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Introduction to Neutrino Oscillation Physics

Carlo Giunti

INFN, Sezione di Torino, and Dipartimento di Fisica Teorica, Universit`a di Torino mailto://[email protected]

Neutrino Unbound:http://www.nu.to.infn.it

9-13 June 2008, Benasque, Spain NUFACT’08 School

C. Giunti and C.W. Kim

Fundamentals of Neutrino Physics and Astrophysics

Oxford University Press 15 March 2007 – 728 pages

(2)

Part I: Theory of Neutrino Masses and Mixing Dirac Neutrino Masses

Majorana Neutrino Masses Dirac-Majorana Mass Term

(3)

Part II: Neutrino Oscillations in Vacuum and in Matter Neutrino Oscillations in Vacuum

CPT, CP and T Symmetries Two-Neutrino Oscillations Neutrino Oscillations in Matter

(4)

Part I

Theory of Neutrino Masses and Mixing

(5)

Dirac Neutrino Masses

Dirac Neutrino Masses Dirac Mass

Higgs Mechanism in SM Dirac Lepton Masses

Three-Generations Dirac Neutrino Masses Massive Chiral Lepton Fields

Massive Dirac Lepton Fields Quantization

Mixing

Flavor Lepton Numbers Total Lepton Number Mixing Matrix

Standard Parameterization of Mixing Matrix CP Violation

Example: #12= 0 Example: #13==2 Example: m2= m3

Jarlskog InvariantC. Giunti Neutrino Oscillation Physics 9-13 June 2008, Benasque, Spain 5

(6)

Dirac Mass

Dirac Equation: (i / m)(x) = 0 (/ )

Dirac Lagrangian: L(x) =(x) (i / m)(x)

Chiral decomposition: L 

1 5

2 ; R  1 + 5

2 

=L+R

L =Li/ L+Ri/ R m(LR+RL)

In SM only L =) no Dirac mass

Oscillation experiments have shown that neutrinos are massive

Simplest extension of the SM: addR

(7)

Higgs Mechanism in SM

SM: fermion masses are generated through the Higgs mechanism

Higgs Doublet: Φ(x) = 

+(x)



0(x)

!

Higgs Lagrangian: LHiggs= (DΦ)y(DΦ) V(Φ)

Higgs Potential: V(Φ) =2ΦyΦ +yΦ)2

2

<0,>0=) V(Φ) =



ΦyΦ v22

2

, withv 

q



2



Vacuum: Vmin for ΦyΦ = v22 =)hΦi= p1

2

0 v

!

Spontaneous Symmetry Breaking: SU(2)LU(1)Y !U(1)Q

Unitary Gauge: Φ(x) = p1

2

0 v+ H(x)

!

(8)

Dirac Lepton Masses

LL L

`L

!

`R R

Lepton-Higgs Yukawa Lagrangian LH

;L= y`LLΦ`R yLLΦeR + H.c.

Unitary Gauge

Φ(x) = 1

p

2

0 v+ H(x)

!

Φ = ie 2Φ= 1

p

2

v+ H(x) 0

!

LH

;L= y`

p

2



L `L

 0

v+ H(x)

!

`R

y

p

2



L `L

 v+ H(x) 0

!

R + H.c.

(9)

LH

;L= y` v

p

2

`L`R y v

p

2

LR

y`

p

2

`L`RH y

p

2

LRH+ H.c.

m`= y` v

p

2 m = y v

p

2 g`H = y`

p

2 = m`

v gH = y

p

2 = m

v

(10)

Three-Generations Dirac Neutrino Masses

L0eL 

0



 0

eL

` 0

eL eL0

1

A L0

L 

0



 0

L

` 0

L

0

L

1

A L0

L

0



 0

L

` 0

L

0

L

1

A

` 0

eR eR0 `0R 

0

R `

0

R 

0

R

 0

eR 

0

R 

0

R

Lepton-Higgs Yukawa Lagrangian LH

;L=

X

; =e;;

h

Y0`

L0

LΦ`0 R + Y 0

L0

LΦe 0R

i

+ H.c.

Unitary Gauge

Φ(x) = p1

2

0



0 v+ H(x)

1

A

Φ = ie 2Φ= p1

2

0



v+ H(x) 0

1

A

(11)

LH

;L=

v+ H

p

2



X

; =e;;

h

Y 0`

` 0

L`

0

R + Y 0

 0

L

0

R

i

+ H.c.

LH

;L=

v+ H

p

2



h

0LY0`0R + νL0 Y0νR0

i

+ H.c.

0L 0

B



eL0

 0

L

 0

L

1

C

A0R  0

B



eR0

 0

R

 0

R

1

C

A νL0  0

B



 0

eL

 0

L

 0

L

1

C

A νR0  0

B



 0

eR

 0

R

 0

R

1

C

A

Y0`

0

B



Yee0` Ye0`



Ye0`



Y0`

e Y0`



Y0`



Y0`e Y0` Y0` 1

C

A Y0 

0

B



Yee0 Ye0



Ye0



Y0

e Y0



Y0



Y0

e Y0



Y0



1

C

A

M0`= v

p

2Y0` M0 = v

p

2Y0

(12)

LH

;L=

v+ H

p

2



h

0LY0`0R + νL0 Y0νR0

i

+ H.c.

Diagonalization of Y0` andY0 withunitary VL`,VR`,VL,VR0L= VL`L0R = VR`R νL0 = VLnL νR0 = VRnR

Kinetic terms are invariant under unitary transformations of the fields

LH

;L=

v+ H

p

2



h

LVL`yY0`VR`R+ νLVLyY0VRνR

i

+ H.c.

VL`y Y0` VR` = Y` Y ` = y ` Æ

( ; = e;;) VLy Y0 VR = Y Ykj = ykÆkj (k;j = 1;2;3)

Real and Positive y `,yk

(13)

VLyY0VR = Y () Y0 = VRy Y VL 2N2 N2 N N2

18 9 3 9

(14)

Massive Chiral Lepton Fields

L= VL`y0L 0

B

B

B

B



eL

L

L

1

C

C

C

C

A

R = VR`y0R  0

B

B

B

B



eR

R

R

1

C

C

C

C

A

nL= VLyνL0  0

B

B

B

B



1L

2L

3L

1

C

C

C

C

A

nR = VRyνR0  0

B

B

B

B



1R

2R

3R

1

C

C

C

C

A

LH

;L=

v+ H

p

2



h

LY`R + nLYnR

i

+ H.c.

=

v+ H

p

2



"

X

=e;;

y `

`

L` R +

3

X

k=1

ykkLkR

#

+ H.c.

(15)

Massive Dirac Lepton Fields

`

`

L+` R ( = e;;)

k =kL+kR (k = 1;2;3) LH

;L=

X

=e;;

y `v

p

2

`

`

3

X

k=1

ykv

p

2

kk Mass Terms

X

=e;;

y ` p

2

`

`

H

3

X

k=1

yk

p

2

kkH Lepton-Higgs Couplings Charged Lepton and Neutrino Masses

m = y`

v

p

2 ( = e;;) mk = ykv

p

2 (k = 1;2;3) Lepton-Higgs coupling /Lepton Mass

(16)

Quantization

k(x) =

Z d3p (2)32Ek

X

h=1



a(h)k (p) uk(h)(p) e ipx+ b(h)k

y

(p) vk(h)(p) eipx



p0 = Ek =

q

~p2+ m2k (/p mk) u(h)k (p) = 0 (/p+ mk) vk(h)(p) = 0

~p~Σ

j~pj u(h)k (p) = h uk(h)(p)

~p~Σ

j~pj vk(h)(p) = h vk(h)(p)

fa(h)k (p);a(h

0)y

k (p0)g=fb(h)k (p);b(h

0)y

k (p0)g= (2)32EkÆ3(~p ~p0)Æhh0

fa(h)k (p);a(h

0)

k (p0)g=fa(h)k y(p);a(h

0)y

k (p0)g= 0

fb(h)k (p);b(h

0)

k (p0)g=fbk(h)y(p);b(h

0)y

k (p0)g= 0

fa(h)k (p);b(h

0)

k (p0)g=fa(h)k y(p);b(h

0)y

k (p0)g= 0

fa(h)k (p);b(h

0)y

k (p0)g=fa(h)k y(p);b(h

0)

k (p0)g= 0

(17)

Mixing

Charged-Current Weak Interaction Lagrangian L(CC)

I = g

2

p

2jW W+ H.c.

Weak Charged Current: jW = jW

;L+ jW

;Q

Leptonic Weak Charged Current jW

;L =

X

=e;;

 0





1 5



` 0

= 2

X

=e;;

 0

L



` 0

L= 2 νL0 0L0

L= VL`L ν0

L= VLnL

jW

;L= 2 nLVLy VL`L= 2 nLVLyVL` L= 2 nLUy L Mixing Matrix

Uy= VLyVL` U = VL`yVL

(18)

Definition: Left-Handed Flavor Neutrino Fields νL= U nL= VL`yνL0 =

0

B



eL



L



L

1

C

A

They allow us to write theLeptonic Weak Charged Currentas in the SM:

jW

;L= 2 νL

L= 2

X

=e;;



L



`

L

Each left-handed flavor neutrino fieldis associated with the

corresponding charged lepton fieldwhich describes a massive charged lepton (e,,).

In practiceleft-handed flavor neutrino fields are useful for calculations in the SM approximation of massless neutrinos (interactions).

If neutrino masses must be taken into account, it is necessary to use jW

;L= 2 nLUy L= 2

3

X

k=1

X

=e;;

U kkL



`

L

(19)

Flavor Lepton Numbers

Flavor Neutrino Fields are useful for defining Flavor Lepton Numbers

as in the SM

Le L L

(e;e ) +1 0 0 (

; ) 0 +1 0 (

; ) 0 0 +1

Le L L

(ec;e+) 1 0 0





c



;

+



0 1 0

(c

;

+) 0 0 1

L= Le+ L+ L

Standard Model: Lepton numbers are conserved

(20)

Leptonic Weak Charged Current is invariant under the globalU(1) gauge transformations

`

L!ei' ` L  L!ei'  L ( = e;;)

If neutrinos are massless (SM), Noether’s theorem implies that there is, for each flavor, a conserved current:

j

= L





L+`



`



j

= 0 and a conserved charge:

L =

Z

d3x j0

(x) 0L = 0

: L : =

Z d3p (2)32E

h

a( ) y(p) a( ) (p) b(+) y(p) b(+) (p)

i

+

Z d3p (2)32E

X

h=1

h

a(h)y

`

(p) a(h)

`

(p) b(h)y

`

(p) b(h)

`

(p)

i

(21)

Lepton-Higgs Yukawa Lagrangian:

LH

;L=

v+ H

p

2



"

X

=e;;

y `

`

L` R +

3

X

k=1

ykkLkR

#

+ H.c.

Mixing:  L=

3

X

k=1

U kkL () kL =

X

=e;;

U

k L

LH

;L=

v+ H

p

2



X

=e;;

"

y`

`

L` R+ L 3

X

k=1

U kykkR

#

+ H.c.

Invariant for

`

L!ei' ` L;  L!ei'  L

`

R !ei' ` R; 3

X

k=1

U kykkR !ei'

3

X

k=1

U kykkR

But kinetic part of neutrino Lagrangian is not invariant L()

kinetic =

X

=e;;



Li/ L+

3

X

k=1

kRi/ kR

because P3k=1U kykkR is not a unitary combination of the kR’s

(22)

LD

mass=



eL L L

 0

B



mDee mDe meD

mD

e mD



mD



mDe mD mD

1

C

A 0

B



eR



R



R

1

C

A+ H.c.

Le,L,L are not conserved

Lis conserved: L( R) = L( L) ) j∆Lj= 0

(23)

Total Lepton Number

Dirac neutrino masses violateconservation of Flavor Lepton Numbers

Total Lepton Number is conserved, because Lagrangian is invariant under the global U(1)gauge transformations

kL!ei'kL; kR !ei'kR (k = 1;2;3)

`

L!ei'` L; ` R !ei'` R ( = e;;)

From Noether’s theorem:

j =

3

X

k=1

k



k +

X

=e;;

`



`



j = 0 Conserved charge: L =

Z

d3x j0

(x) 0L = 0 : L : =

3

X

k=1

Z d3p (2)32E

X

h=1

h

a(h)ky(p) a(h)k (p) b(h)ky(p) b(h)k (p)

i

+

X

=e;;

Z d3p (2)32E

X

h=1

h

a(h)y

`

(p) a(h)

`

(p) b(h)y

`

(p) b(h)

`

(p)

i

(24)

Mixing Matrix

Leptonic Weak Charged Current: jW

;L= 2 nLUy L

U = VL`yVL =

0

B



U11 U12 U13 U21 U22 U23 U31 U32 U33

1

C

A

 0

B



Ue1 Ue2 Ue3 U1 U2 U3

U1 U2 U3

1

C

A

UnitaryNN matrix depends on N2 independent real parameters

N = 3 =)

N(N 1)

2 = 3 Mixing Angles N(N + 1)

2 = 6 Phases

Not all phases are physical observables

Only physical effect of mixing matrix occurs through its presence in the Leptonic Weak Charged Current

(25)

Weak Charged Current: jW

;L = 2

3

X

k=1

X

=e;;

kLU k



`

L

Apart from theWeak Charged Current, the Lagrangian is invariant under the global phase transformations

k !ei'kk (k = 1;2;3); ` !ei' ` ( = e;;)

Performing this transformation, theCharged Currentbecomes jW

;L= 2

3

X

k=1

X

=e;;

kLe i'kU

kei' ` L

jW

;L= 2 e i('1 'e)

| {z }

1 3

X

k=1

X

=e;;

kL e i('k '1)

| {z }

N 1=2

U k ei(' 'e)

| {z }

N 1=2



`

L

There are 1 + (N 1) + (N 1) = 2 N 1 = 5 arbitrary phases of the fields that can be chosen to eliminate 5 of the 6 phases of the mixing matrix

2N 1 and not2N phases of the mixing matrix can be eliminated because a common rephasing of all the fields leaves the Charged Current invariant() conservation of Total Lepton Number.

(26)

The mixing matrix contains N(N + 1)

2 (2 N 1) = (N 1) (N 2)

2 = 1 Physical Phase

It is convenient to express the33 unitary mixing matrix only in terms of the four physical parameters:

3 Mixing Anglesand1 Phase

(27)

Standard Parameterization of Mixing Matrix

0

B



eL



L



L

1

C

A=

0

B



Ue1 Ue2 Ue3 U1 U2 U3

U1 U2 U3

1

C

A 0

B



1L

2L

3L

1

C

A

U = R23W13R12

=

0

B



1 0 0 0 c23 s23 0 s23 c23

1

C

A 0

B



c13 0 s13e iÆ13

0 1 0

s13eiÆ13 0 c13

1

C

A 0

B



c12 s12 0 s12 c12 0 0 0 1

1

C

A

=

0

B



c12c13 s12c13 s13e iÆ13 s12c23 c12s23s13eiÆ13 c12c23 s12s23s13eiÆ13 s23c13

s12s23 c12c23s13eiÆ13 c12s23 s12c23s13eiÆ13 c23c13

1

C

A

cab cos#ab sabsin#ab 0#ab 



2 0Æ132 3 Mixing Angles#12,#23,#13 and1 Phase Æ13

(28)

CP Violation

U = U () CP symmetry

General conditions for CP violation (14 conditions):

1. No two charged leptons or two neutrinos are degenerate in mass (6 conditions)

2. No mixing angle is equal to0or =2 (6 conditions) 3. The physical phase is different from 0or(2 conditions)

These 14 conditions are combined into the single condition det C 6= 0 C = i[M0M0y;M0`M0`y]

det C = 2 J



m2

2 m2

1



m2

3 m2

1



m2

3 m2

2





m2



m2e



m2



m2e



m2



m2





Jarlskog invariant: J ==m

h

U3Ue2U2Ue3

i

[C. Jarlskog, Phys. Rev. Lett. 55 (1985) 1039, Z. Phys. C 29 (1985) 491]

[O. W. Greenberg, Phys. Rev. D 32 (1985) 1841]

[I. Dunietz, O. W. Greenberg, Dan-di Wu, Phys. Rev. Lett. 55 (1985) 2935]

(29)

Example:

#12

= 0

U = R23R13W12

W12=

0

B



cos#12 sin#12e iÆ12 0 sin#12e iÆ12 cos#12 0

0 0 1

1

C

A

#12= 0 =) W12=

0

B



1 0 0 0 1 0 0 0 1

1

C

A= 1 real mixing matrix U = R23R13

(30)

Example:

#13

=

=

2

U = R23W13R12

W13=

0

B



cos#13 0 sin#13e iÆ13

0 1 0

sin#13eiÆ13 0 cos#13

1

C

A

#13==2 =) W13=

0

B



0 0 e iÆ13

0 1 0

eiÆ13 0 0

1

C

A

U =

0

B



0 0 e iÆ13

s12c23 c12s23eiÆ13 c12c23 s12s23eiÆ13 0 s12s23 c12c23eiÆ13 c12s23 s12c23eiÆ13 0

1

C

A

(31)

U =B

0 0 e iÆ13

jU1jei1 jU2jei2 0

jU1jei1 jU2jei2 0

C

A



1 2=1 2 1 1 =2 2

k !ei'kk (k = 1;2;3); `

!ei' ` ( = e;;) U !



e i'e 0 0 0 e i' 0 0 0 e i'

 0 0 e iÆ13

jU1jei1 jU2jei2 0

jU1jei1 jU2jei2 0

!



ei'1 0 0 0 ei'2 0 0 0 ei'3



U = 0 0

ei( Æ13 'e +'3)

jU1jei(1 '+'1)jU2jei(2 '+'2) 0

jU1jei(1 '+'1) jU2jei(2 '+'2) 0

!

'1= 0 '=1 ' =1 '2=' 2=1 2

'2=' 2=1 2=1 2 OK!

U =

 0 0 1

jU1j jU2j 0

jU1j jU2j 0



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