Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

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Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.
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Transcript of Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Page 1: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Neutrino Mass and Grand Unification of Flavor

R. N. Mohapatra

Goranfest, June 2010Split.

Page 2: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Brief Remembrances CCNY-70’s: Turbulent times

Look back, Look at, Look ahead Joy was doing physics…

Page 3: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Two Outstanding Problems in Particle Physics Today

Origin of Mass: --Higgs, SUSY, Extra D --LHC will probe this:

Origin of Flavor: (this talk)

-- Many non-collider probes:

Page 4: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Quark, Lepton flavor:Definitions

Masses and mixings- two aspects of flavor Def.

Mass basis: and for neutrinos

.., chmlMlQMQL TRlLRduqLmass

diaglqRlqL MUMU ,,

tbtstd

cbcscd

ubusud

VVV

VVV

VVV

321

321

321

UUU

UUU

UUU eee

duCKM UUV UUU lPMNS

Page 5: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Flavor Puzzle < 1998: Quark masses and mixings (at GUT

scale) Up quarks:

Down quarks: Mixings: Leptons: Note:

WHY ?

1:03.0:002.0:: bsd mmm003.0;037.0;22.0 ubcbus VVV

58.1:093.0:0005.0:: mmme

sb mmmm 3;

82:2.0:0008.0

Page 6: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Attempts to Understandusing texture zeros

Relation: d-s mass matrix

(Weinberg;

Wilczek,Zee; Fritzsch)

Also GUT scale relations: and Finally at GUT scale, This implies: Md= whereas Ml = (Georgi, Jarlskog)

s

dus m

mV

ba

a0

s

d

m

m

][][ dlsde MDetMDetmmmm

mmb

smm 3

ba

a0

ba

a

3

0

Page 7: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Neutrino mass discovery has added to this puzzle !

What we know about neutrino masses ? Masses: ; Mixings:

; Overall mass scale: < .1- 1 eV (roughly) To be determined (expts in progress or planning)

(i) Majorana or Dirac ? (ii) Mass ordering: normal or inverted? (iii) Value of (iv) Any possible CP violation ?

252 1067.7 eVmsol 232 1039.2 eVmAtm

;312.sin 122 466.sin 23

2 04.sin 132

13

Page 8: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

An Interesting mixing pattern ?

Tri-bi-maximal mixing for neutrinos:

U=

(Harrison, Perkins, Scott; Xing; He, Zee)

Is it exact ? If not how big are corrections ?

Page 9: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

New Challenges posed by neutrino masses

(i) ? (ii) Flavor issues : A.

B.

lqmm ,

04.07.0 2323 CKMl VV

b

sC

atm

sol

m

m

m

m

m

m,

Quarks and leptons so different- is a unified description of

Flavor possible ?

Page 10: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Hints for a strategy for flavor

Small quark mixings:

Mass hierarchy for quarks and charged leptons: suggests:

Large mixings for leptons unrelated.

Unifying quark-lepton flavors: GUTs

00du MM

,,

,,0

00

000

000

~

bt

ldu

m

M

MM l ,

Page 11: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Basic strategy to unify quark-lepton flavor:

Assumption (I): Suppose a theory gives: (Dutta, Mimura, RNM’PRD-

09)

Choose basis sof diagonal. Then lepton mixings are given by the matrix that diagonalizes;

For anarchic M0, quark mixings are small while

lepton mixings are large.

dd rMM 0 Lfvm

uu MM 0

0,, Mldu

ll rMM 0

Page 12: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

How to see that ? Suppose: Then Since off-diagonal

elements of V are small.

On the other hand, whose matrix

elements are large.

diagMUMU 000

VVUUVCKM 00

0,, Mldu

0UPMNSU

diagdMVU

0

Page 13: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Rank One mechanism and mass hierarchy

Assumption (II): M0 has rank one i.e.

gives mass to third gen fermions: t, b, tau + others are massless. Turn on Other fermions c,s,mu pick up mass with and relates mixings to

masses

0M

0,, Mldu

,,,, btsc mm

mmb

Page 14: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Illustration for 2-Gen. case

Suppose and

angle; chosen large; f <<h.

Predictions: consistent

with

observations:

),( 32 diagf

.Atm

bmm tancb

b

s Vm

m

0M du ,

Page 15: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Making model predictive

Key idea: SM sym for massless fermions :[SU(3)]^5;

Choose subgroup: Discrete subgroup with 3-d. rep.

Replace Yukawa’s by scalar fields (flavons);

Minima of the flavon theory Yukawas:

GUT theory that realizes the new ansatz for flavor

Page 16: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

What kind of GUT theory ?

Recall ansatz: as

In SM, singlets- so Mu, Md unrelated. We need a theory where, are in a

doublet.

Left-Right symmetric and SO(10) (which contains LR) are precisely

such theories.

uu MM 0

dd rMM 0

dudu MM ,0,

Ru Rd

R

R

d

u

cLBRL SUUSUSU )3()1()2()2(

Page 17: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Neutrino mass and seesaw also suggest LR and SO(10)

SM: nu mass Add

Adding RH neutrino for nu mass left-right

sym.unification based on SU(2)LxSU(2)RxU(1)B-L xSU(3)C and SO(10)

L

L

d

u

L

L

e

Ru

Rd

Re R

L

L

d

u

R

R

d

u

L

L

e

R

R

e

P

P

Page 18: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

SUSY SO(10) Features Minimal GUT group with complete fermion

unification (per family) is SO(10)-its spinor rep contains all 16 SM fermions (including RH nu) in single rep.

Has B-L needed to understand why MR<< M_Pl Theory below GUT scale is MSSM: B-L needed for naturally stable dark matter.

Page 19: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

From SO(10) down to the Std Model

SO(10) Nu mass

LR Sym.

Standard Model- -> seesaw

M

0

0

0

M

m

m

0

0)( LB

emc USU )1()3(

cLBRL SUUSUSU )3()1()2()2(

cYL SUUSU )3()1()2(

Page 20: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

SUSY SO(10) and unified understanding of flavor

Fermions in {16}: 16mx16m={10}H+{120}H+{126}H

Only renorm. couplings for fermion masses:

Has SM doublets contributes to fermion mass

{126}H responsible for both neutrino masses and quark masses: helps to connect quark mixings to neutrino mixings: Unifies quark and lepton flavors: (Babu, Mohapatra, 93)

HHHY hfhL ]10,120[1616'6211616101616

Page 21: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Fermion mass formulae in renormalizable SO(10)

Define The mass formulae: Compare with

ansatz

Both sets of formulae identical for f, h’<< h

wkff vMY /

uu MM 0

dd rMM 0

ll rMM 0

Page 22: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Neutrino mass in Renormalizable SO(10):

{126} has an SU(2)L triplet with B-L=2: New formula for nu-mass:

Type II seesaw: gives naturally small v

Two independent parameters:

2

2

M

vv wk

TD

BLD M

fvMfvm

1

Lazaridis, Shafi, Wetterich; R.N.M.,Senjanovic; Schecter, Valle’81RvM ,2

UMM

Page 23: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Type II dominance: If ,first term dominates Then the fermion mass formula become:

: (Bajc, Senjanovic,Vissani’02)

(Babu, Mohapatra’92)

Neutrino mass and quark and charged lepton masses connected and all ingredients of our ansatz are realized in SO(10) .

BLfvM

fvm

Page 24: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Rank One mechanism for Flavor

Generic case does not explain mass hierarchies

Assume h is rank 1 +

For f, h’=0, only 3rd gen. pick up mass. Leads to with f,

h’<<h Gives and ;

fvm

cba

c

b

a

h

hhf ',

mmmm ebds ,, ;

smm 3bmm Catm

sol

m

m ~

Page 25: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Origin of Rank one SO(10)

Rank one model as an effective theory at GUT scale:

Add one vector like matter and singlets: Superpotential: +

Flavor texture depends on < >; with symmetries it can be predicted.

}61{}16{ VV

V V

H

VVM i

ViiW

i

Page 26: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

VEV alignment from flat directions in an S4 model

Examples: S4 triplet flavon case:

While for

Page 27: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

A specific realization with predictive textures:

Group: SO(10)xS4

Consider flavons ; matter {16} Inv effective superpotential at GUT scale:

The flavon vevs align as:

Leading to f= and h’=

Gives realistic model for fermion masses and mixings

2121 11233 3,2,1 2,13 23

Page 28: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Prediction of a specific theory with S4-

symmetry Solar mass

Bottom-tau: and

Leading order PMNS: U

Testable prediction: Bjorken, King, Pakvasa Ferrandis (2004-05)

Double beta mass 3 meV. Dutta, Mimura, RNM

arXiv:0911.2242

catm

solar

m

m

mmb smm 3

05.023

13 c

Page 29: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Prospects for measuring Reactor, Long base line e.g. T2K, NoVA: (Lindner, Huber,Schwetz,Winter’09)

Our prediction 01.02sin 132

Page 30: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

GUTs and Proton decay Proton decay in SUSY GUTs have two

generic sources: (i) Gauge exchange:

(ii) Higgsino exchange:

Present limit: yrsK

33103.2

Page 31: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Present experimental limits

Super-K, Soudan, IMB, Frejus

Page 32: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Rank one also solves the proton decay problem

Proton decay problem in SU(5): one Higgs pair s

In SO(10), there are more Higgs fields and if flavor structure is such that triplet Higgs do not connect, no p-decay problem: Choice flavor structure that does it( Dutta,

Mimura, RNM’05)

dup YYA

Page 33: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Conclusion:(i) New ansatz to unify diverse profiles

of quark and lepton flavor patterns.(ii) SO(10) GUT with type II seesaw

provides a natural framework for realization of this ansatz.

(iii) Predicts measurable and solves proton decay problem of susy GUTs.

Happy Birthday, Goran !

13

Page 34: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Some examples: SUSY Non-SUSY SO(10) SM with seesaw

Page 35: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Simplest example: SUSY SU(5)

Page 36: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Why minimal SU(5) not satisfactory

Minimal model ruled out by proton decay !

Not predictive for neutrinos- so no advantage of GUTs except scale !

However one nice feature: A small piece of the flavor puzzle !!

mmb

Page 37: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Grand unification hypothesis:

• All forces and all matter become one at high energies no matter how different

they are at low energies. Leptons quarks become

same.

Page 38: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

What we need to know: (i) Majorana or Dirac (Nucl matrix element )

(ii) Absolute mass scale: (iii) Mass ordering: (iv) Value of (v) CP phase

13

0

Page 39: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Unified understanding of Flavor in SO(10)

Fermion masses depend on 3 matrices: h, f, h’

Suppose, h >> f and h’=0 and h is anarchic: Choose basis so with Dominant contributions to VCKM cancel out

explaining why CKM angles are small VCKM coming from .

large neutrino mixngs come entirely from charged lepton sector; and hence are large!!

fvm

),,( 321 diagf

3,2,1

llPMNS UUUU

abh

Page 40: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Realistic 3-generation model for Flavor:

Our proposal after diagonalization of h with appropriately rotated f and h’.

Different ansatzes for f and h’ lead to different

realizations of this idea:

Page 41: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

More general Rank one model Predictions for

Depends on solar and atm masses:

13

05.013

Page 42: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Why GUT theory for neutrinos ?

Seesaw paradigm to explain Add right handed neutrinos to SM with

Majorana mass: Breaks B-L : New scale and new physics beyond SM. After EWSB -neutrino mass tiny and neutrino Majorana

RNNNMHNLhL RRY

RM

R

wk

M

vhm

22

Minkowski,Gell-Mann, Ramond, Slansky,Yanagida, Mohapatra, Senjanovic,Glashow

lqmm ,

Page 43: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Seesaw scale Neutrino masses seesaw scale much lower

than Planck scale New symmetry (B-L). Type I seesaw + GUT scale GeV- -Small neutrino mass strong indication for SUSYGUT; Seesaw scale is around TeV Accessible at LHC, other signals, ,

tD mm GeVM R

1410 1610

2atmm

eD mm

e 0

Page 44: Neutrino Mass and Grand Unification of Flavor R. N. Mohapatra Goranfest, June 2010 Split.

Why Supersymmetry ?

Simple picture of force Unification:

Predicts correct Weinberg angle

Candidate for Dark matter