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GUT and Supersymmetry Hitoshi Murayama 129A F2002 semester

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Page 1: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

GUT and Supersymmetry

Hitoshi Murayama129A

F2002 semester

Page 2: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Grand Unified Theories

Page 3: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Motivations for GUT

• Charge quantization, anomaly cancellation,bizarre hypercharge assignments in theStandard Model

• Three seemingly unrelated forces yet allgauge forces

• Einstein’s dream towards a unifieddescription of all forces

• Baryogenesis no longer a prime motivation

Page 4: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Quantum Numbers in theStandard Model

• I didn’t become a physicist to memorizethese weird numbers...

ud

Ê

Ë Á

ˆ

¯ ˜

L(3,2, - 1

6) uR(3,1,+ 23) dR(3,1, - 1

3)

n

Ë Á

ˆ

¯ ˜

L(1,2,- 1

2) lR (1,1,-1)

Page 5: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Quantum Numbers in theStandard Model

• To treat them on equal footing, make allparticles left-handed using CP

ud

Ê

Ë Á

ˆ

¯ ˜

L(3,2, - 1

6) u L (3*,1,- 23) d L (3*,1,1

3)

n

Ë Á

ˆ

¯ ˜

L(1,2,- 1

2) l L (1,1,1)

Page 6: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Gauge Anomaly

• Gauge symmetry crucial to keep quantum fieldtheories (including the SM) under control

• Triangle diagrams:

• May spoil the gauge invariance at quantum levelfi disaster

• Anomalies must all vanish for three gauge vertices(not for global currents, e.g. B, L)

• Sum up all standard model fermions and see ifthey indeed vanish

Page 7: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Anomaly Cancellation

• U(1)3

• U(1)(gravity)2

• U(1)(SU(2))2

• U(1)(SU(3))2

• (SU(3))3

• (SU(2))3, (SU(3))2SU(2), SU(3)(SU(2))2

• SU(2)Non-trivial connection between q & l

3 ⋅ 2 16( )3

+ 3 - 23( )3

+ 3 13( )3

+ 2 - 12( )3

+ 1( )3 = 03 ⋅ 2 1

6( ) + 3 - 23( ) + 3 1

3( ) + 2 - 12( ) + 1( ) = 0

3 ⋅ 2 16( ) + 2 - 1

2( ) = 03 ⋅ 2 1

6( ) + 3 - 23( ) + 3 1

3( ) = 0

# 3-# 3* = 2 - 1 -1 = 0

# 2 = 3 + 1 = 4 = even0

Page 8: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

SU(5) GUT

• SU(3)¥SU(2)¥U(1)ÃSU(5)• U(1) must be traceless: try 5*:• 5¥5 matrices

SU(3) SU(2)

U(1)

- 12 la* 00 0

Ê

Ë Á

ˆ

¯ ˜ 0 0

0 12t a

Ê

Ë Á

ˆ

¯ ˜

13 I3 00 - 1

2 I2

Ê

Ë Á Á

ˆ

¯ ˜ ˜

dddn

l

Ê

Ë

Á Á Á Á Á Á

ˆ

¯

˜ ˜ ˜ ˜ ˜ ˜

Page 9: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

SU(5) GUT

• Then the rest belongs to 10• All quantum numbers work

out this way

• Anomaly cancellation:

0 u -u d -u-u 0 u d -uu -u 0 d -u

-d -d -d 0 lu u u -l 0

Ê

Ë

Á Á Á Á Á Á

ˆ

¯

˜ ˜ ˜ ˜ ˜ ˜

#10-#5* = 0

ud

Ê

Ë Á

ˆ

¯ ˜

L(3,2, - 1

6) ~n

Ë Á

ˆ

¯ ˜

L(1,2, - 1

2) ƒ d L (3*,1,13)

È

Î Í

˘

˚ ˙

*

u L (3*,1,- 23) ~ d L (3*,1,1

3) ƒ d L (3*,1, 13)[ ]*

l L (1,1,1) ~n

Ë Á

ˆ

¯ ˜

L(1,2, - 1

2) ƒn

Ë Á

ˆ

¯ ˜

L(1,2,- 1

2)È

Î Í

˘

˚ ˙

*

Page 10: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Fermion Mass Relation

• Down- and lepton-Yukawa couplings comefrom the same SU(5) operator 10 5* H

• Fermion mass relationmb= mt, ms = mm, md = me

• Reality:mb= mt, 3ms = mm, md = 3me

• Not bad!

Page 11: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

SO(10) GUT

• SU(5)¥U(1)ÃSO(10)

• Come with right-handed neutrinos!– anomaly-free for any multiplets– Smallest simple anomaly-free group with chiral

fermions– Smallest chiral representation contains all

standard model fermions

16 = (10, +1) + (5*,-3) + (1, +5)

Page 12: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Seesaw Mechanism

• Once SO(10) broken to the standard model,right-handed neutrino mass becomesallowed by the gauge invariance M~ h MGUT

n L nR( )mD

mD

Ê

Ë Á

ˆ

¯ ˜

n Ln R

Ê

Ë Á

ˆ

¯ ˜ n L nR( )

mDmD M

Ê

Ë Á

ˆ

¯ ˜

n Ln R

Ê

Ë Á

ˆ

¯ ˜ mn =

mD2

M<< mD

To obtain m3~(Dm2atm)1/2, mD~mt, M3~1015GeV (GUT!)

Page 13: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Gauge Coupling Unification

Page 14: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Einstein’s Dream

• Is there an underlyingsimplicity behind vastphenomena in Nature?

• Einstein dreamed tocome up with a unifieddescription

• But he failed to unifyelectromagnetism andgravity (GR)

Page 15: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

History of Unification

gravity

electric magnetic

a-decay

b-decay

g-decay

planets apple

electromagnetiesm

atoms

Quantum mechanicsmechanics

Special relativity

Quantum ElectroDynamics Weak force

Strong forceElectroweak theory

Grand Unification?

GR

String theory?

Page 16: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Proton Decay

• Quarks and leptons in the same multiplet• Gauge bosons can convert q to l• Cause proton decay!

G µg2

MX2

Ê

Ë Á Á

ˆ

¯ ˜ ˜

2mp

5

Page 17: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Supersymmetric Proton Decay

G µg2

(4p )2hshcqC

2

MHC mSUSY

Ê

Ë Á Á

ˆ

¯ ˜ ˜

2

mp5

Suppressed only by thesecond power of GUTscale vs fourth in X-bosonexchange

Page 18: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Proton Decay

• No sign of protondecay yet!– Non-SUSY GUT does

not unify couplings• Minimal SUSY

particle content– Couplings unify!– t(pÆK+n) > 6.7 1032

years (90% CL) fromSuperK

Page 19: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Rest In PeaceMinimal SUSY SU(5) GUT

• RGE analysis • SuperK limitMHc>7.6 1016 GeV

• Even if 1st, 2ndgeneration scalars“decoupled”, 3rdgeneration contribution(Goto, Nihei)

MHc>5.7 1016 GeV(HM, Pierce)

Page 20: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Avoiding Proton Decay

• Unfortunately, proton decay rate/mode ishighly model-dependent– more threshold corrections (HM, Pierce)

– Some fine-tuning (Babu, Barr)

– GUT breaking by orbifolds (Kawamura; Hall, Nomura)

– Depends on the triplet-doublet splittingmechanism, Yukawa (non-)unification

Page 21: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Don’t give up!

• Still, proton decay unique window tophysics at >1015 GeV

• Suppression by fine-tuning: pÆK+n may bejust around the corner

• Flipped SU(5): pÆe+p0 possible• We still need SuperK!• Eventually with ~1000kt detector

Page 22: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Supersymmetry

Page 23: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Why was Anti-Matter Needed?

• At the end of 19th century: a “crisis” aboutelectron– Like charges repel: hard to keep electric charge

in a small pack– Electron is point-like– At least smaller than 10-17 cm

• Need a lot of energy to keep it small!

Page 24: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

E=mc2

• Need more than 109 eV ofenergy to pack electriccharge tightly inside theelectron

• But the observed energy ofthe electron is only 5 105 eV

• Electron cannot be smallerthan 10–13 cm??

• Breakdown of theory ofelectromagnetism

Page 25: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Uncertainty Principle

• Energy-Time UncertaintyPrinciple:You can violate energyconservation if it is only for ashort time

• Vacuum is full of quantum bubbles!

Werner Heisenberg

Page 26: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Anti-Matter Helps

• Electron creates aforce to repel itself

• Vacuum bubble ofmatter anti-mattercreation/annihilation

• Electron annihilatesthe positron in thebubblefi only 10% of mass

Page 27: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Anti-Matter Helps

• “Anti-matter attraction” cancels “Like-charge repulsion”

• It does not cost too much energy to tightlypack the electric charge inside the electron

• Needed anti-matter: double #particles• Theory of electromagnetism now works at

very short distances (12 digits accuracy!)

Page 28: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Higgs repels itself, too

• Just like electronrepeling itself becauseof its charge, Higgsboson also repels itself

• Requires a lot ofenergy to contain itselfin its point-like size!

• Breakdown of theoryof weak force

Page 29: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

But there is gravity

• Gravity and quantum mechanics unify at anextremely short distance 10–33 cm

• Higgs boson must be this small, too, to havea sensible unified theory of gravity andquantum mechanics

• But current theory of weak force breaksdown already at 10–17 cm

Page 30: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

History repeats itself?

• Double #particles again fisuperpartners

• “Vacuum bubbles” ofsuperpartners cancels the energyrequired to contain Higgs bosonin itself

• Theory of weak force madeconsistent with unification ofgravity and quantum mechanics

Page 31: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Where are the superpartners?

• They need to cancel self-repelling energy ofthe Higgs boson

• Cannot be too heavy to do this job• Have to be below 1012 eV or “Fermi

energy”• We are getting there this decade

– Tevatron (Fermilab, Illinois) 2001–– LHC (CERN, Switzerland) 2006–

Page 32: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Superpartners everywhere?

• There are unknown“Dark Matter” in ourgalaxy and outside

• It amounts for about30% of the Universe

• Lightest superpartnerone of the bestcandidates

Page 33: GUT and Supersymmetry - Hitoshi Murayamahitoshi.berkeley.edu/129A/GUT+SUSY.pdfallowed by the gauge invariance M~ h MGUT (nL nR) mD mD Ê Ë Á ˆ ¯ ˜ nL nR Ê Ë Á ˆ ¯ ˜ M mn

Superpartners as probe

• Most exciting thingabout superpartnersbeyond existence:They carryinformation of small-distance physics tosomething we canmeasuree.g., “Is GrandUnification true?”