The Standard Model. The Standard Model combines the electromagnetic, weak, and strong forces (= interactions).

Size: px
Start display at page:

Download "The Standard Model. The Standard Model combines the electromagnetic, weak, and strong forces (= interactions)."

Transcription

1 The Standard Model fermion boson fermion The Standard Model combines the electromagnetic, weak, and strong forces (= interactions). Bosons with spin 1 communicate the force between fermions with spin ½. Glashow Salam Weinberg An extra feature is the Higgs boson with spin 0.

2 Bosons Three sets of bosons mediate three interactions: Electromagnetic Weak Strong photon Z, W gluons The principle stays the same, only the players change: Bosons communicate interactions between fermions. Each interaction has its characteristic set of bosons.

3 The Higgs boson The Higgs boson is unique. There is no other fundamental particle with spin 0. It was concocted by theorists to explain why the Z,W bosons have mass while the photon and the gluons don t. It also describes the mass of fermions (electron, quarks).* The Higgs particle was observed at the LHC in * However, the influence of the Higgs boson on the mass of humans, stars, and galaxies is negligible. These are made of atoms, whose mass is dominated by the mass of their nucleons. Those consist of quarks and gluons. The quark mass is < 2% of the nucleon mass (Slide 7) and the gluon mass is zero. Instead, the nucleon mass is dominated by the kinetic energy of quarks and gluons, converted to mass using E=mc 2.

4 How the Higgs field creates mass Mathematically, the mass comes from a clever manipulation of quantum fields. But it is hard to describe in plain words.the British Science Minister Waldegrave challenged physicists in 1993 to produce an explanation on a single sheet of paper. The result can be condensed into a few bullets: The Higgs field fills space like molasses, attaching itself to particles. When a particle is accelerated, it has to drag the Higgs field along. That reduces its acceleration a. Newton s F=ma tells us that a smaller acceleration a for the same force F implies a larger mass m.

5

6 The Higgs field is different The Higgs field oscillates around a non-zero average. All other fields oscillate around zero, for example the electric and magnetic field of an electromagnetic wave. Higgs field All other fields 0 0 non-zero average

7 Fermions Three generations, each consisting of lepton and quark pairs. light heavier heaviest Who ordered that? (Isaac Rabi)

8 Is there a 4 th generation? Are there more than three particle generations? This question can be answered by measuring the number of particles that originate from the decay of a Z boson.the Z itself is produced by an electron-positron pair. The green curve is calculated for 3 neutrino generations. It fits the data perfectly.the red curves for 2 and 4 generations don t fit. Number of observed particles Z boson Energy (GeV)

9 Why are there three generations of fermions? We are still clueless.

10 Convergence of the three interactions The strength of an interaction is determined by its coupling constant. Inverse coupling constant Electromagnetic Weak Strong 1 Energy (GeV) TeV Planck Energy Coupling constants are not constant. They change with energy. At energies approaching the Planck energy they seem to converge to a single, unified coupling constant. This convergence is improved by introducing a new symmetry called supersymmetry, which predicts a new set of supersymmetric particles with masses >1TeV.The coupling constants converge to a value close to the number 1/8. Caution! This is an extrapolation over 13 orders of magnitude in energy.

11 The anthropic principle The Standard Model does extremely well at predicting all kinds of measurements done by accelerators. But it is not able to calculate coupling constants. Some argue that coupling constants cannot be calculated: Different universes may have different coupling constants. Our universe has a particular set of coupling constants because otherwise humans would not exist and contemplate this question. For example, the Sun can t be too hot or too cold for life. That would happen with an electromagnetic coupling constant slightly smaller or larger than 1/137. This is a slick excuse for our inability to predict the many numbers that the Standard Model cannot calculate ( 20).

An Introduction to Particle Physics

An Introduction to Particle Physics An Introduction to Particle Physics The Universe started with a Big Bang The Universe started with a Big Bang What is our Universe made of? Particle physics aims to understand Elementary (fundamental)

More information

Particle + Physics at ATLAS and the Large Hadron Coillder

Particle + 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 information

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

I. Antoniadis CERN. IAS CERN Novice Workshop, NTU, 7 Feb 2014 I. Antoniadis CERN IAS CERN Novice Workshop, NTU, 7 Feb 2014 1 2 3 the Large Hadron Collider (LHC) Largest scientific instrument ever built, 27km of circumference >10 000 people involved in its design

More information

A first trip to the world of particle physics

A 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 information

Overview. 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. 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 information

Physics 662. Particle Physics Phenomenology. February 21, Physics 662, lecture 13 1

Physics 662. Particle Physics Phenomenology. February 21, Physics 662, lecture 13 1 Physics 662 Particle Physics Phenomenology February 21, 2002 Physics 662, lecture 13 1 Physics Beyond the Standard Model Supersymmetry Grand Unified Theories: the SU(5) GUT Unification energy and weak

More information

Chapter 22: Cosmology - Back to the Beginning of Time

Chapter 22: Cosmology - Back to the Beginning of Time Chapter 22: Cosmology - Back to the Beginning of Time Expansion of Universe implies dense, hot start: Big Bang Future of universe depends on the total amount of dark and normal matter Amount of matter

More information

Introduction to the Standard Model

Introduction to the Standard Model Introduction to the Standard Model Bill Murray, RAL, Quarks and leptons Bosons and forces The Higgs March 2002 1 Outline: An introduction to particle physics What is the Higgs Boson? Some unanswered questions

More information

1. What does this poster contain?

1. 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 information

Particle physics: what is the world made of?

Particle 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 information

Beyond the standard model? From last time. What does the SM say? Grand Unified Theories. Unifications: now and the future

Beyond the standard model? From last time. What does the SM say? Grand Unified Theories. Unifications: now and the future From last time Quantum field theory is a relativistic quantum theory of fields and interactions. Fermions make up matter, and bosons mediate the forces by particle exchange. Lots of particles, lots of

More information

Physics Beyond the Standard Model. Marina Cobal Fisica Sperimentale Nucleare e Sub-Nucleare

Physics Beyond the Standard Model. Marina Cobal Fisica Sperimentale Nucleare e Sub-Nucleare Physics Beyond the Standard Model Marina Cobal Fisica Sperimentale Nucleare e Sub-Nucleare Increasingly General Theories Grand Unified Theories of electroweak and strong interactions Supersymmetry

More information

Lecture 39, 40 Supplement: Particle physics in the LHC era

Lecture 39, 40 Supplement: Particle physics in the LHC era Lecture 39, 40 Supplement: Particle physics in the LHC era The Matter Particles (Fermions) plus their antiparticles... What is measured? quarks confined into hadrons A zoo of strongly interacting particles...

More information

Chapter 22 Back to the Beginning of Time

Chapter 22 Back to the Beginning of Time Chapter 22 Back to the Beginning of Time Expansion of Universe implies dense, hot start: Big Bang Back to the Big Bang The early Universe was both dense and hot. Equivalent mass density of radiation (E=mc

More information

The God Particle and what it means. Peter Bussey. CiS Northern Meeting, April

The God Particle and what it means. Peter Bussey. CiS Northern Meeting, April The God Particle and what it means. Peter Bussey CiS Northern Meeting, April 27 2013 2010,2012 1993 Good publicity for an elementary particle! The CERN laboratory site, Geneva, Switzerland. Photographs

More information

Beyond Standard Models Higgsless Models. Zahra Sheikhbahaee

Beyond Standard Models Higgsless Models. Zahra Sheikhbahaee Beyond Standard Models Higgsless Models Zahra Sheikhbahaee Standard Model There are three basic forces in the Universe: 1. Electroweak force, including electromagnetic force, 2. Strong nuclear force, 3.

More information

Lecture 03. The Standard Model of Particle Physics. Part II The Higgs Boson Properties of the SM

Lecture 03. The Standard Model of Particle Physics. Part II The Higgs Boson Properties of the SM Lecture 03 The Standard Model of Particle Physics Part II The Higgs Boson Properties of the SM The Standard Model So far we talked about all the particles except the Higgs If we know what the particles

More information

Astronomy 182: Origin and Evolution of the Universe

Astronomy 182: Origin and Evolution of the Universe Astronomy 182: Origin and Evolution of the Universe Prof. Josh Frieman Lecture 12 Nov. 18, 2015 Today Big Bang Nucleosynthesis and Neutrinos Particle Physics & the Early Universe Standard Model of Particle

More information

Name : Physics 490. Practice Final (closed book; calculator, one notecard OK)

Name : Physics 490. Practice Final (closed book; calculator, one notecard OK) Name : Physics 490. Practice Final (closed book; calculator, one notecard OK) Problem I: (a) Give an example of experimental evidence that the partons in the nucleon (i) are fractionally charged. How can

More information

Black holes in D>4 dimensional space-times

Black holes in D>4 dimensional space-times Black holes in D>4 dimensional space-times Key-words: extra dimensions, string theory, brane world models, LHC, stability, perturbations, quasinormal modes, Hawking radiation R. A. Konoplya May 20, 2010

More information

Photon Coupling with Matter, u R

Photon Coupling with Matter, u R 1 / 16 Photon Coupling with Matter, u R Consider the up quark. We know that the u R has electric charge 2 3 e (where e is the proton charge), and that the photon A is a linear combination of the B and

More information

Mysteries of the Standard Model

Mysteries of the Standard Model Mysteries of the Standard Model Methods of exploring the nature of the Electroweak force at the Compact Muon Solenoid [CMS] experiment. Final REU presentation given by Kellen McGee in partial fulfillment

More information

Wesley Smith, U. Wisconsin, January 21, Physics 301: Introduction - 1

Wesley 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 information

Source:CERN. Size and Scale

Source:CERN. Size and Scale Table of Contents Introduction Unification of Forces Size and Scale Standard Model Summary Standard Model Particles and Force Carriers About Mass and Energy Standard Model Fermions: Generations and Masses

More information

Particles and Interactions. Prof. Marina Cobal Corso Particelle ed interazioni fondamentali 2013/2014

Particles and Interactions. Prof. Marina Cobal Corso Particelle ed interazioni fondamentali 2013/2014 Particles and Interactions Prof. Marina Cobal Corso Particelle ed interazioni fondamentali 2013/2014 What is the world made of? In the ancient time: 4 elements 19 century atoms Beginning 20 th century

More information

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

The first one second of the early universe and physics beyond the Standard Model The first one second of the early universe and physics beyond the Standard Model Koichi Hamaguchi (University of Tokyo) @ Colloquium at Yonsei University, November 9th, 2016. Credit: X-ray: NASA/CXC/CfA/M.Markevitch

More information

Lecture 03. The Standard Model of Particle Physics. Part III Extensions of the Standard Model

Lecture 03. The Standard Model of Particle Physics. Part III Extensions of the Standard Model Lecture 03 The Standard Model of Particle Physics Part III Extensions of the Standard Model Where the SM Works Excellent description of 3 of the 4 fundamental forces Explains nuclear structure, quark confinement,

More information

Cosmology and particle physics

Cosmology 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 information

The 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. 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 information

Most of Modern Physics today is concerned with the extremes of matter:

Most of Modern Physics today is concerned with the extremes of matter: Most of Modern Physics today is concerned with the extremes of matter: Very low temperatures, very large numbers of particles, complex systems Æ Condensed Matter Physics Very high temperatures, very large

More information

Particle Theory Beyond the Standard Model. Ann Nelson University of Washington August 9, 2010

Particle Theory Beyond the Standard Model. Ann Nelson University of Washington August 9, 2010 Particle Theory Beyond the Standard Model Ann Nelson University of Washington August 9, 2010 The world physics community has spent > 4B dollars (including 600M from American taxpayers) on the Large Hadron

More information

Essentials of Particle Physics

Essentials of Particle Physics Essentials of Particle Physics Kajari Mazumdar Department of High Energy Physics Tata Institute of Fundamental Research Mumbai http://www.tifr.res.in/~mazumdar Kajari.Mazumdar@gmail.com KSTA Lecture Series

More information

Most of Modern Physics today is concerned with the extremes of matter:

Most of Modern Physics today is concerned with the extremes of matter: Most of Modern Physics today is concerned with the extremes of matter: Very low temperatures, very large numbers of particles, complex systems Æ Condensed Matter Physics Very high temperatures, very large

More information

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

The Early Universe. Overview: The Early Universe. Accelerators recreate the early universe. Simple Friedmann equation for the radiation era: The Early Universe Notes based on Teaching Company lectures, and associated undergraduate text with some additional material added. ) From µs to s: quark confinement; particle freezout. 2) From s to 3

More information

Supersymmetry. Keywords: standard model, grand unified theories, theory of everything, superpartner, higgs boson, neutrino oscillation.

Supersymmetry. Keywords: standard model, grand unified theories, theory of everything, superpartner, higgs boson, neutrino oscillation. Supersymmetry Min Raj Lamsal Department of Physics, Prithvi Narayan Campus, Pokhara min_lamsal@yahoo.com Abstract : This article deals with the introduction of supersymmetry as the latest and most emerging

More information

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

John Ellison University of California, Riverside. Quarknet 2008 at UCR Overview of Particle Physics John Ellison University of California, Riverside Quarknet 2008 at UCR 1 Particle Physics What is it? Study of the elementary constituents of matter And the fundamental forces

More information

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

FACULTY OF SCIENCE. High Energy Physics. WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON FACULTY OF SCIENCE High Energy Physics WINTHROP PROFESSOR IAN MCARTHUR and ADJUNCT/PROFESSOR JACKIE DAVIDSON AIM: To explore nature on the smallest length scales we can achieve Current status (10-20 m)

More information

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

Particle 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 information

Large Hadron Collider

Large Hadron Collider Large Hadron Collider Himadri Barman TSU, JNCASR September 18, 2008 0-0 Large Hadron Collider (LHC): Plan We ll see 4 short videos. In between I ll give you a little guideline. Purpose is to understand

More information

Le Modèle Standard et ses extensions

Le Modèle Standard et ses extensions Particules Élémentaires, Gravitation et Cosmologie Année 2007-08 08 Le Modèle Standard et ses extensions Cours III: 15 février f 2008 Weak Interactions: from Fermi s s model to a gauge theory 15 fevrier

More information

UNVEILING THE ULTIMATE LAWS OF NATURE: DARK MATTER, SUPERSYMMETRY, AND THE LHC. Gordon Kane, Michigan Center for Theoretical Physics Warsaw, June 2009

UNVEILING THE ULTIMATE LAWS OF NATURE: DARK MATTER, SUPERSYMMETRY, AND THE LHC. Gordon Kane, Michigan Center for Theoretical Physics Warsaw, June 2009 UNVEILING THE ULTIMATE LAWS OF NATURE: DARK MATTER, SUPERSYMMETRY, AND THE LHC Gordon Kane, Michigan Center for Theoretical Physics Warsaw, June 2009 OUTLINE! Some things we ve learned about the physical

More information

Fundamental Forces. David Morrissey. Key Concepts, March 15, 2013

Fundamental Forces. David Morrissey. Key Concepts, March 15, 2013 Fundamental Forces David Morrissey Key Concepts, March 15, 2013 Not a fundamental force... Also not a fundamental force... What Do We Mean By Fundamental? Example: Electromagnetism (EM) electric forces

More information

The Discovery of the Higgs boson Matthew Herndon, University of Wisconsin Madison Physics 301: Physics Today. M. Herndon, Phys

The Discovery of the Higgs boson Matthew Herndon, University of Wisconsin Madison Physics 301: Physics Today. M. Herndon, Phys The Discovery of the Higgs boson Matthew Herndon, University of Wisconsin Madison Physics 301: Physics Today M. Herndon, Phys 301 2018 1 The Periodic Table: The early 20 th century understanding of the

More information

Chapter 32 Lecture Notes

Chapter 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 information

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

The 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 information

Physics 214 Experimental Particle Physics. Lecture 1 What to expect.

Physics 214 Experimental Particle Physics. Lecture 1 What to expect. Physics 214 Experimental Particle Physics Lecture 1 What to expect. We ll start with a grand tour. I do not expect you to understand this tour in detail. Instead, think of it as an orientation to which

More information

SUPERSYMETRY FOR ASTROPHYSICISTS

SUPERSYMETRY FOR ASTROPHYSICISTS Dark Matter: From the Cosmos to the Laboratory SUPERSYMETRY FOR ASTROPHYSICISTS Jonathan Feng University of California, Irvine 29 Jul 1 Aug 2007 SLAC Summer Institute 30 Jul 1 Aug 07 Feng 1 Graphic: N.

More information

The Physics of Particles and Forces David Wilson

The 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 information

Astro-2: History of the Universe

Astro-2: History of the Universe Astro-2: History of the Universe Lecture 11; May 21 2013 Previously on astro-2 In an expanding universe the relationship between redshift and distance depends on the cosmological parameters (i.e. the geometry

More information

Elementary particles and typical scales in high energy physics

Elementary particles and typical scales in high energy physics Elementary particles and typical scales in high energy physics George Jorjadze Free University of Tbilisi Zielona Gora - 23.01.2017 GJ Elementary particles and typical scales in HEP Lecture 1 1/18 Contents

More information

Particle Physics Lectures Outline

Particle Physics Lectures Outline Subatomic Physics: Particle Physics Lectures Physics of the Large Hadron Collider (plus something about neutrino physics) 1 Particle Physics Lectures Outline 1 - Introduction The Standard Model of particle

More information

Hunting for the Higgs Boson. Ulrich Heintz Brown University

Hunting for the Higgs Boson. Ulrich Heintz Brown University Hunting for the Higgs Boson Ulrich Heintz Brown University the standard model electromagnetism acts on all charged particles strong force acts on all quarks weak force acts on all particles spin ½ spin

More information

PH5211: High Energy Physics. Prafulla Kumar Behera Room: HSB-304B

PH5211: High Energy Physics. Prafulla Kumar Behera Room: HSB-304B PH5211: High Energy Physics Prafulla Kumar Behera E-mail:behera@iitm.ac.in Room: HSB-304B Information Class timing: Wed. 11am, Thur. 9am, Fri. 8am The course will be graded as follows: 1 st quiz (20 marks)

More information

Physics 214 Experimental Particle Physics. Lecture 1 What to expect.

Physics 214 Experimental Particle Physics. Lecture 1 What to expect. Physics 214 Experimental Particle Physics Lecture 1 What to expect. We ll start with a grand tour. I do not expect you to understand this tour in detail. Instead, think of it as an orientation to which

More information

Chapter 46. Particle Physics and Cosmology

Chapter 46. Particle Physics and Cosmology Chapter 46 Particle Physics and Cosmology Atoms as Elementary Particles Atoms From the Greek for indivisible Were once thought to be the elementary particles Atom constituents Proton, neutron, and electron

More information

Gravity, Strings and Branes

Gravity, Strings and Branes Gravity, Strings and Branes Joaquim Gomis Universitat Barcelona Miami, 23 April 2009 Fundamental Forces Strong Weak Electromagnetism QCD Electroweak SM Gravity Standard Model Basic building blocks, quarks,

More information

SUSY Phenomenology & Experimental searches

SUSY Phenomenology & Experimental searches SUSY Phenomenology & Experimental searches Slides available at: Alex Tapper http://www.hep.ph.ic.ac.uk/~tapper/lecture.html Objectives - Know what Supersymmetry (SUSY) is - Understand qualitatively the

More information

Grand Unified theory, God Particle and the Missing Universe

Grand Unified theory, God Particle and the Missing Universe Grand Unified theory, God Particle and the Missing Universe Presented by Abraham A. Christian College Chengannur 5/18/2012 1 Warning What you will hear in this session may alter your perception of reality

More information

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

Democritus, a fifth century B.C. philosopher, is credited with being the first This paper will give a general overview of the current thoughts on the building blocks of atoms through the scope of the Standard Model. There will be an abridged explanation of the interactions that these

More information

Bosons in the Zoo of Elementary Particles

Bosons in the Zoo of Elementary Particles Bosons in the Zoo of Elementary Particles Daniele Sasso * Abstract In this paper we want to raise the question concerning the physical identity of bosons and the function that they perform in the Non-Standard

More information

Gravitinos, Reheating and the Matter-Antimatter Asymmetry of the Universe

Gravitinos, Reheating and the Matter-Antimatter Asymmetry of the Universe Gravitinos, Reheating and the Matter-Antimatter Asymmetry of the Universe Raghavan Rangarajan Physical Research Laboratory Ahmedabad with N. Sahu, A. Sarkar, N. Mahajan OUTLINE THE MATTER-ANTIMATTER ASYMMETRY

More information

PARTICLE PHYSICS COLUMBIA SCIENCE HONORS PROGRAM WEEK 7 OVERVIEW OF THE STANDARD MODEL (CONT ED) LIMITATIONS OF THE STANDARD MODEL

PARTICLE PHYSICS COLUMBIA SCIENCE HONORS PROGRAM WEEK 7 OVERVIEW OF THE STANDARD MODEL (CONT ED) LIMITATIONS OF THE STANDARD MODEL PARTICLE PHYSICS COLUMBIA SCIENCE HONORS PROGRAM WEEK 7 OVERVIEW OF THE STANDARD MODEL (CONT ED) LIMITATIONS OF THE STANDARD MODEL COURSE POLICIES Attendance Up to four excused absences Two with notes

More information

Electroweak Symmetry Breaking

Electroweak Symmetry Breaking Electroweak Symmetry Breaking An enduring mystery of the standard model of particle physics and how we hope to solve it David Schaich Department of Physics and Center for Computational Science Boston University

More information

The Building Blocks of Nature

The 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 information

Essential Physics II. Lecture 14:

Essential 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 information

The Particle Physics Odyssey [Where are we? Where are we going?]

The Particle Physics Odyssey [Where are we? Where are we going?] The Particle Physics Odyssey [Where are we? Where are we going?] The Particle Physics Odyssey [Where are we? Where are we going?] The Particle Physics Odyssey [Where are we? Where are we going?] Introduction

More information

Finish up our overview of small and large

Finish up our overview of small and large Finish up our overview of small and large Lecture 5 Limits of our knowledge Clicker practice quiz Some terminology... "Elementary particles" = objects that make up atoms (n,p,e) or are produced when atoms

More information

Lecture 18 - Beyond the Standard Model

Lecture 18 - Beyond the Standard Model Lecture 18 - Beyond the Standard Model Why is the Standard Model incomplete? Grand Unification Baryon and Lepton Number Violation More Higgs Bosons? Supersymmetry (SUSY) Experimental signatures for SUSY

More information

INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS

INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS Class Mechanics My office (for now): Dantziger B Room 121 My Phone: x85200 Office hours: Call ahead, or better yet, email... Even better than office

More information

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

Elementary 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 information

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

The 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 information

L23/24, part 1: let s end up with the story of relativity

L23/24, part 1: let s end up with the story of relativity L23/24, part 1: let s end up with the story of relativity Special relativity showed that space and time are not absolute Instead they are inextricably linked in a fourdimensional combination called spacetime

More information

Open Questions in Particle Physics. Carlos Wagner Physics Department, EFI and KICP, Univ. of Chicago HEP Division, Argonne National Laboratory

Open Questions in Particle Physics. Carlos Wagner Physics Department, EFI and KICP, Univ. of Chicago HEP Division, Argonne National Laboratory Open Questions in Particle Physics Carlos Wagner Physics Department, EFI and KICP, Univ. of Chicago HEP Division, Argonne National Laboratory Society of Physics Students, Univ. of Chicago, Nov. 21, 2016

More information

PARTICLE PHYSICS COLUMBIA SCIENCE HONORS PROGRAM WEEK 7 OVERVIEW OF THE STANDARD MODEL (CONT ED) LIMITATIONS OF THE STANDARD MODEL

PARTICLE PHYSICS COLUMBIA SCIENCE HONORS PROGRAM WEEK 7 OVERVIEW OF THE STANDARD MODEL (CONT ED) LIMITATIONS OF THE STANDARD MODEL PARTICLE PHYSICS COLUMBIA SCIENCE HONORS PROGRAM WEEK 7 OVERVIEW OF THE STANDARD MODEL (CONT ED) LIMITATIONS OF THE STANDARD MODEL COURSE POLICIES Attendance Up to four excused absences Two with notes

More information

The Higgs boson. Johann Collot Laboratoire de Physique Subatomique et de Cosmologie de Grenoble. Université Grenoble Alpes, CNRS/IN2P3

The Higgs boson. Johann Collot Laboratoire de Physique Subatomique et de Cosmologie de Grenoble. Université Grenoble Alpes, CNRS/IN2P3 The Higgs boson Johann Collot Laboratoire de Physique Subatomique et de Cosmologie de Grenoble Université Grenoble Alpes, CNRS/IN2P3 1 Higgs boson : a very simple particle No electrical charge No spin

More information

Chapter 27 The Early Universe Pearson Education, Inc.

Chapter 27 The Early Universe Pearson Education, Inc. Chapter 27 The Early Universe Units of Chapter 27 27.1 Back to the Big Bang 27.2 The Evolution of the Universe More on Fundamental Forces 27.3 The Formation of Nuclei and Atoms 27.4 The Inflationary Universe

More information

XI. Beyond the Standard Model

XI. Beyond the Standard Model XI. Beyond the Standard Model While the Standard Model appears to be confirmed in all ways, there are some unclear points and possible extensions: Why do the observed quarks and leptons have the masses

More information

Plasma Universe. The origin of CMB

Plasma Universe. The origin of CMB Plasma Universe As we go back in time, temperature goes up. T=2.73(1+z) K At z~1100, T~3000 K About the same temperature as M-dwarfs Ionization of hydrogen atoms H + photon! p + e - Inverse process: recombination

More information

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

Quantum 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 information

Contents. Objectives Newton s Laws preliminaries 1 st Law pushing things 2 nd Law 3 rd Law A Problem Fundamental Forces Fundamental Particles Recap

Contents. Objectives Newton s Laws preliminaries 1 st Law pushing things 2 nd Law 3 rd Law A Problem Fundamental Forces Fundamental Particles Recap Physics 121 for Majors Class 9 Newton s Laws Standard Model Last Class Matrices Classical boosts Lorentz boosts Space-time four-vectors Space and time problems in relativity Today s Class Newton s Laws

More information

Particles, Energy, and Our Mysterious Universe

Particles, Energy, and Our Mysterious Universe Particles, Energy, and Our Mysterious Universe 1 The End of Physics "The more important fundamental laws and facts of physical science have all been discovered, and these are now so firmly established

More information

Gravity, Strings and Branes

Gravity, Strings and Branes Gravity, Strings and Branes Joaquim Gomis International Francqui Chair Inaugural Lecture Leuven, 11 February 2005 Fundamental Forces Strong Weak Electromagnetism QCD Electroweak SM Gravity Standard Model

More information

Review Chap. 18: Particle Physics

Review Chap. 18: Particle Physics Final Exam: Sat. Dec. 18, 2:45-4:45 pm, 1300 Sterling Exam is cumulative, covering all material Review Chap. 18: Particle Physics Particles and fields: a new picture Quarks and leptons: the particle zoo

More information

Weak interactions and vector bosons

Weak interactions and vector bosons Weak interactions and vector bosons What do we know now about weak interactions? Theory of weak interactions Fermi's theory of weak interactions V-A theory Current - current theory, current algebra W and

More information

Flavor oscillations of solar neutrinos

Flavor oscillations of solar neutrinos Chapter 11 Flavor oscillations of solar neutrinos In the preceding chapter we discussed the internal structure of the Sun and suggested that neutrinos emitted by thermonuclear processes in the central

More information

The Standard Model and Beyond

The Standard Model and Beyond The Standard Model and Beyond Nobuchika Okada Department of Physics and Astronomy The University of Alabama 2011 BCVSPIN ADVANCED STUDY INSTITUTE IN PARTICLE PHYSICS AND COSMOLOGY Huê, Vietnam, 25-30,

More information

Einige interessante Aspekte der in der Zielsetzung genannten Fragestellungen. Appetithappen -> Antworten spaeter in der Vorlesung.

Einige interessante Aspekte der in der Zielsetzung genannten Fragestellungen. Appetithappen -> Antworten spaeter in der Vorlesung. 0. Einführung Einige interessante Aspekte der in der Zielsetzung genannten Fragestellungen. Appetithappen -> Antworten spaeter in der Vorlesung. Folien auf Englisch (aus anderer Vorlesung ausgeliehen)

More information

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

The Exchange Model. Lecture 2. Quantum Particles Experimental Signatures The Exchange Model Feynman Diagrams. Eram Rizvi The Exchange Model Lecture 2 Quantum Particles Experimental Signatures The Exchange Model Feynman Diagrams Eram Rizvi Royal Institution - London 14 th February 2012 Outline A Century of Particle Scattering

More information

F. TASNÁDI LINKÖPING UNIVERSITY THEORETICAL PHYSICS NEUTRINO OSCILLATIONS & MASS

F. TASNÁDI LINKÖPING UNIVERSITY THEORETICAL PHYSICS NEUTRINO OSCILLATIONS & MASS F. TASNÁDI LINKÖPING UNIVERSITY THEORETICAL PHYSICS NEUTRINO OSCILLATIONS & MASS the fundamental discoveries in physics con4nues 1 CONGRATULATIONS - NOBEL PRIZE IN PHYSICS 2016 the secrets of exotic matter

More information

Particle Physics. Dr Victoria Martin, Spring Semester 2012 Lecture 1: The Mysteries of Particle Physics, or Why should I take this course?

Particle Physics. Dr Victoria Martin, Spring Semester 2012 Lecture 1: The Mysteries of Particle Physics, or Why should I take this course? Particle Physics Dr Victoria Martin, Spring Semester 2012 Lecture 1: The Mysteries of Particle Physics, or Why should I take this course? Contents: Review of the Standard Model! What we know! What we don

More information

Truth and Beauty and the Physics of the Dark

Truth and Beauty and the Physics of the Dark Truth and Beauty and the Physics of the Dark Robert Kehoe QuarkNet Mtg. Aug. 2009 forces of nature Greece (atomism) India (vaisesika) China Zulu (amandala) Yoruba building blocks of matter structure of

More information

An Introduction to Modern Particle Physics

An Introduction to Modern Particle Physics An Introduction to Modern Particle Physics Mark Thomson University of Cambridge Y Z X Science Summer School: 30 th July - 1 st August 2007 1 Course Synopsis Introduction : Particles and Forces - what are

More information

Lecture 11. Weak interactions

Lecture 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 information

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

Origin of the Universe - 2 ASTR 2120 Sarazin. What does it all mean? Origin of the Universe - 2 ASTR 2120 Sarazin What does it all mean? Fundamental Questions in Cosmology 1. Why did the Big Bang occur? 2. Why is the Universe old? 3. Why is the Universe made of matter?

More information

The 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 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 information

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

Lecture PowerPoint. Chapter 32 Physics: Principles with Applications, 6 th edition Giancoli Lecture PowerPoint Chapter 32 Physics: Principles with Applications, 6 th edition Giancoli 2005 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the

More information

Introduction to Particle Physics and the Standard Model. Robert Clare UCR

Introduction to Particle Physics and the Standard Model. Robert Clare UCR Introduction to Particle Physics and the Standard Model Robert Clare UCR Timeline of particle physics Ancient Greeks Rutherford 1911 Rutherford Chadwick Heisenberg 1930 s Hofstader Gell-Mann Ne eman 1960

More information

Kiwoon Choi (KAIST) 3 rd GCOE Symposium Feb (Tohoku Univ.)

Kiwoon Choi (KAIST) 3 rd GCOE Symposium Feb (Tohoku Univ.) Exploring New Physics beyond the Standard Model of Particle Physics Kiwoon Choi (KAIST) 3 rd GCOE Symposium Feb. 2011 (Tohoku Univ.) We are confronting a critical moment of particle physics with the CERN

More information

Option 212: UNIT 2 Elementary Particles

Option 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 information

Particle Physics (concise summary) QuarkNet summer workshop June 24-28, 2013

Particle Physics (concise summary) QuarkNet summer workshop June 24-28, 2013 Particle Physics (concise summary) QuarkNet summer workshop June 24-28, 2013 1 Matter Particles Quarks: Leptons: Anti-matter Particles Anti-quarks: Anti-leptons: Hadrons Stable bound states of quarks Baryons:

More information