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Stuart Raby 2009 Workshop on Lepton and Baryon Number Violation U. Wisconsin, Madison September 22, 2009 Testing an SO(10) SUSY GUT + Family Symmetry

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Testing an SO(10) SUSY GUT + Family Symmetry. Stuart Raby. 2009 Workshop on Lepton and Baryon Number Violation U. Wisconsin, Madison September 22, 2009. Outline. Minimal SO(10) SUSY Model 3 rd family only changing BCs at M GUT - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: Stuart Raby

Stuart Raby

2009 Workshop on Lepton and Baryon Number Violation

U. Wisconsin, Madison September 22, 2009

Testing an SO(10) SUSY GUT + Family Symmetry

Page 2: Stuart Raby

Outline Minimal SO(10) SUSY Model

3rd family only changing BCs at MGUT

SO(10) + Family Symmetry

3 family model Conclusions

Page 3: Stuart Raby

Blazek, Dermisek & Raby PRL 88, 111804 (2002) PRD 65, 115004 (2002)Baer & Ferrandis, PRL 87, 211803 (2001)Auto, Baer, Balazs, Belyaev, Ferrandis & Tata JHEP 0306:023 (2003)Tobe & Wells NPB 663, 123 (2003)Dermisek, Raby, Roszkowski & Ruiz de Austri JHEP 0304:037 (2003) JHEP 0509:029 (2005)Baer, Kraml, Sekmen & Summy JHEP 0803:056 (2008) JHEP 0810:079 (2008)

Yukawa Unification & Soft SUSY breaking

Page 4: Stuart Raby

Title of talk 4

16 16 145

10 10 M

6 16 W

Albright, Anderson, Babu, Barr, Barbieri, Berezhiani, Blazek, Carena, Chang, Dermisek, Dimopoulos, Hall, Masiero, Murayama, Pati, Raby, Romanino, Rossi, Starkman, Wagner, Wilczek, Wiesenfeldt, WillenbrockPossible UV completion to strings !!

Effective higher dimension operators, Small rep’s + Many predictions !!

Hierarchical SO(10) Yukawas

Page 5: Stuart Raby

t b Note, CANNOT predict top mass due to large SUSY threshold corrections to bottom and tau mass

So instead use Yukawa unification to predictsoft SUSY breaking masses !!

3 316 1 0 16

Page 6: Stuart Raby

3 316 1 0 16

t b

0 16 10 16

16 1/2 16

2 2

TeV , <<

A m m m

m few M m

tan 50

MSO10SM

Fit t,b,tau requires

TM

Page 7: Stuart Raby

2 2

2

2

10

13%2

d uH H

H

m mm

m

Roughly ½ comes From RG running from G

M m

20 10Varying , ,

arbitraryH

A

A m m

m

Radiative EWSB requires

Blazek, Dermisek & Raby “Just so”

Note, this is difficult in bottom – up approach !!

Page 8: Stuart Raby

2 2

2

2

10

13%2

d uH H

H

m mm

m

BDR “Just so”

22 0ii X X im Q D m

0

16 10

Q U D L E | H H

1 1 -3 -3 1 5 | -2 2

m | m

U D

i

X

i

Q

m

Baer, Kraml & Sekmen arXiv:0908.0134 “DR3”

3 1,216 16m m

Page 9: Stuart Raby

Gauge coupling unification Yukawa unification Inverted scalar mass hierarchy

Bagger, Feng, Polonsky & Zhang PLB473, 264 (2000) Suppresses flavor & CP violation Nucleon decay

MSO10SMTM

Page 10: Stuart Raby

MSO10SM1. Extend to 3 family model in 4D ( Dermisek & Raby PLB 622, 327

(2005). )

2. Extend to orbifold GUT in 5D ( HD Kim, Schradin & Raby, JHEP 0301, 056 (2003) & JHEP 0505, 036

(2005) )

3. Extend to heterotic string in 10D compactified on Z3xZ2 orbifold ( Kobayashi, Raby & Zhang, PLB 593, 262 (2004) & NPB 704, 3

(2005))

TM

Page 11: Stuart Raby

c2 analysis - 3rd family

11 Parameters :

3

01 10/ 2 16tanG G

HM m

M

A m m

9 Observables ( included in c2) :

EM s Z W NEW

t b b

G M M

M m m M

Dermisek, Raby, Roszkowski and Ruiz de Austri

JHEP 09 (2005) 029

Page 12: Stuart Raby

Results

1. Dark Matter & WMAP2. Bs -> m+ m-

3. Light Higgs mass - mh

4. Upper bound on mA

Lower bound on BR(Bs -> m+ m-)

Page 13: Stuart Raby

Dark Matter & WMAP

Neutralino LSP

1 1 A f f

tanAb b

A : broad resonance, mA arbitrary

Page 14: Stuart Raby

Results - m16 & mA fixed

Green band consistent with WMAP Light Higgs mass contours

Page 15: Stuart Raby

Br( Bs -> m+ m- )

SM : 3 x 10-9

MSSM : ~ (tan )b 6 /mA4

DZero < 4.7 x 10-8 (95% CL) w/ 5.0 fb-1

“expected sensitivity”

CDF bound < 4.3 x 10-8 (95% CL) w/ 3.7 fb-1

Page 16: Stuart Raby

Title of talk 16

Page 17: Stuart Raby

Results - m16 & mA fixed

Constant Bs -> m+ m- contoursConstant c2 contours

Page 18: Stuart Raby

Light Higgs mass

|At| increases mh decreases

Carena,Quiros &Wagner ‘95

Page 19: Stuart Raby

Light Higgs mass

2

3 g

2 2

tan tanlog .

2%

t tb

bb t

b

b

M Am corrm m m

mm

Needed to fit data

M1/2 increases -At increases

mh decreases

Page 20: Stuart Raby

Light Higgs mass contours

Page 21: Stuart Raby

mA[max] Br[ Bs -> m+ m- ][min]

Fermilab ??

-8

1.3 TeV

Br( )

10

A

s

m

B

Page 22: Stuart Raby

22

Baer, Kraml, Sekmen and Summy JHEP 03 (2008) 056

Bottom – Up and Down and Up …

Dermisek, Raby, Roszkowski and Ruiz de Austri JHEP 09 (2005) 029

Top - Down

max( , , )

min( , , )t b

t b

f f fR

f f f

2

Page 23: Stuart Raby

Summary - MSO10SM

1. Gauge & Yukawa unification2. Suppresses flavor & CP viol. &

N decay3. Dark Matter consistent

w/WMAP4. 114 < mh < 121 GeV5. mA < 1.3 TeV

BR(Bs -> m+ m-) > 10-8

TM

Page 24: Stuart Raby

Balazs & Dermisek JHEP 0306:024 (2003) non universal gaugino massesAltmannshofer, Guadagnoli, Raby & Straub PLB 668, 385 (2008) Baer, Kraml & Sekmen arXiv:0908.0134 [hep-ph] D term splitting &

Guadagnoli, Raby & Straub arXiv:0907.4709 [hep-ph]

Varying BCs at MGUT 3rd Family only

t b

2 2 & U Dt b H HA A m m

3 1,216 16 m m

Page 25: Stuart Raby

Balazs & Dermisek JHEP 0306:024 (2003) non universal gaugino masses (gauginoMSB) squark & slepton masses zero at GUT scale

Bottom line

Heavy squarks and gluinosPossibly light sleptons, neutralinos and light Higgs

Varying BCs at MGUT 3rd Family only

Page 26: Stuart Raby

Altmannshofer, Guadagnoli, Raby & Straub PLB 668, 385 (2008)

Varying BCs at MGUT 3rd Family only

t b

Bottom line

Good fits with 10 – 20 % top – bottom Yukawa splitting & m16 = 7 TeV

Observable stop, gauginos and Higges at LHC !

Page 27: Stuart Raby

Baer, Kraml & Sekmen arXiv:0908.0134 [hep-ph] D term splitting &

Varying BCs at MGUT 3rd Family only

3 1,216 16 m m

Bottom line

Good fits with Yukawa unification and m16 = 10 TeV or greaterObservable gauginos and light Higgs at LHCsmoking gun : light sbottom mixing

Page 28: Stuart Raby

Guadagnoli, Raby & Straub arXiv:0907.4709 [hep-ph]

Varying BCs at MGUT 3rd Family only

2 2 & U Dt b H HA A m m

Bottom line

Good fits with m16 = 4 TeV or greater

Observable stop, gauginos and light Higgs

Page 29: Stuart Raby

Dermisek & Raby PLB 622:327 (2005).

Dermisek, Harada & Raby PRD74, 035011 (2006)

Albrecht, Altmannshofer, Buras, Guadagnoli & Straub JHEP 0710:055 (2007)

3 Family SO(10) + family symmetry

Page 30: Stuart Raby

3 family SO10 SUSY Model

D3 x U(1) Family Symmetry Superpotential Yukawa couplings c2 analysis Charged fermion masses &

mixing Neutrino masses & mixing

Page 31: Stuart Raby

Title of talk 31

Superpotential for charged fermion Yukawa couplings

. 3 3

3

16 1016 16 10

45 16 45 16 16

ch fermions a a

a aa a a a

W

M AM M

1

2

2

0

45 GB L M

Familon VEVs

assumed

Page 32: Stuart Raby

Title of talk 32

SO(10) x [ D3 x U(1) family sym. ]Yukawa Unification for 3rd Family

Dermisek & Raby PLB 622:327 (2005).

7 real para’s + 4 phases

+ 3 real MajoranaNeutrino masses

Page 33: Stuart Raby

Title of talk 33

Effective higher

dimension operators

Page 34: Stuart Raby

Title of talk 34

2 3 3 3

12 3 3 3

16 16 16neutrino a a

a a a

W N N

S N N S N N

3 3a aS M S M 1616 v

Extend to neutrino sector

Assume 3 new real para’s

Page 35: Stuart Raby

Title of talk 35

12neutrino NW m VN NM N

sin2

vm Y

32

32

0

3

3 3 1

Y

2

2 1

2

16 2

3

0 0

0 0

0 0

V v

1 2 3NM diag M M M

Page 36: Stuart Raby

Title of talk 36

1 1T T Te N eM U m V M V m U

Using c2 analysis, fit

15 charged fermion & 4 neutrino low energy observables with

11 arbitrary Yukawa & 3 Majorana mass parameters

4 & 1 d. o. f.or 5 predictions

Page 37: Stuart Raby

Title of talk 37

compared to SM - 27 parameters CMSSM - 32 parameters

24 parameters at GUT scale

Global c2 analysis

Page 38: Stuart Raby

Title of talk 38

Global c2 analysis – good fits to charged fermion masses & mixing angles neutrino masses & mixing angles naturally satisfies Lepton Flavor Violation and electron electric dipole moment bounds Dermisek, Harada & Raby PRD74, 035011 (2006)

Page 39: Stuart Raby

Title of talk 39

16

1/2

4 TeV

= 300 GeV

M 200 GeV

m

Page 40: Stuart Raby

Title of talk 40

Page 41: Stuart Raby

Title of talk 41

Results for 7 < c2 < 8

16

213

14

29

4 TeV

114 < m 129 GeV

0.010 < sin 2 0.015

1 < BR( e ) 10 < 7

2 < d ( cm) 10 < 5

h

e

m

e

Page 42: Stuart Raby

Title of talk 42

c2 analysis including B physics

Albrecht, Altmannshofer, Buras, Guadagnoli, & Straub JHEP 0710:055 (2007)

Find good fits to quark, charged lepton & neutrino masses and mixing angles & test flavor violation in b physics

some tension between b s g & b s l+ l-

m16 ~ 10 TeV

Page 43: Stuart Raby

Title of talk 43

SM SM7 t 7 7A tan sign 2C C C

g

b s

t

SMs 7 7favors C

BR(B

at

X

)

2

l l C

SM SM7 7 7 7C C C C

tA 0

What is the tension ?

Page 44: Stuart Raby

Title of talk 44

7 7SMC C

Belle arXiv:0904.0770

However …

*B K l l

Page 45: Stuart Raby

Title of talk 45

Albrecht et al. JHEP 0710:055 (2007)

7 7Required SMC C

Page 46: Stuart Raby

Title of talk 46

MSO10SM & Large tan( b ) Fits WMAP Predicts light Higgs with mass of order 120 – 130 GeV Predicts lighter 3rd and heavy 1st & 2nd gen.

squarks and sleptons (inverted scalar mass hier.) LFV bounds satisfied Enhances Br[ Bs m+ m- ] Suppresses Br( B t n ) & DMBs

B Xs g , Xs l+ l- tension ??

LHCb

Page 47: Stuart Raby

Title of talk 47

MSO10SM & Large tan( b )

predicts light gluinos ~ 300 – 500 GeV predicts light charginos and neutralinos

LHC

MSO10SM : Beautiful symmetry Many experimental tests !!

Page 48: Stuart Raby

Title of talk 48

Backup slides

Page 49: Stuart Raby

Title of talk 49

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Title of talk 50

Page 51: Stuart Raby

Title of talk 51

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Title of talk 52

Page 53: Stuart Raby

Title of talk 53

Balazs & Dermisek JHEP 0306:024

(2003)

Gaugino mediated SUSY breaking

Observablesleptons, neutralino &light higgs ??

Heavy gluino &squarks

Page 54: Stuart Raby

Title of talk 54

Altmannshofer, Guadagnoli, Raby & Straub PLB 668, 385

(2008)

3rd family only with free parameterb

t

Page 55: Stuart Raby

Title of talk 55

Baer, Kraml & Sekmen

arXiv:0908.0134

D term Higgs splitting & DR3

3 1,216 16m m

Page 56: Stuart Raby

Title of talk

Guadagnoli, Raby & Straub arXiv:0907.4709 [hep-ph]

A term & “Just so” Higgs splitting