1. Feb 6, 2003M. Fincke-Keeler, Univ. of Victoria Motivation A little bit of history Orders of magnitude Elementary particles Tools: Accelerators and Detectors How to go about More things to find out…. Exploring the World of Elementary Particles

2. Motivation: Some people are just plain curious about the things around them and like to understand them at a deeper level.

3. 400-500 BC Democritus - Atoms ~ 1700 Newton: F=ma ~ 1800 Atoms are the smallest building blocks of matter ~ 1880 All physics is essentially understood ~ 1900 Big confusion: * What are “rays” ? * Energy comes in “lumps” (Planck). * Atoms are mainly empty (Rutherford). * It is impossible to measure the position and the momentum of a particle simultaneously to any desired precision (Heisenberg).

4. When we say we “understand something” we usually mean “it makes sense” (within the framework of experiences we have gathered in our lives so far). Scientists like to be slightly more objective: Mathematical frameworks exist, which describe many processes and phenomena very accurately - i.e. the results of the mathematical formalism agrees with the results observed in nature or in an experiment. Such frameworks are called: “Models” What do we mean when we say “we understand something” ?

5. Orders of Magnitude 1m 0.1m (10cm) 10 -2 m (1cm) 10 -3 m (1mm) 10m 100m 10 3 m (1km) 10 -4 m (0.1mm) 10 4 m (10km)

6. Orders of Magnitude ct’d 10 -4 m 10 -5 m 10 -6 m 10 -7 m 10 -8 m 10 -9 m 10 -10 m 10 -11 m 10 -12 m 10 -13 m 10 -14 m 10 -15 m (  ) 10 -18 m leptons, quarks (still ?) “pointlike” 10 -16 m 10 -17 m (  ) (  smaller than )

7. Understanding what matter is made of also involves an understanding of the origins of “mass”. Recent theories for a mechanism that could explain the origin of mass imply the existence of a so far undetected “Higgs particle” H Leptons Quarks t e u  c g dsb  ZW Electroweak and Strong Exchange Bosons Today we believe that “matter” as we know it is composed out of Leptons, Quarks and Exchange Bosons of the strong and electroweak forces: (carry colour, but have to form “colourless” observable particles) e  

8. The Higgs Mechanism A room full of physicists chattering quietlyis like space filled with the Higgs field A well known scientist walks in, creating a disturbance as he moves across the room and attracting a cluster of admirers with each step......this increases his resistance to movement - he acquires mass, just like a particle moving through the Higgs field. © CERN

9. Next, a rumor crosses the room... …it creates the same kind of clustering, but this time among the scientists themselves. In this analogy, these clusters are the Higgs particles.

10. Some Mesons: _  + : ud charge: +1  : 2.6 ·10 -8 s  +   +  _ _  o : (uu - dd)/  2 charge: 0  : 0.8 ·10 -16 s  o   _ _  - : du charge: -1  : 2.6 ·10 -8 s  -   -  Some Baryons: p : uud charge: +1  : > 10 31 s _ n : udd charge: 0  : 885 s n  p e -  + : uus charge: +1  : 0.8 ·10 -10 s  +  p  o ; n  +

11. What we are able to “see” depends on the wavelength Visible light: 500 nm (green) = 5 10 -7 m This is good for looking at “macroscopic” things:  object A good optical microscope resolves distances of about 1  m. Electron microscopes can resolve smaller distances. Make use of the wave attributes of the electron: = h/p With: h  4 10 -15 eV s and p  20 keV/c  0.06 nm (Resolution of an electron microscope: 0.2nm)

12. This experiment has also been done with electrons!

13. What we are able to “see” depends on the wavelength Good: small compared to object Not so good: large compared to object

14. Particle Energy Proton structure as predicted by: de Broglie wavelength Simple parton modelQCD 10 7 eV 10 11 eV 10 -14 m 10 -16 m 10 -17 m 10 -18 m 10 9 eV  2·10 10 eV

15. We can probe different aspects of particles depending on the type of particles we choose to accelerate Electrons: - no substructure  We have a good idea of what actually collides Protons: - are made up of “partons”  It can be difficult to untangle what happened in the collision  We get a chance to probe the partons

16. Two electrons collide at high energy: 50 GeV qq pairs e e ZoZo “jet”..

17. Two Protons collide at high energy: 7 TeV qq pairs p p “spectators” gluon “jet”

18. Some accelerators and experiments: Accelerator: SPS LEP LHC Particles: p e + e - p CM Energy: 5.4·10 11 eV (540 GeV) 0.9-2·10 11 eV (90-200 GeV) 1.4·10 13 eV (14 TeV) Experiment: UA1 OPAL ATLAS

19. The LEP (e + e - ) accelerator at CERN (Geneva)

21. UA1(1980’s) OPAL (1990’s) ATLAS (2007+) LEP/LHC SPS

22. Inside the LEP tunnel

23. L3 Experiment

24. OPAL experiment

25. How do we find things out? Particle properties that can be measured: Trajectory - fast moving charged particles leave a trail of ionization in their wake. Mass - particles ionize matter differently, depending on their mass Charge - a charged particle has a curved trajectory in a magnetic field. Energy - particles lose some or all of their energy as they travel through matter - this energy can be detected. These measurements are done simultaneously or consecutively, in order to gather the maximum amount of information.

26. tracking of charged particles (p,q,vertex) e.m. calorimeter (e,  stop here) hadronic calorimeter (  stop here)  detectors (with 4T toroidal B field) coil (2T solenoid) A typical collider experiment: Hermeticity missing energy (jets)

27. “Signatures” of particles in a high energy physics detector

29. OPAL calorimeter

30. Inside the tracking chamber of the UA1 experiment

31. Reconstructed particle tracks of the UA1 experiment

32. e+e+ e-e- ZoZo q q p p

33. e+e+ e-e- ZoZo q q

34. e+e+ e-e- ZoZo ++ -- e+e+ e-e- ZoZo e+e+ e-e-

35. e+e+ e-e- ZoZo e +,  +, q,... e -,  -, q, …. ~10 -25 seconds Many more possibilities: e+e+ e-e- Zo/Zo/ e+e+ e-e- e+e+ e-e- Zo/Zo/ e-e- e+e+ and all of them contribute...

36. Heisenberg’s Uncertainty Relation:  E  t  ћ  p  x  ћ If the lifetime  t of a particle is very short, it’s rest mass ( in terms of energy/c ) cannot possibly be determined any more precise than ћ/  t. We can determine the lifetime of the particle by measuring the “width” of the rest mass. Z o :  E = 2.5 GeV   t  ћ/  E = 6.6·10 -25 GeV·s/2.5GeV = 2.6 ·10 -25 s

37. q e+e+ e-e- /Zo/Zo q _ e+e+ e-e-  q _ q

38. Hot topics at the moment: Looking for a Higgs particle Neutrinos “oscillate” (and have mass!) Unification of all forces? Are there more particles than we know? (e.g. Supersymmetry) - More dimensions? Gravitational waves ? How did and does the universe evolve? Lots more mass in the universe than we had thought … “dark matter” (what actually is that?) W H Y …... ? ? ( http://pdg.web.cern.ch/pdg/particleadventure/ )

40. There are more things in heaven and earth, Horatio, Than are dreamt of in your philosophy. Hamlet, Act1, Scene5

42. A little bit of kinematics: For any particle with mass m: “Four momentum”: For several particles (eg: decay products):