The Leptonic Dirac CP-Violating Phase from Sum Rules · 2015-09-09 · The Leptonic Dirac...
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The Leptonic Dirac CP-Violating Phase from Sum Rules
Arsenii Titov
in collaboration with I. Girardi and S.T. Petcov
SISSA and INFN, Trieste, Italy
XIV International Conference on Topics in Astroparticle and Underground Physics
9 September 2015, Turin, Italy
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Outline
• 3-neutrino mixing
• General setup
• Sum rules
• Predictions
• Conclusions
Based on I. Girardi, S.T. Petcov, A.T., NPB 894 (2015) 733 [arXiv:1410.8056]
I. Girardi, S.T. Petcov, A.T., EPJC 75 (2015) 7, 345 [arXiv:1504.00658]
209.09.2015 Arsenii Titov | TAUP 2015 | Turin
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U is the Pontecorvo-Maki-Nakagawa-Sakata neutrino mixing matrix
Best fit 3σ range
sin2 θ12 0.308 0.259 ÷ 0.359
sin2 θ23 (NO) 0.437 0.374 ÷ 0.626
sin2 θ23 (IO) 0.455 0.380 ÷ 0.641
sin2 θ13 (NO) 0.0234 0.0176 ÷ 0.0295
sin2 θ13 (IO) 0.0240 0.0178 ÷ 0.0298
δ/π (NO) 1.39 0 ÷ 2
δ/π (IO) 1.31 0 ÷ 2
Capozzi et. al., PRD 89 (2014) 093018
309.09.2015 Arsenii Titov | TAUP 2015 | Turin
θ12 ≈ π/4 − 0.20
θ23 ≈ π/4 − 0.06
θ13 ≈ 0 + 0.15
Symmetry?
3-neutrino mixing
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Me is the charged lepton mass matrix
Mν is the neutrino Majorana mass matrix
General setup
409.09.2015 Arsenii Titov | TAUP 2015 | Turin
Ũe and Ũν are CKM-like 3×3 unitary matrices
Ũν is assumed to have a symmetry form which is dictated by, or associated with, a flavour (discrete) symmetry, e.g., A4, S4, A5, T’
Frampton, Petcov, Rodejohann, NPB 687 (2004) 31
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General setup
509.09.2015 Arsenii Titov | TAUP 2015 | Turin
Symmetry forms of Ũν : bimaximal, tri-bimaximal, golden ratio, hexagonal…
• Tri-bimaximal (TBM) A4/T’ θν12 = arcsin (1/√3) ≈ 35°
• Bimaximal (BM) S4 θν12 = π/4 = 45°
• Golden ratio A (GRA) A5 θν12 = arcsin (1/√(2+r)) ≈ 31°
• Golden ratio B (GRB) D10 θν12 = arcsin (√(3−r)/2) = 36°
• Hexagonal (HG) D12 θν12 = π/6 = 30°
θν23 = − π/4
for all these symmetry forms
r is the golden ratio:r = (1 + √5)/2
where
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General setup
609.09.2015 Arsenii Titov | TAUP 2015 | Turin
Charged lepton (CL) corrections:
• 1 rotation from the CL sector and 2 rotations from the neutrino sector
• 2 rotations from the CL sector and 2 rotations from the neutrino sector
• 1 rotation from the CL sector and 3 rotations from the neutrino sector
=> sum rules for cos δ, i.e., cos δ as a function of the observable mixing angles θ12, θ23, θ13 and the angles θν
ij, whose values are fixed
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Sum rules
709.09.2015 Arsenii Titov | TAUP 2015 | Turin
1 rotation from the CL sector and 2 rotations from the neutrino sector
R12(θe12)
R13(θe13)
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Sum rules
809.09.2015 Arsenii Titov | TAUP 2015 | Turin
2 rotations from the CL sector and 2 rotations from the neutrino sector
R12(θe12) R23(θe
23)
R13(θe13) R23(θe
23)
Petcov, NPB 892 (2015) 400
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Sum rules
909.09.2015 Arsenii Titov | TAUP 2015 | Turin
R12(θe12)
R13(θe13)
%
1 rotation from the CL sector and 3 rotations from the neutrino sector
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Predictions for cos δ
1009.09.2015 Arsenii Titov | TAUP 2015 | Turin
Using best fit values of mixing angles for NO neutrino mass spectrum
θν23 = − π/4 [θν
13, θν12]
a = arcsin (1/3) b = arcsin (1/√(2+r)) c = arcsin (1/ √3) d = arcsin (√(3−r)/2)
Non-zero values of θν13: Bazzocchi, arXiv:1108.2497, Toorop et. al., PLB 703 (2011) 447,
Rodejohann and Zhang, PLB 732 (2014) 174
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Predictions for JCP: statistical analysis
1109.09.2015 Arsenii Titov | TAUP 2015 | Turin
R12(θe12) R23(θe
23)
JCP determines the magnitude of CP-violating effects in neutrino oscillations
NO schemeIO scheme
NO global fitIO global fit
Relatively large CP-violating effects in neutrino oscillations in the cases of TBM, GRA, GRB, HG: JCP ≈ − 0.03, |JCP | ≥ 0.02 @ 3σand suppressed ones in the case of BM:JCP ≈ 0
Krastev and Petcov, PLB 205 (1988) 84
Using latest results on sin2 θij and δ, obtained in global analysis of neutrino oscillation data in Capozzi et. al., PRD 89 (2014) 093018
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Predictions for cos δ: statistical analysis
1209.09.2015 Arsenii Titov | TAUP 2015 | Turin
Likelihood function
R12(θe12) R23(θe
23)
Using current best fit values and prospective 1σ uncertainties for sin2 θij: 0.7% for sin2 θ12 (JUNO), 3% for sin2 θ13 (Daya Bay), 5% for sin2 θ23 (NOvA and T2K) + Gaussian approximation
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Predictions for cos δ: statistical analysis
1309.09.2015 Arsenii Titov | TAUP 2015 | Turin
Likelihood function
R13(θe13) R23(θe
23)
Using current best fit values and prospective 1σ uncertainties for sin2 θij: 0.7% for sin2 θ12 (JUNO), 3% for sin2 θ13 (Daya Bay), 5% for sin2 θ23 (NOvA and T2K) + Gaussian approximation
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Extension of the study
1409.09.2015 Arsenii Titov | TAUP 2015 | Turin
Today on arXiv:
I. Girardi, S.T. Petcov, A.J. Stuart, A.T., arXiv:1509.02502
𝐺𝑓
𝐺𝑒 𝐺ν
Flavour symmetry group (non-Abelian discrete)
Residual symmetries of the CL and neutrino mass matrices
=>Sum rules for cos δ
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Exact (within the schemes considered) sum rules for cos δ
Relatively large CP-violating effects in neutrino oscillations in the cases of TBM, GRA, GRB, HG and suppressed ones in the case of BM
Sufficiently precise measurement of δ combined with prospective precision on the neutrino mixing angles can provide information about the existence of a new type of fundamental symmetry in the lepton sector
Conclusions
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Backup
1609.09.2015 Arsenii Titov | TAUP 2015 | Turin
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1) χi2 being extracted from Capozzi et. al., PRD 89 (2014) 093018
2) Gaussian approximation:
Statistical details
and are b.f.v. and 1σ uncertainties
are parameters of the scheme
1709.09.2015 Arsenii Titov | TAUP 2015 | Turin
Future:
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Statistical details: comparison
1809.09.2015 Arsenii Titov | TAUP 2015 | Turin
1)
2)
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Predictions for cos δ: statistical analysis
1909.09.2015 Arsenii Titov | TAUP 2015 | Turin
Likelihood function
R12(θe12) R23(θe
23)
Using latest results on sin2 θij and δ, obtained in global analysis of neutrino oscillation data in Capozzi et. al., PRD 89 (2014) 093018
Using prospective 1σ uncertainties on sin2 θij:0.7% for sin2 θ12 (JUNO)
3% for sin2 θ13 (Daya Bay)5% for sin2 θ23 (NOvA and T2K)
+ Gaussian approximation
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Dependence on best fit values
2009.09.2015 Arsenii Titov | TAUP 2015 | Turin
Likelihood function
R12(θe12) R23(θe
23)
(sin2 θ12)bf = 0.304
(sin2 θ23)bf = 0.579
(sin2 θ13)bf = 0.0219
(sin2 θ12)bf = 0.332
(sin2 θ23)bf = 0.437
(sin2 θ13)bf = 0.0234Gonzalez-Garcia et. al., JHEP 1411 (2014) 052
IO neutrino mass spectrum
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Predictions for δ: statistical analysis
2109.09.2015 Arsenii Titov | TAUP 2015 | Turin
R12(θe12) R23(θe
23)
NO schemeIO scheme
NO global fitIO global fit
Using latest results on sin2 θij and δ, obtained in global analysis of neutrino oscillation data in Capozzi et. al., PRD 89 (2014) 093018
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Results for sin2 θ23: statistical analysis
2209.09.2015 Arsenii Titov | TAUP 2015 | Turin
R12(θe12) R23(θe
23)
NO schemeIO scheme
NO global fitIO global fit
Using latest results on sin2 θij and δ, obtained in global analysis of neutrino oscillation data in Capozzi et. al., PRD 89 (2014) 093018
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Predictions for cos δ: statistical analysis
2309.09.2015 Arsenii Titov | TAUP 2015 | Turin
Likelihood function
R13(θe13) R23(θe
23)
Using latest results on sin2 θij and δ, obtained in global analysis of neutrino oscillation data in Capozzi et. al., PRD 89 (2014) 093018
Using prospective 1σ uncertainties on sin2 θij:0.7% for sin2 θ12 (JUNO)
3% for sin2 θ13 (Daya Bay)5% for sin2 θ23 (NOvA and T2K)
+ Gaussian approximation
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Results for sin2 θ23: statistical analysis
2409.09.2015 Arsenii Titov | TAUP 2015 | Turin
NO schemeIO scheme
NO global fitIO global fit
R13(θe13) R23(θe
23)
Using latest results on sin2 θij and δ, obtained in global analysis of neutrino oscillation data in Capozzi et. al., PRD 89 (2014) 093018
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Predictions for cos δ: statistical analysis
2509.09.2015 Arsenii Titov | TAUP 2015 | Turin
Likelihood function
R12(θe12)
Using latest results on sin2 θij and δ, obtained in global analysis of neutrino oscillation data in Capozzi et. al., PRD 89 (2014) 093018
[θν13, θν
12]: Case I = [π/10, − π/4] Case II = [π/20, arcsin (1/√(2+r))]Case III = [π/20, − π/4] Case IV = [arcsin (1/3), − π/4] Case V = [π/20, π/6]
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Predictions for cos δ: statistical analysis
2609.09.2015 Arsenii Titov | TAUP 2015 | Turin
R12(θe12)
[θν13, θν
12]: Case I = [π/10, − π/4] Case II = [π/20, arcsin (1/√(2+r))]Case III = [π/20, − π/4] Case IV = [arcsin (1/3), − π/4] Case V = [π/20, π/6]
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Predictions for cos δ: statistical analysis
2709.09.2015 Arsenii Titov | TAUP 2015 | Turin
Likelihood function
R13(θe13):
Using latest results on sin2 θij and δ, obtained in global analysis of neutrino oscillation data in F. Capozzi et. al., PRD 89 (2014) 093018
[θν13, θν
12]: Case I = [π/20, π/4] Case II = [arcsin (1/3), π/4]Case III = [π/20, arcsin (1/√3)] Case IV = [π/10, π/4] Case V = [π/20, arcsin (√(3−r)/2)]
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Predictions for cos δ: statistical analysis
2809.09.2015 Arsenii Titov | TAUP 2015 | Turin
R13(θe13)
[θν13, θν
12]: Case I = [π/20, π/4] Case II = [arcsin (1/3), π/4]Case III = [π/20, arcsin (1/√3)] Case IV = [π/10, π/4] Case V = [π/20, arcsin (√(3−r)/2)]