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Search for L epton F lavor V iolation in the m + N -> t + N conversion (preliminary). S.N. Gninenko INR, Moscow. SPSC meeting, Villars, September 22-28, 2004. Outline. Introduction m +N-> t +N conversion Choice of signature Experimental setup - PowerPoint PPT Presentation
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SPSC, Villars, September 22-28, 2004 S.N.Gninenko
Search for Lepton Flavor Violation in the + N -> + N conversion
(preliminary)
S.N. Gninenko INR, Moscow
SPSC meeting, Villars, September 22-28, 2004
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
Outline
Introduction +N->+N conversion Choice of signature Experimental setup Signal/Background simulations Results Summary
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
Introduction
SuperK'98 result: u and/or are not massless, u-mixing is large. First observation of the LFV process with neutral leptons. SM has no LFV: New physics. Suggests LFV for associated –leptons
LFV involving charged leptons has never been observed. In many models LVF is natural - SUSY - Left-Right Symmetric Model - Top seesaw, - Extra dimensions - Higgs mediated LFV
In some models LFV processes for tau are enhanced over muon processes
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
Experimental Limits on LFV
Future Plans
BNL:-+Al->e-+Al < 10-16
PSI: -->e-+< 10-14
J- Parc : -->e- < 10-18
For sectorlimits are quite modest
Focus on -e sector:
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
Why + N -> + N ?
Inverse process + N->+N is possible for muon energy E> ~3 GeV at p or n.
s it interesting? Gninenko at el.(2002), Sher & Turan. (2004)
More theoretical attention is required compare to +A->e+A
The similar experiment to search for +A->+A would be very interesting, but too short -lifetime (< 0.3 ps) makes it unrealistic.
What is the +A->e+A conversion?
capture
target
stop
atom g.s.
conversion
e ~105 MeV
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
Phenomenology
c : week limit on for ()(u c)
enhances motivation to search for conversion emphasizes need to test LFV in both rare decays and in conversion at high energies
Note: Br->. . .-1/4
1/2() (qq)
q q’
Limits on Black et al.
S PS V A
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
Cross section for DIS + N -> + N
Vector
=2.6 TeV
=12 TeV
Scalar
cross section is model dependent
S cross section is ~ 1fb at ~100 GeV
V cross section is suppressed by the limit on ~1/4
primary muon energy should be more than ~20 GeV
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
Rate estimate for + N -> + N
muon energy E=100 GeV cross section fb muon integral flux N =10 15
target length L = 100 cm target density ~10 g/cm3, e.g. PWO crystals branching ratio Br(->..) ~ 17 %e efficiency ~100 %
N = NL N ABr(->..)
For ()(u c) N ->
could be much higher
For ()(q q), q=u,dN= 120 events
Target
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
+ N -> + N: Choice of the Signature DIS: + N -> +X (e, h, ..)
• for any decay mode, the photoproduction is the main source of background, • complicated final state and analysis• many possibilities for background
quasi-elastic (QE) + N -> + N’, and/or coherent + A-> + A (?)
• two-body reaction,• low momentum transfer• smaller cross sections• enhancement for coherent • monoenergetic • small energy of N’ or N* , < ~ 1 GeV
So farSo far Signature:Signature:
• single single
• large missing Elarge missing E
• missing Ptmissing Pt
• small Esmall ETARGETTARGET
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
Comment on background
If detector is hermetic- leakages are mostly due to X
neutrino decays: X -> + L
(associated lepton, LF conservation !).
If neutrino energy is ~a few 10s GeV, small E L from X ->
+ L is very unlikely.
High suppression of photoproduction.
Week reactions are another source of background,
N
L
100 GeV <50 GeV
>50 GeV of missing E
X
Large missing energy is one of the keys,good hermiticity is important
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
high rate capability: simple design
active target with low energy threshold
hermetic (good ~4 coverage) detector
electromagnetic & hadronic calorimeter energy resolution, granularity
high in/out going muon momentum resolution
particles ID
Experimental Setup
Signature:Signature:
• single single
• large missing large missing EE
• missing Ptmissing Pt
• small Esmall ETARGETTARGET
• no Eno EHCALHCALHermiticity might confront precision measurements
HCAL
ECAL target
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
Simulations
+ n -> + p
+ n -> + n
+ p -> + n
+ p -> + p
CC CC
. . . . . .
Nomad configuration/software (WA-96, Search for )
Analogy with induced reactionsused in simulations, e.g. :
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
QE: signal simulation
monochromatic below 50 GeV
ECAL energy <1 GeV
Pt < 1.5 GeV/c
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
Background sources for QE (
CC: X->…
QE or Coherent trilepton
production
Coherent production
Single charm production:
d,s->c -> s+
(beam sign is important !)
. . . .
final state
Beam related:
- low energy tail E < 50 GeV
- decays in flight:
f x PDec x P(E<E cut) x PECAL
K decays are more dangerous
DIS like QEL
- ’+ neutrals + leakage
- ’+ X->L+ ……
The goal is to search for a few, at most ~100 induced events among ~1012
interactions. Background sources have to be explored down to 10-12
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
X (CC) sample simulated events at 100 GeV 1 event found
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
Coherent Additional suppression
due to decay in flight < 10 GeV
ECAL < 1 GeV
Pt < 1.5 GeV/c
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
CHARM II ’91: ~0.03 fb at <E>~24 GeV
Coherent trilepton production
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
Summary of background for the QE reaction :
Source of background
Rate per interaction(very preliminary)
E< ~50 GeV muons in the
beam from decaystbd
photoproduction tbd
DIS CC ~10-14
Coherent trilepton
~10-14
Coherent production
~10-15
single charm in CC
<10-14
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
People/Institutes involved
Experimental groups LAPP, Annecy INR, Moscow IHEP, Protvino ETH, Zurich (help/experience with simulations, A.Rubbia’s group)
Theoretical groups College William and Merry, Williamsburg INR, Moscow Also, Osaka Univ. , S. Kanemura et al., talk at Tau’04, 16 Sept. 2004. JINR, Dubna, S. Kovalenko H. Kosmas’s group (Ioannina and Tuebingen) , coherent cross section
SPSC, Villars, September 22-28, 2004 S.N.Gninenko
Summary search for LFV in muon to tau conversion would be interesting
and challenging
further work is required to study
• muon beam : energy, intensity, purity, …
• target: composition, mass, …
• detector: rate capability, precision, ...
• production mechanism and cross sections
• best experimental signature
• signal/background: MC simulations, tools, …
and demonstrate feasibility of the experiment