Material for speakers: Difference between revisions
Jump to navigation
Jump to search
| Line 10: | Line 10: | ||
=Tracking= | =Tracking= | ||
[[File:TrackerResolutionRequirement.png|thumb|Slide illustrating the requirement on track resolution for Mu2e-II compared with Mu2e. | [[File:TrackerResolutionRequirement.png|thumb|Slide illustrating the requirement on track resolution for Mu2e-II compared with Mu2e. | ||
| Line 15: | Line 16: | ||
electron spectrum from muon decays in orbit (DIOs). The red curves show the conversion electron spectrum for the | electron spectrum from muon decays in orbit (DIOs). The red curves show the conversion electron spectrum for the | ||
values of <math>R_{\mu e}</math> indicated in the legends.]] | values of <math>R_{\mu e}</math> indicated in the legends.]] | ||
[[File:AmbroseCPAD_Mu2e_Tracker_18.jpg|100px]] | |||
=Calorimeter= | =Calorimeter= | ||
=Cosmic Ray Veto= | =Cosmic Ray Veto= | ||
Revision as of 17:32, 16 June 2021
Mu2e
Mu2e public results and material for speakers
PIP-II accelerator
Production target
Tracking
Slide illustrating the requirement on track resolution for Mu2e-II compared with Mu2e. Noe that the resolution has contributions from several sources. The blue dashed curve on each plot indicates the electron spectrum from muon decays in orbit (DIOs). The red curves show the conversion electron spectrum for the values of [math]\displaystyle{ R_{\mu e} }[/math] indicated in the legends.
Error creating thumbnail: File with dimensions greater than 12.5 MP