Changes

Here, Δλ denotes the difference between the wavelengths  of the incoming and the scattered ray, while θ is the angle of scattering.

Here, Δλ denotes the difference between the wavelengths  of the incoming and the scattered ray, while θ is the angle of scattering.

The probability for Compton scattering is approximately proportional to the [[atomic number]] Z, and for energies greater than 500 [[keV]] approximately proportional to <math>\frac{1}{E^\gamma}</math><ref>{{cite web|url=http://ie.lbl.gov/education/glossary/glossaryf.htm|title=Glossary of Nuclear Science Terms|accessdate=January 10, 2013}}</ref>, the energy of the gamma ray [[photon]].

The probability for Compton scattering is approximately proportional to the [[atomic number]] Z, and for energies greater than 500 [[keV]] approximately proportional to <math>\frac{1}{E^\gamma}</math>,<ref>{{cite web|url=http://ie.lbl.gov/education/glossary/glossaryf.htm|title=Glossary of Nuclear Science Terms|accessdate=January 10, 2013}}</ref> the energy of the [[gamma ray]] [[photon]].

== Reference ==

== Reference ==

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[[category:physics]]

[[category:physics]]