oscillation analyses at t2k
play

oscillation analyses at T2K Raj Shah (STFC/Oxford) 19/07/16 1 - PowerPoint PPT Presentation

oscillation analyses at T2K Raj Shah (STFC/Oxford) 19/07/16 1 Outline Neutrino oscillations The T2K experiment Analysis strategy Results Raj Shah - STFC/Oxford Oscillation analysis @ T2K 2 Neutrino Mixing


  1. ν̅ oscillation analyses at T2K Raj Shah (STFC/Oxford) 19/07/16 1

  2. Outline •Neutrino oscillations � •The T2K experiment � •Analysis strategy � •Results Raj Shah - STFC/Oxford Oscillation analysis @ T2K 2

  3. Neutrino Mixing Atmospheric Reactor | LBL Solar θ 13 θ 23 ∆ m 2 12 ∆ m 2 δ CP 23 ∆ m 2 13 Raj Shah - STFC/Oxford Oscillation analysis @ T2K 3

  4. CP Violation P ( ν µ → ν e ) − P ( ν ¯ e ) µ → ν ¯ = − 16 S 12 C 12 S 13 C 2 13 S 23 C 23 Sin ( δ ) Sin ( ∆ 12 ) Sin ( ∆ 23 ) Sin ( ∆ 13 ) ∆ ij = ∆ m ij L ∝ Sin ( ∆ 12 ) Sin ( ∆ 23 ) Sin ( ∆ 13 ) 4 E ∝ Sin ( θ 12 ) Sin ( θ 23 ) Sin ( θ 13 ) ∝ Sin ( δ CP ) P ( ν µ ! ν µ ) 6 = P (¯ ν µ ! ¯ ν µ ) CPT Violation!! Raj Shah - STFC/Oxford Oscillation analysis @ T2K 4

  5. T2K Tokai to Kamioka μ -like e-like Raj Shah - STFC/Oxford Oscillation analysis @ T2K 5

  6. Detectors + Beam Ingrid ND280 Raj Shah - STFC/Oxford Oscillation analysis @ T2K 6

  7. Oscillation analysis Flux SK Efficiencies ND Constraint Cross section Oscillation Prob MC Prediction Data Oscillation fit Raj Shah - STFC/Oxford Oscillation analysis @ T2K 7

  8. Oscillation analysis Flux SK Efficiencies ND Constraint Cross section Oscillation Prob MC Prediction Data Oscillation fit Good Fit! Raj Shah - STFC/Oxford Oscillation analysis @ T2K 8

  9. Predicted spectra μ -like e-like ν � 7.00e20 POT ν̅� 7.41e20 POT Raj Shah - STFC/Oxford Oscillation analysis @ T2K 9

  10. Joint analysis results ν : 7.00e20 POT ν ̅ : 7.41e20 POT Nuisance parameters marginalised Raj Shah - STFC/Oxford Oscillation analysis @ T2K 10

  11. ν̅ e appearance μ -like e-like ν � 7.00e20 POT ν̅� 7.41e20 POT Raj Shah - STFC/Oxford Oscillation analysis @ T2K 11

  12. ν̅ e appearance 7.41e20 POT Do ν̅ μ oscillate into ν̅ e ? Signal: ν ̅ μ ➡ ν ̅ e 2.786 Osc 𝝃 e Beam 𝝃 e NC Tot Background 0.71 1.04 1.47 3.22 Raj Shah - STFC/Oxford Oscillation analysis @ T2K 12

  13. Frequentist analysis P Value: Probability to observe data as or more extreme than what was observed under the null hypothesis Null hypotheses No ν ̅ e appearance PMNS ν ̅ e appearance ( 𝛾 =0) ( 𝛾 =1) P osc ( ν ̅ μ ➡ ν ̅ e ) = 𝛾 · P osc (PMNS) P osc ( 𝝃 x ➡ 𝝃 y ) = P osc (PMNS) Statistic Δ 𝝍 2 = 𝝍 2 ( 𝛾 =0) - 𝝍 2 ( 𝛾 =1) Raj Shah - STFC/Oxford Oscillation analysis @ T2K 13

  14. Results ) 2 χ -1.93 Data P-Value 0.07 ∆ ))/d( =1 0.099 β 0.06 2 χ =0 0.374 β ∆ 0.05 d(p( 0.04 0.03 0.02 0.01 0 5 0 5 10 15 20 − 2 2 2 = ( =0) - ( =1) ∆ χ χ β χ β Raj Shah - STFC/Oxford Oscillation analysis @ T2K 14

  15. Bayesian results B 01 = Marginal Likelihood ratio P ( β = 0 | D ) P ( β = 1 | D ) = π ( β = 0) π ( β = 1) B 01 = π ( β = 0) π ( β = 1) e − 0 . 5 × ∆ χ 2 marg B 01 = 2.62 Weak preference for 𝛾 =0 Raj Shah - STFC/Oxford Oscillation analysis @ T2K 15

  16. ν̅ μ Disappearance ν : 6.57e20 POT vs ν ̅ : 4.01e20 POT • Introduce new separate parameters sin 2 ( θ ̅ 23 ) and Δ m ̅ 232 for 𝝃 oscillations. • Fix all ν oscillation (background) PMNS parameters • Fit ν ̅ oscillation parameters and compare with ν fit. Raj Shah - STFC/Oxford Oscillation analysis @ T2K 16

  17. Summary Joint Analysis � •Constraints on all ν oscillation parameters •Hint towards maximal CP violation � ν̅ e Appearance � •Preference for no ν̅ e appearance •10% p-value for PMNS appearance � ν̅ μ Disappearance � •Consistent constraints for ν and ν̅ oscillations Raj Shah - STFC/Oxford Oscillation analysis @ T2K 17

  18. Back ups Raj Shah - STFC/Oxford Oscillation analysis @ T2K 18

  19. Data vs Expectation 𝜉 𝜉̅ 1Rµ 1Re Raj Shah - STFC/Oxford Oscillation analysis @ T2K 19

  20. ν̅ e Appearance Raj Shah - STFC/Oxford Oscillation analysis @ T2K 20

  21. Null distribution #1 Prior knowledge : ν 1Re, ν 1R 𝜈 , ν̅ 1R 𝜈 � Method: � 1. Throw model parameters (osc and syst) based on priors 2. Generate all 4 predicted spectra (N exp ) 3. Compute likelihood ℒ ( ν 1R 𝜈 , ν 1Re, ν̅ 1R 𝜈 | data) � � � 4. Any toy dataset derived from N exp has a weight given by ℒ when filling the null hypothesis statistic distribution � Raj Shah - STFC/Oxford Oscillation analysis @ T2K 21

  22. Null distribution #2 (1) Take N exp from method in previous slide � (2) Throw poisson from N exp ν̅ 1Re � (3) Calculate statistic Δ 𝜓 2 with ν̅ 1Re toy and ν 1Re, ν 1Rµ and ν̅ 1Rµ real data � (4) Fill distribution with null hypothesis statistic � (5) Repeat from (1) 10k times Raj Shah - STFC/Oxford Oscillation analysis @ T2K 22

  23. Signal vs Background χ 2 ( β = 0) χ 2 ( β = 1) ∆ χ 2 # Obs # Exp ( β = 1) # Exp ( β = 0) 4 6.00 3.22 326.865 328.795 -1.930 Δ 𝜓 2 = 𝜓 2 ( β =0) - 𝜓 2 ( β =1) Raj Shah - STFC/Oxford Oscillation analysis @ T2K 23

  24. Sensitivity vs datafit β = 1 β = 0 Asimov Data fit Raj Shah - STFC/Oxford Oscillation analysis @ T2K 24

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend