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)
Marciano, William J. and Mori, Toshinori and Roney, J. Michael, Charged Lepton Flavor Violation Experiments, Annual Review of Nuclear and Particle Science, 58 (2008) 315-341.
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)
[16] Charged Lepton Flavor Violation Experiments (2008)
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<li> [https://journals.aps.org/prd/abstract/10.1103/PhysRevD.80.013002 Vincenzo Cirigliano, Ryuichiro Kitano, Yasuhiro Okada, and Paula Tuzon, Phys. Rev. D 80, 013002 (2009)] | <li> [https://journals.aps.org/prd/abstract/10.1103/PhysRevD.80.013002 Vincenzo Cirigliano, Ryuichiro Kitano, Yasuhiro Okada, and Paula Tuzon, Phys. Rev. D 80, 013002 (2009)] | ||
<li> Marciano, William J. and Mori, Toshinori and Roney, J. Michael, Charged Lepton Flavor Violation Experiments, Annual Review of Nuclear and Particle Science, 58 (2008) 315-341. | |||
=PIP-II accelerator= | =PIP-II accelerator= |
Revision as of 20:59, 10 August 2021
Mu2e
Mu2e public results and material for speakers
Theory
We measure
[math]\displaystyle{ \begin{equation} R_{\mu e} \equiv \frac{\Gamma(\mu^-N(A,Z)\to e^-N(A,Z)}{\Gamma(\mu^-N(A,Z)\to \nu_\mu N(A,Z-1)^*)}. \end{equation} }[/math] In the standard model, this is very small. On aluminum it is estimated to be [math]\displaystyle{ \begin{equation} R(\mu^-\hbox{Al}\to e^- \hbox{Al}) \sim 2\times10^{-52}\frac{\sin^2\theta_{13}}{0.15}. \end{equation} }[/math]
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.