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Physics: Understanding Neutrino Oscillation Parameters and the Role of PX435, Study notes of Engineering Physics

An overview of neutrino oscillation experiments, focusing on the measurement of neutrino mixing parameters, specifically ฮธ13. It discusses various experiments, their sensitivities, limitations, and improvements. The document also touches upon the role of px435 in the field and the expected discoveries in the near future.

Typology: Study notes

2010/2011

Uploaded on 09/10/2011

melanycox
melanycox ๐Ÿ‡ฌ๐Ÿ‡ง

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PX435 โ€“ ๏ฎ Physics
Current state of knowledge
The Future and Beyond
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Download Physics: Understanding Neutrino Oscillation Parameters and the Role of PX435 and more Study notes Engineering Physics in PDF only on Docsity!

Current state of knowledge

The Future and Beyond

To the Future and Beyond!

The next 20 years Measurement Method Experiments Why? When Is it maximal? 2009 Equal to 0? Can't 2012 Reactor 2012 T2KK, neutrino Unification, GUT 2025? Factory, ??? Lepton asymmetry

23

๏ญ Disapp. T2K, NovA ๏ฑ 13

e Appear. T2K, NovA measure ๏ค CP if it is Anti-๏ฎ e Disapp. Sgn(๏„m 23 2 ) ๏ฎ e / anti-๏ฎ e ๏ค CP

CP violation? Measuring ๏ค CP is the ultimate goal of neutrino oscillation experiments. How? P ๎‚ž๎ƒƒ ๎ƒ‚ ๎‚Œ๎ƒƒ e ๎‚Ÿโ‰  P ๎‚ž๎ƒƒ ๎ƒ‚ ๎‚Œ ๎ƒƒ e Look for ๎‚Ÿ Prob ๎‚ž๎ƒƒ ๎‚ท ๎‚Œ ๎ƒƒ ๎‚ธ ๎‚Ÿ=๎‚บ ๎‚ท ๎‚ธ โˆ’ (^4) โˆ‘ i ๎‚… j โ„œ๎‚ž U ๎‚ท i

U ๎‚ธ i U ๎‚ท j U ๎‚ธ j

๎‚Ÿ sin 2 ๎‚ž๎‚ญ m ij 2 L 4 E ๎‚Ÿ ๎‚ƒ (^2) โˆ‘ i ๎‚… j โ„‘๎‚ž U ๎‚ท i

U ๎‚ธ i U ๎‚ท j U ๎‚ธ j

๎‚Ÿ sin๎‚ž๎‚ญ m ij 2 L 2 E ๎‚Ÿ = 0 if ๏ก๏€ ๏€ฝ๏€ ๏ข CP violation can only take place in appearance experiments

13 determines the next 15-30 years or so of the field

How large is it? sin 2 ( 2 ฮธ 13 )=0.063ยฑ0. Real or accidental? Need more data... Fogli et al - arXiv:0809.

CHOOZ sin 2 ( 2 ฮธ 13 )<0.16 @ 90 % CL Limitations: Large radioactive background Limited statistics Stability of detector Reactor was not always on

Improving CHOOZ Statistical Error Systematic Error 2.8% 0.5%

CHOOZ

DoubleCHOOZ 5 m 3 to 10 m 3 detector Longer running time Near and Far detector helps eliminate some systematics errors Improved design with lower threshold Lower background

Sensitivity sin 2 ( 2 ฮธ 13 )โ‰ค0. sin 2 ( 2 ฮธ 13 )โ‰ค0. Discovery @ 3๏ณ if sin 2 (2๏ฑ 13

Sensitivity Far detector has been running since September 2010 Expect first appearance result at the summer conference round

How do we get to ๏ฑ 13 ? P๎‚ž๎ƒƒ ๎ƒ‚

e ๎‚Ÿ=sin 2 2 ๎‚พ 13 sin 2 ๎‚พ 23 sin 2 ๎‚ž1.27๎‚ญ m 23

2 L

E

๏ญ

e oscillations with atmospheric L/E

P๎‚ž๎ƒƒ

e

x

๎‚Ÿ=sin

2

13

๎‚Ÿ sin

2

๎‚ž1.27๎‚ญ m

23

2 L

E

e

x disappearance oscillations with atmospheric L/E ๏ฎ e

x disappearance oscillations with atmospheric L/E P๎‚ž๎ƒƒ e

x

C^ ๎‚‘ P๎‚‘ P๎‚ž๎ƒƒ e

x

Next Generation T2K NOvA Site Beam <E ๏ฎ

Distance Far Det mass Tokai,Japan JPARC 0.7 GeV 295 km Super-K 22.5 kton USA NuMI 2.2 GeV 812 km to be built 30.0 kton Long enough for matter effects

Who we are...

PX435 โ€“ ๏ฎ Physics First Off-axis Neutrino Beam Proton Beam Target ๏ฐ,K Decay pipe

    • ฯ€,K

Magnetic Focusing Near Far ๏ฑ E ๎ƒƒ = 0.43 E ๎ƒ† 1 ๎‚ƒ๎‚น 2 ๎‚พ 2 Energy tuned to oscillation max.