Particle Physics WS 2015/16

Similar documents
Introduction to Elementary Particle Physics. Note 01 Page 1 of 8. Natural Units

Periodic Table of Particles/Forces in the Standard Model. Three Generations of Fermions: Pattern of Masses

Accelerator Physics WS 2011/12

Concepts in Theoretical Physics

Theoretical Particle Physics FYTN04: Oral Exam Questions, version ht15

High Energy Physics. Lecture 4 More kinematics and a picture show of particle collisions

Weak Interactions: towards the Standard Model of Physics

REALIZING EINSTEIN S DREAM Exploring Our Mysterious Universe

Selected Topics in Elementary Particle Physics ( Haupt-Seminar )

hij Teacher Resource Bank GCE Physics A Other Guidance: Particle Physics By J Breithaupt

How To Find The Higgs Boson

Pearson Physics Level 30 Unit VIII Atomic Physics: Chapter 17 Solutions

The Standard Model and the LHC! in the Higgs Boson Era Juan Rojo!

Masses in Atomic Units

The Standard Model of Particle Physics - II

How To Teach Physics At The Lhc

Particle Physics. The Standard Model. A New Periodic Table

1 Introduction. 1 There may, of course, in principle, exist other universes, but they are not accessible to our

The Higgs Boson. Linac08 Victoria BC, Canada CANADA S NATIONAL LABORATORY FOR PARTICLE AND NUCLEAR PHYSICS

STRING THEORY: Past, Present, and Future

Searching for the Building Blocks of Matter

Discovery of neutrino oscillations

THREE QUARKS: u, d, s. Precursor 2: Eightfold Way, Discovery of Ω - Quark Model: first three quarks and three colors

Launching DORIS II and ARGUS. Herwig Schopper University Hamburg and CERN

The Wilson Chamber. Karlsruhe, Fall 2002

The OPERA Emulsions. Jan Lenkeit. Hamburg Student Seminar, 12 June Institut für Experimentalphysik Forschungsgruppe Neutrinophysik

Unification - The Standard Model

Curriculum for Excellence. Higher Physics. Success Guide

Spontaneous symmetry breaking in particle physics: a case of cross fertilization

Gauge theories and the standard model of elementary particle physics

The origin of neutrino mass

A Study of the Top Quark Production Threshold at a Future Electron-Positron Linear Collider

Highlights of Recent CMS Results. Dmytro Kovalskyi (UCSB)

Relativistic kinematics basic energy, mass and momentum units, Lorents force, track bending, sagitta. First accelerator: cathode ray tube

Experimental Particle Physics PHYS6011 Southampton University Lecture 1

Quark Model. Quark Model

Big Bang Nucleosynthesis

Physics for the 21 st Century. Unit 1: The Basic Building Blocks of Matter. Bonnie Fleming and Mark Kruse

The Elegant Universe Teacher s Guide

The Standard Model of Particle Physics. Tom W.B. Kibble Blackett Laboratory, Imperial College London

Elementary Particle Physics Fall Term Course Information

HIGH-ENERGY COLLIDER PARAMETERS: e + e Colliders (I)

The Physics Graduate Program

Topic 3. Evidence for the Big Bang

Evolution of the Universe from 13 to 4 Billion Years Ago

PHYSICS WITH LHC EARLY DATA

FCC JGU WBS_v0034.xlsm

0.33 d down c charm s strange t top b bottom 1 3

A Guide to Detectors Particle Physics Masterclass. M. van Dijk

Toward a PhD Degree in Physics

The standard model of particle physics

Objectives 404 CHAPTER 9 RADIATION

Universe. Can scientists theory of everything really explain all the weirdness the universe displays? /// BY EDWARD WITTEN

Where is Fundamental Physics Heading? Nathan Seiberg IAS Apr. 30, 2014

Top rediscovery at ATLAS and CMS

NIKHEF Annual Report 2004

The Universe. The Solar system, Stars and Galaxies

UN PICCOLO BIG BANG IN LABORATORIO: L'ESPERIMENTO ALICE AD LHC

Cross section, Flux, Luminosity, Scattering Rates

Directed by: Prof. Yuanning Gao, IHEP, Tsinghua University Prof. Aurelio Bay, LPHE, EPFL

thermal history of the universe and big bang nucleosynthesis

Theory of electrons and positrons

Big Bang Cosmology. Big Bang vs. Steady State

Olga Botner, Uppsala. Photo: Sven Lidström. Inspirationsdagar,

Middle East Technical University. Studying Selected Tools for HEP: CalcHEP

Calorimetry in particle physics experiments

Your years of toil Said Ryle to Hoyle Are wasted years, believe me. The Steady State Is out of date Unless my eyes deceive me.

Phase Transitions in the Early Universe

Extensions of the Standard Model (part 2)

PHOTOELECTRIC EFFECT AND DUAL NATURE OF MATTER AND RADIATIONS

Build Your Own Universe

Measurement of the Mass of the Top Quark in the l+ Jets Channel Using the Matrix Element Method

Cosmic Ray Astrophysics with AMS-02 Daniel Haas - Université de Genève on behalf of the AMS collaboration

Information about the T9 beam line and experimental facilities

Real, False and Missed Discoveries in High Energy Physics

Transcription:

Particle Physics Lecture WS 2015/16 Prof. A. Schöning Physikalisches Institut der Universität Heidelberg 1

Goal of this Lecture Introduction to particle physics for master students Comprehensive overview about particle physics: Experiments and experimental methods phenomenology theoretical concepts and fundamental laws 2

Particle Physics Related Courses Winter term 2015/16: Higgs, Precision Tests and New Physics at the LHC lecture + seminar: Wed 14h15, Fri, 14h15 (Dunford) Accelerator Physics lecture + tutorial: Wed 11h15, 16h15 (Schöning) Statistical Methods in Particle Physics lecture + tutorial: Mon 14h14, Mon 16h15 (Brandt) LHC analyses and their physics impact master seminar: Mon 16h15 (Brandt/Plehn/Uwer) Nobel Prizes in Particle Physics master seminar: Fri 9h00 (Reygers/Stachel) Particle Physics Colloquium Tue 17h15 http://www.physi.uni-heidelberg.de/veranstaltungen/vortraege.php?kol=pc [Standard Model Theory II] Wed 16h15, Fri 9h00 (Rodejohann/Lindner) Summer term 2016: Particle Physics, Detector Physics, Standard Model I, seminars,... 3

Organisation of PP lecture Prerequisites: Knowledge: Quantum Mechanics (Schrödinger Eq.), special relativity Lectures: Physics I-V, Introduction to Nuclear and Particle Physics Focus and content of this lecture: Accelerators, Detectors, Relativisitc Kinematics, Symmetries, Quantum Electrodynamics, Weak Interaction, Quantum Chromodynamics, Standard Model, Beyond the Standard Model, Flavor Physics, Astroparticle Physics This course is a basis for more specialised lectures: LHC Physics, Standard Model, Beyond the SM, Supersymmetry Other useful lectures: Quantum Field Theory (Mon+Wed, 11h15, A. Hebecker) more information: http://www.physi.uni-heidelberg.de/~schoning/vorlesungen/particlephysics/ 4

Tutorials + Requirements Tutorials: 11 series of exercises to be handed in Thursday 14h15 beginning of lecture typically ~4 exercises/sheet (up to three names) exercises are checked and corrected target: 60% of the maximum score registration deadline for PP lecture November 27 (point of no return...) written examination 4.2.2015 (repetition 18.2.2015) number of credit points = 8 (lecture+tutorial) Dates of tutorials (start in 2nd lecture week): Thu; 16:15-18:00; INF 501 / FP (R.102); group 1; Thu; 16:15-18:00; INF 501 / CIP R. 103; group 2; Mon; 11:00-13:00; INF 227 / SR 3.402; group 3; [Fri; 09:15-11:00; INF 226, K2,3; group 4;] Fri; 11:15-13:00; INF 227 / SR 3.404; group 5; Registration: https://uebungen.physik.uni-heidelberg.de/v/580 Coordinator: Christoph Anders <anders@physi.uni-heidelberg.de> 5

Literature on Particle Physics Ch. Berger: Elementarteilchenphysik, 2014, in German, Springer Verlag, ISBN 978-3-642-41752-8 M. Thompson: Modern Particle Physics, 2013, engl., ISBN-13: 978-1107034266 B.R. Martin, Nuclear and Particle Physics, An Introduction, 2009, Wiley, ISBN 9780-470-74275-4 Povh, Rith, Scholz and Zetsche, Particles and Nuclei, An Introduction, 2008, Springer Verlag ISBN 978-3-540-79368-7 D.Griffith, Introduction to Elementary Particle Physics, 2008, Wiley, ISBN: 9783527406012 D.H. Perkins, Introduction to High Energy Physics, 2000, Addison Wesley (older standard book) P. Schmüser, Feynmann Graphen, 1995, Springer Verlag Particle Data Group, K.A. Olive et al., Chin. Phys. C, 38, 090001 (2014) and 2015 update [http://pdg.lbl.gov/] by far not complete. Many, many more books... 6

Lecture Dates Tuesday 14:15-16:00 and Thursday 14:15-16:00 7

Master Thesis in Particle Physics Nuclear and Heavy Ion Physics: Prof. N.Herrmann (CBM) Prof. J.Stachel (ALICE) High Energy Physics: Dr. O Brandt (ATLAS) Prof. S.Hansmann Menzemer (LHCb) Prof. H.C. Schultz-Coulon (ATLAS,CALICE, MU3E) Prof. (ATLAS, MU3E) Prof. M Schmelling (LHCb) Prof. U. Uwer (LHCb) Neutrino Physics: Prof. M.Lindner (GERDA,XENON100,...) Prof. Enss (ECHO, ) Astroparticle Physics: Prof. W.Hoffmann (HESS, CTA) Theory Prof. J.Jäckel (Beyond the Standard Model) Prof. T.Plehn (LHC Phenomenology) 8 + research groups

give feedback! 9

Introduction 100 years of particle physics......more than a success story! a historical overview 10

Ionisation Measurement Victor Hess discovery of cosmic showers 1912 Nobel Prize (1936) 11

1912 100 years 2012 electron photons nuclei (protons, neutrons) 12

1912 100 years 2012 electron photons nuclei (protons, neutrons) Standard Model Lagrangian 13

Anti-Particle Hypothesis Paul Dirac (1928): Field equation for a relativistic Quantum Mechanics based on Einsteins special relativity relation: 2 2 E =m + p 2 Dirac equation has solutions for positively and negatively polarised particles and for positive and negative energies: negative energy antiparticles! Later, Feynman-Stückelberg interpretation: antiparticles are particles travelling in reverse time direction 14

Discovery of the Positron first observed by D.Skobeltsyn in cosmic rays using a Wilson (cloud) chamber (1929) C.D. Anderson: study of cosmic rays in a cloud chamber (1932) positrons are bent due to magnetic field proof of existence of anti-particles Carl D. Anderson Nobel Prize (1936) 15

Muon Discovery (1936) Muon discovery in cosmic rays by Carl Anderson + Seth Nedermeyer mass: mµ ~100 MeV Nobel Prize (1936) myon was first exotic particle and believed to be the meson predicted by Yukawa 16

Prediction of the Pion H.Yukawa predicted 1935 mesons as carriers of the strong force Nobel Prize (1949) meson mass ~ ħc / (range of force) range ~ 1 fm mmeson = 200 MeV Note 1: mesons are quark-anti-quark states and not elementary Note 2: meson = mean, intermediate state 17

Discovery of the Pion 1947 discovered by Perkins, Ochialini and Powell emulsions μ e π Nobel Prize (Powell 1950) 18

Discovery of Neutrinos _ beta decay: n p e ν - e- me = 0.511 MeV mn = 939.565 MeV n missing energy? p mp = 938.272 MeV _ ν W. Pauli predicted in a letter to E.Fermi the existence of neutrinos (1930) 19

Discovery of the Electron-Neutrino Discovery of the electron neutrino (Cowan, Reines, 1957) Nobel Prize (1995) Anti-Electron-Neutrino 20

Existence of Muon-Neutrinos proton accelerator berylium plate dipole magnets iron absorber pion decay tunnel decay: π μνμ big sparc chamber 10 tons νμn μ p Discovery of the muon neutrino (Ledermann, Schwartz, Steinberger 1962) Nobel Prize (1988) 21

Discovery of Strangeness Surprise! V-particles Production of Kaons and Lambda-Baryons in pp Collisions Long Lifetime! neither electromagnetic nor strong force bubble chamber (1950ties) 22

Status in 1962 (50 years after Hess's baloon trip) known fermions M. Gell-Mann and G. Zweig hypothised existence of quarks: up-quark down-quark strange-quark in the year 1964 Nobel Prize (1969) 23

Prediction of the Charm Quark How explain non-observation of Flavor Changing Neutral Currents? K π γ γ K us ud? π Such a flavor changing decay is frobidden if fourth quark exists (Glashow, Iliopoulos, Maiani) Note: not the first time that a new particle was predicted! 24

Observation of the Charm Quark cc resonance e+ e- J/Psi e+ e- (μ+,μ-),(π+ π-) SLAC: B.Richter et al. (1974) p Be X J/Psi X e+ ebnl: S.Ting et al. (1974) Nobel Prizes 1976 25

Status in 1975 known fermions no anti-matter in universe! Charge and Parity Conservation must be broken! (2nd A.Sakharovs condition) third quark family could explain matter-antimatter asymmetry Nambu, Kobayashi, Maskawa Nobel Prize 2008 Note: particle physics and evolution of universe are closely related! 26

Discovery of the Third Family Tau Lepton discovered by MARK1 at SPEAR (1974-1976) + + e e τ τ τ eνν τ μ ν ν discovery of tau-lepton (Reines et al., M.Perl) Nobel Prize (1995) meµ mτ=1.777 GeV Discovery of the Bottom-Quark (1977) by M.Ledermann et al. at Fermilab Nobel Prize (1988) 27

Top Quark Discovery at Tevatron Fermilab Tevatron p p collider s1/2 =2 TeV 28

Top Quark Discovery in 1995 CDF Collaboration D0 Collaboration Top-quark mass ~175 GeV Top production: Top decay: pp tt X t W b and W qq or lv 29

Status in 2000 (~90 years after Hess's baloon trip) all fermions discovered tau neutrino discovered in 2000 by Donut experiment 30

Status in 2002 (90 years after Hess's baloon trip) Nobel Prize 2015 neutrinos have mass! Takaaki Kajita + Arthur B. McDonald SNO experiment (2001/2) Super-kamiokande (1998) 31

Discovery of Vector Bosons Photons: X-rays (Röntgen 1995) Nobel Prize 1901 photo-electric effect (Einstein 1905) Nobel Prize 1921 Gluons: carriers of strong force predicted by Gell-Mann et al. experimentally discovered as jets of hadrons e.g. at PETRA W± bosons: carriers of weak interactions responsible for weak decays. building blocks of Standard Model Glashow, Salam, Weinberg Nobel Prize 1979 W-boson discovered at CERN SppS in 1983 C.Rubbia and S. van d. Meer Nobel Prize 1984 32

Observation of Neutral Currents Bubble Chamber Gargamelle (1974) νe νe e ν e e νe Z e e 33

Discovery of Vector Bosons Z bosons: indirectly observed at Gargamelle discovered at at CERN SppS in 1983 C.Rubbia and S. van d. Meer Nobel Prize 1984 precision studies at LEP accelerator 34

Large Electron-Positron Collider CERN 1989-2000 s1 / 2=90-200 GeV 26.7 km circumference Four experiments: ALEPH DELPHI L3 OPAL 35

Large Hadron Collider (CERN) LHC (pp) s1/2 <= 14 TeV 26.7 km circumference! 36

The Higgs Boson ATLAS CMS mh=125 GeV Nobel Prize 2013 F.Englert P.Higgs 37

Experimental Tools CMS (LHC) ATLAS (LHC) ZEUS (HERA) H1 (HERA) CDF (Tevatron) 38

Supermikroskop HERA 920 GeV Protonen x 26.7 GeV Elektronen HERMES H1 ZEUS (1992-2007 Hamburg) 39

Study of the Proton Structure Recent results on proton structure H1 + ZEUS experiments (2015) important for other (future) experiments and LHC 40

Theoretical Problems of the SM Grand Unification??? 41

Dark Matter dark matter in filaments between galaxies (simulation) [R.Kaehler et al. (KIPAC)] 42

The SM and Astro- Particle Physics Matter-Antimatter Asymmetry in Universe N B 10 9 N Dark Matter Problem (only 1% of the mass is visible in the universe) Formation of galaxies and structures in the universe Dark energy (from microwave background anisotropy) Nucleosynthesis constraints Big-Bang 43

era of gravitation era of particle physics 44

1874 "in this field (physics), almost everything is already discovered, and all that remains is to fill a few unimportant holes." (1874) Philipp von Jolly (1809 1884) Prof. in Heidelberg (physicist and mathematician) Max Planck: 1858-1947 45

46