Quantum Chromo Dynamics
|
|
- Ethelbert Baldwin
- 5 years ago
- Views:
Transcription
1 Quantum Chromo Dynamics Evidence for Fractional Charges Color Gluons Color Transformations Quark Confinement Scaling Violations The Ratio R Deep Inelastic Scattering Structure of the Proton
2 Introduction QUANTUM ELECTRODYNAMICS: is the uantum theory of the electromagnetic interaction. mediated by massless photons photon couples to electric charge, Strength of interaction :. QUANTUM CHROMO-DYNAMICS: is the uantum theory of the strong interaction. mediated by massless gluons, i.e. propagator gluon couples to strong charge Only uarks have non-zero strong charge, therefore only uarks feel strong interaction
3 Introduction Basic QCD interaction looks like a stronger version of QED, QED Q α α = e 2 /4π ~ 1/137 γ QCD α S α S = g S 2/4π ~ 1 g ( subscript em is sometimes used to distinguish the of electromagnetism from ). In QED: Charge of QED is electric charge. Electric charge - conserved uantum number. In QCD: Charge of QCD is called COLOUR COLOUR is a conserved uantum number with 3 VALUES labelled red, green and blue
4 Evidence for Fractional Charge Production of lepton pairs in Pion-Carbon scattering: Electromagnetic annihilation of a uark and an anti-uark in pionnucleon collisions: a virtual photon converts into a muon pair annihilate photon μ + μ + The cross section σ ~ charge of charge of Since the and have opposite charges: σ ~ [charge of ] 2
5 Evidence for Fractional Charge Use an 'Isoscalar' target same number of u and d uarks 12 C has 6 protons (uud) and 6 neutrons (udd) 6 18 u + 18 d For π (ud) uu annihilation to μ μ + For π + (ud) dd annihilation to μ μ + σ(π C µ + µ + anything) 18 Q u 2 =18 4 /9 σ(π + C µ + µ + anything) 18 Q d 2 =18 1/9 Good agreement with experiment Also results from electron and neutrino scattering from nuclei
6 Quark Colour Why do we need coloured uarks? In the baryon decuplet J P = 3 /2 +, the Δ ++ is u u u with angular momentum l = 0 i.e. 3 fermions in the same state violates Pauli Exclusion Principle Wavefunction symmetric in space, spin and flavour not allowed for fermions Introduce a new Degree of Freedom Colour 3 'colours' red r, blue b, green g Now the 3 fermions are in different states: u (red) u (blue) u (green) Not real colour just a new uantum number that distinguishes them!
7 The corner states of the decuplet (uuu), (ddd) and (sss) are symmetric under flavorinterchange (therefore, also the other states are assumed to behave the same). The decuplet members are indeed the 10 uark combinations (out of 27) symmetric under space, spin and flavor exchange We also assume that each baryon is a properly normalized combination of permuted states, e.g. : Colour (ddu) = 1 (ddu + udd + dud) 3 (dus) = 1 6 (dsu + uds + sud + sdu + dus + usd) Since the decuplet members are spin 3/2 baryons of the lowest mass, we assume the three uarks are in the (spatially symmetric) ground state (l=0). This implies that the three spins are parallel: is the Pauli principle violated? Need another degree of freedom (uantum number) that can be different for the three uarks: color(red, blue, green) such that the hadron net color is 0. Indeed, experimentally one only detects protons and not red or green protons. The three colors are the source of the strong-force charge. The strong force is independent of the uark color, i.e. the SU(3) color symmetry is exact.
8 Quark Colour However they work like colours on a computer red green blue Red Green Blue Cyan = anti-red r Magenta = anti-green g Yellow = anti-blue b White Black Baryons consist of r + g + b = = white colourless Mesons consist of r + r = = = white colourless (or g + g or b + b)
9 Gluons These are: Expect 9 combinations (r, g, b) (r, g, b) r b r g g r g b b g b r r r g g b b mix Colourless and symmetric under r b g colour change. Doesn't interact 8 interacting gluons
10 Colour Charge The 'Color Charge' is the Strong Interaction euivalent of Electric Charge in Electromagnetism Quantum Chromodynamics (QCD) is the uantum field theory of the strong 'color' interaction between uarks The strong force is carried by 8 massless vector gluons (J P = 1 ). They are euivalent to pairs i.e. rb, gr,.. etc.. This is an non-abelian theory where the force carriers have the charge and can interact with each other unlike electromagnetism where the photons carry NO charge and don't interact with each other
11 QCD Colour Transformations QCD is a gauge theory. Gauge means scale or absolute potential. Consider a proton made up of one red, one green and one blue uark. Do a global colour transformation red green everywhere Still 'colourless' nothing has changed
12 QCD Colour Transformations Local Colour Transformations Now do a local colour transformation red green at one uark only Can be made colourless if A emits an rg gluon which is absorbed at C. When the gluon is absorbed at C the green and anti-green annihilate to make C red. No longer colourless g + rg r Colourless again Local colour transformation exchange of gluons force
13 The Local Gauge Principle The Local Gauge Principle All the interactions between fermions and spin-1 bosons in the SM are specified by the principle of LOCAL GAUGE INVARIANCE To arrive at QED, reuire physics to be invariant under the local phase transformation of particle wave-functions Note that the change of phase depends on the space-time coordinate: Under this transformation the Dirac Euation transforms as To make physics, i.e. the Dirac euation, invariant under this local phase transformation FORCED to introduce a massless gauge boson,. + The Dirac euation has to be modified to include this new field: The modified Dirac euation is invariant under local phase transformations if: Gauge Invariance
14 The Local Gauge Principle For physics to remain unchanged must have GAUGE INVARIANCE of the new field, i.e. physical predictions unchanged for Hence the principle of invariance under local phase transformations completely specifies the interaction between a fermion and the gauge boson (i.e. photon): interaction vertex: QED! The local phase transformation of QED is a unitary U(1) transformation i.e. with Now extend this idea
15 From QED to QCD Suppose there is another fundamental symmetry of the universe, say invariance under SU(3) local phase transformations i.e. reuire invariance under where are the eight 3x3 Gell-Mann matrices introduced in handout 7 are 8 functions taking different values at each point in space-time 8 spin-1 gauge bosons wave function is now a vector in COLOUR SPACE QCD! QCD is fully specified by reuire invariance under SU(3) local phase transformations Corresponds to rotating states in colour space about an axis whose direction is different at every space-time point interaction vertex: Predicts 8 massless gauge bosons the gluons (one for each ) Also predicts exact form for interactions between gluons, i.e. the 3 and 4 gluon vertices the details are beyond the level of this course
16 Colour in QCD Colour in QCD The theory of the strong interaction, Quantum Chromodynamics (QCD), is very similar to QED but with 3 conserved colour charges In QED: In QCD: the electron carries one unit of charge the anti-electron carries one unit of anti-charge the force is mediated by a massless gauge boson the photon uarks carry colour charge: anti-uarks carry anti-charge: The force is mediated by massless gluons In QCD, the strong interaction is invariant under rotations in colour space i.e. the same for all three colours SU(3) colour symmetry This is an exact symmetry, unlike the approximate uds flavour symmetry discussed previously.
17 Colour in QCD Represent SU(3) colour states by: Colour states can be labelled by two uantum numbers: colour isospin colour hypercharge Exactly analogous to labelling u,d,s flavour states by Each uark (anti-uark) can have the following colour uantum numbers: and uarks anti-uarks
18 Colour Confinement It is believed (although not yet proven) that all observed free particles are colourless i.e. never observe a free uark (which would carry colour charge) conseuently uarks are always found in bound states colourless hadrons Colour Confinement Hypothesis: only colour singlet states can exist as free particles All hadrons must be colourless i.e. colour singlets To construct colour wave-functions for hadrons can apply results for SU(3) flavour symmetry to SU(3) colour with replacement g r just as for uds flavour symmetry can define colour ladder operators b
19 Colour Singlets It is important to understand what is meant by a singlet state Consider spin states obtained from two spin 1/2 particles. Four spin combinations: Gives four eigenstates of spin-1 triplet spin-0 singlet The singlet state is spinless : it has zero angular momentum, is invariant under SU(2) spin transformations and spin ladder operators yield zero In the same way COLOUR SINGLETS are colourless combinations: they have zero colour uantum numbers invariant under SU(3) colour transformations ladder operators all yield zero NOT sufficient to have : does not mean that state is a singlet
20 Meson Colour Wave-function Wavefunction Consider colour wave-functions for The combination of colour with anti-colour is mathematically identical to construction of meson wave-functions with uds flavour symmetry Coloured octet and a colourless singlet Colour confinement implies that hadrons only exist in colour singlet states so the colour wave-function for mesons is: Can we have a state? i.e. by adding a uark to the above octet can we form a state with. The answer is clear no. bound states do not exist in nature.
21 Baryon Colour Wavefunction Do bound states exist? This is euivalent to asking whether it possible to form a colour singlet from two colour triplets? Following the discussion of construction of baryon wave-functions in SU(3) flavour symmetry obtain No colour singlet state Colour confinement bound states of do not exist BUT combination of three uarks (three colour triplets) gives a colour singlet state (pages )
22 Baryon Color Wavefunction The singlet colour wave-function is: Check this is a colour singlet It has : a necessary but not sufficient condition Apply ladder operators, e.g. (recall ) Similarly Colourless singlet - therefore bound states exist! Anti-symmetric colour wave-function Allowed Hadrons i.e. the possible colour singlet states Mesons and Baryons Exotic states, e.g. pentauarks To date all confirmed hadrons are either mesons or baryons. However, some recent evidence for pentauark states (LHCb experiment).
23 Gluons In QCD uarks interact by exchanging virtual massless gluons, e.g. b r b r b rb br r r b r Gluons carry colour and anti-colour, e.g. b r r r b r b br rb rr Gluon colour wave-functions (colour + anti-colour) are the same as those obtained for mesons (also colour + anti-colour) OCTET + COLOURLESS SINGLET
24 Gluons So we might expect 9 physical gluons: OCTET: SINGLET: BUT, colour confinement hypothesis: only colour singlet states can exist as free particles Colour singlet gluon would be unconfined. It would behave like a strongly interacting photon infinite range Strong force. Empirically, the strong force is short range and therefore know that the physical gluons are confined. The colour singlet state does not exist in nature! NOTE: this is not entirely ad hoc. In the context of gauge field theory (see minor option) the strong interaction arises from a fundamental SU(3) symmetry. The gluons arise from the generators of the symmetry group (the Gell-Mann matrices). There are 8 such matrices 8 gluons. Had nature chosen a U(3) symmetry, would have 9 gluons, the additional gluon would be the colour singlet state and QCD would be an unconfined long-range force. NOTE: the gauge symmetry determines the exact nature of the interaction FEYNMAN RULES
25 Self Interaction Gluons that carry colour charges can interact with each other (Non-Abelian) 16 gluons 8 gluons 4 gluons 'Strength' of the colour charge appears to decrease as distance decreases (energy increases)
26 Gluon-Gluon Interactions Gluon-Gluon Interactions In QED the photon does not carry the charge of the EM interaction (photons are electrically neutral) In contrast, in QCD the gluons do carry colour charge Gluon Self-Interactions Two new vertices (no QED analogues) triple-gluon vertex uartic-gluon vertex In addition to uark-uark scattering, therefore can have gluon-gluon scattering e.g. possible way of arranging the colour flow
27 Free Quarks? Many searches for 'free' uarks not bound into hadrons: Search for stable fractional charged particles 'exotic' atoms - Moon rock, deep sea sludge,... Search for fractional charges in Millikan oil drop type experiments Look in accelerators and cosmic rays for particles with 1/9 or 4/9 ionisation of normal particles No evidence for isolated free fractionally charged uarks Why?
28 Quark Confinement The reason there are no free uarks, and the only stable configurations are and (and possible gg 'glueball' states) is due to the fact that α S decreases with increasing energy and increases with increasing distance At short distance, inside a proton, α S is small and the uarks are 'free' Try and pull one out and α S increases and the force tries to keep it in
29 Gluon Self-Interaction and Confinement Gluon self-interactions and Confinement Gluon self-interactions are believed to give rise to colour confinement Qualitative picture: Compare QED with QCD In QCD gluon self-interactions sueeze lines of force into a flux tube What happens when try to separate two coloured objects e.g. e + e - Form a flux tube of interacting gluons of approximately constant energy density Reuire infinite energy to separate coloured objects to infinity Coloured uarks and gluons are always confined within colourless states In this way QCD provides a plausible explanation of confinement but not yet proven (although there has been recent progress with Lattice QCD)
30 Hadronization and Jets Hadronisation and Jets Consider a uark and anti-uark produced in electron positron annihilation i) Initially Quarks separate at high velocity ii) Colour flux tube forms between uarks iii) Energy stored in the flux tube sufficient to produce pairs iv) Process continues until uarks pair up into jets of colourless hadrons This process is called hadronisation. It is not (yet) calculable. The main conseuence is that at collider experiments uarks and gluons observed as jets of particles e + e
31 Hadronization In high energy interactions you don't see the produced uarks but 'jets' of hadrons Analogy: Gluons are like bits of elastic and uarks are the ends There are no free ends If you pull hard enough you get two bits of elastic but still no free ends
32 Quark Gluon Interaction The Quark Gluon Interaction Representing the colour part of the fermion wave-functions by: Particle wave-functions The QCD g vertex is written: Only difference w.r.t. QED is the insertion of the 3x3 SU(3) Gell-Mann matrices Gluon a Isolating the colour part: Hence the fundamental uark - gluon QCD interaction can be written colour i! j
33 External Lines spin 1/2 spin 1 Feynman Rules of QCD Feynman Rules for QCD incoming uark outgoing uark incoming anti-uark outgoing anti-uark incoming gluon outgoing gluon Internal Lines (propagators) spin 1 gluon Vertex Factors spin 1/2 uark a, b = 1,2,,8 are gluon colour indices i, j = 1,2,3 are uark colours, a = 1,2,..8 are the Gell-Mann SU(3) matrices + 3 gluon and 4 gluon interaction vertices Matrix Element -im = product of all factors
34 Quark Quark Scattering Consider QCD scattering of an up and a down uark u d u d The incoming and out-going uark colours are labelled by In terms of colour this scattering is The 8 different gluons are accounted for by the colour indices NOTE: the -function in the propagator ensures a = b, i.e. the gluon emitted at a is the same as that absorbed at b Applying the Feynman rules: where summation over a and b (and and ) is implied. Summing over a and b using the -function gives: Sum over all 8 gluons (repeated indices)
35 QCD vs QED QCD vs QED QED e e QCD u u QCD Matrix Element = QED Matrix Element with: or euivalently d d + QCD Matrix Element includes an additional colour factor
36 Colour Factors QCD colour factors reflect the gluon states that are involved Gluons: Configurations involving a single colour r r Only matrices with non-zero entries in 11 position are involved r r Similarly find
37 r r Colour Factors Other configurations where uarks don t change colour e.g. Only matrices with non-zero entries in 11 and 33 position are involved b b Similarly Configurations where uarks swap colours r g e.g. Only matrices with non-zero entries in 12 and 21 position are involved g r Gluons Configurations involving 3 colours r b b g e.g. Only matrices with non-zero entries in the 13 and 32 position But none of the matrices have non-zero entries in the 13 and 32 positions. Hence the colour factor is zero colour is conserved
38 Colour Factors Recall the colour part of wave-function: The QCD g vertex was written: Now consider the anti-uark vertex The QCD g vertex is: Note that the incoming anti-particle now enters on the LHS of the expression For which the colour part is i.e indices ij are swapped with respect to the uark case Hence c.f. the uark - gluon QCD interaction
39 Colour Factors Finally we can consider the uark anti-uark annihilation QCD vertex: with Conseuently the colour factors for the different diagrams are: e.g. Colour index of adjoint spinor comes first
40 Quark-Quark Scattering Quark-Quark Scattering Consider the process which can occur in the high energy proton-proton scattering jet There are nine possible colour configurations of the colliding uarks which are all eually likely. Need to determine the average matrix element which is the sum over all possible colours divided by the number of possible initial colour states p jet d u d u p The colour average matrix element contains the average colour factor For rr rr,.. rb rb,.. rb br,..
41 Quark-Quark Scattering Previously derived the Lorentz Invariant cross section for e e elastic scattering in the ultra-relativistic limit. QED For ud ud in QCD replace and multiply by QCD Never see colour, but enters through colour factors. Can tell QCD is SU(3) Here is the centre-of-mass energy of the uark-uark collision The calculation of hadron-hadron scattering is very involved, need to include parton structure functions and include all possible interactions e.g. two jet production in proton-antiproton collisions
42 QED Running Coupling Constants Running Coupling Constants bare charge of electron screened by virtual e + e pairs behaves like a polarizable dielectric In terms of Feynman diagrams: -Q +Q Same final state so add matrix element amplitudes: Giving an infinite series which can be summed and is euivalent to a single diagram with running coupling constant Note sign
43 Running Coupling Constants Might worry that coupling becomes infinite at i.e. at OPAL Collaboration, Eur. Phys. J. C33 (2004) But uantum gravity effects would come in way below this energy and it is highly unlikely that QED as is would be valid in this regime In QED, running coupling increases very slowly Atomic physics: High energy physics:
44 Running of α S Running of s QCD Similar to QED but also have gluon loops Fermion Loop Boson Loops Remembering adding amplitudes, so can get negative interference and the sum can be smaller than the original diagram alone Bosonic loops interfere negatively with = no. of colours = no. of uark flavours S decreases with Q2 Nobel Prize for Physics, 2004 (Gross, Politzer, Wilczek)
45 Colour Charge Strength s for strong α S ~ 0.2 at E = 30 GeV Compare with electromagnetic interaction α EM ~ 1/137 ~ Low energy Long distance High energy Short distance
46 Running of α S Measure S in many ways: jet rates DIS tau decays bottomonium decays α (µ) 0.2 QCD Prediction As predicted by QCD, S decreases with Q µ (GeV) At low : S is large, e.g. at find S ~ 1 Can t use perturbation theory! This is the reason why QCD calculations at low energies are so difficult, e.g. properties hadrons, hadronisation of uarks to jets, At high : S is rather small, e.g. at find S ~ 0.12 Asymptotic Freedom Can use perturbation theory and this is the reason that in DIS at high uarks behave as if they are uasi-free (i.e. only weakly bound within hadrons)
47 QCD in e + e - Annihilation e - e + Cleanest laboratory for studying perturbative QCD: No hadrons in initial state No remnants of initial proton(s) Quarks and gluons produced at short distances and emerge as jets
48 Two Jet Event e - e + Distribution follows dσ d(cosϑ) cm (1 + cos 2 ϑ) Just like e + e - -> µ + µ - -> uarks have spin 1/2
49 Proof that Gluons Exist e- e- e- e- Gluons fragment into jets similarly to uarks so expect 3 jet events
50 Proof that Gluons Exist 3 jet events observed at rate consistent with expectations
51 The Ratio R [ some threshold kinematics factors] Sum over all contributing uarks Charge of μ 2 As uarks come in 3 colours: The fact that the factor of 3 is necessary is very strong evidence in support of the colour hypothesis
52 The Ratio R Flavour : u d s c b t Charge 2 : (⅔) 2 (-⅓) 2 (-⅓) 2 (⅔) 2 (-⅓) 2 (⅔) 2 For ECM ~ 2 GeV have uu, dd, ss R = 3 (4/9 + 1/9 + 1/9) = 2 For ECM ~ 5 GeV have uu, dd, ss, cc R = 3 (4/9 + 1/9 + 1/9 + 4/9) = 3⅓ Need ~3 GeV to make cc Need ~10 GeV to make bb For ECM ~ 11 GeV have uu, dd, ss, cc, bb R = 3 (4/9 + 1/9 + 1/9 + 4/9 + 1/9) = 3⅔
53 The R Ratio e - e + PDG
54 The Ratio R u + d + s 2 u + d + s + c 3.3 u + d + s + c + b 3.7 colour factor of 3
55 u, d, s: R 0 = 3 ( u2 + d2 + s2 ) = 2 u, d, s, c: R 0 = 3 ( u2 + d2 + 2 s + c2 ) = 10/3 = 3.3 u, d, s, c, b: R 0 = 3 ( u2 + d2 + 2 s + 2 c + b2 ) = 11/3 = 3.7 u, d, s, c, b, t: R 0 = 3 ( u2 + d2 + 2 s + 2 c + 2 b + t2 ) = 5
56 Any more Quarks? We have 3 full generations. We only need one (u, d, e, ѵe) for everyday life So if 3 why not more? Since it is not understood why there are 3 generations there is no theoretical reason why there shouldn't be more (Periodic Table again?) However, experimental evidence now suggests only 3 In early 1990s LEP measured the width of the Z 0 to very high precision. The Z 0 can decay into any fermion pairs with a combined mass less than the Z 0 mass (~90 GeV/c 2 ) f = u, d, s, c, b, e, μ, τ, ѵe, ѵμ, ѵτ The more ways the Z 0 can decay, the shorter its lifetime τ and the larger its width Γ (Γ τ ~ ħ)
57 Any more Quarks? Generation u c t h... Z 0 tt since M Z 0 < 2M t d s b l... e μ τ χ... ѵe ѵμ ѵτ ν χ... The Z 0 can decay into all these The Z 0 would decay into any new neutrinos assuming they were massless (or light compared with M Z 0)
58 The Width of the Z 0 We know how much each uark/lepton pair contributes to Γ Z 0 Γ Z 0 = Γ uu + Γ dd + Γ ss + Γ cc + Γ bb + Γ e + e + Γ μ + μ + Γ τ + τ + N ѵ Γ ѵѵ Each of the Γ uu etc are known as partial widths A measurement of Γ Z 0 is euivalent to measuring the number of neutrino species N ѵ If there is one neutrino species per generation as now total number of generations Result from LEP: N ѵ = ± i.e. only 3 generations This is only true if the new neutrinos are light but they cannot be too heavy or they would contribute too much mass to the Universe Astrophysical constraint on neutrino masses
59 The Width of the Z 0 Data points
60 Deep Inelastic Scattering Shoot high energy electrons at protons Scattering angle θ related to momentum transfer = (k k') x is the fraction of the proton's momentum carried by the struck uark 0 x 1 The total energy of the hadrons from the struck uark is + xp Measure hadron energy + scattering angle θ deduce x
61 Scaling Violations x is a 'scaled' parameter i.e. x = p uark / p proton - so naively expect uark and antiuark distributions to depend on x and not energy But see 'scaling violations' at higher energies probe deeper into the proton and see more 'structure i.e. more of the proton's momentum appears to be carried by gluons and pairs and less by valence uarks valence uarks high energy valence uarks low energy Distribution depends on x and energy
62 Structure of the Proton Protons are very complicated and have a lot more in them than just two up uarks and a down uark. There are zillions of gluons, antiuarks, and uarks in a proton. The standard shorthand, the proton is made from two up uarks and one down uark, is really a statement that the proton has two more up uarks than up antiuarks, and one more down uark than down antiuarks. The proton consists of partons: three valence uarks (uud), an infinite sea of light uarkantiuark pairs (sea uarks), and gluons. The protons viewed at ever higher resolution appears more and more as field energy (soft glue).
63 Parton Distribution Functions Introduced by Feynman (1969) in the parton model, to explain Bjorken scaling in deep inelastic scattering data The number densities of the partons in the proton depend on the probing energy scale, Q 2, and parton momentum fraction, x, with respect to the momentum of the proton, expressed by a parton distribution function (PDF), f i (x,q 2 ), for each parton i. Interpretation as probability distributions: P uv `x1, x 2, Q 2 Z x2 According to the QCD factorization theorem for inclusive hard scattering processes, universal distributions containing long-distance structure of hadrons; related to parton model distributions at leading order, but with logarithmic scaling violations. PDFs are extracted from fits to the deep inelastic lepton-hadron scattering experimental data using the Dokshitzer-Gribov-Lipatov- Altarelli-Parisi (DGLAP) evolution euations. x 1 dxu V (x, Q 2 )
64 Proton Structure The proton consists of u u d + pairs At energies ~ 10 GeV Valence uarks Sea uarks valence uarks antiuarks
65 Parton Distribution Functions The curves all fall off very uickly as x increases; you are very unlikelyindeed to hit anything with more than 50% of the proton s energy. Most particles in the proton carry much less than 10% (that is, x< 0.1) of the proton s energy, and you are more likely to hit one of those, with lower energies than with higher ones. If you do hit something that carries less than 10% of the proton s energy, then it is most likely a gluon; and uarks and antiuarks are about eually likely once you get below about 2% of the proton s energy. If you hit something with much above 20% (that is, x>0.2) of the proton s energy which is very rare it is most likely a uark, and about twice as likely to be an up uark as a down uark
66 Structure of the Proton U U d d d s s Proton is composed of u,d valence uarks which carry uantum numbers and " sea" of u, u, d, d, s, s, g with _ no _ net _ uantum _ number
67 Constraints on Parton Density Functions The charm, beauty and top compositions are negligible so proton is composed of u, d, s uarks and anti uarks and glue. The observed uantum number constraints No net strangeness ( s( x) s( x)) dx = 0 Charge =1 Isospin I 3 =1/2 1 1 [ ( u( x) u( x)) ( d( x) d ( x))] dx = ( u( x) u( x)) ( d( x) d ( x)) ( s( x) s( x)) dx = Leads to: ( u( x) u( x)) dx = 2 ( d( x) d ( x)) dx = 1 Two u uarks and 1 d uark as expected. These are called sum rules and there is one for every uantum number. Momentum sum rule: x[ u( x) + u( x) + d( x) + d ( x) + s( x) + s( x) g( x)] dx = 1
68 Early Data on Proton Structure SLAC-MIT ~20 GeV electrons, protons at rest, Q 2 = few GeV 2 BCDMS GeV muons, protons at rest, Q 2 = tens of GeV 2
69 PDFs u(x) and d(x) parton distributions for proton µ = Q x(x) u(x) d(x) x
70 PDFs u(x) and u(x) parton distributions for proton x(x) u(x) valence + sea u ( x) sea only x
71 Gluon Distribution Quark distributions can be measured by e or µ scattering but not the gluon distribution as gluons are not electrically charged. A nonzero gluon distribution can be inferred from the momentum sum rule: so: x( u( x) + u( x) + d( x) + d ( x) + s( x) + s( x) + g( x) ) dx = 1. 0 xg( x) dx 1.0 ( u( x) + u( x) + d( x) + d ( x) + s( x) + = s( x)) dx More generally, Q 2 evolution of (x,q 2 ), and hence F i (x,q 2 ), involves g(x,q 2 ), so gluon distribution can be extracted that way. Nevertheless, it is not as well known as the uark distributions.
72 PDFs Gluons carry 50% of proton momentum xg ( x) dx = 0. 5 x(x) g(x) u(x) +d(x) x
73 PDFs At high Q 2 = µ 2 see more of sea x(x) u(x) 500 GeV u(x) 5 GeV x
74 PDFs At high Q 2 see less valence uarks more sea antiuarks x(x) u( x) 500 GeV u( x) 5 GeV u(x) 5 GeV x
75 PDFs More low x gluons less high x valence uarks at high Q 2 x(x) g( x) 500 g( x) 5 GeV GeV x
76 Quark uantum numbers Flavor I I 3 S C B* T Q/e u 1/2 1/ /3 d 1/2-1/ /3 s /3 c /3 b /3 t /3 Q/e = I (B + C + S + B *+T) 2 Baryon number :1/3 for all uarks
Kern- und Teilchenphysik II Lecture 1: QCD
Kern- und Teilchenphysik II Lecture 1: QCD (adapted from the Handout of Prof. Mark Thomson) Prof. Nico Serra Dr. Marcin Chrzaszcz Dr. Annapaola De Cosa (guest lecturer) www.physik.uzh.ch/de/lehre/phy213/fs2017.html
More informationKern- und Teilchenphysik I Lecture 13:Quarks and QCD
Kern- und Teilchenphysik I Lecture 13:Quarks and QCD (adapted from the Handout of Prof. Mark Thomson) Prof. Nico Serra Dr. Patrick Owen, Dr. Silva Coutinho http://www.physik.uzh.ch/de/lehre/phy211/hs2016.html
More informationOverview. The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions.
Overview The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions. Our understanding is about to take a giant leap.. the Large Hadron Collider
More informationDEEP INELASTIC SCATTERING
DEEP INELASTIC SCATTERING Electron scattering off nucleons (Fig 7.1): 1) Elastic scattering: E = E (θ) 2) Inelastic scattering: No 1-to-1 relationship between E and θ Inelastic scattering: nucleon gets
More information7. QCD. Particle and Nuclear Physics. Dr. Tina Potter. Dr. Tina Potter 7. QCD 1
7. QCD Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 7. QCD 1 In this section... The stron vertex Colour, luons and self-interactions QCD potential, confinement Hadronisation, jets Runnin
More informationHigh Energy Physics. Lecture 9. Deep Inelastic Scattering Scaling Violation. HEP Lecture 9 1
High Energy Physics Lecture 9 Deep Inelastic Scattering Scaling Violation HEP Lecture 9 1 Deep Inelastic Scattering: The reaction equation of DIS is written e+ p e+ X where X is a system of outgoing hadrons
More informationSubatomic Physics: Particle Physics Study Guide
Subatomic Physics: Particle Physics Study Guide This is a guide of what to revise for the exam. The other material we covered in the course may appear in uestions but it will always be provided if reuired.
More informationElectron-positron pairs can be produced from a photon of energy > twice the rest energy of the electron.
Particle Physics Positron - discovered in 1932, same mass as electron, same charge but opposite sign, same spin but magnetic moment is parallel to angular momentum. Electron-positron pairs can be produced
More informationParticle Physics. All science is either physics or stamp collecting and this from a 1908 Nobel laureate in Chemistry
Particle Physics JJ Thompson discovered electrons in 1897 Rutherford discovered the atomic nucleus in 1911 and the proton in 1919 (idea of gold foil expt) All science is either physics or stamp collecting
More informationMost of Modern Physics today is concerned with the extremes of matter:
Most of Modern Physics today is concerned with the extremes of matter: Very low temperatures, very large numbers of particles, complex systems Æ Condensed Matter Physics Very high temperatures, very large
More informationINTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS
INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS Class Mechanics My office (for now): Dantziger B Room 121 My Phone: x85200 Office hours: Call ahead, or better yet, email... Even better than office
More informationIntroduction to Quantum Chromodynamics (QCD)
Introduction to Quantum Chromodynamics (QCD) Jianwei Qiu Theory Center, Jefferson Lab May 29 June 15, 2018 Lecture One The plan for my four lectures q The Goal: To understand the strong interaction dynamics
More informationMost of Modern Physics today is concerned with the extremes of matter:
Most of Modern Physics today is concerned with the extremes of matter: Very low temperatures, very large numbers of particles, complex systems Æ Condensed Matter Physics Very high temperatures, very large
More informationDr Victoria Martin, Prof Steve Playfer Spring Semester 2013
Particle Physics Dr Victoria Martin, Prof Steve Playfer Spring Semester 2013 Lecture 12: Mesons and Baryons Mesons and baryons Strong isospin and strong hypercharge SU(3) flavour symmetry Heavy quark states
More informationGian Gopal Particle Attributes Quantum Numbers 1
Particle Attributes Quantum Numbers Intro Lecture Quantum numbers (Quantised Attributes subject to conservation laws and hence related to Symmetries) listed NOT explained. Now we cover Electric Charge
More informationParticle Physics. Dr Victoria Martin, Spring Semester 2012 Lecture 10: QCD at Colliders
Particle Physics Dr Victoria Martin, Spring Semester 2012 Lecture 10: QCD at Colliders! Renormalisation in QCD!Asymptotic Freedom and Confinement in QCD! Lepton and Hadron Colliders!R = (e + e!!hadrons)/(e
More informationThe Standard Model. 1 st 2 nd 3 rd Describes 3 of the 4 known fundamental forces. Separates particle into categories
The Standard Model 1 st 2 nd 3 rd Describes 3 of the 4 known fundamental forces. Separates particle into categories Bosons (force carriers) Photon, W, Z, gluon, Higgs Fermions (matter particles) 3 generations
More informationIntroduction to Particle Physics strong interactions
Introduction to Particle Physics strong interactions isto Orava Spring 6 the standard model strong interactions properties of the Strong Interaction colour the basic process comparison between QED and
More informationQuantum ChromoDynamics (Nobel Prize 2004) Chris McLauchlin
Quantum ChromoDynamics (Nobel Prize 2004) Chris McLauchlin Outline The Four Fundamental Forces The Strong Force History of the Strong Force What These People Did Experimental Support 1 Fundamental Forces
More information1 Introduction. 1.1 The Standard Model of particle physics The fundamental particles
1 Introduction The purpose of this chapter is to provide a brief introduction to the Standard Model of particle physics. In particular, it gives an overview of the fundamental particles and the relationship
More informationThe Strong Interaction and LHC phenomenology
The Strong Interaction and LHC phenomenology Juan Rojo STFC Rutherford Fellow University of Oxford Theoretical Physics Graduate School course Lecture 2: The QCD Lagrangian, Symmetries and Feynman Rules
More informationElementary particles, forces and Feynman diagrams
Elementary particles, forces and Feynman diagrams Particles & Forces quarks Charged leptons (e,µ,τ) Neutral leptons (ν) Strong Y N N Electro Magnetic Y Y N Weak Y Y Y Quarks carry strong, weak & EM charge!!!!!
More informationLecture 9. Isospin The quark model
Lecture 9 Isospin The quark model There is one more symmetry that applies to strong interactions. isospin or isotopic spin It was useful in formulation of the quark picture of known particles. We can consider
More informationQuark model. Jan 30, 2006 Lecture 8 1
Quark model Jan 30, 2006 Lecture 8 1 Quark model of hadrons!!!! Developed long before QCD was recognized as the appropriate quantum field theory of the strong interactions Postulate that 1.! All baryons
More informationIntroduction to particle physics Lecture 7
Introduction to particle physics Lecture 7 Frank Krauss IPPP Durham U Durham, Epiphany term 2009 Outline 1 Deep-inelastic scattering and the structure of protons 2 Elastic scattering Scattering on extended
More informationIntroduction to High Energy Nuclear Collisions I (QCD at high gluon density) Jamal Jalilian-Marian Baruch College, City University of New York
Introduction to High Energy Nuclear Collisions I (QCD at high gluon density) Jamal Jalilian-Marian Baruch College, City University of New York Many thanks to my colleagues, A. Deshpande, F. Gelis, B. Surrow
More informationPhysics 7730: Particle Physics
Physics 7730: Particle Physics! Instructor: Kevin Stenson (particle physics experimentalist)! Office: Duane F317 (Gamow tower)! Email: kevin.stenson@colorado.edu! Phone: 303-492-1106! Web page: http://www-hep.colorado.edu/~stenson/!
More informationParticle Physics. Lecture 11: Mesons and Baryons
Particle Physics Lecture 11: Mesons and Baryons Measuring Jets Fragmentation Mesons and Baryons Isospin and hypercharge SU(3) flavour symmetry Heavy Quark states 1 From Tuesday: Summary In QCD, the coupling
More informationThe Quark Parton Model
The Quark Parton Model Quark Model Pseudoscalar J P = 0 Mesons Vector J P = 1 Mesons Meson Masses J P = 3 /2 + Baryons J P = ½ + Baryons Resonances Resonance Detection Discovery of the ω meson Dalitz Plots
More informationElectron-Positron Annihilation
Evidence for Quarks The quark model originally arose from the analysis of symmetry patterns using group theory. The octets, nonets, decuplets etc. could easily be explained with coloured quarks and the
More informationThe SU(3) Group SU(3) and Mesons Contents Quarks and Anti-quarks SU(3) and Baryons Masses and Symmetry Breaking Gell-Mann Okubo Mass Formulae Quark-Mo
Lecture 2 Quark Model The Eight Fold Way Adnan Bashir, IFM, UMSNH, Mexico August 2014 Culiacán Sinaloa The SU(3) Group SU(3) and Mesons Contents Quarks and Anti-quarks SU(3) and Baryons Masses and Symmetry
More informationLecture 8. CPT theorem and CP violation
Lecture 8 CPT theorem and CP violation We have seen that although both charge conjugation and parity are violated in weak interactions, the combination of the two CP turns left-handed antimuon onto right-handed
More informationPhysics at Hadron Colliders Partons and PDFs
Physics at Hadron Colliders Partons and PDFs Marina Cobal Thanks to D. Bettoni Università di Udine 1 2 How to probe the nucleon / quarks? Scatter high-energy lepton off a proton: Deep-Inelastic Scattering
More informationOutline. Charged Leptonic Weak Interaction. Charged Weak Interactions of Quarks. Neutral Weak Interaction. Electroweak Unification
Weak Interactions Outline Charged Leptonic Weak Interaction Decay of the Muon Decay of the Neutron Decay of the Pion Charged Weak Interactions of Quarks Cabibbo-GIM Mechanism Cabibbo-Kobayashi-Maskawa
More informationQuantum Chromodynamics at LHC
Quantum Chromodynamics at LHC Zouina Belghobsi LPTh, Université de Jijel EPAM-2011, TAZA 26 Mars 03 Avril Today s high energy colliders past, present and future proton/antiproton colliders Tevatron (1987
More informationParticle Physics Lecture 1 : Introduction Fall 2015 Seon-Hee Seo
Particle Physics Lecture 1 : Introduction Fall 2015 Seon-Hee Seo Particle Physics Fall 2015 1 Course Overview Lecture 1: Introduction, Decay Rates and Cross Sections Lecture 2: The Dirac Equation and Spin
More informationDeep Inelastic Scattering in Lepton-Hadron Collisions Probing the Parton Structure of the Nucleon with Leptons Basic Formalism (indep.
Deep Inelastic Scattering in Lepton-Hadron Collisions Probing the Parton Structure of the Nucleon with Leptons Basic Formalism (indep. of strong dynamics and parton picture) Experimental Development Fixed
More informationOption 212: UNIT 2 Elementary Particles
Department of Physics and Astronomy Option 212: UNIT 2 Elementary Particles SCHEDULE 26-Jan-15 13.00pm LRB Intro lecture 28-Jan-15 12.00pm LRB Problem solving (2-Feb-15 10.00am E Problem Workshop) 4-Feb-15
More informationThe Standard Model (part I)
The Standard Model (part I) Speaker Jens Kunstmann Student of Physics in 5 th year at Greifswald University, Germany Location Sommerakademie der Studienstiftung, Kreisau 2002 Topics Introduction The fundamental
More informationExperimental Aspects of Deep-Inelastic Scattering. Kinematics, Techniques and Detectors
1 Experimental Aspects of Deep-Inelastic Scattering Kinematics, Techniques and Detectors 2 Outline DIS Structure Function Measurements DIS Kinematics DIS Collider Detectors DIS process description Dirac
More informationThe Strong Interaction and LHC phenomenology
The Strong Interaction and LHC phenomenology Juan Rojo STFC Rutherford Fellow University of Oxford Theoretical Physics Graduate School course Introduction and motivation: QCD and modern high-energy physics
More informationNuclear and Particle Physics 3: Particle Physics. Lecture 1: Introduction to Particle Physics February 5th 2007
Nuclear and Particle Physics 3: Particle Physics Lecture 1: Introduction to Particle Physics February 5th 2007 Particle Physics (PP) a.k.a. High-Energy Physics (HEP) 1 Dr Victoria Martin JCMB room 4405
More informationLecture 02. The Standard Model of Particle Physics. Part I The Particles
Lecture 02 The Standard Model of Particle Physics Part I The Particles The Standard Model Describes 3 of the 4 known fundamental forces Separates particles into categories Bosons (force carriers) Photon,
More informationLecture 3 (Part 1) Physics 4213/5213
September 8, 2000 1 FUNDAMENTAL QED FEYNMAN DIAGRAM Lecture 3 (Part 1) Physics 4213/5213 1 Fundamental QED Feynman Diagram The most fundamental process in QED, is give by the definition of how the field
More informationPhysics 161 Homework 2 - Solutions Wednesday August 31, 2011
Physics 161 Homework 2 - s Wednesday August 31, 2011 Make sure your name is on every page, and please box your final answer. Because we will be giving partial credit, be sure to attempt all the problems,
More informationProblem Set # 1 SOLUTIONS
Wissink P640 Subatomic Physics I Fall 2007 Problem Set # 1 S 1. Iso-Confused! In lecture we discussed the family of π-mesons, which have spin J = 0 and isospin I = 1, i.e., they form the isospin triplet
More informationLecture 9 Valence Quark Model of Hadrons
Lecture 9 Valence Quark Model of Hadrons Isospin symmetry SU(3) flavour symmetry Meson & Baryon states Hadronic wavefunctions Masses and magnetic moments Heavy quark states 1 Isospin Symmetry Strong interactions
More informationEvidence for the Strong Interaction
Evidence for the Strong Interaction Scott Wilbur Scott Wilbur Evidence for the Strong Interaction 1 Overview Continuing search inside fundamental particles Scott Wilbur Evidence for the Strong Interaction
More information2. HEAVY QUARK PRODUCTION
2. HEAVY QUARK PRODUCTION In this chapter a brief overview of the theoretical and experimental knowledge of heavy quark production is given. In particular the production of open beauty and J/ψ in hadronic
More informationModern Physics: Standard Model of Particle Physics (Invited Lecture)
261352 Modern Physics: Standard Model of Particle Physics (Invited Lecture) Pichet Vanichchapongjaroen The Institute for Fundamental Study, Naresuan University 1 Informations Lecturer Pichet Vanichchapongjaroen
More informationSECOND PUBLIC EXAMINATION. Honour School of Physics Part C: 4 Year Course. Honour School of Physics and Philosophy Part C C4: PARTICLE PHYSICS
A047W SECOND PUBLIC EXAMINATION Honour School of Physics Part C: 4 Year Course Honour School of Physics and Philosophy Part C C4: PARTICLE PHYSICS TRINITY TERM 05 Thursday, 8 June,.30 pm 5.45 pm 5 minutes
More informationPhysics 4213/5213 Lecture 1
August 28, 2002 1 INTRODUCTION 1 Introduction Physics 4213/5213 Lecture 1 There are four known forces: gravity, electricity and magnetism (E&M), the weak force, and the strong force. Each is responsible
More informationCosmology and particle physics
Cosmology and particle physics Lecture notes Timm Wrase Lecture 5 The thermal universe - part I In the last lecture we have shown that our very early universe was in a very hot and dense state. During
More informationDiscovery of Pions and Kaons in Cosmic Rays in 1947
Discovery of Pions and Kaons in Cosmic Rays in 947 π + µ + e + (cosmic rays) Points to note: de/dx Bragg Peak Low de/dx for fast e + Constant range (~600µm) (i.e. -body decay) small angle scattering Strange
More informationHadron Spectroscopy Lecture 1 Introduction and Motivation
Hadron Spectroscopy Lecture 1 Introduction and Motivation National Nuclear Physics Summer School at MIT Matthew Shepherd Indiana University Outline 1. Overview and Motivation 1.1.Uniue features of QCD
More informationQuarks and hadrons. Chapter Quark flavor and color
Chapter 5 Quarks and hadrons Every atom has its ground state the lowest energy state of its electrons in the presence of the atomic nucleus as well as many excited states which can decay to the ground
More informationChapter 32 Lecture Notes
Chapter 32 Lecture Notes Physics 2424 - Strauss Formulas: mc 2 hc/2πd 1. INTRODUCTION What are the most fundamental particles and what are the most fundamental forces that make up the universe? For a brick
More information1. Introduction. Particle and Nuclear Physics. Dr. Tina Potter. Dr. Tina Potter 1. Introduction 1
1. Introduction Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 1. Introduction 1 In this section... Course content Practical information Matter Forces Dr. Tina Potter 1. Introduction 2 Course
More informationwave functions PhD seminar- FZ Juelich, Feb 2013
SU(3) symmetry and Baryon wave functions Sedigheh Jowzaee PhD seminar- FZ Juelich, Feb 2013 Introduction Fundamental symmetries of our universe Symmetry to the quark model: Hadron wave functions q q Existence
More informationHc 5: Outline. Book by Tipler, chapter 12.2
Hc 5: Outline Introduc:on Produc:on and iden:fica:on of par:cles Basic concepts: par:cle- an:par:cle, leptons and hadrons Fundamental interac:ons and force carriers Conserva:on laws and symmetries The
More information.! " # e " + $ e. have the same spin as electron neutrinos, and is ½ integer (fermions).
Conservation Laws For every conservation of some quantity, this is equivalent to an invariance under some transformation. Invariance under space displacement leads to (and from) conservation of linear
More informationLecture 10. September 28, 2017
Lecture 10 September 28, 2017 The Standard Model s QCD theory Comments on QED calculations Ø The general approach using Feynman diagrams Ø Example of a LO calculation Ø Higher order calculations and running
More informationOutline. Charged Leptonic Weak Interaction. Charged Weak Interactions of Quarks. Neutral Weak Interaction. Electroweak Unification
Weak Interactions Outline Charged Leptonic Weak Interaction Decay of the Muon Decay of the Neutron Decay of the Pion Charged Weak Interactions of Quarks Cabibbo-GIM Mechanism Cabibbo-Kobayashi-Maskawa
More informationParticle Physics. Lecture 12: Hadron Decays.!Resonances!Heavy Meson and Baryons!Decays and Quantum numbers!ckm matrix
Particle Physics Lecture 12: Hadron Decays!Resonances!Heavy Meson and Baryons!Decays and Quantum numbers!ckm matrix 1 From Friday: Mesons and Baryons Summary Quarks are confined to colourless bound states,
More information6. QED. Particle and Nuclear Physics. Dr. Tina Potter. Dr. Tina Potter 6. QED 1
6. QED Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 6. QED 1 In this section... Gauge invariance Allowed vertices + examples Scattering Experimental tests Running of alpha Dr. Tina Potter
More informationIntroduction to particle physics Lecture 6
Introduction to particle physics Lecture 6 Frank Krauss IPPP Durham U Durham, Epiphany term 2009 Outline 1 Fermi s theory, once more 2 From effective to full theory: Weak gauge bosons 3 Massive gauge bosons:
More informationIntroduction to Quantum Chromodynamics (QCD)
Introduction to Quantum Chromodynamics (QCD) Jianwei Qiu August 16 19, 018 Four Lectures The 3 rd WHEPS, August 16-4, 018, Weihai, Shandong q The Goal: The plan for my four lectures To understand the strong
More informationQuantum Numbers. Elementary Particles Properties. F. Di Lodovico c 1 EPP, SPA6306. Queen Mary University of London. Quantum Numbers. F.
Elementary Properties 1 1 School of Physics and Astrophysics Queen Mary University of London EPP, SPA6306 Outline Most stable sub-atomic particles are the proton, neutron (nucleons) and electron. Study
More informationM. Cobal, PIF 2006/7. Quarks
Quarks Quarks Quarks are s = ½ fermions, subject to all kind of interactions. They have fractional electric charges Quarks and their bound states are the only particles which interact strongly Like leptons,
More informationParticle Physics. Tommy Ohlsson. Theoretical Particle Physics, Department of Physics, KTH Royal Institute of Technology, Stockholm, Sweden
Particle Physics Tommy Ohlsson Theoretical Particle Physics, Department of Physics, KTH Royal Institute of Technology, Stockholm, Sweden International Baccalaureate T. Ohlsson (KTH) Particle Physics 1/
More informationSECOND PUBLIC EXAMINATION. Honour School of Physics Part C: 4 Year Course. Honour School of Physics and Philosophy Part C C4: PARTICLE PHYSICS
754 SECOND PUBLIC EXAMINATION Honour School of Physics Part C: 4 Year Course Honour School of Physics and Philosophy Part C C4: PARTICLE PHYSICS TRINITY TERM 04 Thursday, 9 June,.30 pm 5.45 pm 5 minutes
More informationStructure of Hadrons. gluons. gluons
gluons Gluons are the exchange particles which couple to the color charge. They carry simultaneously color and anticolor. What is the total number of gluons? According to SU 3, 3x3 color combinations form
More informationOUTLINE. CHARGED LEPTONIC WEAK INTERACTION - Decay of the Muon - Decay of the Neutron - Decay of the Pion
Weak Interactions OUTLINE CHARGED LEPTONIC WEAK INTERACTION - Decay of the Muon - Decay of the Neutron - Decay of the Pion CHARGED WEAK INTERACTIONS OF QUARKS - Cabibbo-GIM Mechanism - Cabibbo-Kobayashi-Maskawa
More informationSU(3) symmetry and Baryon wave functions
INTERNATIONAL PHD PROJECTS IN APPLIED NUCLEAR PHYSICS AND INNOVATIVE TECHNOLOGIES This project is supported by the Foundation for Polish Science MPD program, co-financed by the European Union within the
More informationLecture 01. Introduction to Elementary Particle Physics
Introduction to Elementary Particle Physics Particle Astrophysics Particle physics Fundamental constituents of nature Most basic building blocks Describe all particles and interactions Shortest length
More informationParticle Physics Outline the concepts of particle production and annihilation and apply the conservation laws to these processes.
Particle Physics 12.3.1 Outline the concept of antiparticles and give examples 12.3.2 Outline the concepts of particle production and annihilation and apply the conservation laws to these processes. Every
More informationDiscrete Transformations: Parity
Phy489 Lecture 8 0 Discrete Transformations: Parity Parity operation inverts the sign of all spatial coordinates: Position vector (x, y, z) goes to (-x, -y, -z) (eg P(r) = -r ) Clearly P 2 = I (so eigenvalues
More informationIsospin. K.K. Gan L5: Isospin and Parity 1
Isospin Isospin is a continuous symmetry invented by Heisenberg: Explain the observation that the strong interaction does not distinguish between neutron and proton. Example: the mass difference between
More informationPHYS 420: Astrophysics & Cosmology
PHYS 420: Astrophysics & Cosmology Dr Richard H. Cyburt Assistant Professor of Physics My office: 402c in the Science Building My phone: (304) 384-6006 My email: rcyburt@concord.edu My webpage: www.concord.edu/rcyburt
More informationLecture 6:Feynman diagrams and QED
Lecture 6:Feynman diagrams and QED 0 Introduction to current particle physics 1 The Yukawa potential and transition amplitudes 2 Scattering processes and phase space 3 Feynman diagrams and QED 4 The weak
More informationPhysicsAndMathsTutor.com 1
Q1. (a) The K meson has strangeness 1. State the quark composition of a meson... State the baryon number of the K meson... (iii) What is the quark composition of the K meson?.... The figure below shows
More informationFundamental Forces. David Morrissey. Key Concepts, March 15, 2013
Fundamental Forces David Morrissey Key Concepts, March 15, 2013 Not a fundamental force... Also not a fundamental force... What Do We Mean By Fundamental? Example: Electromagnetism (EM) electric forces
More informationDerivation of Electro Weak Unification and Final Form of Standard Model with QCD and Gluons 1 W W W 3
Derivation of Electro Weak Unification and Final Form of Standard Model with QCD and Gluons 1 W 1 + 2 W 2 + 3 W 3 Substitute B = cos W A + sin W Z 0 Sum over first generation particles. up down Left handed
More informationWeak interactions and vector bosons
Weak interactions and vector bosons What do we know now about weak interactions? Theory of weak interactions Fermi's theory of weak interactions V-A theory Current - current theory, current algebra W and
More informationFundamental Interactions (Forces) of Nature
Chapter 14 Fundamental Interactions (Forces) of Nature Interaction Gauge Boson Gauge Boson Mass Interaction Range (Force carrier) Strong Gluon 0 short-range (a few fm) Weak W ±, Z M W = 80.4 GeV/c 2 short-range
More informationElementary Particles, Flavour Physics and all that...
Elementary Particles, Flavour Physics and all that... 1 Flavour Physics The term Flavour physics was coined in 1971 by Murray Gell-Mann and his student at the time, Harald Fritzsch, at a Baskin-Robbins
More informationPHYS 3446 Lecture #21
PHYS 3446 Lecture #21 Monday, Nov. 27, 2006 Dr. 1. The Standard Model Quarks and Leptons Gauge Bosons Symmetry Breaking and the Higgs particle Higgs Search Strategy Issues in the Standard Model Neutrino
More informationParticle Physics Lectures Outline
Subatomic Physics: Particle Physics Lectures Physics of the Large Hadron Collider (plus something about neutrino physics) 1 Particle Physics Lectures Outline 1 - Introduction The Standard Model of particle
More informationQuark Model. Mass and Charge Patterns in Hadrons. Spin-1/2 baryons: Nucleons: n: MeV; p: MeV
Mass and Charge Patterns in Hadrons To tame the particle zoo, patterns in the masses and charges can be found that will help lead to an explanation of the large number of particles in terms of just a few
More informationParticle physics today. Giulia Zanderighi (CERN & University of Oxford)
Particle physics today Giulia Zanderighi (CERN & University of Oxford) Particle Physics Particle Physics is fundamental research, as opposed to many applied sciences (medicine, biology, chemistry, nano-science,
More informationBooks: - Martin, B.R. & Shaw, G Particle Physics (Wiley) (recommended) - Perkins, D.H. Introduction to High Energy Physics (CUP) (advanced)
PC 3 Foundations of Particle Physics Lecturer: Dr F. Loebinger Books: - Martin, B.R. & Shaw, G Particle Physics (Wiley) (recommended) - Perkins, D.H. Introduction to High Energy Physics (CUP) (advanced)
More informationThe symmetries of QCD (and consequences)
The symmetries of QCD (and consequences) Sinéad M. Ryan Trinity College Dublin Quantum Universe Symposium, Groningen, March 2018 Understand nature in terms of fundamental building blocks The Rumsfeld
More informationAN OVERVIEW OF QUANTUM CHROMODYNAMICS UNIVERSITY OF WASHINGTON PHYS575 FARRAH TAN 12/10/2015
AN OVERVIEW OF QUANTUM CHROMODYNAMICS UNIVERSITY OF WASHINGTON PHYS575 FARRAH TAN 12/10/2015 1 AGENDA SOME DEFINITIONS (QCD, FUNDAMENTAL FORCES) SOME HISTORY (THEORY, SLAC) GAUGE THEORY FLAVORS AND COLORS
More informationLecture PowerPoint. Chapter 32 Physics: Principles with Applications, 6 th edition Giancoli
Lecture PowerPoint Chapter 32 Physics: Principles with Applications, 6 th edition Giancoli 2005 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the
More informationLecture II. QCD and its basic symmetries. Renormalisation and the running coupling constant
Lecture II QCD and its basic symmetries Renormalisation and the running coupling constant Experimental evidence for QCD based on comparison with perturbative calculations The road to QCD: SU(3) quark model
More informationAn Introduction to Particle Physics
An Introduction to Particle Physics The Universe started with a Big Bang The Universe started with a Big Bang What is our Universe made of? Particle physics aims to understand Elementary (fundamental)
More informationPHYSICS PARTICLE. An Introductory Course of. Palash B. Pal. CRC Press. Saha Institute of Nuclear Physics. Kolkata, India. Taylor &.
An Introductory Course of PARTICLE PHYSICS Palash B. Pal Saha Institute of Nuclear Physics Kolkata, India W CRC Press Taylor &. Francis Croup Boca Raton London New York CRC Press is an imprint of the &
More informationDEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS
DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS LSN 7-3: THE STRUCTURE OF MATTER Questions From Reading Activity? Essential Idea: It is believed that all the matter around us is made up of fundamental
More informationPARTICLE PHYSICS Major Option
PATICE PHYSICS Major Option Michaelmas Term 00 ichard Batley Handout No 8 QED Maxwell s equations are invariant under the gauge transformation A A A χ where A ( φ, A) and χ χ ( t, x) is the 4-vector potential
More informationFundamental Particles and Forces
Fundamental Particles and Forces A Look at the Standard Model and Interesting Theories André Gras PHYS 3305 SMU 1 Overview Introduction to Fundamental Particles and Forces Brief History of Discovery The
More information