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Probing the Structure of Matter A History of Fundamental Particle Physics Steve Schnetzer Rutgers University 1 Fundamental Particle Physics 2 Fundamental Particle Physics ä What are the fundamental constituents of the universe? 2 Fundamental Particle Physics ä What are the fundamental constituents of the universe? ä How do they interact with each other? 2 How to Judge How We’re Doing Constituents • Number: economical • Properties: few and simple • Point-like? (no structure) Theory • Mathematically consistent • Explains all observations • Able to make predictions 3 Ancient Greece Plato Aristotle 4 Ancient Greece All is mathematical form Plato Aristotle 4 Ancient Greece All is mathematical form I can figure out the universe by pure thought Plato Aristotle 4 Fundamental Physics Circa 500 B.C. The universe is built on the five Platonic solids Democritus 5 Fundamental Physics Circa 500 B.C. PSST! The universe is made up of atoms The universe is built on the five Platonic solids Democritus 5 The Classical Period 1687 − 1897 6 Newton 7 Newton The world is made of point particles 7 Newton 8 Newton The world is I made have of no point idea what they are particles 8 Chemists Discover Evidence for Atoms 1802 John Dalton • • • • Gay-Lussac’s Law Boyle’s Law Charles’s Law Law of Multiple Proportions 9 World’s First Particle Physicist 1827 Discovered Brownian Motion Robert Brown Botanist movie 10 Periodic Table 1869 a classification scheme Mendeleev 11 Periodic Table 1869 a classification scheme Mendeleev 11 Fundamental Particle Physics End of 19th century 92 Atoms 12 The Romantic Period 1897 − 1932 NJAAPT Banquet March 14, 2008 13 The Cavendish World’s premier physics laboratory late 19th century The Cavendish Cambridge University Bunsen Cell A Typical Lab 14 Discovery of the Electron J. J. Thomson A new particle Thomson’s CRT electrically charged 15 The Plum Pudding Model can knock electrons out of atoms (photoelectric effect) ⇒ electrons are a part of atoms How to make a stable electrically neutral atom? negatively charged electrons distributed like raisins in a positively charged “pudding” 16 Lord Rutherford World’s first high energy physicist 1910 Use high energy (5 MeV) alpha particles from radium decay to study structure of the atom. Ernest Rutherford very light electrons should have no effect on the alpha’s scattering of the alpha’s will indicate structure of the “pudding” 17 Rutherford Scattering A surprise some of the alpha’s scattered at large angles Data is described by assuming alpha’s scattered of a massive point charge 18 Rutherford Scattering A surprise some of the alpha’s scattered at large angles Data is described by assuming alpha’s scattered of a massive point charge 18 The Nuclear Atom Nearly all of the mass of the atom concentrated in a very small positively charged nucleus. How small is the nucleus? 19 Heisenberg Uncertainty Principle precision of measurement Why we need large, expensive high energy accelerators if you want to probe something at small distances, you have to kick it hard momentum transferred Rutherford couldn’t resolve the nucleus. It looked like a point. 20 Discovery of the Neutron 1932 James Chadwick Alpha particles interacting in air found to knock out neutral particles. Rutherford had earlier discovered the proton (the nucleus of the hydrogen atom) Atoms made out of: protons, neutrons, electrons 21 The Neutrino A free neutron decays to a proton and electron in about 15 minutes • not a 2-body decay • must be a third unseen particle Ghost-like neutrino Predicted in 1930 by Pauli Discovered in 1956 by Cowan and Reines Pauli 22 Fundamental Particle Physics 1932 neutrino electron photon proton neutron 23 The Modern Period 1932 − 1974 24 Cosmic Rays The cosmic accelerator much higher energies than available in the lab with higher energies can produce more massive particles cloud chamber 25 26 Antimatter 1932 Carl Anderson discovers anti-electrons (positrons) positron track 27 Discovery of the Muon 1937: the muon a heavy electron discovered by Anderson Just like electron except about 200 times more mass I.I. Rabi 28 Discovery of the Muon 1937: the muon a heavy electron discovered by Anderson Who ordered that? Just like electron except about 200 times more mass I.I. Rabi 28 Particle Discoveries 29 Particle Discoveries 1947: pions discovered using photographic emulsions at high altitudes .jpg (JPEG Image, 600 × 400 pixels) http://static01.nyt.com/images/2012/08/07/science/07HESS_SPAN/07HESS-articleLarge.jpg 30 Structure of the Nucleus 1953 Scattered 125 MeV electrons off of nuclei Hofstadter nuclear size: cm 31 Structure of the Proton Scattered 550 MeV 1956 electrons off of nuclei Hofstadter’s spectrometer Mark 3 electron linac at Stanford University The proton has a size it is not a point-like object 32 The Bevatron 6 GeV proton synchrotron in the hills of Berkeley Designed to discover the anti-proton 33 “Seeing” Particles The bubble chamber Donald Glaser Luis Alvarez 34 The Particle Zoo Hundreds of new particles discovered 1955 - 1965. What does it all mean? 35 Quarks 1964 Three quarks up down strange mesons: baryons: Murray Gell-Mann d d d u proton neutron u u 36 Classification Again meson octet baryon octet prediction: bound state of 3 strange quarks baryon decaplet 37 Brookhaven The AGS 33 GeV proton synchrotron 38 Discovery of the Omega Minus 1964 Nick Samios 80 - inch bubble chamber 39 Discovery of the Omega Minus 40 Stanford Linear Accelerator Center SLAC 30 GeV electrons 2-mile long linear accelerator 41 Inside the Proton 1968 SLAC - MIT Group Kendall Friedman deep inelastic scattering Taylor proton 42 Inside the Proton 1968 SLAC - MIT Group Kendall Friedman deep inelastic scattering Taylor Rutherford scattering off of point objects again 43 Fundamental Particle Physics 1974 leptons gauge boson quarks 44 The Golden Period 1974 − 1982 45 Discovery of a New Quark 1974 resonance SPEAR Electron-positron collider Burt Richter bound state of charm and anti-charm quarks Charmonium 46 Simultaneous Discovery AGS Experiment Sam Ting Double-arm spectrometer 47 Discovery of a New Heavy Electron 1975 The tau lepton Just like electron except about 2000 times more mass Marty Perl 48 Fermilab 400 GeV Proton Synchrotron 2 km diameter ring Robert Wilson 49 Discovery of Another New Quark 1976 bound state of bottom and anti-bottom quarks Leon Lederman 50 Discovery of Another New Quark 1976 bound state of bottom and anti-bottom quarks Leon Lederman 50 Discovery of the Gluon 1979 30 GeV e+e- Collider Sau Lan Wu PETRA carrier of the strong force Quantum Chromo Dynamics binds quarks together to make proton 51 The Standard Model Quantum Electrodynamics charged particles interacting by photon exchange atomic physics Quantum Chromodynamics quarks interacting by gluon exchange binding of quarks Weak Force particles interacting by W and Z exchange heavy lepton decay heavy quark decay neutrino interactions 52 CERN Off to the French Alps proton − antiproton collisions at 450 GeV 53 Discovery of the W and Z 1982 Rubbia UA 1 Detector 54 Fundamental Particle Physics 1982 leptons gauge bosons quarks 55 The Recent Period 1982 − 2008 56 LEP 1989 - 2000 100 GeV electron - positron collisions at CERN 27 kilometer tunnel 57 Z Factory Over 10 million Z’s produced and decays studied by four large detectors Aleph Detector 58 Precision Tests of Standard Model • Standard Model tested to 0.1% level in agreement with all measurements down to 10-16 cm • Only three light neutrinos • Higgs still missing 59 Discovery of the Top Quark 1995 2 TeV Proton - Antiproton collisions Fermilab Tevatron Collider Production top anti-top D0 Collaboration 60 Fundamental Particle Physics 2008 leptons quarks gauge bosons Higgs missing NJAAPT Banquet March 14, 2008 61 SM Summary Complete, consistent theory of fundamental physics ✹ Fundamental constituents: 6 quarks and 6 leptons plus antiparticles ✹ Three fundamental forces: Electromagnetic mediated by photons Strong mediated by gluons Weak mediated by W+ W- Z0 ✹ Agrees with all experiments to 10-16 cm ✹ Needs Higgs particle to be complete 62 The Large Hadron Collider 14 TeV proton antiproton collisions in the LEP tunnel 2008 probing matter at the 10-17 cm scale Atlas Detector CMS Detector 63 The Current Period 2009 − 2015 NJAAPT Banquet March 14, 2008 64 The Large Hadron Collider 65 Big Detectors, Big Collaborations The CMS Collaboration The CMS Collaboration ~ 1/4 of the people who made CMS possible 3170 scientists and engineers (including ~800 66 Higgs Decay Fractions H ! bb 58% H ! W +W 22% H ! gg 8.6% H ! ⌧ +⌧ 6.3% H ! cc 2.9% H ! ZZ 2.6% H! 0.2% 67 The Higgs Discovery CMS ATLAS 1 of 1 68 Problems with the Standard Model • “Natural” mass of the Higgs is 1019 GeV/c2. Why is it 17 orders of magnitude smaller? • The Standard Model does not include gravity. • Why does matter dominate over antimatter? • Why are there three generations of matter particles? • What explains the values of the masses? • Too many parameters (27). • Higgs mechanism seems ad hoc. • Doesn’t account for Dark Matter • Doesn’t account for Dark Energy 69 LHC Physics Discovery of the Higgs Boson • Missing ingredient of the Standard Model (SM) • Now have complete mathematically consistent theory • Agrees with all experiments down to 10-18 m scale What lies beyond the SM at smaller distance (higher energy) scales? • Measure decay fractions of Higgs to 1% precision • Search for Supersymmetry (SUSY) - Might explain why Higgs is unnaturally light - Lightest SUSY particle provides Dark Matter candidate • Search for other exotics - Vector - Like quarks, . . . • Find the unexpected 70 Future Circular Collider A 100 TeV collider under discussion at CERN / China No guarantee of new physics de-image-2.jpg (PNG Image, 517 × 272 pixels) http://tlep.web.cern.ch/sites/tlep.web.cern.ch/themes/profe Design report in 2018 Turn on in the 2050?