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High Energy Accelerators

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SLAC Accelerator PEP rings. BaBar Detector. Typical collider detector elements ... LHC Tunnel and Accelerator. Cross Section of Two Beam Path. Magnets ... – PowerPoint PPT presentation

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Title: High Energy Accelerators


1
High Energy Accelerators
  • Dennis Silverman
  • Physics and Astronomy
  • U. C. Irvine

2
SLAC B Meson Factory
  • Neutral B0 mesons are composed of a u quark and a
    b antiquark.
  • They live long enough to go some distance in the
    detector, called BaBar.
  • They oscillate to their anti- B0 through
    annihilating to a W and W- pair.
  • In this oscillation there is a discrepancy
    between particle and antiparticle rates.
  • This allows us to learn about such a discrepancy
    that allowed the universe to remain one part in a
    billion matter after matter and antimatter
    annihilated in the big bang.
  • A similar B factory called Belle is producing
    similar results in Japan.

3
B Anti-B pairs formed by e e-Annihilation
  • B anti-B pair created through virtual photon

b-gtanti-B
e-
virtual photon
e
anti-b-gt B
4
SLAC Accelerator PEP rings
5
BaBar Detector
6
Typical collider detector elements
7
Fermilab Tevatron
  • Rings allow collisions of protons and
    anti-protons in their center of mass, each of
    1TeV energy.
  • Included quarks and anti-quarks colliding at a
    typical 1/3 of a TeV each.

Anti-proton
8
CDF (and D0) Detectors
9
LHC at CERN
  • Large Hadron Collider at CERN Geneva
  • 7 TeV protons on 7 TeV protons in their center of
    mass, 27 km long ring tunnel
  • Cost of 2.5 billion to international
    collaboration, U.S. about 0.5 billion share,
    including much manpower
  • Atlas and CMS detectors
  • Capable of producing Higgs and SUSY particles
  • Starting in 2007

10
LHC Ring Layout
11
LHC Tunnel and Accelerator
12
Cross Section of Two Beam PathMagnets
13
Atlas Detector Five Stories Tall
14
Neutrino Detectors
  • Large water detectors
  • Charged particles produce Cherenkov light cones
  • Detect atmospheric produced neutrinos from cosmic
    rays, and their oscillations
  • Detect solar neutrinos and their oscillations
  • Detect supernova produced neutrinos
  • Search for proton decay
  • Talk in the Fall from Hank Sobel

15
Super-K (Kamiokande)
16
Super-K
  • 11,000 20 inch phototubes
  • 50 kilotons of purified water
  • In a deep mine
  • Dimensions 40 m diameter, 40 m high

17
New Phototube layout
18
SNO (Sudbury Neutrino Detector)
  • 1 kiloton of Canadian
  • heavy water D20
  • 7 kilotons of normal
  • water surrounding
  • 18 m sphere
  • surrounding
  • 10,000 phototubes
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