Four Roads to the neutrino magnetic moment - PowerPoint PPT Presentation

About This Presentation
Title:

Four Roads to the neutrino magnetic moment

Description:

Origin of the Magnetic Moment. Actually, the 'effective moment' ... c.f.: Miranda, Segura, Semikoz, and Valle, hep-ph/9906328. Calculation of e cross section ... – PowerPoint PPT presentation

Number of Views:51
Avg rating:3.0/5.0
Slides: 11
Provided by: wwwd
Category:

less

Transcript and Presenter's Notes

Title: Four Roads to the neutrino magnetic moment


1
Four Roads to the neutrino magnetic moment
  • Traditional ? e cross section
  • Cerenkov Radiation
  • Transition Radiation
  • Resonant Cavities

2
Origin of the Magnetic Moment
  • Actually, the effective moment µeff
    (µ2d2)1/2
  • also R-parity violating SUSY
  • limited to lt10-10 µB expected 109 smaller yet
  • If neutrinos are massive, then to first order, µ
    linearly dependent on neutrino mass (?)

c.f. Lee and Shrock,PRD 16 1444 (1977)or
Marciano and
Sanda,Phys Lett 67B 303 (1977)
3
Road OneThe ? e cross section
c.f. Miranda, Segura, Semikoz, and Valle,
hep-ph/9906328
  • Traditional approach followed by NuMu, HELLAZ,
    etc. SM EM

4
Calculation of ? e cross section
  • High neutrino E does not help
  • Quadratic dependence on mag moment
  • Need a dedicated detectoryet cant do much
    better than others

5
Road 2Cerenkov Radiation
  • K.McF. 1 km long water tank
  • Quadratic in µ
  • Numerical calculation for 2E20 0.00033 photons
    per year

c.f. Grimus and Neufeld,Phys Lett B315 129 (1993)
6
Road 3Transition Radiation
  • From solar neutrino calculationsc.f. Grimus and
    Neufeld hep-ph 9410245
  • Still quadratic in µ
  • Numerical calculation for 2E20, 1E6 foils4.5E-5
    X-ray photons per year This is a hard
    calculation!The conversion factors are not
    smallnonetheless this should be the final
    answer for given input

Several approximations here
7
Small Adjustments, big gains?
  • Small gains from ?p in standard materials. (?)We
    dont have the usual limits a TRD would
    have.Still prefer to avoid X-ray attenuation
    i.e. high Z materials.
  • Lowering X-ray detection threshold from 20 keVto
    5 keV gives you a factor of 100 but low
    efficiency in real detectors
  • Originally I was looking at a big reactor2
    meters away I think I still am.

8
Road 4The Resonant Cavity
Thanks Fritz DeJongh C.f. Vannucci, hep-ex
9911025
  • Essentially a low-energy photon target
  • Stimulate radiative decays
  • Rotate neutrinos to sterile statesby
    introducing a relative phase to the helicity
    componentsthus reducing the event rate at a
    detector when the cavity is powered-up.
  • NOT quadratic in µ!

I havent thoughtabout this yet
9
Resonant Cavity the only remaining option?
  • Its at least as attractive as the others!
  • There exists a CERN proposal for this
    one.(Vanucci Achievable limits)
  • Does not require a dedicated detector
  • Detector systematics cancel

10
Four Difficult Roads
  • I recommend the traditional search only if it
    comes for free.
  • Cerenkov is out
  • TR looks bad, at least at NuFact Any
    ideas are welcome!
  • More to come on ResCav
Write a Comment
User Comments (0)
About PowerShow.com