and Applications
