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

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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 20, 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


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String Theory in the LHC Era

1

J Marsano (marsano@uchicago.edu)

Friday, April 20, 12

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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

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3

Quantum Electrodynamics (QED) works incredibly well

Richard Feynman Julian Schwinger Sin-Itiro Tomonoga

L ∼ ¯ ψ (iγµDµ − m) ψ − 1 4e2 FµνF µν

Photon Electron Charge Electron mass

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4

L ∼ ¯ ψ (iγµDµ − m) ψ − 1 4e2 FµνF µν

Photon Electron Charge Electron mass

Mass without Higgs...... so why all the fuss......

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5

Quantum Electrodynamics works fine without a Higgs ...but nuclear interactions don’t

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  • A. Henri Becquerel

Test to see if various materials glow when exposed to sunlight ...weather was cloudy for several days led to discovery of natural radioactivity!

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7

  • A. Henri Becquerel

Pierre Curie Marie Curie

Radioactivity!

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8

Decay classified according to penetration depth

Ernest Rutherford

Sheet of paper Aluminum Lead

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Decay classified according to penetration depth

Photons He nuclei Electrons Ernest Rutherford

Sheet of paper Aluminum Lead

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Decays can change one element into another

Frederick Soddy Ernest Rutherford

e.g. β decay +e− + . . .

60 27Co → 60 28Ni

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Decays can change one element into another

Frederick Soddy Ernest Rutherford

e.g. β decay +e− + . . .

60 27Co → 60 28Ni

# protons + neutrons # protons

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10

+ e− + . . .

Why?

Electron energy should be fixed by change in atomic mass

60 27Co → 60 28Ni

n → p+ + e− + . . .

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10

+ e− + . . .

Why?

Electron energy should be fixed by change in atomic mass

  • G. J. Neary, Roy. Phys. Soc. (London), A175, 71 (1940).

...but it isn’t...varies continuously ...something else is carrying away energy

60 27Co → 60 28Ni

n → p+ + e− + . . .

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Neutrino! Wolfgang Pauli Enrico Fermi

60 27Co → 60 28Ni + e− + νe

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12

Enrico Fermi

Interaction strength

GF (~c)3 = 1.11637(1) × 10−5 GeV −2 ∼ 1 (300 GeV )2

Fermi constant

60 27Co → 60 28Ni

e− n → p+ + e− + νe n p+

νe

+ e− + νe

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13

Interaction strength

GF (~c)3 = 1.11637(1) × 10−5 GeV −2 ∼ 1 (300 GeV )2

Fermi constant

Conventional to choose units so that ~ = c = 1 E = hc λ → E ∼ 1 λ

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Interaction strength

GF (~c)3 = 1.11637(1) × 10−5 GeV −2 ∼ 1 (300 GeV )2

Fermi constant

Conventional to choose units so that ~ = c = 1 E = hc λ → E ∼ 1 λ Energy = 1 Distance

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Interaction strength

GF (~c)3 = 1.11637(1) × 10−5 GeV −2 ∼ 1 (300 GeV )2

Fermi constant

Conventional to choose units so that ~ = c = 1 E = hc λ → E ∼ 1 λ Energy = 1 Distance e ∼ r 4π 137

Fermi interaction Electromagnetic interaction

mproton ∼ 0.938 GeV

GF ∼ 1 (300 GeV)2 ∼

  • 10−16 cm

2 `proton ∼ 10−13 cm

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No units No characteristic length or energy scale Physical length/energy scale

(Length)2 ∼ (Energy)−2

‘Short range force’ ‘Long range force’

e ∼ r 4π 137

Fermi interaction Electromagnetic interaction

mproton ∼ 0.938 GeV

GF ∼ 1 (300 GeV)2 ∼

  • 10−16 cm

2 `proton ∼ 10−13 cm

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No units No characteristic length or energy scale Physical length/energy scale

(Length)2 ∼ (Energy)−2

‘Short range force’ ‘Long range force’

Some funny business around 100 GeV

(more on this later)

e ∼ r 4π 137

Fermi interaction Electromagnetic interaction

mproton ∼ 0.938 GeV

GF ∼ 1 (300 GeV)2 ∼

  • 10−16 cm

2 `proton ∼ 10−13 cm

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15

+ e− + νe

60 27Co → 60 28Ni

Weak nuclear force Quantum Electrodynamics works perfectly well without a Higgs boson ...but the Weak nuclear force doesn’t!

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60 27Co → 60 28Ni

Weak nuclear force Focus on two puzzles:

  • Parity violation (problems with mirrors)
  • Unitarity violation (problems with probabilities)

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  • 1. Parity

Violation

(problems with mirrors)

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Parity is essentially reflection in a mirror flips right and left

Looking right Looking left For years people assumed that our world respected parity

i.e. the laws of physics do not distinguish right from left

Real world ‘Mirror’ world

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Photo Credit: Alan W. Richards from physics.nist.gov

  • C. N.

Yang

  • T. D. Lee

Parity seems natural Why should right and left be different?

In 1956, Lee and Yang pointed out that parity of weak interactions hadn’t been strongly tested Many people doubted that parity could actually be violated

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Photo Credit: Alan W. Richards from physics.nist.gov

  • C. N.

Yang

  • T. D. Lee

Parity seems natural Why should right and left be different?

In 1956, Lee and Yang pointed out that parity of weak interactions hadn’t been strongly tested Many people doubted that parity could actually be violated Feynman bet $50 that parity is not violated in nature

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Photo Credit: Alan W. Richards from physics.nist.gov

  • C. N.

Yang

  • T. D. Lee

Lee and Yang suggested several experimental tests

Spin

Use fact that parity flips the spin of a particle

Real world ‘Mirror’ world Spin

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Chien-Shiung Wu

60 27Co Nuclei

Spinning

β rays (electrons)

Parity = ⇒ same # of e− going ↑ and ↓

Real world ‘Mirror’ world

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Chien-Shiung Wu

60 27Co Nuclei

Spinning

β rays (electrons)

Parity = ⇒ same # of e− going ↑ and ↓

Left ⬌ Right flips direction of spin

Real world ‘Mirror’ world

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Chien-Shiung Wu

In reality, see more going ↓ than ↑!

60 27Co Nuclei

Spinning

β rays (electrons)

Real world ‘Mirror’ world

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Chien-Shiung Wu

In reality, see more going ↓ than ↑!

60 27Co Nuclei

Spinning

β rays (electrons)

Real world ‘Mirror’ world

Different result in real and mirror worlds

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Chien-Shiung Wu

Text

  • C. N.

Yang

  • T. D. Lee

Weak interactions can tell right from left!

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→ Weak interactions distinguish left- and right-handed particles

Weak interactions can tell right from left! Spin Momentum Spin Momentum

right-handed left-handed

Participate in Weak Interaction DO NOT Participate in Weak Interaction

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Spin

For a massive particle, the direction of motion depends on the observer!

Looks left-handed to us but if the race car is moving fast enough...... Momentum that we see Race car speed

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Spin

For a massive particle, the direction of motion depends on the observer!

Looks left-handed to us but if the race car is moving fast enough...... Momentum that we see Race car speed Momentum seen by race car

Particle looks right-handed to the race car!

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Spin

For a massive particle, the direction of motion depends on the observer!

We think the left-handed particle should participate in Weak Interaction Momentum that we see Race car speed Momentum seen by race car Race car thinks right-handed particle should not participate in Weak Interaction

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Spin Momentum that we see Race car speed Momentum seen by race car

If particle is massless, it moves at speed of light

Race car can never ‘catch up’ to it we always agree on the ‘handedness’

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Summary of Parity Puzzle:

  • Massless particles can be right-handed or left-handed
  • A massive particle can have either ‘handedness’ depending
  • n the observer
  • The weak interaction couples only to left-handed and not

to right-handed particles

→ ALL PARTICLES MUST BE FUNDAMENTALLY MASSLESS

Spin Momentum Spin Momentum right-handed left-handed

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→ ALL PARTICLES MUST BE FUNDAMENTALLY MASSLESS

Wait what?!?!?!?!?

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How to generate mass?

Start with massless ‘right-handed’ and ‘left-handed’ electrons

eL eR

h

eR and eL

Add a new ‘Higgs field’ that couples to them

h

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How to generate mass?

Start with massless ‘right-handed’ and ‘left-handed’ electrons

eL eR

h

eR and eL

Add a new ‘Higgs field’ that couples to them

h

Electrons can acquire a mass if the vacuum has a ‘bath’ of Higgs fields Like having a constant electric field everywhere in the universe

→ Higgs boson is a small fluctuation of this field

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Crowded room of physicists Einstein walks in People crowd around Einstein and slow him down (Higgs bath in vacuum) (Particle comes along) (Particle becomes massive)

Cartoons from CERN

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Cartoons from CERN

What about the Higgs boson?

Someone introduces a rumor in the room, say some new discovery at CERN Physicists cluster as the rumor passes through the room (A small excitation is introduced) (The excitation, a Higgs boson, propagates in the room)

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Resolution of Parity Puzzle:

  • Massless (charged) particles are right-handed or left-handed
  • Pairs of massless particles can become massive by

interacting with the ‘Higgs bath’

  • Weak force can violate parity because the ‘Higgs field’

carries ‘weak charge’

→ REQUIRES FUNDAMENTAL SCALAR PARTICLE: HIGGS BOSON

Spin Momentum Spin Momentum right-handed left-handed

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Peter Higgs Tom Kibble Gerald Guralnik C Richard Hagen Francois Englert Robert Brout

First Second Third Not just Higgs....3 Papers and 6 Authors

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  • 2. Unitarity

Violation

(problems with probabilities)

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Enrico Fermi

Interaction strength

GF ∼ 1 (300 GeV)2

Fermi’s theory is badly behaved if we do scattering experiments at energies much beyond 300 GeV

n → p+ + e− + νe e−

n

p+ νe

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GF ∼ 1 (300 GeV)2

Fermi’s theory is badly behaved if we do scattering experiments at energies much beyond 300 GeV → violates ‘unitarity’

Unitarity ⬌

If we sum the probabilities of everything that can happen in a given experiment, the answer better be 1 (i.e. 100%)

Fermi’s theory starts violating this condition for scattering experiments at energies much beyond 300 GeV

e− n p+ νe

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GF ∼ 1 (300 GeV)2

Unitarity ⬌

If we sum the probabilities of everything that can happen in a given experiment, the answer better be 1 (i.e. 100%)

Fermi’s theory starts violating this condition for scattering experiments at energies much beyond 300 GeV Very roughly, grows too large at large energy E

e− n p+ νe ’Probability’ ∼ GF E2 ∼ ✓ E 300 GeV ◆2

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GF ∼ 1 (300 GeV)2

Fermi’s theory is an ‘effective theory’, valid only at low enough energies

New physics must appear before we get far above 300 GeV. ‘Naturalness‘ principle says that the new physics should appear very close to 300 GeV

‘Naturalness’

e− n p+ νe

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At high energies, it becomes evident that Fermi’s interaction is mediated by a heavy particle

not too far from 300 GeV

e− n p+

νe

e− W − n p+

νe MW ∼ 80 GeV

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νe e− W + νe νe Z0

In fact we get 3 new heavy particles Like massive photons Carriers of ‘Weak nuclear force’ Mass sets ‘distance scale’ of force

e− W − n p+

νe

n → p+ + e− + νe n + νe → p+ + e− p+

n

n + νe → n + νe

n n

MW ∼ 80 GeV MZ ∼ 91 GeV

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νe e− W + νe νe Z0

In fact we get 3 new heavy particles Like massive photons Carriers of ‘Weak nuclear force’ Mass sets ‘distance scale’ of force

e− W − n p+

νe

n → p+ + e− + νe n + νe → p+ + e− p+

n

n + νe → n + νe

n n

MW ∼ 80 GeV MZ ∼ 91 GeV

e− e− e− e− γ

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Carlo Rubbia Simon van der Meer

W and Z bosons discovered at CERN in 1983

UA1 and UA2 SPS: Proton-antiproton collider Now injector for LHC

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e−

νe q q

W e− q q Z e+

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Quantum theory tricky

Hard to give mass to vector particles like photon To get an idea why, we return, to the classical electromagnetic wave (an ensemble of photons)

e− W − n p+

νe

n → p+ + e− + νe

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Light has two physical polarizations (ie ways to oscillate)

Electric field oscillates in horizontal direction Electric field oscillates in vertical direction

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In principle, there is a third polarization: Longitudinal polarization

Some parts of slinky move faster than

  • thers...gives a ‘lump’ that propagates

→ like polarization along direction of motion

Light cannot do this because every part of the wave moves at a fixed ‘speed of light’ and nothing can go faster

...but a wave made from massive force carriers could do this!

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Massless force carriers Massive force carriers

Photon γ

Long range force

→ Electromagnetism

Weak bosons W ±, Z0

Short range force

Range set by 1 Mass of W ±, Z0

→ Weak nuclear force

n νe e− p+ W −

γ e− e−

2 degrees of freedom 3 degrees of freedom

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Massless force carriers Massive force carriers

Photon γ

Long range force

→ Electromagnetism

Weak bosons W ±, Z0

Short range force

Range set by 1 Mass of W ±, Z0

→ Weak nuclear force

n νe e− p+ W −

γ e− e−

2 degrees of freedom 3 degrees of freedom

Extra degree of freedom can cause unitarity problems in quantum theory

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W-W scattering badly behaved around 1 TeV Divergences from the ‘extra longitudinal mode’ Idea: W and Z fundamentally massless Get mass from Higgs bath

Where does the ‘longitudinal mode’ come from?

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Higgs to the rescue

Rolls to nonzero field values

→ Generates ‘Higgs bath’

Motion along bottom

→ Longitudinal modes of

Motion up hill

→ ‘Higgs boson’

W ±, Z0

(rough picture)

‘Spontaneous symmetry breaking’

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Without Higgs, W-W scattering badly behaved around 1 TeV Higgs contributions can cure this

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Summary of our Two Puzzles:

  • Parity violation (problems with mirrors)
  • Does not allow massive particles
  • Mass from interaction with ‘Higgs bath’
  • Unitarity violation (problems with probabilities)
  • Fermi’s theory breaks down at high energies
  • Requires massive force carriers (like massive photons)
  • Mass from Higgs field

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Summary of our Two Puzzles:

  • Parity violation (problems with mirrors)
  • Does not allow massive particles
  • Mass from interaction with ‘Higgs bath’
  • Unitarity violation (problems with probabilities)
  • Fermi’s theory breaks down at high energies
  • Requires massive force carriers (like massive photons)
  • Mass from Higgs field

Higgs solves two problems of mass:

1.Mass to ordinary particles 2.Mass to carriers of weak nuclear force

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Electroweak theory

✓A sin θW + Z0 cos θW √ 2W − √ 2W + −A sin θW − Z0 cos θW ◆ ⊗ A cos θW − Z0 sin θW

  • Photon

Weak bosons SU(2) U(1)

Broken to quantum electrodynamics by Higgs mechanism

Steven Weinberg Abdus Salam Sheldon Glashow

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Looking for the Higgs ATLAS CMS

A Toroidal Lhc ApparatuS Compact Muon Solenoid

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Image from CDF website

p p

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Image from CDF website

Look for Higgs through its decay products Best channel is

h → γγ

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[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%)

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SUMMARY

  • Radioactive decay requires new ‘weak interaction’
  • Fermi wrote down a quantum model that works for sufficiently low scales
  • ‘Weak interaction’ introduces two puzzles related to mass
  • ‘Weak interactions violate parity’
  • Nature distinguishes between ‘right’ and ‘left’
  • Massive particles can be left-handed or right-handed to different observers
  • All particles must be fundamentally massless
  • Particles get mass from a ‘Higgs bath’ in the vacuum
  • Excitations are Higgs bosons!
  • Fermi’s theory of ‘Weak interactions’ violates unitarity
  • Probability of all events is not 1...requires new physics at a higher scale
  • New physics is set of massive force carriers
  • Force carriers get mass through ‘Higgs mechanism’
  • Resulting ‘Electroweak theory’ unifies Weak interactions and

electromagnetism

Friday, April 20, 12