AWhat changed
Constrains full temperature-dependent equilibrium spectra through reversible compression/Doppler reasoning, preserving a constant wavelength-temperature coordinate and appropriate spectral-density rescaling.
Scientific scope
Constrains full temperature-dependent equilibrium spectra through reversible compression/Doppler reasoning, preserving a constant wavelength-temperature coordinate and appropriate spectral-density rescaling. The displacement/scaling relation concerns the stated equilibrium blackbody radiation and thermodynamic argument. It does not determine the complete spectral function or guarantee a model for arbitrary nonequilibrium emitters. The later 1896 exponential spectral proposal and Planck’s law are separate contributions.
Evidence
Source-linked, scoped account of the original work. The published scope states the scientific assumptions and remaining verification limits. WRS has not independently certified the full proof, experimental result or system benchmark.
Contributors
- Wilhelm Wien · SCIENCE: Original source-listed scientific author of this scoped work; byline does not determine effort fractions.
- Wien, Eine neue Beziehung der Strahlung schwarzer Koerper zum zweiten Hauptsatz der Waermetheorie,1893
- Ci Nii scholarly bibliography: Wilhelm Wien,1893 Akademie 55-62
- Collected Einsteinpapers scholarly bibliography, selected Wien 1893/1894/1896 identities
Provisional WRS assessment, edition 2026-10-16.1. Independent expert calibration is pending. This grade does not certify correctness or assign ownership.
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