flavor mixing, neutrino masses, and neutrino oscillations

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Flavor Mixing, Neutrino Masses, and Neutrino Oscillations. H. Fritzsch CERN. Standard Model. 28 fundamental constants. 4. G. 14. G. 28. G. (22 related to fermion masses). Masses of W-Bosons:. ? Higgs Mechanism ?. Mass and Symmetry Breaking. Brout-Englert, Higgs, Kibble. - PowerPoint PPT Presentation

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Page 1: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 2: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 3: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

G s

w

Page 4: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

G s

wu

d

wM

HM

sun

atm

choozl

Page 5: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

G

um

s

w

dm

tmbm

em

m

cm

u

d

sm

m

wM

HM2m

1m

3m

sun

atm

choozl

2

3

Page 6: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 7: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

GeV2462

v

Page 8: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Fermion Masses: ArbitraryFermion Masses: Arbitrary

L

R

lbGeVMeVme30100002246000002105110 ...

GeVMEVm

GeVMeVm

_246...0072.0__1777

_24600043.0_66.105

Page 9: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 10: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Quark Masses:Quark Masses:

Observed:Observed:

m(c) : m(t) = m(u):m(c) m(c) : m(t) = m(u):m(c) 1/207 1/2071/207 1/207

m(s):m(b) = m(d):m(s)m(s):m(b) = m(d):m(s) 1/23 1/231/23 1/23

Page 11: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 12: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 13: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 14: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 15: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

III

II

I

Page 16: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

ba

a0

Page 17: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 18: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Relations between masses and Relations between masses and

mixing anglesmixing angles

c

uu m

marctan

s

dd m

marctan

c

ui

s

dc m

me

m

m

21.0s

d

m

m07.0

c

u

m

m

o13

Page 19: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

c

u

m

m

090sd mm /

Page 20: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

2sin / /c d s u cm m m m

0 a

a b

Page 21: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

III

II

I

Page 22: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

100

0

0

0

0

00

100

0

0

dd

ddi

uu

uu

cs

sc

cs

sc

e

cs

sc

V

Page 23: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

tan /d d sm m tan /u u cm m

0 0

0

A

A C B

B D

0 0

0

A

A C B

B D

Page 24: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 25: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

c

u

m

m

090sd mm /

Page 26: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 27: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Thus far neutrinos have been used as tools, Thus far neutrinos have been used as tools, likelike

electrons, to study nuclear matterelectrons, to study nuclear matter(quark distributions etc.)(quark distributions etc.)

New focus now: New focus now: What type of mass? What type of mass? How big or small are masses?How big or small are masses?How big are the mixing angles?How big are the mixing angles?Relations among angles and masses?Relations among angles and masses?

Page 28: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

23322 105.2 eVm

25221 108 eVm

Page 29: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Ewigkeit ist lang, speziell gegen dem Ende zu.W.A.

Page 30: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 31: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Neutrino masses:Neutrino masses: A: masses about 1 eVA: masses about 1 eV m(1) = 0.94 eV m(1) = 0.94 eV m(2) = 0.95 eV m(2) = 0.95 eV m(3) = 1 eV (nearly m(3) = 1 eV (nearly degenerate)degenerate)

Page 32: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Neutrino masses:Neutrino masses: B: masses much smaller than 1 eV B: masses much smaller than 1 eV m(1) = 0 eV m(1) = 0 eV m(2) = 0.009 eV m(2) = 0.009 eV m(3) = 0.06 eV (strong m(3) = 0.06 eV (strong hierarchy)hierarchy)

Page 33: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Neutrino masses:Neutrino masses: C: neither hierarchy nor degeneracy C: neither hierarchy nor degeneracy m(1) = 0.10 eV m(1) = 0.10 eV m(2) = 0.14 eV m(2) = 0.14 eV m(3) = 0.29 eV m(3) = 0.29 eV

Page 34: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

See-saw mechanism:See-saw mechanism:

Mm

mM

0

Mm

Mmm

2

21 /

Page 35: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Ex.: tau-neutrino mass at Ex.: tau-neutrino mass at about 1 eV:about 1 eV:

GeVM

eVMGeV9

2

1016.3

_1/)777,1(

Page 36: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 37: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

SU(5) theory SU(5) theory with with

supersymmetry supersymmetry okok

Page 38: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 39: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 40: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Electroweak theory:Electroweak theory:

SU(2) x SU(2) x U(1)SU(2) x SU(2) x U(1)

U(1): (B-L)U(1): (B-L)

Page 41: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Electroweak theory:Electroweak theory:

SU(2) x SU(2) x U(1)SU(2) x SU(2) x U(1)

U(1): (B-L)U(1): (B-L)

Page 42: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 43: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

O(10)

Page 44: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 45: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Neutrino Masses: Neutrino Masses:

Mass terms for Mass terms for charged leptons and charged leptons and neutrinos are not neutrinos are not parallel parallel

Neutrino MixingNeutrino Mixing

Page 46: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

321 ......... e

Page 47: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

321

321

321

VVV

VVV

VVV

Veee

Page 48: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

332211 eeee VVV

332211 VVV

332211 VVV

Page 49: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Neutrino mixingNeutrino mixing

V=UxPV=UxP

100

00

00

i

i

e

e

P

100

0

0

0

0

00

100

0

0

cs

sc

cs

sc

e

cs

sc

U

i

ll

ll

sun at anglereactorl

Page 50: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

oat

o

osun

o

2.538.36

2.3930

23322 105.2 eVm 252

21 108 eVm

70.060.038.0

70.060.038.0

05.054.084.0

V

Page 51: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

34.6

45

4.6

0.821 0.568 0.08

0.047 0.40 0.03 0.58 0.70

0.047 0.40 0.03 0.58 0.70

osun

oatm

ochooz

i i

i i

V e e

e e

Page 52: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

100

0

0

0

0

00

100

0

0

cs

sc

cs

sc

e

cs

sc

U

i

ll

ll

2

1tanm

m 0695.0tan

m

mel

Page 53: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Observation:Observation:

oo 45__33

42.0/

:

21 mm

Page 54: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Neutrino masses fixed, Neutrino masses fixed, sincesincethe mass differences are the mass differences are given by the experiment,given by the experiment,and the angles are fixed and the angles are fixed by the mass matrixby the mass matrix

Page 55: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

19.0/ 32

3

2

1

mm

m

m

m

Page 56: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 57: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Neutrino masses less Neutrino masses less hierarchical than the hierarchical than the masses of the charged masses of the charged leptonsleptons

Page 58: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 59: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 60: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Double Beta DecayDouble Beta Decay

Page 61: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

DB

BA

A

M

0

0

00

Page 62: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

1

2 2 3

2

/ 14

/ 26

40

sin 0.97

o

o

o

m m

m m

1 2

Page 63: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

The atm. angle is the sum of the two large The atm. angle is the sum of the two large angles (14 and 26 degrees).angles (14 and 26 degrees).

Page 64: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

321

321

321

VVV

VVV

VVV

Veee

Page 65: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

052.02

13

m

mV ee

Page 66: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations
Page 67: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

Conclude:Conclude:

Fermion masses remain a mystery.Fermion masses remain a mystery.Neutrino masses might be Dirac masses or Neutrino masses might be Dirac masses or Majorana masses.Majorana masses.

Mixing angles for quarks are fixed by ratios of Mixing angles for quarks are fixed by ratios of quark masses. Very good agreement with quark masses. Very good agreement with experiment.experiment.

Page 68: Flavor Mixing,  Neutrino Masses, and Neutrino Oscillations

This works also well for leptons. One finds, This works also well for leptons. One finds, using the observed mass differences:using the observed mass differences:

m(1)/m(2)=0.42, m(2)/m(3)=0.19.m(1)/m(2)=0.42, m(2)/m(3)=0.19.

m(1): 0.0041 eV m(1): 0.0041 eV m(2): 0.0097 eVm(2): 0.0097 eV m(3): 0.051 eVm(3): 0.051 eV

Atmospheric angle about 40 degreesAtmospheric angle about 40 degreesNeutrinoless double beta decay: difficultNeutrinoless double beta decay: difficultReactor neutrinos: V (3e) ~ 0.052Reactor neutrinos: V (3e) ~ 0.052