cosmological matter-antimatter asymmetry and neutrino oscillations

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Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations Zhi-zhong Xi ng (IHEP, Beiji ng) A Conjecture + An Ans atz Seesaw + Leptogenesis -Mixing + Baryogenes is Space Part 06, Beijing, 19-21 April 2006

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Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations. Zhi-zhong Xing (IHEP, Beijing).  A Conjecture + An Ansatz  Seesaw + Leptogenesis   - Mixing + Baryogenesis. Space Part 06, Beijing, 19-21 April 2006. Motivation: the new minimal SM. - PowerPoint PPT Presentation

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Page 1: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

Zhi-zhong Xing

(IHEP, Beijing)

A Conjecture + An Ansatz

Seesaw + Leptogenesis

-Mixing + Baryogenesis

Space Part 06, Beijing, 19-21 April 2006

Page 2: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

Motivation: the new minimal SM

Experimental/Observational Evidence for NP:

• Dark Matter

• Dark Energy

• Cosmic Inflation

• Cosmic Baryon Asymmetry

• Atmospheric & Solar Neutrino Oscillations

Davoudiasl, Kitano, Li, Murayama, hep-ph/0405097NMSM = MSM + New Physics(Minimal number of new degrees of freedom)

Page 3: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

Can one stone kill two big birds?

2 Right-handed neutrinos added:

• Principle of minimal particle content

• SU(2)U(1) gauge symmetry preserved

2

1R N

Nv

The minimal seesaw model:Frampton, Glashow, Yanagida, hep-ph/0208157; ……

Seesaw+Leptogenesis {Neutrino OscillationsBaryon Asymmetry

Page 4: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

3 Right-handed neutrinos more freedomConjecture: Universal Geometric Neutrino Mass Hierarchy

Light Heavy

Quarks

Is there special -mass hierarchy?

Z.Z.X., hep-ph/0406047 (for both light and heavy );Kaus, Meshkov, hep-ph/0410024 (for light );Tsujimoto, hep-ph/0501023 (for heavy ).

?

Page 5: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

A plot of fermion mass spectrum

(a nomal neutrino mass hierarchy is assumed)

Gaps: eV — MeV; and TeV — RH -mass scale

Page 6: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

Quantum correction

10 GeV10 M3

M2M1

Leptogenesis

10 GeV 2

m3

m2

m1

Oscillations

Seesaw

A phenomenological picture:

Page 7: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

AtmSun

3Geometric -mass hierarchy:

at electroweak scale

Page 8: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

Renormalization-group equations

Further Conjecture:

Minimal SM case

at the seesaw scale

Page 9: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

Seesaw-invariant Fritzsch texture

Seesaw invariance!

Conjecture: Y_ and M_R Fritzsch Texture

Phase condition

Seesaw relation:

Page 10: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

MNS lepton flavor mixing matrixCharged leptons: at the seesaw scale

The MNS matrix V arises from mismatch between the diagonalizations of Y_l and Y_ . Due to the normal hierarchy of m_i , RGE effects on V is negligibly small from seesaw to electroweak scales.

At low scales, the Fritzsch-like texture of lepton mass matrices is found to be compatible with the present neutrino data at the 3 level. (Z.Z.X. 02; Z.Z.X., S. Zhou 04)

Page 11: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

Isomeric textures and FTY seesawIf M_l and M_ take a parallel a

nd Fritzsch-like form, there are 6 different combinations. Their consequences on lepton flavor mixing are exactly the same --- an isomeric feature! (This feature is also true when the leptogenesis is concerned.)

A seesaw ansatz with Fritzschform of M_l and M_D , but M_R = 11 (3 degenerate heavyneutrinos) by Fukugita, Tanimoto, Yanagida (93, 03): At low scales: better fit to current neutrino oscillations; At seesaw scale: no leptogenesis due to N-degeneracy.

Page 12: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

Leptogenesis at the seesaw scale

lN i c

i lN

CP violation

Lepton-number-violating decays:

Fukugita, Yanagida 86

Page 13: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

Baryogenesis via Leptogenesis

Out of thermal equilibrium and N_1 decay

Net baryon asymmetry via sphaleron

Net lepton asymmetry

Observation:

Page 14: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

CP asymmetry in our ansatz

where

Dilution factor

(A)

(B)

in which

{

Page 15: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

Input

M1, random

The allowed ranges of M_1 and

Page 16: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

L

Page 17: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

Some further comments:

• The cosmological baryon asymmetry and the present -oscillation data can simultaneously be interpreted in this phenomenological ansatz

50tan • YB can be extended to the MSSM for • The CP-violating asymmetry has no direct connection with the low-energy CP violation in neutrino oscillations

1

• Replace

by

The result is stable, but more free parameters.

Page 18: Cosmological Matter-Antimatter Asymmetry and Neutrino Oscillations

Leibniz: why is there something rather than

nothing?

Concluding question

Thanks