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T2K Experiment Results & Prospects

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T2K Experiment Results & Prospects. Alfons Weber University of Oxford & STFC/RAL For the T2K Collaboration. Content. Neutrino Oscillations I ntroduction The T2K Experiment Beam Near Detector Far Detector Results Disappearance analysis Appearance search Future potential - PowerPoint PPT Presentation
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T2K Experiment Results & Prospects Alfons Weber University of Oxford & STFC/RAL For the T2K Collaboration
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T2K ExperimentResults & Prospects

Alfons WeberUniversity of Oxford &

STFC/RAL

For the T2K Collaboration

FLASY2014

Content

• Neutrino Oscillations– Introduction

• The T2K Experiment– Beam – Near Detector– Far Detector

• Results – Disappearance analysis– Appearance search

• Future potential– The hunt for CP-violation

Jun-2014 A.Weber, FLASY2014, Brighton 2

FLASY2014

Neutrino MixingThe PMNS Matrix

• Assume that neutrinos do have mass:– mass eigenstates weak interaction eigenstates– Analogue to CKM-Matrix in quark sector!

1

2

3

e

U

weak“flavour eigenstates”

Mass eigenstatesm1, m2, m3

Unitary mixing matrix:3 mixing angles

& complex phases

Pontecorvo-Maki-Nakagawa-Sakata

2 2ijwith cos( ), sin , mixing angle and mass differenceij ij ij ij ijc s (θ ) θ Δm

2

3

1 2 3 13 13 12 12

1 2 3 23 23 12 12

1 2 3 23 23 13 13

1 0 0 0 0 1 0 0

0 0 1 0 0 0 0

0 0 0 0 1 0 0

ie e e

i

ii

U U U c s e c s

U U U U c s s c e

U U U s c s e c e

3Jun-2014 A.Weber, FLASY2014, Brighton

FLASY2014

Oscillation Signatures

Jun-2014 4A.Weber, FLASY2014, Brighton

, or e 1 2 3, ,

e appearance: determine 13 constrain dCP disappearance: determine 23 and m232

Reconstructed ν Energy (MeV) Reconstructed ν Energy (MeV)Reconstructed ν Energy (MeV)

Eve

nts

Rat

io o

f ob

s/ex

pect

ed

FLASY2014

The T2K Experiment

• A Long-baseline Experiment to study neutrino oscillations– Baseline 295 km– Beam power up to 230 kW– Detectors Near and far

Jun-2014 5A.Weber, FLASY2014, Brighton

FLASY2014

Producing Neutrinos

6

π→μν118 m

off-axis (2.5°)

(30 GeV from MRsynchrotron)

Jun-2014

2 2

0.431

EE π

νγ θ

A.Weber, FLASY2014, Brighton

Using NA61 data to constrain

hadron production

FLASY2014

Data Taken

• Data Set: 6.57 x 1020 PoT (8% of design goal)• Increase power in future

– More protons / bunch– Higher repetition rate

Jun-2014 7A.Weber, FLASY2014, Brighton

FLASY2014

ND280 detector

• Off-axis: ND280– 0.2 T magnet (UA1/NOMAD)– Plastic scintillator detectors:

Fine Grained Detector (FGD), π0 detector (P0D), ECals and SMRD, Time projection chambers (TPC)

• On-axis: INGRID

8Jun-2014

νμ

FGD2FGD2

TPC3TPC3TPC2TPC2TPC1TPC1

FGD1FGD1

A.Weber, FLASY2014, Brighton

FLASY2014

Some ND distribution

• Select different event classes in near detector– Negative muon & something/nothing

• Constrains flux and cross section uncertainties

Jun-2014 9A.Weber, FLASY2014, Brighton

CC 1π+CC 0π CC Other

BEFO

RE F

ITAF

TER

FIT

FLASY2014

Reduced Systematics

Jun-2014 10A.Weber, FLASY2014, Brighton

FLASY2014

Far Detector

Jun-2014 11A.Weber, FLASY2014, Brighton

FLASY2014

Far Detector Events

Jun-2014 12A.Weber, FLASY2014, Brighton

FLASY2014

Electron Neutrino Appearance

• Event Selection– Fully contained, – no π0

– No decay electrons

Jun-2014 13A.Weber, FLASY2014, Brighton

FLASY2014

Appearance Result

Jun-2014 14A.Weber, FLASY2014, Brighton

Phys. Rev. L

ett. 112, 061802

(2014)

FLASY2014

Compare with Reactors

Jun-2014 15A.Weber, FLASY2014, Brighton

• Comparing with reactor measurements• best overlap is for the

normal hierarchy δcp=–π/2.

• Need to increase θ23 to account for high event rate Note: Marginalized

over 23 and m232

Lucky point!

FLASY2014

Disappearance Measurement

Jun-2014 16A.Weber, FLASY2014, Brighton

Maximal mixing is not the same as maximumdisappearance if θ13 is not zero!

NH: sin2(θ23) = 0.514NH: Δm2

32 = 2.51x10-3 eV2

120 selected events

FLASY2014

The World Scene

Jun-2014 17A.Weber, FLASY2014, Brighton

Best-fit ± FC 68% CL (Δm2 units 10-3 eV2/c4)

NHsin2θ23 0.514+0.055

-0.056

Δm232 2.51 ± 0.10

IHsin2θ23 0.511 ± 0.055

Δm213 2.48 ± 0.10

FLASY2014

Putting it All Together

Jun-2014 18A.Weber, FLASY2014, Brighton

FLASY2014

The width of the beam is comparable to the measured Gaussians in the previous runs.

ND280 anti-ν event

The detectors are all working well.

Here is our first identified anti-neutrino event from an anti-neutrino test run!

Measured with INGRID

μ+

Run Status

Jun-2014 A.Weber, FLASY2014, Brighton 19

FLASY2014

Future Sensitivity

No systematics

5% error on signal, 10% on background

T2K best sensitivity: 50% ν/50% anti-ν Anti-nu running: large new physics program.

50% ν/50% anti-ν (true NH)100% ν (true NH)

50% ν/50% anti-ν (true NH)w/ Reactor constraint

100% ν (true NH)w/ Reactor constraint

“Lucky! (+: Sin22θ=0.1, δCP=-90)”

NH

T2K: 50% ν/50% anti-ν

Jun-2014 A.Weber, FLASY2014, Brighton 20

FLASY2014

Future Sensitivity (II)

50% ν/50% anti-ν (true NH)

50% ν/50% anti-ν (true NH)w/ Reactor constraint

100% ν (true NH)w/ Reactor constraint

100% ν (true NH)

“Unlucky! (+: Sin22θ=0.1, δCP=0)”

Jun-2014 A.Weber, FLASY2014, Brighton 21

FLASY2014

T2K and NOvA

T2K: 50% ν/50% anti-ν

NH IH

No systematics

5% error on signal, 10% on background

Jun-2014 A.Weber, FLASY2014, Brighton 22

FLASY2014

Summary and Conclusion

• T2K has taken 8% of its nominal PoT• World leading results

– 7.3σ electron neutrino appearance– Most precise measurement of θ23

• Combination with reactor measurements– Hint that δCP = -π/2

• Improved sensitivity with data to come– Can be lucky to “discover” CP violation

• More results to come– Cross sections, sterile neutrinos, exotics…

Jun-2014 23A.Weber, FLASY2014, Brighton

Backup

FLASY2014

Who is Who

Jun-2014 25

νμ disappearance

ν–less double beta decay

Solar neutrino oscillation

νe disappearance inνμ beam Or

reactor neutrino experiments

A.Weber, FLASY2014, Brighton

FLASY2014

Ubi es?

26

Normal Hierarchy or Inverted Hierarchy?Open questions:

smaller) little a(or 45

eV104.2

23

23232

m

?0

?232

m

Jun-2014 A.Weber, FLASY2014, Brighton

913

FLASY2014

NA61/SHINE

• hadron(π, K) yield – 30 GeV p + C

• High-acceptance – ToFs and spectrometers

• 2cm thin target (4%λI)• π+ analysis:

– dE/dx only analysis low momenta (Phys.Rev.C84.2011.034604)

– dE/dx+ToF analysishigh momenta(Phys.Rev.C85.2011.035210)

27

~13m

~1

0m

Jun-2014 A.Weber, FLASY2014, Brighton

FLASY2014

Predicted Flux

• Primary pions modelled with NA61 data

• νμ flux– Pions dominant at low energy– Kaons important in tail

• νe flux – For low energy from muons

28

νμ

νμνe

Jun-2014 A.Weber, FLASY2014, Brighton

FLASY2014

CC Interaction

Jun-2014 29A.Weber, FLASY2014, Brighton


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