Skip to content

ROOT Class to plot effects on energy resolution due to Doppler Broadening.

Notifications You must be signed in to change notification settings

ksmith0/DopplerBroadening

Repository files navigation

Doppler Broadening

The project provide the DopplerBroadening class as well as a simple method to create plots. This method can be envoked from root by the following:

.x DopplerBroadeningCalc.C(energyMeV, beta, dThetaDeg, resolutionConst, dBeta)

where the arguments are as follows:

  • energyMeV The energy of the emitted gamma-ray in MeV.
  • beta The fraction of the speed of light of incoming beam.
  • dThetaDeg The angular coverage of the detector in degrees.
  • resolutionConst The constant term in the 1/sqrt(e) resolution term.
  • dBeta The change in beta.

Further documentation is available at https://ksmith0.github.io/DopplerBroadening.

About

ROOT Class to plot effects on energy resolution due to Doppler Broadening.

Resources

Stars

Watchers

Forks

Releases

No releases published

Packages

No packages published