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Particle Detection and Identification

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Presentation on theme: "Particle Detection and Identification"— Presentation transcript:

1 Particle Detection and Identification
Roger Barlow Particle Physics Masterclass Manchester, March 20th 2008

2 Studying Particles Detection: Where are they? Very small
Too small to see Identification: What are they? The particle-spotters’ guide

3 Detecting particles Rule 1: You can’t detect neutral particles, only charged particles. Rule 2: You can only detect charged particles if they’re moving – quite fast. Rule 3: Even then the signals are small and need amplifying Rule 4: You can only detect charged particles with ‘long’ lifetimes, i.e. >~1 ns. That basically means e, , , K, p

4 Small but with a big kick
Charged Particle Excited electron Electric Field What next? Two options ATOM

5 Option 1: Excited to a higher level
Photon Drops back

6 Many atoms – many photons
Scintillation particle Light Good for measuring Timing Energy loss Bad for measuring position Collected and amplified by photomultiplier

7 Option 2: Excited all the way out
Positive ion Free electron

8 Tracking detectors Electrons=charge=current
Wire in a gas Big field near wire Amplification through avalanche process Good for position Wire At ~1 kV Geiger counter Multiwire chambers Drift chambers

9 Tracking Chambers + - - + - + + - - + + - - + + - - + - +

10 Summary so far We can detect a fast charged particle in all sorts of ways, based on Scintillation Ionisation What next?

11 Identification: What are they?
Birds: Size Shape Colour Sound Behaviour Particles Size Shape Colour Sound Behaviour electron Hadron (pi, K) muon proton positron

12 What Charge is it? + or - ? Apply a magnetic field
Particle curves to right or left depending on its charge Bonus: faster particles curve less Bend depends on momentum This measures momentum and direction

13 Tracking B Path of a charged particle A measured point

14 Spotting electrons/positrons
Intersperse Sensitive material – scintillators or tracking chambers Dense material – sheets of iron or lead (or …) Electrons and positrons shower rapidly e- e-    e+ e- Hadrons shower more slowly Collide with protons/neutrons and produce more hadrons Muons don’t shower No strong interaction Bonus: photons convert to electrons and then shower Bonus: size of shower gives the energy

15 Calorimeters Incoming electron, positron or photon Electron-positron Pair Shower of secondary particles Count number of secondary particles in showerenergy of incoming particle

16 Spotting muons Do not interact much No shower in calorimeter
Penetrate through shielding Muon detector = charged particle detector put where other charged particles would be screened out Muon in Muon out Absorber

17 Spotting hadrons Anything that is not a muon or an electron is a hadron (pion, kaon, proton) Telling the difference is possible but more complicated and less reliable…

18 Parts of a Detector Muon chambers Calorimeters Tracking B

19 DELPHI Detector

20 Another detector: BaBar

21 Yet another detector: ATLAS

22 What about quarks? u,d,s,c,b,t Never been seen directly
Manifest as jets of hadrons Bonus: gluons look almost just like quarks

23 Quarks are jets e+ e-  q q Many tracks Mostly hadrons
Hadrons collimated into jets Jets back to backs

24 Conclusion Elementary particles are very small BUT we can detect them
Lots of different techniques – no single best method New ideas evolving all the time Yesterday’s detectors look primitive compared to today’s sophisticated and ingenious devices Tomorrow’s will be even better.


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