Neutrino Physics

34
Neutrino Physics MEMBER ERIKO KUSUNOKI KENJI SHU TAKESHI SAITO MESANORI IWAMOTO MITSUTAKA NAKAO NISHIMURA GROUP

description

Neutrino Physics. Member Eriko kusunoki Kenji shu Takeshi saito Mesanori iwamoto Mitsutaka nakao. NISHIMURA Group. CONTENTS. ν - Source. Theory of Neutrino Physics Super Kamiokande (Super K) Measuring Cosmic Rays T2K Experiment Analyzing T2K data. ν - Oscillation. - PowerPoint PPT Presentation

Transcript of Neutrino Physics

Page 1: Neutrino Physics

Neutrino PhysicsMEMBER

ERIKO KUSUNOKIKENJI SHUTAKESHI SAITOMESANORI IWAMOTOMITSUTAKA NAKAO

NISHIMURA GROUP

Page 2: Neutrino Physics

CONTENTS

• Theory of Neutrino Physics• Super Kamiokande (Super K)• Measuring Cosmic Rays• T2K Experiment• Analyzing T2K data

ν- Source

ν- Oscillation

ν- Detector

Page 3: Neutrino Physics

Theory of Neutrino Physics

Page 4: Neutrino Physics

What is neutrino?

・ Three Flavors・ Neutral (no charge)・ Only Weak Interaction・ Very Tiny Mass

very difficult for detecting…

Page 5: Neutrino Physics

The interesting point is…

Neutrino Oscillation

Page 6: Neutrino Physics

Neutrino Oscillation(Two mixing case)

・ The mass basis is different from the interaction basis.

flavour massΘ:mixing angle

The probability to change νμ into ντ is… L : Length [km]E : energy[GeV]Δm2 : mass square difference[eV2]but nature is more complex…

✔✔✔

Page 7: Neutrino Physics

Neutrino Oscillation(Three mixing case)

Atmospheric Neutrinos

νμ→ντ

Solar Neutrinos

νe→νxAccelerator

νμ→νe

What we want to know is …

Mixing Parameter

✔ ✔❓~45° ~34°

T2K

Page 8: Neutrino Physics

CP violation~What is δCP in PMNS matrix?~

This parameter leads to CP violation.

CP term

Leading Term

Page 9: Neutrino Physics

How can we detect neutrinos?

The answer is…

Super K

Page 10: Neutrino Physics

Super-Kamiokande1km

Kamioka

39.3m

41.4m

50,000 t

Inner tank

outer tank

11,129 PMTs (50cm)detect neutrinos.

1,885 PMTs (20cm)distinguish neutrinos from muons coming from outside.

water

We can block muons that originate from cosmic ray.

1km Underground

Page 11: Neutrino Physics

Red : strong light

Blue : weak lightVertex

1. Timing of detection2. Vertex position 3. Finding Cherenkov ring4. Neutrino traveling

direction and energy

Event display

OH

p n

𝝂𝒆

𝑒+¿ ¿𝑊+¿¿

Cherenkov light

inverse beta decay

Neutrino detection @Super-Kamiokande

Neutrinos interact with particle in water.

→ SK detect Cherenkov light that is created when a charged particle travels faster than the speed of light in water.

neutrino

Page 12: Neutrino Physics

Next: Hyper-Kamiokande

HK might uses HPDs instead of PMT.

ee

~8kV

Avalanche diode

Super-Kamiokande

eMetal dynode

~2kV

Photon

To measure the light energy, we use PMTs.

Neutrino detectors

HPD accomplish superior performance in low cost !!

Improving performance(Volume of tank) ×25

PMT (PhotoMultiplier-tube) HPD (Hybrid-Photo Detector)‐

photoelectric effect

Let’s use HPD !!!!

Page 13: Neutrino Physics

These PMT are used in super-Kto measure the cosmic rays. HPDs may be used in Hyper-K . We tested an HPD and a PMT to measure the angular Distribution of cosmic ray muons .   

HPD

PMT

Testing PMTs and HPDs

Page 14: Neutrino Physics

The Angular Distribution of Cosmic ray Muons

The flux is given by J(x,θ) = J(x,0) (n =   Where λ is mean free pathThe purpose of thisexperiment was finding the value of n.

Page 15: Neutrino Physics

Set up We used two sets of two detectors to measure the angular distribution.  

Scintillator(20cm×20cm)

PMT

HPD

PMT

Scintillator(50cm×50cm)

First detector Second detector

μ

Page 16: Neutrino Physics

We made a coincident circuit to count muons which activated all detectors.

Page 17: Neutrino Physics

Resultsangle[degree] measuring

time[second]

count flux[Hz/counter]

0 15502.80 1276 0.0823

30 23489.36 1015 0.0397

50 42961.68 1345 0.0241

70 50647.65 817 0.00901

We corrected flux by a solid angle

Page 18: Neutrino Physics

We fitted a× and determined n = 2.470.53 .

fitting

Page 19: Neutrino Physics

T2K Experiment

Page 20: Neutrino Physics

What is T2K?

• Tokai(J-PARC) to Kamioka(SK)

• Pure • SK can distinguish

and  • Observe

appearing and   disappearing

http://t2k-experiment.org/ja/

𝑣𝜇

?

Page 21: Neutrino Physics

Devices to discovery

• Distance • Off axis

2.5。𝜋+¿¿

E ~ 0.6 GeV

L = 295 km

𝜈𝜇 (on axis)

SK

appearensae in E = 0.6 GeV

disappearing in L =295 km

Page 22: Neutrino Physics

Enrichment signals

• Reduce BG cuts using Monte Carlo calculations

193

60

cut BG

377 events is first selected by timing

Number of rings e -like evernts

cut NC,μ

cut collapse π,μ   cut in beam 57 44 39 28

• Selection one ring -like events

Page 23: Neutrino Physics

events

• Proton created in J-PARC :• expected BG : 4.92• So we calculate expectation and estimate

6.57

28 -like single ring events were found𝜈𝑒

Was happened?     ?

Page 24: Neutrino Physics

Analyzing T2K data

Page 25: Neutrino Physics

What we have• T2K result

number :

Proton number :

Very new : Physical Review Letters, 2014 Feb

• Theory

Page 26: Neutrino Physics
Page 27: Neutrino Physics

Maximum Likelihood Method to find • Likelihood function : ← maximize L• ← minimize

Compare numbers obs. vs exp.

Poisson distribution

Restrict systematic parameters

f : systematic errors ← parametersExpectation of numbers observed

: signal of oscillation depends on ←par : background appeared as by M.C. simulation (depends on , , , function was given)

Page 28: Neutrino Physics

Get

sin22 𝜃13=0.137

• Best fitChange minimizing That = experimental result!!!

Page 29: Neutrino Physics

Get errors• Error(1 sigma)

get at

+0 .0370 .137−0 .032

Page 30: Neutrino Physics

Get confidence level for

get at

Significance : 6.9s

actually exists and non-zero!!!

√ 46.9=6.9𝜎

Page 31: Neutrino Physics

Comparison with actual T2K

ACTUAL T2K

• C.L. :

OUR VERIFICATION

• C.L. :

Same value, same error

T2K was correct!!!

(C.L. is better by using energy likelihood function)

Page 32: Neutrino Physics

In actual T2K experiment…• Likelihood function

: oscillation parameter : systematic error parameterf are more than 49!

Page 33: Neutrino Physics

Future experiment

• T2K is just in beginning• Continue to get 10 times more data• Check the sensitivity ()

(We did)→ twice more precise

• Anti-Neutrino experiment by Hyper-K can measure

Page 34: Neutrino Physics

Summary

Theory

Experiment Analyzing