Future Neutrino Oscillation Experiments - PowerPoint PPT Presentation

About This Presentation
Title:

Future Neutrino Oscillation Experiments

Description:

Future Neutrino Oscillation Experiments – PowerPoint PPT presentation

Number of Views:45
Avg rating:3.0/5.0
Slides: 34
Provided by: edblu
Learn more at: http://hep.uchicago.edu
Category:

less

Transcript and Presenter's Notes

Title: Future Neutrino Oscillation Experiments


1
Future Neutrino Oscillation Experiments
Ed Blucher
  • Neutrino oscillations, CP violation, and
    importance of ?13
  • Accelerator vs. reactor experiments
  • Future reactor experiments to measure sin22?13

2
Neutrino Oscillations
  • During last few years, oscillations among
    different flavors of neutrinos have been
    established physics beyond the S.M.
  • Mass eigenstates and flavor eigenstates are not
    the same (similar to quarks)

mass eigenstates
flavor eigenstates
MNSP matrix
  • Raises many interesting questions including
    possibility of CP violation in neutrino
    oscillations.
  • CP violation in neutrino sector could be
    responsible for the matter-antimatter asymmetry.

3
Quark and Neutrino Mixing Matrices
4
2 Flavor Neutrino Mixing
The time evolution of the flavor states is
For a beam that is pure ?? at t0,
5
MNSP Matrix
?12 30
?23 45
sin2 2?13 lt 0.2 at 90 CL
What is ?e component of ?3 mass eigenstate?
6
CP Violation in Neutrino Oscillations
Minakata and Nunokawa, hep-ph/0108085
7
Methods to measure sin22?13
  • Appearance nm?ne (Accelerator Exp)
  • Use fairly pure, accelerator produced nm beam
    with a detector at long distance (300 km - 900
    km) from the source
  • Look for the appearance of ne events
  • Use near detector to measure background nes (beam
    and misid)

150m
1500m
  • Disappearance (Reactor Exp)
  • Use a set of reactors as a source of
  • ne's with a detector at few km
  • Look for a non- 1/r2 behavior of the ne rate
  • Use near detector to measure the unoscillated
    flux

Diablo Canyon, CA
overburden
8
Accelerator and reactor measurements of ?13
Accelerator experiments measure
Reactor measurement of ?13 is independent of
matter effects and CP violation
9
Reactor Measurements of Neutrino Oscillations
Reactors are copious sources of
per second.
Detection of antineutrino by
followed by
or for Gd-loaded scintillator
10
Long history of neutrino experiments at reactors
20 m
KamLAND
6 m
CHOOZ
Current interest is focused mainly on possibility
of measuring ???
11
Reactor Measurements of
Future Search for small oscillations at 1-2 km
distance (corresponding to
Pee
Reactor experiments allow direct measurement of
sin22??? no matter effects, no CP
violation, almost no correlation with other
parameters.
Sensitivity goal sin22???0.01. Level at which
long-baseline superbeams can be used to measure
mass hierarchy, CPV sensitivity goal of
proposed accel. expts.
Distance to reactor (m)
12
Previous Reactor ??? Experiments
CHOOZ Systematic Errors
  • CHOOZ and Palo Verde Experiments
  • Single detector experiments
  • Detectors used liquid scintillator with
    gadolinium and buffer zones for background
    reduction
  • Shielding
  • CHOOZ 300 mwe
  • Palo Verde 32 mwe
  • Fiducial mass
  • CHOOZ 5 tons _at_ 1km, 5.7 GW
  • 2.2 evts/day/ton with 0.2-0.4 bkg evts/day/ton
  • 3600 n events
  • Palo Verde 12 tons _at_ 0.85km, 11.6 GW
  • 7 evts/day/ton with2.0 bkg evts/day/ton
  • 26000 n events

13
CHOOZ
Target 5 ton Gd-doped scintillator
14
Is it possible to improve the Chooz experiment by
order of magnitude (i.e., sensitive to sin22???
0.01)? Add second detector bigger detectors
better control of systematics.
200 m
1500 m
  • What systematic error is attainable?
  • Efficiency and energy calibration strategy
    (movable detectors?)
  • Backgrounds
  • Multiple reactor cores
  • Site / depth
  • Choice of scintillator (stability of
    Gd-loaded scintillator)
  • Size, distance of detectors

15
Normalization and spectral information
Predicted spectrum ?130
Observed spectrum sin22?130.04
  • Counting Experiment
  • Compare number of events in near and far detector
  • Energy Shape Experiment
  • Compare energy spectrum in near and far detector

E? (MeV)
E? (MeV)
16
Analysis Using Counting and Energy
Spectrum(Huber et al. hep-ph/0303232)
scal relative near/far energy calibrationsnorm
relative near/far normalization
90CL at Dm2 310-3 eV2
  • Counting exp. region
  • Spectrum Rate region

ScenariosReactor I 12ton7GW5yrsReactor II
250ton7GW5yrs
17
Worldwide interest in two-detector reactor
experiment
Workshops Alabama, June 2003 Munich, October
2003 Niigata, Japan, March 2004
Based on early workshops, a whitepaper
describing physics possibilities of reactor
experiment has been written.
18
  • Sites under discussion
  • Kraznoyarsk (Russia)
  • Chooz (France)
  • Kashiwazaki (Japan)
  • Diablo Canyon (California)
  • Braidwood, Byron (Illinois)
  • Wolf Creek (Kansas)
  • Brazil
  • Taiwan
  • China

19
Kr2Det Reactor ?13 Experiment at Krasnoyarsk
Features - underground reactor - existing
infrastructure
Detector locations constrained by existing
infrastructure
Reactor
Ref Marteyamov et al, hep-ex/0211070
20
Proposal for Reactor ?13 Experiment in Japan
Kashiwazaki -7 nuclear power stations worlds
most powerful reactors - requires
construction of underground shaft for detectors
far
near
near
Kashiwazaki-Kariwa Nuclear Power Station
21
Kashiwazaki Proposal for Reactor ?13 Experiment
in Japan
far
near
near
70 m
70 m
200-300 m
6 m shaft, 200-300 m depth
22
The Chooz site, Ardennes, France
Double-CH?13?13Z
23
The Chooz site
Type PWR
Cores 2
Power 8.4 GWth
Couplage 1996/1997
(, in to 2000) 66, 57
Constructeur Framatome
Opérateur EDF
?
Near site D100-200 m severall options under
study Far site D1.1 km, overburden 300 mwe
former experimental hall
  • Positive signs from EDF for reusing the former
    CHOOZ site. Near site ? civil engineering
  • 2x11.5 tons, D1100-200m, D21050m. Sensitivity
    3 years ? sin2(2?13) lt 0.03
  • Chooz, 2x10 tonnes, D10.7 km, D21.1 km, 3 ans
    (70 kevts) ? sin2(2?13)lt0.037

24
CHOOZ-Far
25
CHOOZ-Far detector
3.5 m
Existing CHOOZ tub
7 m
26
CHOOZ-Near new Laboratory
10-15 m
High-Z material
5- 15 m
27
U.S. Nuclear Power Plants
28
Braidwood, Illinois 7.17 GW 24 miles SW of Joliet

29
Braidwood site
30
Diablo Canyon Nuclear Power Plant
1500 ft
Powerful Two reactors (3.1 3.1 GW Eth)
Overburden Horizontal tunnel could give 800 mwe
shielding Infrastructure Construction roads.
Controlled access. Close to wineries.
31
  • Weve formed a small collaboration to develop a
    proposal for a
  • midwest site
  • Chicago, Columbia, ANL, FNAL, Kansas, Michigan,
    Oxford, Texas

Chicago involvement Kelby Anderson, Ed Blucher,
Juan Collar, Jim Pilcher, Matt Worcester
(postdoc), Erin Abouzaid (grad), Abby Kaboth
(undergrad), Jennifer Seger (undergrad)
  • Significant effort also underway at LBNL to
    investigate feasibility
  • of experiment at Diablo Canyon.

32
Conclusions
  • Extremely exciting time for neutrino physics!
  • The possibility of observing CP violation in the
    neutrino sector presents a great experimental
    challenge.
  • Reactor and accelerator experiments are
    complementary.
  • Reactor experiment has potential to be faster,
    cheaper, and better for establishing value of ???.

33
Was baryogenesis made possible by leptonic CP
violation?
Leptogenesis may have been the result of direct
CP violation in decays of heavy Majorana
particles
This antilepton excess in converted to a baryon
excess through nonperturbative Standard Model B-L
conserving processes.
- Fukugita and Yanagida, Phys. Lett. B174 (1986)
Write a Comment
User Comments (0)
About PowerShow.com