Wien's approximation (also sometimes called Wien's law or the Wien distribution law) is a law of physics used to describe the spectrum of thermal radiation (frequently called the blackbody function). This law was first derived by Wilhelm Wien in 1896. The equation does accurately describe the short wavelength (high frequency) spectrum of thermal emission from objects, but it fails to accurately fit the experimental data for long wavelengths (low frequency) emission.
The law may be written as
This equation may also be written as
Relation to Planck's lawEdit
The Wien approximation was originally proposed as a description of the complete spectrum of thermal radiation, although it failed to accurately describe long wavelength (low frequency) emission. However, it was soon superseded by Planck's law, developed by Max Planck. Unlike the Wien approximation, Planck's law accurately describes the complete spectrum of thermal radiation. Planck's law may be given as
The Wien approximation may be derived from Planck's law by assuming . When this is true, then
and so Planck's law approximately equals the Wien approximation at high frequencies.
Other approximations of thermal radiationEdit
The Rayleigh-Jeans law developed by Lord Rayleigh may be used to accurately describe the long wavelength spectrum of thermal radiation but fails to describe the short wavelength spectrum of thermal emission.
- ↑ J. Mehra, H. Rechenberg (1982). "1". The Historical Development of Quantum Theory. 1. New York: Springer-Verlag. ISBN 0-387-90642-8.
- ↑ 2.0 2.1 2.2 2.3 R. Bowley, M. Sánchez (1999). Introductory Statistical Mechanics (2nd edition ed.). Oxford: Clarendon Press. ISBN 0-19-850576-0.
- ↑ 3.0 3.1 3.2 3.3 G. B. Rybicki, A. P. Lightman (1979). Radiative Processes in Astrophysics. New York: John Wiley & Sons. ISBN 0-471-82759-2.
- ↑ Equation derived using u=4π/c; see Rybicki, Lightman (1979) reference.