Title: and p0 Decay to Two Neutrinos
1? and p0 Decay to Two Neutrinos
Ali R. Fazely Department of Physics Southern
University Miami Conference, 2008 December 16
-21
2In collaboration with
Richard L. Imlay, Samvel Ter-Antonyan, Xianwu
Xu Department of Physics Southern University
3- Do ? or?0 decay into two neutrinos?
- Standard Model ?0 ? ?? or ? ? ?? is
forbidden, except for massive neutrinos. - The experimental search for such purely NC decays
would shed light on the nature of neutrinos and
weak processes.
4Weak Current
- The ? ? e ?e has a BR of
-
- 1.23 ? 10-4 (pdg)
- The helicity is broken due to the mass of the
electron consistent with the V-A interaction.
5 ?o ? ?? Forbidden in V-A Interaction ?o is
0- and vacuum is 0 For massless neutrinos 0-
? 0 transition is allowed only if Pseudoscalar
(P) is present Same for ? ? ??
6The rate for A and P
- The decay rate for A interaction is proportional
to (1 - ? ). For massless neutrinos ? 1 and the
rate is zero. - The decay rate for P interaction is proportional
to (1 ? ). For massless neutrinos ? 1 and the
rate is maximum. -
7The rate for A and P
- A-coupling
- BR p ? e?e/p ? µ?µ (me/mµ)21/(1-
mµ2/mp2)2 1.27510-4 - P-coupling
- BR p ? e?e/p ? µ?µ 1/(1- mµ2/mp2)2
5.5 -
8Experimental results on ? ? ?? and?0 ? ??
l
q
Z0
Within the SM, the diagram is a simple qq
annihilation to lepton pairs through a Z0
propagator.
l-
q-
9Decay Rate
Arnellos, Marciano, Parsa, Nucl Phy B196 (1982)
10Experimental Results
LSND
pdg, all at 90 CL
11LSND Results PRL 92, 4, 091801-1,
hep-ex/0310060
- Observation of a muon-like, beam-excess above 160
MeV in the LSND detector - 8.7 6.3 (stat) 2.4 (syst) beam-excess events
(pdg) - The possible Branching Ratio of is
12p0 ? ?t?t
- A 95 CL, upper limit of lt18.2 MeV was set
by the ALEPH Collaboration on ?t mass from 3 and
5-prong t decay. (Eu J Phys, 1998, pdg). - However,
- (mt/m?)2 lt 331.24/(134.9)2 0.0182
13p0 ? ?t?t
- Therefore,
- G(p0 ? ?t?t)/G(p0 ? all) lt 5.0 10-10,
- assuming no exotic mechanisms!
- A possible laboratory to set limits on the ?t
- mass!
14? ? ??
(90CL) pdg, BES2 collaboration, 06Q PRL 97
202002
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21muons
neutrons
Photons, from ?0 and ?
Electrons/positrons
22Estimates for the BR of the km3Detectors, e.g.
IceCube
- Dominant interaction inside the ice is
- The signature is an electron or t cascade event
23Primary FluxSolid and dashed lines are those of
Gaisser Honda,(hep-ph/0203272 (2002)).
Symbols are from spectra of Wiebel, Bierman
Meyer, Ast. And Astrophys. 330 (1998), used in
our CORSIKA simulations
24The IceCube Detector
25Atmospheric Neutrino Flux, CORSIKA
26Integral Spectra
27Geant-3.21 Simulation
28Branching Ratio vs. Energy,5-year run
29Conclusions
- Limits can be set for the first time on ????
- with km3 detectors
- ???? limits would not be competitive with
existing limits. - Dedicated experiments can be designed to look for
???t?t yielding limits on - the ?t mass as well as any possible P
interaction in NC sector.