Material for speakers: Difference between revisions
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Vincenzo Cirigliano, Ryuichiro Kitano, Yasuhiro Okada, and Paula Tuzon, Phys. Rev. D 80, 013002 (2009)
PIP-II public web site
E. Pozdeyev, Rare Processes and Precision Frontier Town Hall (2020)
[3] "Pion-production target design for Mu2e-II: status update" 1st Muon Community Meeting (2021)
[4] "Early considerations for muon collider targetry at CERN"
"Design and studies for the Mu2e-II tracker", DPF 2021 [5]
COMET tracker (2020 NIM) [6]
COMET tracker (2016 slides) [7]
[8] "A Novel Scintillator Detector for the Mu2e-II Experiment and a Muon Tomography Probe of the Interior of the Great Pyramid"
[9] Muon-ion collider for BNL (2021)
[10] Mu2e-II Snowmass 22 Letter of Interest (2020)
[11] 1st muon community meeting (CERN), 20-21 May 2020
[12] Mu2e-II theory Snowmass 22 Letter of Interest (2020)
[13] COMET Phase-I TDR (2020)
[14] Muon colliders (2019)
[15] Mu2e-II Expression of Interest (2018)
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<div><ul> | <div><ul> | ||
<li style="display: inline-block; vertical-align: top;"> [[File:TrackerResolutionRequirement.png|thumb|top|Slide illustrating the requirement on track resolution for Mu2e-II compared with Mu2e. | <li style="display: inline-block; vertical-align: top;"> [[File:TrackerResolutionRequirement.png|thumb|top|Slide illustrating the requirement on track resolution for Mu2e-II compared with Mu2e. | ||
Note 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 | 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.]] </li> | values of <math>R_{\mu e}</math> indicated in the legends.]] </li> |
Revision as of 16:04, 27 July 2021
Mu2e
Mu2e public results and material for speakers
Theory
References
PIP-II accelerator
Beamline
Production target
Production solenoid
Tracking
References
Calorimeter
Cosmic Ray Veto
The Mu2e-II Cosmic Ray Veto will need to cope with roughly a factor 3 higher instantaneous rates from accelerator compared with Mu2e as well as a factor of three higher live time (i.e., cosmic rays), because of the higher duty factor for Mu2e-II compared with Mu2e.