String Theory in the LHC Era J Marsano (marsano@uchicago.edu) 1 - - PowerPoint PPT Presentation

string theory in the lhc era
SMART_READER_LITE
LIVE PREVIEW

String Theory in the LHC Era J Marsano (marsano@uchicago.edu) 1 - - PowerPoint PPT Presentation

String Theory in the LHC Era J Marsano (marsano@uchicago.edu) 1 Friday, April 27, 12 String Theory in the LHC Era 1. Electromagnetism and 5. Supersymmetry Special Relativity 2. The Quantum World 6. Einsteins Gravity 3. Why do we need


slide-1
SLIDE 1

String Theory in the LHC Era

1

J Marsano (marsano@uchicago.edu)

Friday, April 27, 12

slide-2
SLIDE 2

String Theory in the LHC Era

  • 1. Electromagnetism and

Special Relativity

  • 2. The Quantum World
  • 3. Why do we need the Higgs?
  • 4. The Standard Model and Beyond
  • 9. String Theory and Particle Physics
  • 5. Supersymmetry
  • 6. Einstein’s Gravity
  • 7. Why is Quantum Gravity so Hard?
  • 8. String Theory and Unification

2

Friday, April 27, 12

slide-3
SLIDE 3

3

We have already encountered essentially 2/3 of the Standard Model Quantum Electrodynamics Weak Interactions

  • Lecture 2
  • Lecture 3

Friday, April 27, 12

slide-4
SLIDE 4

4

In lecture 2, we met Quantum Electrodynamics

Richard Feynman Julian Schwinger Sin-Itiro Tomonoga

Electrons interact by exchange

  • f a photon

Massless force carrier

e ∼ r 4π 137

Dimensionless coupling

Long range force!

e− e− γ e− e−

Friday, April 27, 12

slide-5
SLIDE 5

5

In lecture 3, we met the Weak Interactions e− n → p+ + e− + νe

n

p+ νe

mproton ∼ 0.938 GeV

GF ∼ 1 (300 GeV)2 ∼

  • 10−16 cm

2

`proton ∼ 10−13 cm

MZ ∼ 91 GeV

MW ∼ 80 GeV

νe νe Z0

n n

Friday, April 27, 12

slide-6
SLIDE 6

6

Quantum Electrodynamics Weak Nuclear Force

Long range force

Weak bosons W ±, Z0

Short range force

Range set by 1 Mass of W ±, Z0

n νe e− p+ W −

Photon γ

Massless force carrier Massive force carriers

e− e− γ e− e−

Friday, April 27, 12

slide-7
SLIDE 7

7

Building to the Standard Model....

Electromagnetism Weak Interactions Leptons

(electron, neutrino, and two similar pairs of particles)

Friday, April 27, 12

slide-8
SLIDE 8

8

What about protons and neutrons?

...for that matter what keeps the protons together in the nucleus of an atom?

...we are missing a force...

Friday, April 27, 12

slide-9
SLIDE 9

9

Hideki Yukawa

p+ n π0 p+ n

mπ0 ∼ 0.135 GeV

Yukawa proposed a ‘force carrier’--pion Very short lived particle

τπ0 ∼ 8.4 × 10−17 s π0 → γ + γ

(he didn’t call it that)

How to observe?

Friday, April 27, 12

slide-10
SLIDE 10

10

Cosmic Rays!

Expose special photographic plates at high altitudes (on mountains or balloons)

Cecil Frank Powell

Friday, April 27, 12

slide-11
SLIDE 11

11

Tevatron at Fermilab

Particle accelerators

p p

By the 1960’s, hundreds of particles were discovered that participate in Yukawa’s nuclear interaction

Friday, April 27, 12

slide-12
SLIDE 12

12

By the 1960’s, hundreds of particles were discovered that participate in Yukawa’s nuclear interaction

The Particle Zoo

  • π±
− −
  • π
− −
  • η
  • ρ
− −
  • ω
− − −
  • η′
  • φ
− − −
  • η
  • π
− −
  • π
− −
  • η
  • ω
− − −
  • ρ
− −
  • η
ρ − − − −
  • π
− − −
  • η
  • ω
− − −
  • ω
− − −
  • π
− −
  • φ
− − −
  • ρ
− −
  • ρ
− − −
  • η
  • π
− − −
  • φ
− − − η −
  • π
− − ρ − −
  • ρ
− −
  • π
− − ρ − −
  • φ
− − − η − ρ − −
  • ρ
− − − ±
  • ±
− −
∗ ∗
− − ±
  • ±
±
∗ ±
  • ±
± ∗ ± ±
  • ±
  • ∗±
±
  • ±
  • ±
± ∗ sJ ± sJ ± ±
  • ±
  • ±
  • ±
cb ub
± ∓
∗ sJ ±
  • ±
  • η
− − −
  • χ
  • χ
  • χ
  • η
  • ψ
− − −
  • ψ
− − −
  • χ
  • ψ
− − − ±
  • ψ
− − − ±
  • − −
− −
  • ψ
− − − ± − − η −
− −
  • χ
  • χ
  • χ
− − − − −
  • χ
  • χ
  • χ
− −
− −
− −
− −

Many ad hoc concepts introduced to explain decay patterns, masses, etc

  • Isospin
  • ‘Strangeness’
  • Charm

Friday, April 27, 12

slide-13
SLIDE 13

13

Interesting patterns for particles of similar mass

‘Strangeness’ Charge

Suggestive of underlying mathematical structure

Groups of 8 Groups of 10 η0 Groups of 1

Friday, April 27, 12

slide-14
SLIDE 14

14

This underlying structure is related to the mathematics of symmetries

Friday, April 27, 12

slide-15
SLIDE 15

15

Suppose 31 flavors was really ‘3 flavors’

You and I decide to buy two sundaes but the flavors are chosen at random 3 flavors 3 flavors

×

= 9

fUdge ripple cookie Dough Strawberry

Mine Yours How many possibilities?

Friday, April 27, 12

slide-16
SLIDE 16

16

Suppose instead that both are for me

3 flavors 3 flavors

×

= 9

Mine Also mine U D D U These 2 combinations are effectively the same Less than 9 distinct combinations... how many?

fUdge ripple cookie Dough Strawberry

Friday, April 27, 12

slide-17
SLIDE 17

17

3 flavors 3 flavors

×

= 9

Mine Also mine We can enumerate all possibilities

UU DD SS UD+DU US+SU DS+SD = 6

fUdge ripple cookie Dough Strawberry This set of 6 possibilities is closed under relabeling of flavors

Friday, April 27, 12

slide-18
SLIDE 18

18

3 flavors 3 flavors

×

= 9

Mine Also mine Mathematicians like to divide the 9 combinations into groups that do not mix with one another under relabeling

UD+DU US+SU DS+SD UU DD SS UD-DU US-SU DS-SD

Symmetric under interchange Antisymmetric under interchange

fUdge ripple cookie Dough Strawberry

Friday, April 27, 12

slide-19
SLIDE 19

18

3 flavors 3 flavors

×

= 9

Mine Also mine Mathematicians like to divide the 9 combinations into groups that do not mix with one another under relabeling

UD+DU US+SU DS+SD UU DD SS UD-DU US-SU DS-SD

Symmetric under interchange Antisymmetric under interchange

= 9 6 3 +

fUdge ripple cookie Dough Strawberry

Friday, April 27, 12

slide-20
SLIDE 20

19

3 flavors 3 flavors

×

= 9

Mine Also mine

If we have a set of states made of 2 things that come in 3 flavors

Expect a grouping according to

3 x 3 = 6 + 3

this is not quite what we see in the particle zoo....

fUdge ripple cookie Dough Strawberry

Friday, April 27, 12

slide-21
SLIDE 21

20

Interesting patterns for particles of similar mass

‘Strangeness’ Charge

Suggestive of underlying mathematical structure

Groups of 8 Groups of 10 η0 Groups of 1

Friday, April 27, 12

slide-22
SLIDE 22

20

Interesting patterns for particles of similar mass

‘Strangeness’ Charge

Suggestive of underlying mathematical structure

Groups of 8 Groups of 10 η0 Groups of 1

10 + 8 + 8 + 1 = 27 = 3 x 3 x 3

Friday, April 27, 12

slide-23
SLIDE 23

20

Interesting patterns for particles of similar mass

‘Strangeness’ Charge

Suggestive of underlying mathematical structure

Groups of 8 Groups of 10 η0 Groups of 1

10 + 8 + 8 + 1 = 27 = 3 x 3 x 3

Friday, April 27, 12

slide-24
SLIDE 24

20

Interesting patterns for particles of similar mass

‘Strangeness’ Charge

Suggestive of underlying mathematical structure

Groups of 8 Groups of 10 η0 Groups of 1

10 + 8 + 8 + 1 = 27 = 3 x 3 x 3

Friday, April 27, 12

slide-25
SLIDE 25

21

You and I invite a friend to join us for the sundae... Now how many combinations?

3 flavors 3 flavors 3 flavors

× ×

= 27

Mine Yours Our friend’s

fUdge ripple cookie Dough Strawberry

Friday, April 27, 12

slide-26
SLIDE 26

22

Permutation Groups

Consider all 27 possible permutations of sundaes

UUU, UUD, UDU, DUU, UUS, USU, SUU DDD, DDU, DUD, UDD, DDS, DSD, SDD, SSS, SSU, SUS, USS, SSD, SDS, DSS, UDS, USD, DUS, DSU, SUD, SDU

Mathematicians divide the 27 combinations into groups that do not mix under relabeling

3 x 3 x 3 = 27 = 10 + 8 + 8 + 1

UUU+DDD+SSS

10 ‘symmetric’ combinations

UUU DDD SSS UUD+... UUS+... UDD+... USS+... DDS+... DSS+... UDS+...

Friday, April 27, 12

slide-27
SLIDE 27

23

Interesting patterns for particles of similar mass

‘Strangeness’ Charge

Groups of 8 Groups of 10

27 = 10 + 8 + 8 + 1

Particles display pattern consistent being made of three things that come in three flavors

(mesons too if you think of 3 as product of 30s)

Friday, April 27, 12

slide-28
SLIDE 28

24

‘Strangeness’ Charge

Murray Gell-Mann

Suppose each of these particles is composed of 3 ‘quarks’

3 ‘flavors’ of quark up, down, strange

‘The Eightfold Way’

Very useful organizational principle that gives order to the ‘particle zoo’

Friday, April 27, 12

slide-29
SLIDE 29

25

Murray Gell-Mann

‘The Eightfold Way’

The Ω− was not previously known

Gell-Mann predicted its existence and its mass

Friday, April 27, 12

slide-30
SLIDE 30

26

‘Strangeness’ Charge

Murray Gell-Mann

‘The Eightfold Way’

Quarks introduced as a mathematical tool suggested by symmetry structure and particle mass patterns

Are they real?

Friday, April 27, 12

slide-31
SLIDE 31

27

γ e− e− e− e− γ e− e−

Is my favorite particle fundamental or composite? p+ p+

Energy is conserved

Scattering is ‘elastic’

Appears that energy is not conserved

Scattering is ‘inelastic’

Friday, April 27, 12

slide-32
SLIDE 32

28

γ e− e−

Is my favorite particle fundamental or composite? p+ p+

Appears that energy is not conserved

Scattering is ‘inelastic’

u u d

p+

γ e− e−

Some initial energy deposited in proton structure

Friday, April 27, 12

slide-33
SLIDE 33

29

http://hyperphysics.phy-astr.gsu.edu

Cross section (like probability)

u u d

p+

γ e− e−

At low electron energies, scattering is primarily elastic Becomes inelastic at high electron energies

Friday, April 27, 12

slide-34
SLIDE 34

30

The particles of the ‘Particle Zoo’ are all quark bound states Baryons Triples of quarks Mesons Quark/anti-quark bound states No free quarks: why not?

u u d

p+

u d d

n

u u

π0

Friday, April 27, 12

slide-35
SLIDE 35

31

No free quarks: why not?

We need a theory to describe the physics of quarks

Friday, April 27, 12

slide-36
SLIDE 36

32

Birth of String Theory

Meson spectrum exhibits some ‘string-like’ features Studies of ‘quantized strings’ in 1960’s to describe mesons

  • Strings do describe mesons in a sense, but the

picture is much more involved.....

π0

u u

Some problems....e.g. spin 2 excitations

Friday, April 27, 12

slide-37
SLIDE 37

32

Birth of String Theory

Meson spectrum exhibits some ‘string-like’ features Studies of ‘quantized strings’ in 1960’s to describe mesons

  • Strings do describe mesons in a sense, but the

picture is much more involved.....

π0

u u

Some problems....e.g. spin 2 excitations

Gravity!

Friday, April 27, 12

slide-38
SLIDE 38

33

No free quarks: why not?

We need a theory to describe the physics of quarks

Friday, April 27, 12

slide-39
SLIDE 39

34

What if we model the ‘strong force’ between quarks by analogy with Electromagnetism and the Weak Interactions?

q q q q

g

‘Gluon’

Quark should carry a suitable ‘charge’

s s s

Ω−

Some baryons have three identical quarks ⬌ Pauli exclusion requires three ‘kinds’ of charge

‘color charge’

Friday, April 27, 12

slide-40
SLIDE 40

35

What if we model the ‘strong force’ between quarks by analogy with Electromagnetism and the Weak Interactions?

q q q q

g

‘Gluon’ s s s

Ω−

Quarks carry a ‘color charge’...red, green, blue

Quantum Chromodynamics (QCD)

→ there are 8 types of gluon (rg, rb, etc)

Friday, April 27, 12

slide-41
SLIDE 41

36

Quantum Chromodynamics (QCD)

q q q q

g

‘Gluon’ s s s

Ω−

Can this model explain why we don’t see any free quarks?

Friday, April 27, 12

slide-42
SLIDE 42

37

Key point is how the strong force behaves at different distance scales

As an example, consider QED (electromagnetism)

Interaction receives quantum corrections

+ + + ...

Friday, April 27, 12

slide-43
SLIDE 43

38

Electromagnetic interaction weaker at long distances (low energies) and stronger at short distances (high energies)

Strength of Electromagnetic interaction depends on distance scale

αem ∼ e2 4π Energy scale

Friday, April 27, 12

slide-44
SLIDE 44

39

q q q q

Interaction of quarks with gluons receives many quantum corrections

+ +

q q

g g g

Because there are 8 gluons, they can interact with one another This is unlike QED, where there is

  • nly one photon and it has no self-

interaction

‘Asymptotic Freedom’

Friday, April 27, 12

slide-45
SLIDE 45

39

q q q q

Interaction of quarks with gluons receives many quantum corrections

+ +

q q

g g g

Because there are 8 gluons, they can interact with one another This is unlike QED, where there is

  • nly one photon and it has no self-

interaction

‘Asymptotic Freedom’

Friday, April 27, 12

slide-46
SLIDE 46

40

‘Asymptotic Freedom’

David Gross H David Politzer Frank Wilczek

QCD is strong at large distances (low energies) but weak at small distances (large energies)

Friday, April 27, 12

slide-47
SLIDE 47

41

So why don’t we see free quarks? u u

Friday, April 27, 12

slide-48
SLIDE 48

41

So why don’t we see free quarks? u u

Friday, April 27, 12

slide-49
SLIDE 49

41

So why don’t we see free quarks? u u

Friday, April 27, 12

slide-50
SLIDE 50

41

So why don’t we see free quarks? u u u u

Friday, April 27, 12

slide-51
SLIDE 51

41

So why don’t we see free quarks? u u u u

Separating quarks requires so much energy that we make a quark/anti-quark pair if we try to separate them

No free quarks -- ‘Confinement’

Friday, April 27, 12

slide-52
SLIDE 52

42

The Standard Model of Particle Physics

Electromagnetism Strong nuclear force Weak nuclear force

Leptons

(electrons and neutrinos)

Quarks

Friday, April 27, 12

slide-53
SLIDE 53

43

Electromagnetism Strong nuclear force Weak nuclear force Leptons (electrons and neutrinos) Quarks

The Standard Model of Particle Physics + Higgs Boson

All particle masses from coupling to Higgs

Friday, April 27, 12

slide-54
SLIDE 54

43

Electromagnetism Strong nuclear force Weak nuclear force Leptons (electrons and neutrinos) Quarks

The Standard Model of Particle Physics + Higgs Boson

All particle masses from coupling to Higgs

Photon massless long range force Gluons massless but many

  • f them → confinement

W and Z bosons massive short range force Quark and lepton masses from Higgs

Friday, April 27, 12

slide-55
SLIDE 55

44

The Higgs boson is the missing ingredient

  • 1. Needed to generate particle masses
  • 2. Standard Model violates unitarity (problem

with probability) around 1 TeV without the Higgs

Friday, April 27, 12

slide-56
SLIDE 56

45

Looking for the Higgs ATLAS CMS

A Toroidal Lhc ApparatuS Compact Muon Solenoid

Friday, April 27, 12

slide-57
SLIDE 57

46

Image from CDF website

p p

Friday, April 27, 12

slide-58
SLIDE 58

47

Image from CDF website

Look for Higgs through its decay products Best channel is

h → γγ

Friday, April 27, 12

slide-59
SLIDE 59

48

Friday, April 27, 12

slide-60
SLIDE 60

48

Friday, April 27, 12

slide-61
SLIDE 61

49

[GeV]

H

m 110 115 120 125 130 135 140 145 150

SM

  • /
  • 95% CL Limit on
  • 1

10 1 10 Obs. Exp.

  • 1

±

  • 2

± = 7 TeV s

  • 1

Ldt = 4.6-4.9 fb

  • ATLAS Preliminary

2011 Data CLs Limits

Higgs boson mass (GeV)

110 115 120 125 130 135 140 145

  • f SM Higgs hypothesis

S

CL

  • 3

10

  • 2

10

  • 1

10 1

90% 95% 99%

  • 1

L = 4.6-4.8 fb = 7 TeV s CMS,

Observed Expected (68%) Expected (95%)

Friday, April 27, 12

slide-62
SLIDE 62

50

Beyond the Standard Model

Why?

Friday, April 27, 12

slide-63
SLIDE 63

51

Beyond the Standard Model

Inverse electromagnetic coupling Inverse weak interaction coupling Inverse QCD coupling

  • F. Wilczek, Nature 433, 239

At high energies, electromagnetic coupling becomes large

→ Some new physics must be waiting there.....

Gravity!!!

Friday, April 27, 12

slide-64
SLIDE 64

51

Beyond the Standard Model

Inverse electromagnetic coupling Inverse weak interaction coupling Inverse QCD coupling Grand Unification?

  • F. Wilczek, Nature 433, 239

At high energies, electromagnetic coupling becomes large

→ Some new physics must be waiting there.....

Gravity!!!

Friday, April 27, 12

slide-65
SLIDE 65

52

  • Gravity
  • Neutrino mass
  • Cosmology
  • Dark matter
  • Dark energy (related to gravity?)
  • Matter/antimatter asymmetry
  • Hints of Grand Unification
  • ‘Hierarchy problem’

Why?

Beyond the Standard Model

Friday, April 27, 12

slide-66
SLIDE 66

53

Beyond the Standard Model

Energy Scales

1018 GeV 10−3 GeV

Quantum gravity Weak scale Proton mass Electron mass

16 orders of magnitude

1 GeV 102 GeV

Where did this large scale separation come from?

Higgs boson breaks electroweak symmetry Generates mass for W and Z bosons

Friday, April 27, 12

slide-67
SLIDE 67

54

Beyond the Standard Model

Energy Scales

1018 GeV 10−3 GeV

Quantum gravity Weak scale Proton mass Electron mass

16 orders of magnitude

1 GeV 102 GeV

Determined by ‘infinite’ quantum corrections that must be dealt with Will have much more to say about infinities in coming lectures....for now this hierarchy of scales requires excessive ‘fine-tuning’

Friday, April 27, 12

slide-68
SLIDE 68

55

Many ideas for physics Beyond the Standard Model....

Inverse electromagnetic coupling Inverse weak interaction coupling Inverse QCD coupling Grand Unification?

  • F. Wilczek, Nature 433, 239

Unification improves significantly with ‘Supersymmetry’....

Friday, April 27, 12

slide-69
SLIDE 69

56

Next time: Supersymmetry!

Friday, April 27, 12

slide-70
SLIDE 70

57

SUMMARY

  • Need strong nuclear force to hold atomic nuclei together
  • Can be described by exchange of new particles, the pions
  • Zoo of strongly interacting particles discovered
  • Symmetry brings order to the particle zoo
  • Quarks introduced as mathematical tool -- fiducial components of strongly

interacting particles

  • Strong interaction gets stronger at large distance scales
  • No free quarks at large distances...confinement
  • Quarks are real!
  • Protons and other strongly interacting particles are made of quarks
  • Strong force properly described in terms of strong interaction between quarks
  • Strong interaction couples to ‘color charge’ -- three kinds red, blue, and green
  • Mediated by exchange of 8 types of ‘gluon’
  • Standard Model very successful but not the final story.....

Friday, April 27, 12