Material for speakers: Difference between revisions
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PIP-II public web site
[3] "Early considerations for muon collider targetry at CERN"
COMET tracker (2020 NIM) [4]
COMET tracker (2016 slides) [5]
[6] "A Novel Scintillator Detector for the Mu2e-II Experiment and a Muon Tomography Probe of the Interior of the Great Pyramid"
[7] Muon-ion collider for BNL (2021)
[8] Mu2e-II Snowmass 22 Letter of Interest (2020)
[9] 1st muon community meeting (CERN), 20-21 May 2020
[10] Mu2e-II theory Snowmass 22 Letter of Interest (2020)
[11] COMET Phase-I TDR (2020)
[12] Muon colliders (2019)
[13] Mu2e-II Expression of Interest (2018)
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=PIP-II accelerator= | =PIP-II accelerator= | ||
[https://pip2.fnal.gov/ PIP-II public web site] | <div><ul> | ||
<li style="display: inline-block; vertical-align: top;"> [[File:PIP-II Pozdeyev 7 4MP.png|thumb|top]] </li> | |||
</ul> | |||
==References== | |||
<li> [https://pip2.fnal.gov/ PIP-II public web site] | |||
=Beamline= | =Beamline= |
Revision as of 22:28, 16 July 2021
Mu2e
Mu2e public results and material for speakers
Theory
PIP-II accelerator
References
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.