Material for speakers

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Mu2e

Mu2e public results and material for speakers

Theory

  • Z dependence of µ → e conversion rates for some sample scenarios [1].
  • Tail of the electron spectrum for DIOs and for two [math]\displaystyle{ \mu\to eX }[/math] scenarios [2].

References

  • Vincenzo Cirigliano, Ryuichiro Kitano, Yasuhiro Okada, and Paula Tuzon, Phys. Rev. D 80, 013002 (2009)

    PIP-II accelerator

    • PIP-II Pozdeyev 7 4MP.png
    • PIP-II Pozdeyev 9 4MP.png
    • PIP-II Pozdeyev 10 4MP.png
    • PIP-II Pozdeyev 15 4MP.png
    • PIP-II Pozdeyev 16 4MP.png
    • PIP-II Pozdeyev 17 MP.png


    References

  • PIP-II public web site
  • E. Pozdeyev, Rare Processes and Precision Frontier Town Hall (2020)

    Beamline

    Production target

    • ProductionTargetRotatingRodsWcaption-IPAC214MP.png
    • ProductionTargetDesignsFixedGranular4MP-IPAC21.png
    • ProductionTargetDesignsConveyor4MP-IPAC21.png
    • ComparisonTable4MP-IPAC21.png
    • BallDeformation.png
    • HRScaptioned.png

    References

  • [3] "Pion-production target design for Mu2e-II: status update"
  • [4] "Early considerations for muon collider targetry at CERN"
  • Production solenoid

    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.
    • AmbroseCPAD Mu2e Tracker 184MP.jpg
    • AmbroseCPAD Mu2e Tracker 19.png
    • AmbroseCPAD Mu2e Tracker 20.png

    References

  • COMET tracker (2020 NIM) [5]
  • COMET tracker (2016 slides) [6]
  • Calorimeter

    • Effect of yttrium doping on suppressing the slow component in BaF[math]\displaystyle{ _2 }[/math]
    • Hitlin CPAD 210318- Page 05MP.png
    • Hitlin CPAD 210318 Page 26 4MP.png
    • Hitlin CPAD 210318 Page 274MP.png
    • Hitlin CPAD 210318 Page 28 4MP.png

    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.

    • Crv seminar dpf 2021 16 4MP.png
    • Crv seminar dpf 2021 17 4MP.png
    • Crv seminar dpf 2021 18 4MP.png

    References

  • [7] "A Novel Scintillator Detector for the Mu2e-II Experiment and a Muon Tomography Probe of the Interior of the Great Pyramid"
  • Sensitivity

    References

  • [8] Muon-ion collider for BNL (2021)
  • [9] Mu2e-II Snowmass 22 Letter of Interest (2020)
  • [10] 1st muon community meeting (CERN), 20-21 May 2020
  • [11] Mu2e-II theory Snowmass 22 Letter of Interest (2020)
  • [12] COMET Phase-I TDR (2020)
  • [13] Muon colliders (2019)
  • [14] Mu2e-II Expression of Interest (2018)