Abstract
An implementation of fast simulation models provided by the GEANT4 package for the description of X-ray transition radiation (XTR) produced by a relativistic charged particle in a multi layered medium is discussed. The implementation allows us to calculate the number of XTR photons, their energy and angular spectra in a number of XTR radiators of practical interest. Ionisation produced by the relativistic particle and the XTR photons are also described in terms of fast parameterisation. Comparison of simulation with experimental data from gaseous detectors is presented.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
