High Energy Physics - Purdue University · High Energy Physics QuarkNet summer workshop ... •...

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High Energy Physics QuarkNet summer workshop June 24-28, 2013 1

Transcript of High Energy Physics - Purdue University · High Energy Physics QuarkNet summer workshop ... •...

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High Energy Physics

QuarkNet summer workshopJune 24-28, 2013

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The Birth of Particle Physics

• In 1896, Thompson showed that electrons were particles, not a fluid.

• In 1907, Rutherford showed that the mass of an atom was concentrated in a nucleus.

Particles that should obey the laws of quantum mechanics and relativity.

• In 1905, Einstein argued that photons behave like particles.

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Nuclear Physics

• α, β, ɣ emission

• Properties of neutrons• Fission of heavy elements• Nuclear “chemistry”• Nuclear forces• Beta decay• Neutrino postulated• Theories of beta decay

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Particle Accelerators

• In 1932, Cockroft and Walton accelerated protons to 600 keV, produced the reaction

and verified E=mc2.

• From 1930-1939, Lawrence built bigger and bigger cyclotrons, accelerating protons to higher and higher energies: 80 keV 100 MeV.

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Particle Detectors

• Photographic emulsions exposed by the passage of charged particles

• In 1912, Wilson develops the cloud chamber for seeing the paths of fundamental particles

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Discoveries in Cosmic Rays• Penetrating radiation

observed at high altitudes• Solutions to Dirac’s

equations interpreted as “positive electrons”

• Yukawa proposed a “meson” to explain the strong nuclear force

• Anderson observed positrons in 1932 and muons in 1936

• Perkins discovered pions photographic emulsions in 1947.• In 1912, Viktor Hess investigated

terrestrial radioactivity in balloon experiments.

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The Known Particles in 1950

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New Accelerators: Synchrotrons

1952: Brookhaven 3 GeV “Cosmotron” 1954: Berkeley 6 GeV “Bevatron”

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New Detectors: Bubble Chambers

The Berkeley 72 inch liquid hydrogen bubble chamber

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Known Particles in 1957

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Strongly Interacting Particles: 1961

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Strongly Interacting Particles: 1963

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Organizing the Data

“Strangeness”

Spin

Electric charge

Mas

s

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1964: Quarks?• Murray Gell-Mann: • George Zweig:

Physical meson states are representations of the SU(3) symmetry group:

Physical baryon states are representations of the SU(3) symmetry group:

Hadrons are composed of more elementary objects:

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1964: Observation of the Ω-

Observed in the 80 inch bubble chamber at Brookhaven in 1964.

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1968: Deep Inelastic Scattering

2 mile long, 30 GeV electron accelerator

Hydrogen target

Analyzing magnets

Detector

People

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Elastic Scattering

Proton

Electron

Used to measure the size of the proton.

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Inelastic Scattering

Proton

Electron

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Deep Inelastic Scattering

Proton

Electron

“Partons”

Angular distribution consistent with scattering from point-like spin ½ particles

inside the proton

Exactly the same as the Rutherford scattering experiment

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1974: The November Revolution

The SPEAR synchtrotron: 8 GeV electron-positron collider at SLAC

The Mark-I detector tracked charged particles using spark chambers.The charm quark was heavy and non-relativistic.

Charmonium behaved like a hydrogen atom made of quarks.

Simultaneously observed at Brookhaven where it was called the “J”.

To this day it is called the ...

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Bottom Quarks• Discovered in 1977 at a 400

GeV fixed target experiment, Fermilab E-288.

• Studied in detail with the ARGUS detector at Hamburg and CLEO at Cornell in the 80’s and 90’s.

• B-factories now operate at SLAC (BaBar) and in Japan (Belle)

• Detailed studies of how the weak force interacts with quarks.

Belle

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Fundamental Particles of Matter

• In 1994 the top quark was discovered by the CDF and DØ experiments at Fermilab

• In 2000 the tau neutrino was observed by the DONUT experiment at Fermilab

• The top quark is very heavy (174 GeV/c2) and it decays directly via ....

?

?

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Returning to the 1950’s: Quantum Electrodynamics

• A complete description of electrons, positrons and photons using relativistic quantum mechanics.

• In quantum mechanics, observable quantities are calculated using the “wavefunction” for a particle.

• The definition of the wavefunction is not unique... it could be arbitrarily re-defined at each point in space without changing any observables.

• This works, provided the electron interacts with the photon.

Symmetry Forces

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Quantum Electrodynamics

• Electron-electron scattering:

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Quantum Electrodynamics• Feynman Rules:

– Electron– Photon

– Add together ALL possible Feynman diagrams

Time

Spa

ce e-

e-

e-

e-

Initial state Final state

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Weak Interactions

• Beta decay described by Fermi (1930’s):

• Predicted that the probability of elastic neutrino scattering would exceed unity at energies of around 100 GeV.

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Weak Interactions• A significant improvement:

• A very massive W boson would explain why the interaction is weak.

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Weak Interactions• But hypothetically, at least:

• At high energies, the probability for W+W-

production by “neutrino-neutrino” scattering would exceed unity.

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Weak Interactions• This combination worked:

• But it required adding a new, neutral boson to the theory.

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Observation of Neutral Currents

• Observed in 1973 at CERN in a liquid freon bubble chamber.

• Masses of the W± and Z0 predicted to be of order 100 GeV/c2

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The CERN SPS• Produce W± and Z0

directly by colliding quarks and anti-quarks:

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1983: Observation of W and Z Bosons

W+ µ+ νµZ0 µ+ µ-

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But there’s more...• A theory with explicit mass for W’s and Z’s

is “Non-renormalizable” –• A theory with massless W’s and Z’s is

renormalizable...• By introducing the Higgs mechanism we

get the best of both worlds.• But we’ve added a new particle to the

theory... one that hasn’t yet been observed.

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The Standard ModelQ

uarksLeptons

Gauge

bosons

Higgs boson

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SLAC and LEP

• Masses of the W± and Z0 were known• Build electron-positron colliders to produce

them in large numbers• Make precision measurements tests of the

Standard Model

• SLAC upgraded their linear accelerator...• CERN dug a BIG tunnel...

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1987: Stanford Linear Collider

SLD detector

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Large Electron Positron ColliderSwiss Alps

Geneva

Airport

LEP tunnel

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ALPEH, DELPHI, L3, OPAL

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Z0 Production at LEP

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Physics from LEP

• Only 3 generations of quarks and leptons.

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1997: LEP II – W+W- Production

Weν

WWγ

WWZ

All Feynman diagrams are needed to explain the observed W+W- production cross section.

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The Higgs Boson?

• Direct searches at LEP did not find it.

• Although not directly observed, it should influence precision measurements:

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The Higgs Boson

80.3

80.4

80.5

150 175 200

mH [GeV]114 300 1000

mt [GeV]

mW

[G

eV]

68% CL

∆α

LEP1 and SLD

LEP2 and Tevatron (prel.)

Could it be just around the corner?

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The Large Hadron Collider• Replaced LEP with a proton-proton collider• Seven-fold increase in energy – 14 TeV

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CMS and ATLAS

People

High energy collisions and high intensity beams require complex detectors.

Lots of money, lots of people.

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What we still don’t understand• Why is the Higgs mass finite?

• Supersymmetry would fix this problem but would introduce hundreds of new particles.

• Neutrinos have mass! That breaks the standard model.

• Why are there only three generations of quarks and leptons?

• Are there only 4 space-time dimensions?• No easy way to incorporate gravity...

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Conclusions

• Matter is composed of fundamental, elementary particles.

• We can describe their properties with exquisite precision using Quantum Field Theory.

• We know our knowledge is incomplete.• We hope that the LHC will give us new (and

badly needed) experimental results.