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OPTICAL/PHOTONIC BANDWIDTH Definition: the width of some frequency or wavelength range In photonics, the term bandwidth occurs with a variety of meanings: The bandwidth, or line width = width of the intensity spectrum of the output of some light source—that is, a super luminescent source or a laser; the bandwidth of ultra‒short pulses can be particularly large The width of the frequency range which can be transmitted by some element, e. g. an optical fiber The gain bandwidth of an optical amplifier the width of the range of some other phenomenon, such as a reflection, the phase matching of a nonlinear process—→ phase-matching bandwidth—, or some resonance the maximum modulation frequency—or range of modulation frequencies—of an optical modulator Optical bandwidth values may be specified in terms of frequency or wavelength due to the inverse relationship of frequency and wavelength. The conversion factor between gigahertz and nanometres depends on the centre wavelength or frequency. For converting a—small—wavelength interval into a frequency interval, the equation can be used. This shows that 1 nm is worth more gigahertz if the centre wavelength is shorter. The term bandwidth is also often used for the data rate—that is, in Gigabytes per seconds achieved in an optical communication system. Precisely, the data rate is limited by the optical bandwidth, but is not really itself a bandwidth. The optical bandwidth of a light source is strongly related to the temporal coherence, characterized with the coherence time. Both for passive resonators—that is, optical cavities and for the output of oscillators —that is, lasers, the Q factor is the oscillation frequency divided by the bandwidth. See also: time–bandwidth product, gain bandwidth, coherence time, transform limit, Q factor, phase-matching bandwidth Category: physical foundations