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Spectral linewidth
From Wikipedia, the free encyclopedia
The spectral linewidth characterizes the width of a spectral line, such as in the electromagnetic emission spectrum of an atom, or the frequency spectrum of an acoustic or electronic system. For example, the emission of an atom usually has a very thin spectral linewidth, as only transitions between discrete energy levels are allowed, leading to emission of photons with a certain energy.
Several definitions are used to quantify the spectral linewidth, e.g. the Full width at half maximum (FWHM).
While the spectral width of a resonator in electronics depends on the parameters of the components, and therefore can be easily adjusted over a wide range, linewidths are typically more difficult to adjust in physics. For example, even a resting atom which does not interact with its environment has a non-zero linewidth, called the natural linewidth, which is a consequence of the transform limit (classical description) and the Heisenberg uncertainty principle (quantum mechanical description, ΔE·Δt=ħ/2). As is clear from the latter discription, this linewidth can be adjusted only to the extent that the transition rates can be suppressed or enhanced.
- Spectral lines in optics. (This article also includes a list of sources of linewidth broadening.)
- Q factor and linewidths in electronics, acoustics and optics
- Spectral width in telecommunications
- Doppler broadening, one source of linewidth broadening