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Encyclopedia > Radiative recombination

Radiative recombination is a term used for an electron falling from a high energy orbital into a lower one via the simultaneous emission of a photon.


See Britney's Guide to Semiconductor Physics (http://britneyspears.ac/physics/radiative/radiative.htm) for more info.


  Results from FactBites:
 
Recombination data (283 words)
Radiative recombination rates for H-like, He-like, Li-like and Na-like ions over a broad range of temperature.
We present new calculations and analytic fits to the rates of radiative recombination towards H-like, He-like, Li-like and Na-like ions of all elements from H through Zn (Z=30).
Recombination line intensities for hydrogenic ions: the fine structure components of HI and HeII.
2.11 Carrier generation and recombination (1500 words)
Recombination of electrons and holes is a process by which both carriers annihilate each other: the electrons fall in one or multiple steps into the empty state which is associated with the hole.
Band-to-band recombination occurs when an electron falls from its state in the conduction band into the empty state in the valence band which is associated with the hole.
Recombination in a depletion region and in situations where the hole and electron density are close to each other can not be described with the simple model and the more elaborate expressions for the individual recombination mechanisms must be used.
  More results at FactBites »


 

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