The Blackbody Radiation Spectrum Follows from Zero-Point Radiation and the Structure of Relativistic Spacetime in Classical Physics
Timothy H. Boyer

TL;DR
This paper demonstrates that the Planck blackbody radiation spectrum can be derived from classical zero-point radiation and the structure of relativistic spacetime, without quantum mechanics, using conformal symmetry and acceleration effects.
Contribution
It shows how the blackbody spectrum emerges from classical zero-point radiation through conformal transformations in relativistic spacetime, linking acceleration and thermal radiation.
Findings
Blackbody spectrum derived from classical zero-point radiation.
Conformal symmetry relates zero-point and thermal radiation.
Acceleration in spacetime leads to thermal radiation in classical physics.
Abstract
The analysis of this article is entirely within classical physics. Any attempt to describe nature within classical physics requires the presence of Lorentz-invariant classical electromagnetic zero-point radiation so as to account for the Casimir forces between parallel conducting plates at low temperatures. Furthermore, conformal symmetry carries solutions of Maxwell's equations into solutions. In an inertial frame, conformal symmetry leaves zero-point radiation invariant and does not connect it to non-zero-temperature; time-dilating conformal transformations carry the Lorentz-invariant zero-point radiation spectrum into zero-point radiation and carry the thermal radiation spectrum at non-zero temperature into thermal radiation at a different non-zero-temperature. However, in a non-inertial frame, a time-dilating conformal transformation carries classical zero-point radiation into…
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