PMNS Matrix Elements Without Assuming Unitarity

Slides:



Advertisements
Similar presentations
Measuring Atmospheric Parameters with SuperBeams Enrique Fernández Martínez Departamento de Física Teórica and IFT Universidad Autónoma de Madrid.
Advertisements

1 Probing CP violation in neutrino oscillations with neutrino telescopes Kfir Blum, Yosef Nir, Eli Waxman arXiv: [hep-ph]
Double Chooz: Collaboration, Experimental concept, Detector, Physics Prospect, Status & Schedule, Summary.
High  Li/B  -Beam Enrique Fernández-Martínez, MPI für Physik Munich Based on a collaboration with: P. Coloma, A. Donini and J. López-Pavón.
1 3+2 Neutrino Phenomenology and Studies at MiniBooNE PHENO 2007 Symposium May 7-9, 2007 U. Wisconsin, Madison Georgia Karagiorgi, Columbia University.
Sergio Palomares-Ruiz June 22, 2005 Super-NO A Based on O. Mena, SPR and S. Pascoli hep-ph/ a long-baseline neutrino experiment with two off-axis.
A 10 minutes mini-review on the flavor problem (mixing, CP- violation) Hisakazu Minakata Based on “minus 10 minutes attack” Fully biased 10 minutes counterattack.
Status of Neutrino Science Hitoshi Murayama LBNLnu April 11, 2003.
Neutrino oscillations and non- standard neutrino-matter interactions (NSI) Cecilia Lunardini INT & UW department of Physics, Seattle A.Friedland, C.L.
Non-Standard Neutrino Interactions Enrique Fernández-Martínez MPI für Physik Munich.
Bounds on Neutrino Non-Standard Interactions Enrique Fernández-Martínez MPI für Physik Munich Based on collaborations with: S. Antusch, J. Baumann, C.
Low-energy neutrino physics Belén Gavela Universidad Autónoma de Madrid and IFT.
3+1 sterile Jacobo López–Pavón IFT UAM/CSIC NuFact IIT, Chicago, July
Can we distinguish among different models for mass in the near future? Carla Biggio Max-Planck-Institut für Physik, München, Germany Convegno informale.
Toyota National College of Technology A.Takamura Collaboration with K.Kimura and T.Yoshikawa GLoBES 2007 Measuring the Leptonic CP Phase in Oscillations.
Neutrino oscillation physics II Alberto Gago PUCP CTEQ-FERMILAB School 2012 Lima, Perú - PUCP.
Osamu Yasuda Tokyo Metropolitan University Model independent analysis of New Physics interactions and implications for long baseline experiments INTERNATIONAL.
Sterile Neutrino Oscillations and CP-Violation Implications for MiniBooNE NuFact’07 Okayama, Japan Georgia Karagiorgi, Columbia University August 10, 2007.
Tests of non-standard neutrino interactions (NSI) Cecilia Lunardini Institute for Nuclear Theory University of Washington, Seattle.
Search for Electron Neutrino Appearance in MINOS Mhair Orchanian California Institute of Technology On behalf of the MINOS Collaboration DPF 2011 Meeting.
Measuring Earth Matter Density and Testing MSW Hisakazu Minakata Tokyo Metropolitan University.
NSI versus NU at the Neutrino Factory Euronu meeting Strasbourg June 2-4, 2010 Walter Winter Universität Würzburg TexPoint fonts used in EMF: AAAAA A A.
1 Luca Stanco, INFN-Padova (for the OPERA collaboration) Search for sterile neutrinos at Long-BL The present scenario and the “sterile” issue at 1 eV mass.
Michel Gonin – Ecole Polytechnique – France : SUPER NOVA SN1987A Super-Kamiokande Introduction neutrino oscillations mixing matrices Introduction.
Sterile neutrinos at the Neutrino Factory IDS-NF plenary meeting October 19-21, 2011 Arlington, VA, USA Walter Winter Universität Würzburg TexPoint fonts.
MiniBooNE MiniBooNE Motivation LSND Signal Interpreting the LSND Signal MiniBooNE Overview Experimental Setup Neutrino Events in the Detector The Oscillation.
BEYOND MFV IN FAMILY SYMMETRY THEORIES OF FERMION MASSES Work done with Zygmunt Lalak and Graham Ross Based on existing ideas but, hopefully, contributing.
Future neutrino oscillation experiments J.J. Gómez-Cadenas U. Valencia/KEK Original results presented in this talk based on work done in collaboration.
Neutrino states in oscillation experiments – are they pure or mixd? Pheno 07, May, 07-09, 2007, Madison, Wisconsin Marek Zralek, Univ. of Silesia.
Osamu Yasuda Tokyo Metropolitan University Summary of Phenomenology Subgroup International scoping study of a future Neutrino Factory and super-beam facility.
October 14th, 2006LONU-LENS, Virginia Tech Solar Luminosity by Neutrinos Solar Luminosity by Neutrinos Carlos Pena Garay IFIC, Valencia ~
THE CONNECTION BETWEEN NEUTRINO EXPERIMENTS AND LEPTOGENESIS Alicia Broncano Berrocal MPI.
Near Detector Tasks EuroNu Meeting, CERN 26 March 2009 Paul Soler.
Carla Biggio Universidad Autónoma de Madrid Neutrino masses and new TeV scale HEP 2007, Manchester, England, 19-25/07/07 Based on: Antusch, CB,
1 A.Zalewska, Epiphany 2006 Introduction Agnieszka Zalewska Epiphany Conference on Neutrinos and Dark Matter, Epiphany Conference on Neutrinos.
New Results from MINOS Matthew Strait University of Minnesota for the MINOS collaboration Phenomenology 2010 Symposium 11 May 2010.
Pontecorvo’s idea An introductory course on neutrino physics (IV)
Leptogenesis beyond the limit of hierarchical heavy neutrino masses
A New Family Symmetry: Discrete Quaternion Group
Neutrino Oscillations and T2K
Determining the neutrino flavor ratio at the astrophysical source
Non-unitary deviation from the tri-bimaximal mixing and neutrino oscillations Shu Luo The Summer Topical Seminar on Frontier of Particle Physics.
η and π0 Decay to Two Neutrinos
Neutrinos and the Evolution
Polarization in charmless B VV decays
Beyond the Standard Model: the clue from charm ...
Detector Baseline EuroNu Meeting, RAL 20 January 2010 Paul Soler.
Lecture 14 – Neutral currents and electroweak unification
cLFV in Seesaw Models (after LHC12, θ and MEG13)
SOLAR ATMOSPHERE NEUTRINOS
Neutrino mass and mixing: 2006 Status
On neutrinoless double beta decay in the nMSM
Prospects of J-PARC Neutrino Program
Pauli´s new particle * nt nm ne e m t Beta-Decay Pa 234 b (electron)
T2KK Sensitivity of Resolving q23 Octant Degeneracy
Naotoshi Okamura (YITP) NuFact05
Neutrino oscillation physics
Future neutrino experiments
Double beta decay and Leptogenesis
Neutrino Masses and Mixings
The Neutrino World: Present and Future Boris Kayser
Probing non-standard neutrino physics at T2KK and neutrino factory
High Energy Physics On the Fukugita-Tanimoto-Yanagida Ansatz with Partially Non-degenerate Right-handed Majorana Neutrinos 29 October,
Will T2KK see new physics?
CKM Unitarity and Kaon Decays
Run-Hui Li Yonsei University
Rome Samanta, University of Southampton
2008/01/26 A. Matsuzaki; Nagoya Univ. A. I. Sanda; Kanagawa Univ
The Hunt for right-Handed Neutrinos
Outline Neutrino History n Oscillations World Tour of n Experiments
Presentation transcript:

PMNS Matrix Elements Without Assuming Unitarity NOW06, September 9-16, 2006, Otranto PMNS Matrix Elements Without Assuming Unitarity Enrique Fernández Martínez Universidad Autónoma de Madrid hep-ph/0607020 In collaboration with S. Antusch, C. Biggio, M.B. Gavela and J. López Pavón Thanks also to C. Peña Garay

Motivations n masses and mixing → evidence of New Physics beyond the SM Typical explanations (see-saw) involve NP at higher energies This NP often induces deviations from unitarity of the PMNS at low energy We will analyze the present constraints on the mixing matrix without assuming unitarity

The general idea

Effective Lagrangian 3 light n deviations from unitarity from NP at high energy

Effective Lagrangian 3 light n deviations from unitarity from NP at high energy Diagonal mass and canonical kinetic terms: unitary transformation + rescaling N non-unitary

Effective Lagrangian 3 light n deviations from unitarity from NP at high energy Diagonal mass and canonical kinetic terms: unitary transformation + rescaling unchanged N non-unitary

The effects of non-unitarity… … appear in the interactions ni ni W - Z nj This affects electroweak processes…

The effects of non-unitarity… … appear in the interactions ni ni W - Z nj This affects electroweak processes… … and oscillation probabilities…

n oscillations in vacuum mass basis

n oscillations in vacuum mass basis flavour basis with ≠

n oscillations in vacuum mass basis flavour basis with ≠

n oscillations in vacuum mass basis flavour basis with ≠ Zero-distance effect:

n oscillations in matter VCC VNC 2 families

n oscillations in matter VCC VNC 2 families 1. non-diagonal elements 2. NC effects do not disappear

N elements from oscillations: e-row Only disappearance exps → information only on |Nai|2 CHOOZ: Δ12≈0 K2K (nm→nm ): Δ23 Degeneracy cannot be disentangled UNITARITY

N elements from oscillations: e-row KamLAND: Δ23>>1 KamLAND+CHOOZ+K2K → first degeneracy solved

N elements from oscillations: e-row KamLAND: Δ23>>1 KamLAND+CHOOZ+K2K → first degeneracy solved SNO: SNO → all |Nei|2 determined

N elements from oscillations: m-row Atmospheric + K2K: Δ12≈0 UNITARITY Degeneracy cannot be disentangled

N elements from oscillations only without unitarity OSCILLATIONS 3s with unitarity OSCILLATIONS González-García 04

(NN†) from decays (NN†)aa W ni la W decays ni Z nj Info on Invisible Z Universality tests W ni la lb g Rare leptons decays Info on (NN†)ab

(NN†) and (N†N) from decays Experimentally

(NN†) and (N†N) from decays Experimentally → N is unitary at % level

N elements from oscillations & decays without unitarity OSCILLATIONS +DECAYS 3s with unitarity OSCILLATIONS González-García 04

In the future… MEASUREMENT OF MATRIX ELEMENTS |Ne3|2 , m-row → MINOS, T2K, Superbeams, NUFACT… t-row → high energies: NUFACT phases → appearance experiments: NUFACTs, b-beams

In the future… MEASUREMENT OF MATRIX ELEMENTS |Ne3|2 , m-row → MINOS, T2K, Superbeams, NUFACT… t-row → high energies: NUFACT phases → appearance experiments: NUFACTs, b-beams TESTS OF UNITARITY Rare leptons decays m→eg t→eg t→mg PRESENT

In the future… MEASUREMENT OF MATRIX ELEMENTS |Ne3|2 , m-row → MINOS, T2K, Superbeams, NUFACT… t-row → high energies: NUFACT phases → appearance experiments: NUFACTs, b-beams TESTS OF UNITARITY Rare leptons decays m→eg t→eg t→mg PRESENT FUTURE ~ 10-6 MEG ~ 10-7 NUFACT

In the future… MEASUREMENT OF MATRIX ELEMENTS |Ne3|2 , m-row → MINOS, T2K, Superbeams, NUFACT… t-row → high energies: NUFACT phases → appearance experiments: NUFACTs, b-beams TESTS OF UNITARITY Rare leptons decays m→eg t→eg t→mg ZERO-DISTANCE EFFECT 40Kt Iron calorimeter near NUFACT ne→nm 4Kt OPERA-like near NUFACT ne→nt nm→nt PRESENT FUTURE ~ 10-6 MEG ~ 10-7 NUFACT

In the future… MEASUREMENT OF MATRIX ELEMENTS |Ne3|2 , m-row → MINOS, T2K, Superbeams, NUFACT… t-row → high energies: NUFACT phases → appearance experiments: NUFACTs, b-beams TESTS OF UNITARITY Rare leptons decays m→eg t→eg t→mg ZERO-DISTANCE EFFECT 40Kt Iron calorimeter near NUFACT ne→nm 4Kt OPERA-like near NUFACT ne→nt nm→nt PRESENT FUTURE ~ 10-6 MEG ~ 10-7 NUFACT

Conclusions If we don’t assume unitarity for the leptonic mixing matrix Present oscillation experiments alone can only measure half the elements EW decays confirms unitarity at % level Combining oscillations and EW decays, bounds for all the elements can be found comparable with the ones obtained with the unitary analysis Future experiments can: improve the present measurements on the e- and m-rows give information on the t-row and on phases (appearance exps) test unitarity by constraining the zero-distance effect with a near detector

Back-up slides

…adding near detectors… Test of zero-distance effect: KARMEN: (NN†)me <0.05 NOMAD: (NN†)mt <0.09 (NN†)et <0.013 MINOS: (NN†)mm =1±0.05 BUGEY: (NN†)ee =1±0.04 → also all |Nmi|2 determined

Non-unitarity from see-saw Integrate out NR d=5 operator it gives mass to n d=6 operator it renormalises kinetic energy Broncano, Gavela, Jenkins 02

Number of events n produced and detected in CC Exceptions: measured flux leptonic production mechanism detection via NC

(NN†) from decays: GF (NN†)aa ni W W decays la ni Info on Z GF is measured in m-decay Wˉ m e ni Nmi N*ej ni Z nj Info on (NN†)aa Invisible Z Universality tests

CHOOZ 10-3

Unitarity in the quark sector Quarks are detected in the final state → we can directly measure |Vab| K0 p - d W+ Vus* ni e+ Uei ex: |Vus| from K0 →p - e+ ne → ∑i|Uei|2 =1 if U unitary With Vab we check unitarity conditions: ex: |Vud|2+|Vus|2+|Vub|2 -1 = -0.0008±0.0011 → Measurements of VCKM elements relies on UPMNS unitarity

Unitarity in the quark sector Quarks are detected in the final state → we can directly measure |Vab| K0 p - d W+ Vus* ne e+ ex: |Vus| from K0 →p - e+ ne With Vab we check unitarity conditions: ex: |Vud|2+|Vus|2+|Vub|2 -1 = -0.0008±0.0011 → Measurements of VCKM elements relies on UPMNS unitarity decays → only (NN†) and (N†N) N elements → we need oscillations to study the unitarity of N: no assumptions on VCKM With leptons: