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Particle Physics Particle Physics Chris Parkes April/May 2003 Hydrogen atom Quantum numbers Electron intrinsic spin Other atoms More electrons! Pauli Exclusion Principle Periodic Table Collisions Fixed-Target Colliding beam q 2 Cross-sections Differential xsecs Transition proby Luminosity Luminosity Reaction Kinematics Atomic Structure 2 nd Handout Second Handout http://ppewww.ph.gla.ac.uk/~parkes/teaching/PP/PP.html
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Natural Units, =c=1 Energy GeV Momentum GeV/c (abbreviated to GeV) Mass GeV/c 2 Length (GeV/ c) -1 c=0.197GeVfm=1 [1fm=1E-15m] Natural unit of length 1GeV -1 =0.197fm Time (GeV/ ) -1 =6.6E-25GeVs Natural unit of time 1GeV -1 =6.6E-25s Cross-section (GeV/ c) -2 1barn=10 -28 m 2 Natural unit of xsec =1GeV -2 =0.389mb Charge - ‘Heavyside-Lorenz units’ ε 0 =1 Use dimensionless ‘fine structure constant’
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Fixed Target experiment e.g. NuTeV Scatter neutrinos off nucleons (iron target) Measure sin 2 W Why does this have to be fixed target? Interaction consider with four momenta (E a,p a ) etc.. Total CM energy, a frame invariant [show this] b at rest:E b =m b See Appendix A Martin&Shaw for
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Colliding Beam LEP,Tevatron, LHC – synchotrons. SLC – 1990s e + e- 90GeV Linear Collider ILC – International Linear Collider, 500GeV e + e - ? [Now see Question 2.2] Symmetric beams – lab frame =CM frame Particle & anti-particle collision Four Momentum Transfer Defined as a c b d where ** Scattered through angle (in CM) ** When particles are not changed in the interaction i.e. a=c, b=d – elastic scattering process, magnitudes of momenta unchanged [Here * indicates CM frame] Hence q 2 0, when * 0, forward scattering, otherwise negative [Q 2 =t=-q 2 ] For large momenta in CM, can neglect masses, all momenta same
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Cross-Sections We perform an experiment: How many pions do we expect to see ? Duration of expt(t) Volume of target seen by beam (V) Density of p in target ( ) Beam incident /sec/Unit area (I) Solid angle of detector ( Ω) Efficiency of experiment (trigger/analysis) ( ) (I t) (V ) Ω (1/Area)(N o ) Ω Smashing beam into a target The constant of proportionality – the bit with the real physics in ! – is the differential cross-section NN Integration over 4 gives total cross-section Can divide total xsec into different reactions e.g. Xsec measured in barn, pb etc…
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Luminosity For colliding beams no V (target volume) term. Require two narrow beams with complete overlap at collision point Typical beam sizes 10-100 m in xy and cm in z Interaction rate is n 1,n 2 are number of particles in a bunch f is the frequency of collisions e.g. rotation in circular collider, this can be high, LHC 40 MHz! a is the bunch area of overlap at collision point (100% overlap) jn s -1 is known as the luminosity LHC plans 10 34 cm -2 s -1 Number of events = lumi x xsec x time Typically good machine running time is ~1/3 yr (1x10 7 s)
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Accelerators Considerations Considerations for an accelerator. reaction to be produced Energy required Luminosity required Events expected Particles are accelerated by electric field cavities. Achievable Electric fields few MV/m Higher energy = longer machine Fixed target expt. – not energy efficient but sometimes unavoidable (e.g. neutrino expts) Particles are bent into circles by magnetic fields. Synchrotron radiation – photons radiated as particle travels in circle E lost increases with 4, so heavy particles or bigger ring LEP/LHC 27km ring, long-term future a VLHC of 700km??! Or straight line… Linac – repetition rate slower as beams are not circulating Synchrotron – beams can circulate for several hours
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Deep Inelastic Scattering Quarks confined inside proton by potential [more about this later] Quarks have momentum distribution, each one carries a Varying fraction of the protons E,p call this fraction x At low q 2, scattering shows shape of proton At high q 2, small wavelength, scatter off quarks inside proton electron Proton At rest quark E,p xM E’,p’ m Consider scattered quark in proton v=E-E` q=p`-p Where q is 4-vector v,q Can tell momentum of quark by Looking only at electron! Find only ~½ momentum in quarks! Rest in gluons
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Transition Probability reactions will have transition probability How likely that a particular initial state will transform to a specified final state e.g. decays Interactions We want to calculate the transition rate between initial state i and final state f, We Use Fermi’s golden rule This is what we calculate from our QFT, using Feynman graphs This tells us that fi (transition rate) is proportional to the transition matrix element T fi squared (T fi 2 ) Transition rate Prob y of decay/unit time cross-section x incident flux IV
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