Mid- term exam Content: Specified on Blackboard Date: Thursday, 5 March 2015 Time: 8:30 10:30 Educatorium/Alfa
|
|
- Shawn Shaw
- 5 years ago
- Views:
Transcription
1 Mid- term exam Content: Specified on Blackboard Date: Thursday, 5 March 2015 Time: 8:30 10:30 Room: Educatorium/Alfa Ques/on hour today at 16:00 in room BBL 083 1
2 3. Par/cle Physics André Mischke Utrecht University 2
3 Hc 4: Outline IntroducPon ProducPon and idenpficapon of parpcles Basic concepts: parpcle- anpparpcle, leptons and hadrons Fundamental interacpons and force carriers ConservaPon laws and symmetries The Standard model: Quark model Book by Tipler, chapter
4 ParPcle Physics Structure of maker building blocks: elementary parpcles interacpons between them Elementary parpcles are point- like have no structure are non- excited objects 4
5 Chemistry in the 19 th century Mendeleev s Periodic Table of elements Natural maker: bound states of 92 elements Elementary parpcles in 92 different versions InteracPon: chemical interacpon 5
6 Beginning of the 20 th century 1930s Known elementary parpcles: proton (protos = first), neutron, electron and photon Known interacpons GravitaPon Electro- magnepc interacpon Nuclear interacpon 6
7 Today's Standard Model Elementary parpcles Quarks and leptons (fermions; half- integer spin) InteracPons Exchange parpcles (bosons; integer spin) What was discovered in between? 7
8 ParPcle producpon Cosmic rays: ParPcles from space Balloon experiments (1910s) First evidence for new parpcles = new form of maker ParPcle accelerators - Since 1930 s - Current highest collision energy (8 TeV) reached at the Large Hadron Collider at CERN (Geneva, Switzerland) 8
9 Results from cosmic- ray experiments Balloon experiments in heights up to 5.3 km, V. Hess (1912) Measurement of the ionisapon rate with electrometer RadiaPon increases with increasing height Discovery of AnPmaKer ExoPc parpcles with strange behaviour (= parpcular long life Pmes) 9
10 First apparatuses for arpficially accelerapng parpcles to high energies 27- inch Cyclotron E.O. Lawrence (1934) 3.6 MeV proton beam Cockcrok- Walton accelerator (1932) 300 kev proton beam University grant of
11 ParPcle producpon In parpcles collisions e.g., proton on proton collision at 8 TeV centre- of- mass (cms) energy (at CERN or in the atmosphere) InelasPc collision E = mc 2 ParPcle producpon threshold: cms energy 2 mass RelaPvisPc energy- momentum relaponship (RelaPvisPc mechanics) E 2 = (pc) 2 + (mc 2 ) 2 Lorentz factor (Pme dilatapon) pc = βγ mc 2 and E = γ mc 2 where β = v/c = pc/e and γ = (1- β 2 ) - ½ Book by Tipler, chapter
12 IdenPficaPon of long- lived parpcles Long- lived means that the flight way γτ βc (life Pme Pmes velocity) is at least a few cenpmetre (from observer view) E.g., for typical γ = 200 the life Pme is τ 10-2 m/( m/s) s 12
13 ParPcle idenpficapon methods Aim is to detect a large fracpon of the produced parpcles and its properpes Charge and neutral parpcles ConservaPon laws: momentum, energy and charge Relevant quanppes/properpes type of parpcle (mass/charge m/q) momentum p energy E life Pme τ spin s 13
14 Momentum measurement: DeflecPon of charge parpcle in magnepc field MagnePc field B [Tesla] ParPcle with charge q (negapve in this example) Book by Tipler, page 94 Lorentz force Collision vertex ParCcle trajectory is a helix in 3D space and a circle in the transverse plane p [MeV /c] = 300 q B R 14
15 Charged parpcle idenpficapon: Time of flight Measurement of the Pme of flight (β = v/c) with two scinpllapon counter/detector pc = βγ mc 2, where the momentum is determined in a magnepc field Real data from the ALICE experiment at the CERN- LHC 15
16 Charged parpcle idenpficapon: Specific ionisapon energy loss Specific ionisapon energy loss in maker; from strength of the track charged parpcles ionise material Bethe- Bloch formula: de/dx = - e 2 f(βγ) de/dx β 2 γ 0.7 β 16
17 Charged parpcle idenpficapon in the ALICE* experiment at CERN Specific ionisapon energy loss * Website: hrp://aliceinfo.cern.ch/public/welcome.html 17
18 Energy measurement ElectromagnePc (photon, electron) or hadronic calorimeter (proton, neutron) Several interacpons with detector material à parpcle shower DeterminaPon of the total parpcle energy, deposited in the calorimeter parpcle Detector material read- out sensors 18
19 ReconstrucPon of short- lived parpcle: Invariant mass method B field p (E, p 1 ) 1! Λ π -! (E, p ) 2 2 σ mass = 2.2 MeV The existence of the intermediate state is evident from the peak in the invariant mass distribupon m inv c 2 = (E 1 + E 2 ) 2 - (! p 1 c+! p 2 c) 2 Life Pme: Tipler, chapter 4-2! τ = = Γ σ 2! 2ln 2 19
20 Bubble chamber picture Main measuring device from 1950's to 1980's Beam comes in from this side Features - ParPcles bend in the magnepc field - Neutral parpcles leaves no track, then decays into charge parpcles - Atomic electrons knocked out by parpcles 20
21 Break?! 21
22 Discovery of the positron (first anp- parpcle) Existence of positron (= anp- electron) postulated by P. Dirac (1927): Two solupons of the relapvispc wave equapon Cloud chamber photographs of cosmic ray events; C. Anderson (1932) Electron ionisapon but opposite curvature Discovery of the anp- proton (1955) p + p p + p + p + p E 2 p 2 c 2 = m 2 c 4 E =± p 2 c 2 +m 2 c 4 positron 22
23 Tracks of electron- positron pairs 30 MeV x- ray interacpons with a lead plate MagnePc field points out of the page 23
24 AnPmaKer in medical applicapons Positron emission tomography (PET) (developed at MassachuseKs General Hospital, 1952) 1. Positron- emiyng isotopes ( 11 C, 13 N, 15 O, 18 F) are inserted into physiologically relevant molecules (oxygen, glucose, enzymes) and injected into papent 2. Positron annihilapon is detected with crystal calorimeter 24
25 AnP- hydrogen atom (AnP- ) hydrogen is the simplest atomic system Hot (excited) and cold (slow, using a parpcle trap) anp- hydrogen produced at CERN in 1995 and 2011, respecpvely High- precision spectroscopy Goal: deeper understanding of maker- anpmaker imbalance anpmaker gravity p vacuum wall y φ x z annihilation detector mirror coils electrodes Typical parccle trap octupole e + 25
26 Today s heaviest anpmaker nuclei 18 anp- helium- 4 nuclei, produced in collisions of heavy atomic nuclei STAR experiment at Brookhaven NaPonal Laboratory, USA (2011) 26
27 Discovery of the neutrino n p+e n p+e +ν e # events not this but this # events m n - m p - m e 17 kev E e E e Electron energy spectrum of the β decay Preserve energy and momentum conservapon Existence of neutrino postulated by W. Pauli Discovered by Cowan and F. Reines (1956) 27
28 Discovery of the muon: A surprise! In cosmic ray experiments; C. Anderson (1937) New parpcle behaves like a heavy electron (about 200 Pmes heavier) 28
29 Summary: properpes of electron- like parpcles and neutrinos 29
30 Discovery of the pion Yukawa s predicted meson exchange parpcle In cosmic ray experiments by C. Powel (1947) DetecPon with photo emulsion pictures e + μ + Pion decay π + µ + +ν µ e + +ν e π + 30
31 Discovery of the V 0 parpcle cosmic ray shower Cosmic ray experiment; G. Rochester and C. Butler (1947) 3 cm lead V 0 particle They are produced through strong interacpon but decay very slow (long life Pme τ) τ(strange parpcle) s τ(δ resonance) s CharacterisPc V- decay topology: Discovery of neutral kaon, the K 0 s Cloud chamber picture IndicaPon for a new force: weak force (later more) 31
32 Strange parpcle producpon 32
33 Hundreds of parpcles discovered What are the underlying building blocks? 33
34 Ordering scheme: fundamental consptuent versus Pme 34
35 Ordering scheme (cont d) Ordering of hadrons (hadros = robust) using their measurable properpes (mass, charge, spin, isospin) SeparaPon of light and heavy hadrons and call them baryons and mesons mass [GeV] vector meson (spin 1) pseudo-scalars (spin 0) 35
36 Ordering scheme (cont d) Baryons (baryos = heavy) have half- integer spin proton, anp- proton, neutron Δ(1232) resonances, Λ(1116), Mesons (mesos = middle) have integer spin π 0, π ± (140) η(547), σ(600), ρ(770), ω(782), φ(1019), K ± (493), K 0 s (498), Leptons (leptos = light) do not interact strongly electron, positron, muon, neutrino, Note: Leptons are elementary parpcles, hadrons (baryons and mesons) not; evident from its excitapon spectra. 36
37 Summary Hc 4 ProducPon and idenpficapon of parpcles Every parpcle has an anp- parpcle with exactly the same mass but opposite electrical charge (later: opposite charge, baryon and strange number) New parpcles, with masses between electron and proton mass ExoPc parpcles: strangeness Ordering scheme Hadrons (baryons and mesons) and leptons 37
38 QuesPons? 38
High Energy Physics. QuarkNet summer workshop June 24-28, 2013
High Energy Physics QuarkNet summer workshop June 24-28, 2013 1 The Birth of Particle Physics In 1896, Thompson showed that electrons were particles, not a fluid. In 1905, Einstein argued that photons
More informationOption 212: UNIT 2 Elementary Particles
Department of Physics and Astronomy Option 212: UNIT 2 Elementary Particles SCHEDULE 26-Jan-15 13.pm LRB Intro lecture 28-Jan-15 12.pm LRB Problem solving (2-Feb-15 1.am E Problem Workshop) 4-Feb-15 12.pm
More informationThe Development of Particle Physics. Dr. Vitaly Kudryavtsev E45, Tel.:
The Development of Particle Physics Dr. Vitaly Kudryavtsev E45, Tel.: 0114 2224531 v.kudryavtsev@sheffield.ac.uk Discovery of the muon and the pion Energy losses of charged particles. This is an important
More informationLecture 3. lecture slides are at:
Lecture 3 lecture slides are at: http://www.physics.smu.edu/ryszard/5380fa16/ Proton mass m p = 938.28 MeV/c 2 Electron mass m e = 0.511 MeV/c 2 Neutron mass m n = 939.56 MeV/c 2 Helium nucleus α: 2 protons+2
More informationModern physics 1 Chapter 13
Modern physics 1 Chapter 13 13. Particle physics Particle studied within the ATLAS-project CERN In the beginning of 1930, it seemed that all the physics fundaments was placed within the new areas of elementary
More informationLecture 3. lecture slides are at:
Lecture 3 lecture slides are at: http://www.physics.smu.edu/ryszard/5380fa17/ Proton mass m p = 938.28 MeV/c 2 Electron mass m e = 0.511 MeV/c 2 Neutron mass m n = 939.56 MeV/c 2 Helium nucleus α: 2 protons+2
More informationA brief history of accelerators, detectors and experiments: (See Chapter 14 and Appendix H in Rolnick.)
Physics 557 Lecture 7 A brief history of accelerators, detectors and experiments: (See Chapter 14 and Appendix H in Rolnick.) First came the study of the debris from cosmic rays (the God-given particle
More informationElementary Particle Physics Glossary. Course organiser: Dr Marcella Bona February 9, 2016
Elementary Particle Physics Glossary Course organiser: Dr Marcella Bona February 9, 2016 1 Contents 1 Terms A-C 5 1.1 Accelerator.............................. 5 1.2 Annihilation..............................
More informationThe God particle at last? Science Week, Nov 15 th, 2012
The God particle at last? Science Week, Nov 15 th, 2012 Cormac O Raifeartaigh Waterford Institute of Technology CERN July 4 th 2012 (ATLAS and CMS ) A new particle of mass 125 GeV Why is the Higgs particle
More informationThe Physics of Cosmic Rays
The Physics of Cosmic Rays QuarkNet summer workshop July 23-27, 2012 1 Recent History Most natural phenomena can be explained by a small number of simple rules. You can determine what these rules are by
More informationAt this time the quark model consisted of three particles, the properties of which are given in the table.
*1 In 1961 Murray Gell-Mann predicted the existence of a new particle called an omega (Ω) minus. It was subsequently discovered in 1964. At this time the quark model consisted of three particles, the properties
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 informationenergy loss Ionization + excitation of atomic energy levels Mean energy loss rate de /dx proportional to (electric charge) 2 of incident particle
Lecture 4 Particle physics processes - particles are small, light, energetic à processes described by quantum mechanics and relativity à processes are probabilistic, i.e., we cannot know the outcome of
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 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 informationLecture 11. Weak interactions
Lecture 11 Weak interactions 1962-66: Formula/on of a Unified Electroweak Theory (Glashow, Salam, Weinberg) 4 intermediate spin 1 interaction carriers ( bosons ): the photon (γ) responsible for all electromagnetic
More informationThe Particle World. This talk: What is our Universe made of? Where does it come from? Why does it behave the way it does?
The Particle World What is our Universe made of? Where does it come from? Why does it behave the way it does? Particle physics tries to answer these questions. This talk: particles as we understand them
More informationIonization Energy Loss of Charged Projectiles in Matter. Steve Ahlen Boston University
Ionization Energy Loss of Charged Projectiles in Matter Steve Ahlen Boston University Almost all particle detection and measurement techniques in high energy physics are based on the energy deposited by
More informationWhat is matter and how is it formed?
What is matter and how is it formed? Lesson 6: Subatomic Particles Subatomic particles refers to particles that are more "fundamental" than... Are these fundamental particles or are they made up of smaller,
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 God particle at last? Astronomy Ireland, Oct 8 th, 2012
The God particle at last? Astronomy Ireland, Oct 8 th, 2012 Cormac O Raifeartaigh Waterford Institute of Technology CERN July 4 th 2012 (ATLAS and CMS ) A new particle of mass 125 GeV I The Higgs boson
More informationThe ATLAS Experiment and the CERN Large Hadron Collider
The ATLAS Experiment and the CERN Large Hadron Collider HEP101-2 April 5, 2010 A. T. Goshaw Duke University 1 HEP 101 Plan March 29: Introduction and basic HEP terminology March 30: Special LHC event:
More information9.2.E - Particle Physics. Year 12 Physics 9.8 Quanta to Quarks
+ 9.2.E - Particle Physics Year 12 Physics 9.8 Quanta to Quarks + Atomic Size n While an atom is tiny, the nucleus is ten thousand times smaller than the atom and the quarks and electrons are at least
More information1. What does this poster contain?
This poster presents the elementary constituents of matter (the particles) and their interactions, the latter having other particles as intermediaries. These elementary particles are point-like and have
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 informationLeptons and Weak interactions
PHY771, 8/28/2014 Tomasz Skwarnicki 1 Historical introduction to Elementary Particles: Leptons and Weak interactions Tomasz Skwarnicki Syracuse University Griffiths, 2 nd ed., 1.3-1.5,1.10 PHY771, 8/28/2014
More informationIntroduction to particle physics Lecture 4
Introduction to particle physics Lecture 4 Frank Krauss IPPP Durham U Durham, Epiphany term 2009 Outline 1 Mesons and Isospin 2 Strange particles 3 Resonances 4 The quark model Nuclei, nucleons, and mesons
More informationANTIMATTER MATTER. does the difference between matter and antimatter arise?
WHY ANTIMATTER MATTERS! One of the most striking facts about the Universe is that it is composed almost entirely of matter. At the Big Bang equal amounts of matter and antimatter would have been created.
More information17/01/17 F. Ould-Saada
Chapter 3 3.1 Why Do We Need Accelerators? 3.1.1 The Center-of-Mass (c.m.) System 3.1.2 The Laboratory System 3.1.3 Fixed Target Accelerator and Collider 3.2 Linear and Circular Accelerators 3.2.1 Linear
More informationThe ATLAS Experiment and the CERN Large Hadron Collider
The ATLAS Experiment and the CERN Large Hadron Collider HEP101-4 February 20, 2012 Al Goshaw 1 HEP 101 Today Introduction to HEP units Particles created in high energy collisions What can be measured in
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 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 informationOptimizing Selection and Sensitivity Results for VV->lvqq, 6.5 pb -1, 13 TeV Data
1 Optimizing Selection and Sensitivity Results for VV->lvqq, 6.5 pb, 13 TeV Supervisor: Dr. Kalliopi Iordanidou 215 Columbia University REU Home Institution: High Point University 2 Summary Introduction
More informationcgrahamphysics.com Particles that mediate force Book pg Exchange particles
Particles that mediate force Book pg 299-300 Exchange particles Review Baryon number B Total # of baryons must remain constant All baryons have the same number B = 1 (p, n, Λ, Σ, Ξ) All non baryons (leptons
More informationEssential Physics II. Lecture 14:
Essential Physics II E II Lecture 14: 18-01-16 Last lecture of EP2! Congratulations! This was a hard course. Be proud! Next week s exam Next Monday! All lecture slides on course website: http://astro3.sci.hokudai.ac.jp/~tasker/teaching/ep2
More informationPARTICLE PHYSICS :Higher Level Long Questions
PARTICLE PHYSICS :Higher Level Long Questions Particle Accelerators (including Cockcroft and Walton experiment) 2013 Question 10 (a) In 1932 J.D. Cockroft and E.T.S. Walton accelerated protons to energies
More informationWhy do we accelerate particles?
Why do we accelerate particles? (1) To take existing objects apart 1803 J. Dalton s indivisible atom atoms of one element can combine with atoms of other element to make compounds, e.g. water is made of
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 informationParticle Physics A short History
Introduction to Experimental Particle Physics Heavily indebted to 1. Steve Lloyd Queen Mary s College, London 2004 2. Robert S. Orr University of Toronto 2007 3. Z. Vilakazi University of Cape Town -2006
More informationEarlier in time, all the matter must have been squeezed more tightly together and a lot hotter AT R=0 have the Big Bang
Re-cap from last lecture Discovery of the CMB- logic From Hubble s observations, we know the Universe is expanding This can be understood theoretically in terms of solutions of GR equations Earlier in
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 informationPart II: Detectors. Peter Schleper Universität Hamburg
Part II: Detectors Peter Schleper Universität Hamburg 30.05.2018 Outline of the lecture: 1. Overview on detectors 2. Particle interactions with matter 3. Scintillators and photon detectors 4. Semiconductor
More informationINVASIONS IN PARTICLE PHYSICS
INVASIONS IN PARTICLE PHYSICS Compton Lectures Autumn 2001 Lecture 3 Oct. 20 2001 http://hep.uchicago.edu/compton 1 LECTURE 2 Cosmic Invasion The muon and the pion Previous Lecture 2 3 Orbital n=4 l=3
More informationHand of Anna Röntgen. From Life magazine,6 April 1896
FROM ELECTRONS TO QUARKS The development of Particle Physics QUARKNET 2001, FSU Laura Reina Outline ffl What is Particle Physics? ffl The origins of Particle Physics: the atom (p,e ), radioactivity, and
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 informationHadron Physics & Quantum Chromodynamics Adnan Bashir, IFM, UMSNH, Mexico August 2013 Hermosillo Sonora
Hadron Physics & Quantum Chromodynamics Adnan Bashir, IFM, UMSNH, Mexico August 2013 Hermosillo Sonora Hadron Physics & QCD Part 1: First Encounter With Hadrons: Introduction to Mesons & Baryons, The Quark
More informationPhysics 424: Dr. Justin Albert (call me Justin!)
Physics 424: Dr. Justin Albert (call me Justin!) A Brief History of Particle Physics Discoveries (Or: Figuring out What the Universe is Made Of ) Looking Inside the Atom: e -, p, and n! 1897: J.J. Thomson
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 informationAppendix A2. Particle Accelerators and Detectors The Large Hadron Collider (LHC) in Geneva, Switzerland on the Border of France.
Appendix A. Particle Accelerators and Detectors The Large Hadron Collider (LHC) in Geneva, Switzerland on the Border of France. Prepared by: Arash Akbari-Sharbaf Why Build Accelerators? Probe deeper From
More informationThe Physics of Particle Detectors
The Physics of Particle Detectors Lecture Notes WS 2010/11 Erika Garutti (DESY) Heinz Graafsma (XFEL) 1 On tools and instrumentation New directions in science are launched by new tools much more often
More informationNeutrino Physics. Kam-Biu Luk. Tsinghua University and University of California, Berkeley and Lawrence Berkeley National Laboratory
Neutrino Physics Kam-Biu Luk Tsinghua University and University of California, Berkeley and Lawrence Berkeley National Laboratory 4-15 June, 2007 Outline Brief overview of particle physics Properties of
More informationThe achievements of the CERN proton antiproton collider
The achievements of the CERN proton antiproton collider Luigi DiLella Scuola Normale Superiore, Pisa, Italy Motivation of the project The proton antiproton collider UA1 and UA2 detectors Discovery of the
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 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 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 informationIntroduction to CERN and CMS
Introduction to CERN and CMS and background for the CMS analysis Jamie Gainer University of Hawaii at Manoa April 1, 2017 What do I do? I am a postdoc at UH Manoa I am a theorist In physics there are theorists:
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 informationParticle physics: what is the world made of?
Particle physics: what is the world made of? From our experience from chemistry has told us about: Name Mass (kg) Mass (atomic mass units) Decreasing mass Neutron Proton Electron Previous lecture on stellar
More informationFYS3510 Subatomic Physics. Exam 2016
FYS3510 Subatomic Physics VS 2015 Farid Ould-Saada Exam 2016 In addition to the items marked in blue, don t forget all examples and related material given in the slides, including the ones presented during
More informationUnravelling the Mysteries of Matter with the CERN Large Hadron Collider An Introduction/Overview of Particle Physics
Unravelling the Mysteries of Matter with the CERN Large Hadron Collider An Introduction/Overview of Particle Physics Introductory Lecture August 3rd 2014 International Centre for Theoretical Physics and
More informationSaturday Morning Physics -- Texas A&M University. What is Matter and what holds it together? Dr. Rainer J. Fries. January 27, 2007
Saturday Morning Physics -- Texas A&M University Particles and Forces What is Matter and what holds it together? Dr. Rainer J. Fries January 27, 2007 Zooming in on the World around us Particles and Forces
More informationSaturday Morning Physics -- Texas A&M University Dr. Rainer J. Fries
Saturday Morning Physics -- Texas A&M University Particles and Forces What is Matter and what holds it together? Dr. Rainer J. Fries January 27, 2007 Zooming in on the World around us Particles and Forces
More informationThe Development of Particle Physics. Dr. Vitaly Kudryavtsev E45, Tel.:
The Development of Particle Physics Dr. Vitaly Kudryavtsev E45, Tel.: 0114 2224531 v.kudryavtsev@sheffield.ac.uk Previous lecture New unstable particles discovered in 40s-50s. First hyperons (particles
More informationLHC Detectors and their Physics Potential. Nick Ellis PH Department, CERN, Geneva
LHC Detectors and their Physics Potential Nick Ellis PH Department, CERN, Geneva 1 Part 1 Introduction to the LHC Detector Requirements & Design Concepts 2 What is the Large Hadron Collider? Circular proton-proton
More informationThe Discovery of the Higgs Boson: one step closer to understanding the beginning of the Universe
The Discovery of the Higgs Boson: one step closer to understanding the beginning of the Universe Anna Goussiou Department of Physics, UW & ATLAS Collaboration, CERN Kane Hall, University of Washington
More informationCHAPTER 7 TEST REVIEW
IB PHYSICS Name: Period: Date: # Marks: 94 Raw Score: IB Curve: DEVIL PHYSICS BADDEST CLASS ON CAMPUS CHAPTER 7 TEST REVIEW 1. An alpha particle is accelerated through a potential difference of 10 kv.
More informationFall Quarter 2010 UCSB Physics 225A & UCSD Physics 214 Homework 1
Fall Quarter 2010 UCSB Physics 225A & UCSD Physics 214 Homework 1 Problem 2 has nothing to do with what we have done in class. It introduces somewhat strange coordinates called rapidity and pseudorapidity
More informationThe ATLAS Experiment and the CERN Large Hadron Collider
The ATLAS Experiment and the CERN Large Hadron Collider HEP101-2 January 28, 2013 Al Goshaw 1 HEP 101-2 plan Jan. 14: Introduction to CERN and ATLAS DONE Today: 1. Comments on grant opportunities 2. Overview
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 informationLecture 2 & 3. Particles going through matter. Collider Detectors. PDG chapter 27 Kleinknecht chapters: PDG chapter 28 Kleinknecht chapters:
Lecture 2 & 3 Particles going through matter PDG chapter 27 Kleinknecht chapters: 1.2.1 for charged particles 1.2.2 for photons 1.2.3 bremsstrahlung for electrons Collider Detectors PDG chapter 28 Kleinknecht
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 informationPar$cles. Ma#er is made of atoms. Atoms are made of leptons and quarks. Leptons. Quarks. atom nucleus nucleon quark m m m m
Par$cles Ma#er is made of atoms atom nucleus nucleon quark 10-10 m 10-14 m 10-15 m 10-18 m Atoms are made of leptons and quarks Leptons ν e e Quarks u d What Have We Learned? Rela?vis?c Quantum Mechanics
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 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 informationWesley Smith, U. Wisconsin, January 21, Physics 301: Introduction - 1
Wesley Smith, U. Wisconsin, January 21, 2014 Physics 301: Introduction - 1 Physics 301: Physics Today Prof. Wesley Smith, wsmith@hep.wisc.edu Undergraduate Physics Colloquium! Discussions of current research
More informationThe Building Blocks of Nature
The Building Blocks of Nature PCES 15.1 Schematic picture of constituents of an atom, & rough length scales. The size quoted for the nucleus here (10-14 m) is too large- a single nucleon has size 10-15
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 information32 IONIZING RADIATION, NUCLEAR ENERGY, AND ELEMENTARY PARTICLES
32 IONIZING RADIATION, NUCLEAR ENERGY, AND ELEMENTARY PARTICLES 32.1 Biological Effects of Ionizing Radiation γ-rays (high-energy photons) can penetrate almost anything, but do comparatively little damage.
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 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 informationLecture 2: The First Second origin of neutrons and protons
Lecture 2: The First Second origin of neutrons and protons Hot Big Bang Expanding and cooling Soup of free particles + anti-particles Symmetry breaking Soup of free quarks Quarks confined into neutrons
More informationQuanta to Quarks. Science Teachers Workshop 2014 Workshop Session. Adrian Manning
Quanta to Quarks Science Teachers Workshop 2014 Workshop Session Adrian Manning The Quanta to Quarks module! The Quanta to Quarks module ultimately deals with some of the most fundamental questions about
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 informationA first trip to the world of particle physics
A first trip to the world of particle physics Itinerary Massimo Passera Padova - 13/03/2013 1 Massimo Passera Padova - 13/03/2013 2 The 4 fundamental interactions! Electromagnetic! Weak! Strong! Gravitational
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 informationM. Cobal, PIF 2006/7. Quarks
M. Cobal, PIF 2006/7 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
More informationNUCLEAR AND PARTICLE PHYSICS (PH242) PARTICLE PHYSICS
NUCLEAR AND PARTICLE PHYSICS (PH242) PARTICLE PHYSICS History of Elementary Particles THE CLASSICAL ERA (1897-1932) Elementary particle physics was born in 1897 with J.J. Thomson s discovery of the ELECTRONS
More informationA brief history of neutrino. From neutrinos to cosmic sources, DK&ER
A brief history of neutrino Two body decay m 1 M m 2 Energy-momentum conservation => Energy of the decay products always the same 1913-1930: Puzzle of decay Continuous spectrum of particles Energy is not
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 informationMatter, Antimatter and the Strangeness of CP violation
Matter, Antimatter and the Strangeness of CP violation Angela Romano Angela Romano Masterclass 21/04/10 1 Cambridge, 1928 : Dirac predicted the existence of the positron e+, same mass but opposite charge
More informationParticle detection 1
Particle detection 1 Recall Particle detectors Detectors usually specialize in: Tracking: measuring positions / trajectories / momenta of charged particles, e.g.: Silicon detectors Drift chambers Calorimetry:
More informationExam Results. Force between charges. Electric field lines. Other particles and fields
Exam: Exam scores posted on Learn@UW No homework due next week Exam Results F D C BC B AB A Phy107 Fall 2006 1 Particles and fields We have talked about several particles Electron,, proton, neutron, quark
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 information\ \ \/ \\// (o) (o) U. February 11, UT Saturday Morning Physics. Yuri Kamyshkov University of Tennessee
\ \ \/ \\// (o) (o) U February 11, 2017 @ UT Saturday Morning Physics Yuri Kamyshkov University of Tennessee kamyshkov@utk.edu 1 2 Large Hadron Collider CERN European Centre for Particle Physics Geneva,
More informationThe Physics of Particles and Forces David Wilson
The Physics of Particles and Forces David Wilson Particle Physics Masterclass 21st March 2018 Overview David Wilson (TCD) Particles & Forces 2/30 Overview of Hadron Spectrum Collaboration (HadSpec) scattering
More informationThe first 400,000 years
The first 400,000 years All about the Big Bang Temperature Chronology of the Big Bang The Cosmic Microwave Background (CMB) The VERY early universe Our Evolving Universe 1 Temperature and the Big Bang
More informationParticle + Physics at ATLAS and the Large Hadron Coillder
Particle + Physics at ATLAS and the Large Hadron Coillder Discovering the elementary particles of the Universe Kate Shaw The International Centre for Theoretical Physics + Overview Introduction to Particle
More informationMatter: it s what you have learned that makes up the world Protons, Neutrons and Electrons
Name The Standard Model of Particle Physics Matter: it s what you have learned that makes up the world Protons, Neutrons and Electrons Just like there is good and evil, matter must have something like
More informationMINERVA Masterclass. Teachers Manual. Vera Zimanyine Horvath Francesco Mezzanotte Tom Lambert
MINERVA Masterclass Teachers Manual Vera Zimanyine Horvath Francesco Mezzanotte Tom Lambert 1 Fundamental Particles theoretical background of using Minerva for teachers 1. Standard Model of Fundamental
More informationY2 Neutrino Physics (spring term 2017)
Y2 Neutrino Physics (spring term 2017) Lecture 5 Discoveries of the leptons Dr E Goudzovski eg@hep.ph.bham.ac.uk http://epweb2.ph.bham.ac.uk/user/goudzovski/y2neutrino Previous lecture In 1940s, nuclear
More information