Abstract
The dynamical equations for black-body radiation are derived from the vanishing of the stress-energy tensor and shown to imply a theorem which generalizes that of Tolman and Ehrenfest[Phys. Rev. 36,1791 (1930)]. A method for finding the general solution of these equations is given.
Similar content being viewed by others
References
R. C. Tolman and P. Ehrenfest,Phys. Rev. 36, 1791 (1930).
J. Stachel,Phys. Rev. 180, 1256 (1969).
J. Stachel,J. Math. Phys. 21, 1776 (1980).
J. Stachel,Acta Phys. Polon. 35, 689 (1969).
Author information
Authors and Affiliations
Additional information
Dedicated to Nathan Rosen with the affection of the author.
Rights and permissions
About this article
Cite this article
Stachel, J. The dynamical equations of black-body radiation. Found Phys 14, 1163–1168 (1984). https://doi.org/10.1007/BF01889317
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF01889317