A Brief History of Modern Physics

Similar documents
Lecture 8. CPT theorem and CP violation

Elementary Particle Physics Glossary. Course organiser: Dr Marcella Bona February 9, 2016

Lecture 8. CPT theorem and CP violation

Atoms, nuclei, particles

Chapter 32 Lecture Notes

A first trip to the world of particle physics

Particle Physics Outline the concepts of particle production and annihilation and apply the conservation laws to these processes.

Option 212: UNIT 2 Elementary Particles

FACULTY OF SCIENCE. High Energy Physics. WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON

Units and dimensions

Introduction. Read: Ch 1 of M&S

THE NEUTRINOS. Boris Kayser & Stephen Parke Fermi National Accelerator Laboratory

Quantum Numbers. Elementary Particles Properties. F. Di Lodovico c 1 EPP, SPA6306. Queen Mary University of London. Quantum Numbers. F.

Lecture 2: The First Second origin of neutrons and protons

Atomic emission & absorption spectra

Elementary Particles, Flavour Physics and all that...

Phys 102 Lecture 28 Life, the universe, and everything

1. What does this poster contain?

Overview. The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions.

Quantum Gravity and Entanglement

The Goals of Particle Physics

The 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

Weak Interactions. The Theory of GLASHOW, SALAM and WEINBERG

1. (a) An ion of plutonium Pu has an overall charge of C. (iii) electrons... (3) (2) (Total 5 marks)

Lecture 11. Weak interactions

THE STANDARD MODEL OF MATTER

Option 212: UNIT 2 Elementary Particles

Chapter 46. Particle Physics and Cosmology

FYS3510 Subatomic Physics. Exam 2016

. Thus his equation would have to be of the form. 2 t. but must also satisfy the relativistic energy-momentum relation. H 2 φ = ( p 2 + m 2 )φ (3)

The Standard Model of Particle Physics

E = mc 2 Opening Windows on the World

I. Antoniadis CERN. IAS CERN Novice Workshop, NTU, 7 Feb 2014

Par$cles. Ma#er is made of atoms. Atoms are made of leptons and quarks. Leptons. Quarks. atom nucleus nucleon quark m m m m

Democritus, a fifth century B.C. philosopher, is credited with being the first

Hot Big Bang model: early Universe and history of matter

Nuclear and Particle Physics 3: Particle Physics. Lecture 1: Introduction to Particle Physics February 5th 2007

Cosmology and particle physics

A Tour of the Standard Model of Elementary Particles and Fields

The Physics of Particles and Forces David Wilson

Katsushi Arisaka University of California, Los Angeles Department of Physics and Astronomy

Modern Physics. Luis A. Anchordoqui. Department of Physics and Astronomy Lehman College, City University of New York. Lesson XI November 19, 2015

The Scale-Symmetric Theory as the Origin of the Standard Model

Particle Physics. All science is either physics or stamp collecting and this from a 1908 Nobel laureate in Chemistry

Announcement. Station #2 Stars. The Laws of Physics for Elementary Particles. Lecture 9 Basic Physics

Lecture PowerPoint. Chapter 32 Physics: Principles with Applications, 6 th edition Giancoli

The God particle at last? Astronomy Ireland, Oct 8 th, 2012

The first one second of the early universe and physics beyond the Standard Model

The Discovery of the Higgs Boson: one step closer to understanding the beginning of the Universe

Contents. Preface to the First Edition Preface to the Second Edition

The Four Fundamental Forces. The Four Fundamental Forces. Gravitational Force. The Electrical Force. The Photon (γ) Unification. Mass.

CPT Symmetry and Symmetry-Breaking in the Scale-Symmetric Theory

FYS 3510 Subatomic physics with applications in astrophysics. Nuclear and Particle Physics: An Introduction

FYS3510 Subatomic Physics. Exam 2016

Astro-2: History of the Universe. Lecture 12; May

Spec Content Before Revision After 1st Revision After 2nd Revision

Matter, Antimatter and the Strangeness of CP violation

John Ellison University of California, Riverside. Quarknet 2008 at UCR

Chapter 22 Back to the Beginning of Time

Electron-positron pairs can be produced from a photon of energy > twice the rest energy of the electron.

Quantum Spin Hall Effect

Lecture 9. Isospin The quark model

Physics 4213/5213 Lecture 1

Invariance Principles and Conservation Laws

The Early Universe. Overview: The Early Universe. Accelerators recreate the early universe. Simple Friedmann equation for the radiation era:

Neutron Decay Disagree

The Building Blocks of Nature

An Introduction to Particle Physics

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS

Hot Topics in Physics. OLLI lectures Fall 2016 Horst D Wahl lecture 3, 25 Oct 2016

1 Introduction. 1.1 The Standard Model of particle physics The fundamental particles

Earlier in time, all the matter must have been squeezed more tightly together and a lot hotter AT R=0 have the Big Bang

Hand of Anna Röntgen. From Life magazine,6 April 1896

Quantum Decoherence due to Gravitational Time Dilation

2007 Section A of examination problems on Nuclei and Particles

Chapter 22: Cosmology - Back to the Beginning of Time

Computational Applications in Nuclear Astrophysics using JAVA

Origin of the Universe - 2 ASTR 2120 Sarazin. What does it all mean?

The Uncertainty Principle and the Quarks

Weak interactions. Chapter 7

The Boundary between Classical and Quantum Mechanics

Particle + Physics at ATLAS and the Large Hadron Coillder

Visit for more fantastic resources. OCR. A Level. A Level Physics. Particle physics (Answers) Name: Total Marks: /30

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS

The Exchange Model. Lecture 2. Quantum Particles Experimental Signatures The Exchange Model Feynman Diagrams. Eram Rizvi

Astr 2320 Thurs. May 7, 2015 Today s Topics Chapter 24: New Cosmology Problems with the Standard Model Cosmic Nucleosynthesis Particle Physics Cosmic

Atomic Structure Discovered. Dalton s Atomic Theory. Discovery of the Electron 10/30/2012

Phys 328 Nuclear Physics and Particles Introduction Murat

Extending classical big bang theory

Introduction to Particle Physics. HST July 2016 Luis Alvarez Gaume 1

Neutrino Physics. Kam-Biu Luk. Tsinghua University and University of California, Berkeley and Lawrence Berkeley National Laboratory

Weak interactions and vector bosons

The Standard Model of Particle Physics - I

Quantum Mechanics. Reading: Gray: (1 8) to (1 12) OGN: (15.5)

The God particle at last? Science Week, Nov 15 th, 2012

Frontier Science: The mystery of Antimatter

Introduction to Elementary Particles

3 Dimensional String Theory

Evidence for the Strong Interaction

Physics 424: Dr. Justin Albert (call me Justin!)

Transcription:

A Brief History of Modern Physics Modern Physics rests on two pillars: 1. Theory of Relativity (Einstein) Special Relativity 1905 General Relativity 1915 nature of space and time (phenomena at high speed) gravity as a result of curved spacetime 2. Quantum Mechanics (Bohr, Heisenberg, Schrödinger, ) ~1900-1925 phenomena at very short distance scales structure of the atom behavior of light, subatomic particles

What is Particle Physics About? Experiments can address long standing puzzles / questions: What are the fundamental constituents of matter? What are the fundamental forces between elementary particles? Can the forces of nature be unified? Including gravity? What is the origin of mass? What is the origin of the matter-antimatter asymmetry of the Universe? What is dark matter?

Constituents of Matter (I) Thomson Model of the Atom (early 1900 s) electrons are embedded in homogeneous positively charged mass raisins in plum pudding diffuse positive charge Note: protons not yet discovered in early 1900 s Problems: Emission lines cannot be explained

Constituents of Matter (II) How can we probe the structure of the atom? Perform scattering experiments with high energy particles h with de Broglie wavelength λ = p Rutherford Scattering Expts (1910) Projectiles: α particles (He nucleus) produced in radioactive decays e.g. 232 Th 228 Ra + α Kinetic energy of α particle K = 4 MeV λ 10-14 m Observations: ~1 in 10 4 α particles is back scattered Large angle deflections are due to nearly head-on collisions between the α particles and a very small and dense nucleus

Constituents of Matter (III) Late 1960 s: repeat of Rutherford expt at huge particle accelerators like the 2-mile long linac at the Stanford Linear Accelerator Center (SLAC) Projectiles: linear accelerator takes electrons from rest to K = 50 GeV de Broglie wavelength = 2.5 x 10-17 m moving close to the speed of light: v = 0.999 999 999 95 c Electrons do not see 2 mile-long linac but a contracted length of only 1 in.!

Constituents of Matter (IV) Scattering experiments at SLAC established the existence of quarks as fundamental constituents of protons and neutrons What do we currently know about the structure of matter? Atom Nucleus = bound system of positive nucleus + orbiting electrons ~ 10-10 m = bound system of protons + neutrons (nucleons) ~ 10-15 m Nucleons = bound system of up and down quarks Quarks Name =? no known structure down to < 10-18 m Spin Charge up (u) ½ +⅔ e down (d) ½ strange (s) ½ ⅓ e charmed (c) ½ +⅔ e bottom (b) ½ ⅓ e top (t) ½ +⅔ e ⅓ e mass

Forces How do these fundamental constituents interact with one another? Four different forces are known: Interaction Rel. strength Range Strong 1 ~2 fm Electromagnetic 10-2 Weak 10-5 Gravitational 10-39 ~10-3 fm Forces mediated by particles:

4 Forces

Probing short distance scales (high energy) uncovers deep regularities, symmetries and can lead to unified descriptions of different phenomena

Particle accelerators allow us to peer into the earliest moments of the Universe Forces believed to be unified at extreme energies (or tiny distance scales)

News from the Cosmos Quarks and leptons make up only 5% of the Universe! Deep mystery: what is dark energy and dark matter? Antimatter: 0%

Matter-antimatter Asymmetry (I) Baryogenesis Puzzle Early Universe: matter and antimatter created in equal amounts Universe Today: no antimatter! Big Bang time Mystery: Where did the antimatter go? Why is there any matter left today?

Matter-antimatter Asymmetry (II) A. Sakharov (1967) proposes a mechanism that requires three ingredients to explain the asymmetry: 1. Baryon number violating reactions occur 2. C and CP violation (CPV) take place in these reactions 3. Reactions occur out of thermal equilibrium (Big Bang) Violation of CP-invariance, C-asymmetry and baryon asymmetry of the Universe Sakharov s paper summary in verse: From S. Okubo s effect At high temperature A coat is tailored for the Universe To fit its skewed shape

Matter-antimatter Asymmetry (III) What is CP violation? Observation that the Laws of Physics are not exactly the same under the combined transformation: Charge conjugation C particle antiparticle Parity P left-handed helicity right-handed helicity (mirror symmetry) CP symmetry is preserved in strong and electromagnetic interactions BUT weak interactions violate CP symmetry Cronin, Fitch (1964) Manifestation: different decay rates in K and B meson decays For example, the decay rate for K 0 L π µ + ν µ is slightly higher than that for K 0 L π + µ ν µ (rate asymmetry = 0.3%)

Matter-antimatter Asymmetry (IV) Does the Standard Model provide Sakharov s three ingredients? YES! How much asymmetry do we need? 1 in 10 9 baryons must survive annihilation to generate the baryon asymmetry observed today: (n B n B ) / n γ = 6 x 10-10 (WMAP) Can the Standard Model do that? NO! Amount of CP violation is too small by ~10 orders of magnitude

e + e - ϒ(4S) B B with E(e+) = 3.1 GeV and E(e - ) = 9.0 GeV