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Fromm Institute for Lifelong Learning, University of San Francisco Modern Physics for Frommies III A Universe of Leptons, Quarks and Bosons; the Standard Model of Elementary Particles Lecture 5 9 February 2011 Modern Physics III Lecture 5 1 Agenda • Administrative Matters • Quantum Field Theories • Second or Field Quantization • Electromagnetic Interaction • Weak Interaction • Strong Interaction • Patterns and Symmetries in Nature 9 February 2011 Modern Physics III Lecture 5 2 Administrative Matters •Full schedule of colloquia is posted on the Wiki and should be posted in Fromm Hall •A list of popular books pertaining to Elementary Particle Physics is posted on the Wiki. It will be updated when appropriate. 9 February 2011 Modern Physics III Lecture 5 3 Exchange vector bosons form a T =1 triplet W T3 W 1 0 W0 W or T 0 3 W W T3 1 W0 rather than Z0 for technical reasons involving electro-weak unification W+ (T3 = +1) is emitted in transitions {(T3 = +1⁄2) → (T3 = −1⁄2)} W− boson (T3 = −1) is emitted in transitions {(T3 = −1⁄2) → (T3 =+ 1⁄2)}. e.g. b decay d uW W e 9 February 2011 Modern Physics III Lecture 5 4 It took a great deal of effort to get a renormalizable electro-weak QFT Sheldon Glashow Abdus Salam 1926 - 1996 Steven Weinberg 1979 Nobel Prize 9 February 2011 Modern Physics III Lecture 5 5 Strong Interaction: A little history: 1911 Rutherford discovers the nucleus 1932 Chadwick discovers the neutron → Nucleus is protons + neutrons What holds the nucleus together? Need a strong but short range force. 1947 Powell et al. discover pion, p, in cosmic rays 1935 Yukawa potential g 2 ar g 2 a ar VSI (r ) e or FSI 2 e r r Could be mediated by a scalar boson of mass 200 me P+ p0 P+ Muon, m not it. 9 February 2011 Modern Physics III Lecture 5 6 In the 1960s both theory and experiment began to substructure to “elementary” particles Partons: quarks, antiquarks and gluons Hideki Yukawa 1907 -1981 1949 Nobel Prize Update Yukawa’s picture 9 February 2011 Modern Physics III Lecture 5 7 Simple Quark Model (no color): Baryons: u d Arrows are quark spins u d Sq = 1/2 u d Proton Neutron Mesons: u u d u d u or dd p 9 February 2011 p Modern Physics III Lecture 5 p 8 Color and Color Charge: Color was originally introduced to beat the Pauli principle. u u Arrows are quark spins Sq = 1/2 s3 2 Clearly Pauli blocked u u u Add a new number, color u There are also anticolors for the antiquarks Mrs. Pauli’s favorite son is now happy! 9 February 2011 Modern Physics III Lecture 5 9 Theory of strong interactions between quarks is called quantum chromodynamics (QCD) Mediated by force carriers called gluons Bound states: qq color - color meson 3q 3 different colors baryon 3q 3 different colors antibaryon Note that in all of the above the colors add up to “white”. Color is not observed in our “usual” particles (p, n, p, K etc.). Gluons: 8 of them carrying both color and anticolor BLUE ANTIRED GLUON rb 9 February 2011 Modern Physics III Lecture 5 10 From the 3 color states, one can form 9 bicolor color - anticolor states RR , RB , RG BR , BB , BG GR , GB , GG Removing the colorless state of the trace reduces us to 8 combinations which exchange color between quarks Confinement: Why don’t we see free quarks? Gluons themselves carry color charge (unlike the photon which is electrically neutral). They participate in strong interactions. These g – g interactions constrain color fields to string like objects, flux tubes. 9 February 2011 Modern Physics III Lecture 5 11 Stretching the tube requires more and more energy At some distance it is energetically more favorable to pull a qq pair out of the vacuum than to increase the tubelength. e p K 0 (1-3) e strikes p exciting the d quark (4) An ss pair is created (5) quarks rearrange into color singlets, K and 9 February 2011 Modern Physics III Lecture 5 0 12 Color Screening and Running Coupling Constants: In QED we had some trouble with loop diagrams. We fixed this up by invoking the dressing or screening of the bare electron Vacuum polarization or charge screening reduces the observed charge. As we increase probe energy (probe shorter distances) the observed charge grows The EM, aEM, coupling constant increases with energy What happens in QCD? 9 February 2011 Modern Physics III Lecture 5 13 In QCD the virtual gluons emitted by quarks not only create qq pairs but also more gluons with all the allowed bicolor signatures In QCD the virtual quark-antiquark pairstend to screen the color charge. However, QCD has an additional wrinkle: its force-carrying particles, the gluons, themselves carry color charge, and in a different manner. Each gluon carries both a color charge and an anti-color magnetic moment. The net effect of polarization of virtual gluons in the vacuum is not to screen the field, but to augment it and affect its color. This is sometimes called antiscreening. Getting closer to a quark diminishes the antiscreening effect of the surrounding virtual gluons, so the contribution of this effect would be to weaken the effective charge with decreasing distance. 1 Fermi = 1 fm = 1x10-15 m 9 February 2011 Modern Physics III Lecture 5 14 9 February 2011 Modern Physics III Lecture 5 15 Asymptotic freedom H. David Politzer Frank Wilczek David Gross Nobel Prize 2004 9 February 2011 Modern Physics III Lecture 5 16 Patterns and Symmetries in Nature Our normal space E3, Physics doesn’t change when moved. It is invariant under translation and rotation. Symmetry groups Group: A set of elements closed under a prescription relating the elements. e.g. a and b in the group a b in the group is associative but not necessarily commutative A unit element 1 1 a a 1 a Each element has an inverse a-1 aa-1 = 1 Examples: The integers form a group under addition, 1 + 3 =4. Hours on a clock. A finite number of elements (12). 1 = 12 because h +12 = h If h = 1, h-1 = 11 because 1 + 11 =12 = 1 9 February 2011 Modern Physics III Lecture 5 17 In Physics, groups are associated with manipulations, e.g translation and rotation Translation group: Carry from here to there Rotation group: Rotate so much about a specified axis. Things that remain the same when manipulated by an element are said to be symmetrical. Examples: A sphere under all rotations. A cube under 90° rotations about 3 specific axes. A shoe is not symmetric but a pair is. Approximate symmetries: Still useful. The Earth is not a perfect sphere but can often be treated as one. Some groups can be shown to be equivalent, e.g. group of rotations of 30° is equivalent to the clock number group above. Representation specific instance of a group, e.g. the clock numbers are a representation of the 2-D 30°rotation group 9 February 2011 Modern Physics III Lecture 5 18 NOW RESTRICT OURSELVES TO FINITE GROUPS The elements of a represntation are classified into multiplets e.g. A sphere is a singlet under rotation A square in a plane is a quartet An equilateral triangle in a plane is a triplet A cube about 3 orthogonal axes is an octet Rotations in a plane commute or are Abelian. All 1-D groups are Abelian Finite 3-D rotations are non-Abelian, see Rubik’s Cube Invariants: Symmetries leave something unchanged. e.g. translation maintains the distance between points, r2 = x2 + y2. a conserved quantity, p. Rotations preserve distances and angles conserved quantity, L 9 February 2011 Modern Physics III Lecture 5 19 Symmetries in Relativity: The frame independence of c a “super distance” in 4-D spacetime which is invariant under a corresponding “super rotation”. This is the 4-length or interval s 2 x 2 y 2 z 2 The super rotations are of course the Lorentz trnsforms a.k.a. the Lorentz group. Quantizing Spin: Magnetic fields with their “vector product behavior” arise from the spin of the exchanged g. The occurrence of both repulsive and attractive forces also requires consideration of the exchanged spin (the ball throwing analogy breaks doen here). Recall the wave justification of Bohr’s quantization rule: y must be a standing wave around the equator. 9 February 2011 Modern Physics III Lecture 5 20 2p 2p r n n 1, 2, 3, and = mv mvr n Angular momentum We are dealing here with the rotation of the particle itself so we have the spin angular momentum S n It doesn’t matter that we have used a finite radius for the path of this phase measurement; This is merely an accounting device for the phase, a pure number independent of physical size. Now suppose we measure the phase for multiple loops around the equator rotation marker 9 February 2011 Phase Wheel 1 revolution = 2p radians = 360° Corresponds to 1 complete wavelength n=1 Modern Physics III Lecture 5 21 Our requirement is just that the path closes after an integral number n of revolutions of the wheel. This could easily well happen going around the equator twice Suppose n is even, say n = 4 Clearly mark 3 coincides with 1 and 2 with 4 n=4 1 3 2 4 Superposition of two indistinguishable paths each with n/2 wavelengths n even n/2 = m is also an integer We end up with a class of particles with spin quantized according to S m just as before 9 February 2011 Modern Physics III Lecture 5 22 n=3 Now let n be an odd integer, say 3 3 The pair wise coincidence is replaced by an anticoincidence Each mark on the 2nd loop is midway between 2marks on the 1st. 1 2 The 2 loops are not the same. We obtain a class of particles with an equatorial circumference of n/2 with quantized spin n S 2 n odd This process can be generalized to more looping of the phase wheel.The above 2 classes of particles are the only 2 that appear and are the bosons and fermions respectively. 9 February 2011 Modern Physics III Lecture 5 23 Boson: Phase wrapping is a simple circle. A boson turned 360° is indistinguishable from its original Space is rotationally symmetric so no surprise that 360° turns a particle into itself Fermion: Phase wrapping consists of 2 different loops. A fermion turned 360° does not turn into itself. Instead it requires a turn of 720°. So, what state do we obtain with a 360° rotation? 360°does not return the same amplitude but we really believe space to be rotationally symmetric. Only way out appears to be y → -y for a fermion turned through 360° Remember, we don’t observe amplitudes (y), only probabilities (P). Py 9 February 2011 2 y 2 Modern Physics III Lecture 5 24 What happens if we superpose 2 indistinguishable particles. Distinguishable different quantum numbers, momenta or positions 2 particles in a 1-D box. In analogy to going to a higher D box n1n2 ( x1 , x2 ) y n1 ( x1 )y n2 ( x2 ) Particles are identical so we actually have to write 1 y n1 ( x1 )y n2 ( x2 ) y n2 ( x1 )y n1 ( x2 ) n1n2 ( x1 , x2 ) 2 bosons fermions For fermions: nn ( x, x) 0 9 February 2011 Modern Physics III Lecture 5 25 Truly identical fermions cannot exist. Forces fermions to aggregate in finite sized lumps when piled together Prevents fermions from building up large scale coherent fields when exchanged as virtual particles Identify fermions with matter Bosons have no objection to being identical Bosons aggregate together in the lowest allowed energy state without building up finite sized lumps. Responsible for phenomena such as superconductivity and superfluidty. Identify bosons with forces 9 February 2011 Modern Physics III Lecture 5 26 Fermion Boson? Demo with string Have to change the topology of the phase path. Unless you are allowed to go outside the plane you cannot make these transformations Unless you can step out of space into another dimension, you can never change fermion to boson or vice–versa. It can be shown formally that, unless the universe has extra freedom beyond space-time, spin can only change in whole units of ħ. 9 February 2011 Modern Physics III Lecture 5 27 Polarization and Gauge Invariance: A particle with non-zero-spin can have a certain orientation in space called the polarization. Pick a fixed, but otherwise arbitrary, direction (call it the z-axis) ms = +1/2 ms = +1 s = 1/2 ms = -1/2 s=1 For a given value of s, there are 2s + 1 values for ms ranging from s to –s in steps of 1. 9 February 2011 Modern Physics III Lecture 5 ms = 0 ms = -1 28 Examples of picking a z-axis: Apply a magnetic or electric field Direction of motion The line drawn in the sand by Col. Travis etc. The choice of a direction is called fixing a gauge and the fact that the Physics is independent of this choice is called gauge invariance Zero mass particles: e,g, g Lorentz symmetry s 2 x 2 c 2t 2 is invariant so is m2c 4 p 2c 2 E 2 Let m → 0, so we get E = pc, and apply E = hf and p = h/ pc = hf = (h/)c or c =f a wave propagating with velocity c 9 February 2011 Modern Physics III Lecture 5 29 Now, let’s fix the gauge so that the z-axis is in the direction of motion. This is called the radiation gauge or helicity frame. c ms = -1 ms = 0 ms = +1 A particle with zero rest mass can only have 2 degrees of spin freedom. Similarly the handedness of a massless particle cannot be reversed. c ms = -1/2 9 February 2011 ms = +1/2 Modern Physics III Lecture 5 30 We have seen that the laws of relativity and the law of spin and statistics are consequences of the Lorentz invariance of space time. Can we extend the use of symmetries to Multiplets forces, i.e. the way in which fermions and bosons couple at a vertex Multiplets: Sets of things that have something in common. Singlet an object that is not changed under a symmetry operation e.g. a circle is a singlet under rotation, a square is a singlet under rotations of 90° Doublet a pair of objects that transform into each other. e.g. p,n are a doublet under 180° rotations in strong isospin space. etc.. 9 February 2011 Modern Physics III Lecture 5 31 Rx for invoking a symmetry group at a vertex: 1) Identify or postulate a set of N fermions that are observed, or expected, to act as a ‘fundamental’ multiplet. N is the dimension of a symmetry group G, and the set of fermions is an N-plet under G. 2) An operation from G when applied to a member of the N-plet transmutes it into another member. 3) Every transmutation is interpreted as being due to the emission or absorption of a field boson (aka a gauge boson). e.g. e is a fermion that cannot be changed into something else electromagnetically it is a singlet under some 1-D group, call it U(1) There is only one boson associated with the group, g. 9 February 2011 Modern Physics III Lecture 5 32