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Particle Detectors Thomas Coan SMU What to detect? How to probe?

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Presentation on theme: "Particle Detectors Thomas Coan SMU What to detect? How to probe?"— Presentation transcript:

1 Particle Detectors Thomas Coan SMU What to detect? How to probe?
What is a “detector?” Putting it all together Some examples

2 Particle Properties mass lifetime electric charge ”spin”
Thomas Coan/SMU Quarknet 2001 Particle Properties mass lifetime electric charge ”spin”

3 General Idea of Colliding Particle Experiments
Thomas Coan/SMU Quarknet 2001 General Idea of Colliding Particle Experiments Collide probe particles with target Detect particles from collision Interpret results

4 Early Particle Physics Experiment
Thomas Coan/SMU Quarknet 2001 Early Particle Physics Experiment Ernest Rutherford 1909 Set-up: Interpretation:

5 How do we “shoot” probe particles?
Thomas Coan/SMU Quarknet 2001 How do we “shoot” probe particles? Acquire some probe particles Accelerate the probe particles Final speed  c Steer and aim the probe particles

6 Thomas Coan/SMU Quarknet 2001 Accelerator Types Circular

7 Thomas Coan/SMU Quarknet 2001 Accelerator Types Linear

8 Thomas Coan/SMU Quarknet 2001 Target Types Colliding beam Fixed target

9 Wave Nature of Particles
Thomas Coan/SMU Quarknet 2001 Wave Nature of Particles Waves interfere: Electron diffraction: particle as wave

10 Why use higher and higher energies?
Thomas Coan/SMU Quarknet 2001 Why use higher and higher energies?  = h/p The more energetic the probe, the finer the accessible detail

11 Thomas Coan/SMU Quarknet 2001 Collide

12 Trajectory measurement
Thomas Coan/SMU Quarknet 2001 Trajectory measurement Charged particle Noble “fill gas” Electric field Drifting ionized e- “Drift time”  DOCA Magnetic field curves trajectory “curvature”  1/p

13 Thomas Coan/SMU Quarknet 2001 CLEO Drift Chamber

14 Thomas Coan/SMU Quarknet 2001 CLEO Drift Chamber

15 Thomas Coan/SMU Quarknet 2001 CLEO Calorimeter Measure particle energy (plus position and flight path angle) Good for charged and neutral particles Particles deposit energy in dense, transparent medium Medium produces light, proportional to particle energy

16 Scintillation Complicated phenomenon
Thomas Coan/SMU Quarknet 2001 Scintillation Complicated phenomenon Basic idea: convert particle kinetic energy into light Amount of light proportional to particle energy Light emission is prompt: scintillators useful as timers Scintillators used mostly w/ charged particles

17 Sea-level muon detector
Thomas Coan/SMU Quarknet 2001 Sea-level muon detector PMT Scintillator Discriminator Discriminator PMT Scintillator Photons enter here Photomultiplier tube (PMT)

18 Thomas Coan/SMU Quarknet 2001

19 Determine production height of muons
Thomas Coan/SMU Quarknet 2001 Determine production height of muons 2 1 Atmosphere 3 1 2 3 h Earth Sea level  flux depends on pathlength from production point Changing telescope angle changes pathlength Flux change  production height h

20 Cerenkov Radiation Emitted by charged particles only
Thomas Coan/SMU Quarknet 2001 Cerenkov Radiation Emitted by charged particles only Emitted only when particle’s speed in medium exceeds that of light’s Pattern of light has cone-like shape: Particle’s speed determines shape of cone Cerenkov detectors measure particle speed Particle momentum (mv) and speed (v)  mass

21 Cerenkov Radiation Cerenkov radiator built here at SMU for CLEO
Thomas Coan/SMU Quarknet 2001 Cerenkov Radiation Cerenkov radiator built here at SMU for CLEO

22 Particle “Fingerprints”
Thomas Coan/SMU Quarknet 2001 Particle “Fingerprints”

23 Thomas Coan/SMU Quarknet 2001 Russian Dolls (Anna Kournakova?)

24 Thomas Coan/SMU Quarknet 2001 “Top” event

25 How to “see” neutrinos Sudbury Neutrino Observatory (SNO)
Thomas Coan/SMU Quarknet 2001 How to “see” neutrinos Sudbury Neutrino Observatory (SNO)

26 Cerenkov Light in Action
Thomas Coan/SMU Quarknet 2001 Cerenkov Light in Action

27 Sudbury Neutrino Observatory
Thomas Coan/SMU Quarknet 2001 Sudbury Neutrino Observatory

28 Summary Variety of detector types Detector combinations are the key
Thomas Coan/SMU Quarknet 2001 Summary Variety of detector types Detector combinations are the key Detector behavior is understandable


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