Linked from

The 14 pages that link to Wien's displacement law, each with the reason it gives.

• Thermal radiationRelated: It predicts how the emission peak shifts as matter heats or cools.

• Black-body radiationRelated: It tracks how the spectrum's peak shifts as the emitter heats.

• Color temperatureRelated: It summarizes why hotter blackbodies appear bluer, though color depends on the full spectrum.

• Planck's lawBroader topic: It follows from Planck's spectrum and locates its wavelength peak.

• Stefan–Boltzmann lawRelated: It tracks where emission peaks, while Stefan–Boltzmann gives the integrated total.

• Ultraviolet catastropheRelated: It captures the spectrum’s temperature-dependent peak, distinct from the high-frequency divergence.

• Kirchhoff's law of thermal radiationCompared with: It predicts a spectral peak, whereas Kirchhoff's law equates emission and absorption.

• Rayleigh–Jeans lawCompared with: It concerns the spectrum’s peak, where the Rayleigh–Jeans approximation generally fails.

• Spectral energy distributionRelated: The peak location offers a compact clue to the temperature behind a thermal distribution.

• Wien approximationCompared with: It is a separate result often confused with the high-frequency spectral approximation.

• Wilhelm WienBroader topic: This is Wien’s best-known result and the basis of his 1911 Nobel Prize.

• Black bodyRelated: It shows how heating shifts the black body's spectrum toward shorter wavelengths.

• Stefan–Boltzmann constantCompared with: It predicts spectral peak location, whereas σ governs total emitted power.

• Infrared techniquesRelated: It explains why warmer objects radiate most strongly at shorter infrared wavelengths.