IoP Masterclass. The Physics of Flavour at the Large Hadron Collider. Tim Gershon University of Warwick March 30th 2011

Similar documents
IoP Masterclass. The Physics of Flavour at the Large Hadron Collider. Tim Gershon University of Warwick April

IoP Masterclass B PHYSICS. Tim Gershon University of Warwick March 18 th 2009

IoP Masterclass FLAVOUR PHYSICS. Tim Gershon, University of Warwick April 20 th 2007

Warwick particle physics masterclass 19 March 2014

Matter, Antimatter and the Strangeness of CP violation

Frontier Science: The mystery of Antimatter

e + e - (1) Silicon Vertex Detector

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

Analyzing CMS events

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

Weak Interactions. The Theory of GLASHOW, SALAM and WEINBERG

Lecture 11. Weak interactions

An Introduction to Particle Physics

Elementary Particles, Flavour Physics and all that...

Understanding the balance of matter and antimatter in the Universe

What is matter and how is it formed?

Frontier Particle Accelerators

Quarks and the Cosmos

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

Finish up our overview of small and large

New subatomic particle and the Electro-Strong and -Weak Interaction

Modern physics 1 Chapter 13

LHCb Overview. Barbara Storaci on behalf of the LHCb Collaboration

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

(Heavy Quark) Flavour Physics at LHC

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

CP Violation and Flavor Mixing C O L I N G L E A S O N

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

Observation of a New Particle with a Mass of 125 GeV

Outline. Charged Leptonic Weak Interaction. Charged Weak Interactions of Quarks. Neutral Weak Interaction. Electroweak Unification

the quest for certainty

The physics of elementary particles

Particle physics today. Giulia Zanderighi (CERN & University of Oxford)

The Standard Model of Particle Physics - I

Particle + Physics at ATLAS and the Large Hadron Coillder

1. Introduction. Particle and Nuclear Physics. Dr. Tina Potter. Dr. Tina Potter 1. Introduction 1

Oddelek za fiziko. Top quark physics. Seminar. Author: Tina Šfiligoj. Mentor: prof. dr. Svjetlana Fajfer. Ljubljana, february 2012

Lecture 10: Weak Interaction. 1

The Start of the LHC Era. Peter Wittich Laboratory of Elementary Particle Physics Cornell University

STFC Meet the buyer: CERN experiments and future projects

8.882 LHC Physics. High Energy Physics Overview. [Lecture 16, April 6, 2009] Experimental Methods and Measurements

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

The Physics of Particles and Forces David Wilson

Outline. Charged Leptonic Weak Interaction. Charged Weak Interactions of Quarks. Neutral Weak Interaction. Electroweak Unification

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

Reminder : scenarios of light new physics

Last Friday: pp(bar) Physics Intro, the TeVatron

Parity violation. no left-handed ν$ are produced

ANTIMATTER MATTER. does the difference between matter and antimatter arise?

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

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

The LHCb experiment at Cern

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

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

CP/ Andreas Meyer. Hamburg University. DESY Summer Student Lectures, 1+4 August 2003 (this file including slides not shown in the lecture) Part 1

The Large Hadron Collider, and New Avenues in Elementary Particle Physics. Gerard t Hooft, Public Lecture, IPMU Tokyo, April 16, 2015

Unsolved Problems in Theoretical Physics V. BASHIRY CYPRUS INTRNATIONAL UNIVERSITY

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

OUTLINE. CHARGED LEPTONIC WEAK INTERACTION - Decay of the Muon - Decay of the Neutron - Decay of the Pion

Brief Report from the Tevatron. 1 Introduction. Manfred Paulini Lawrence Berkeley National Laboratory Berkeley, California 94720

Flavour Physics in the LHC Era

Lecture 18 - Beyond the Standard Model

The Particle World. This talk: What is our Universe made of? Where does it come from? Why does it behave the way it does?

MINERVA Masterclass. Teachers Manual. Vera Zimanyine Horvath Francesco Mezzanotte Tom Lambert

Particle Physics. Tommy Ohlsson. Theoretical Particle Physics, Department of Physics, KTH Royal Institute of Technology, Stockholm, Sweden

Optimizing Selection and Sensitivity Results for VV->lvqq, 6.5 pb -1, 13 TeV Data

Particle Physics WS 09/10

BACKGROUND LHC Physics Program Summary LHC PHYSICS. Andrés G. Delannoy 1. 1 Vanderbilt University. 2014/07/21 1

Where is Europe going?

Neutrino Masses & Flavor Mixing 邢志忠. Zhi-zhong Xing. (IHEP, Winter School 2010, Styria, Austria. Lecture B

Large Hadron Collider at CERN

Particle Physics Columbia Science Honors Program

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

LHC & ATLAS. The largest particle physics experiment in the world. Vincent Hedberg - Lund University 1

Yiming Li (LAL, Orsay) On behalf of the LHCb and MoEDAL collaborations

Lecture 8. CPT theorem and CP violation

FYS3510 Subatomic Physics. Exam 2016

This content has been downloaded from IOPscience. Please scroll down to see the full text.

(a) (b) Fig. 1 - The LEP/LHC tunnel map and (b) the CERN accelerator system.

Higgs boson may appear to be a technihiggs

FYS3510 Subatomic Physics. Exam 2016

Wolfgang Pauli, CERN, and the LHC. Rüdiger Voss Physics Department, CERN

Weak interactions, parity, helicity

\ \ \/ \\// (o) (o) U. February 11, UT Saturday Morning Physics. Yuri Kamyshkov University of Tennessee

The first 400,000 years

First some Introductory Stuff => On The Web.

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

1. What does this poster contain?

Today. The nature of the Universe - Beyond the Standard Model

Today. The goals of science. The nature of the Universe - Beyond the Standard Model

Standard Model & Beyond

A Search for the Higgs

LHC Signal Cracks the Standard Model

Baryogenesis and Particle Antiparticle Oscillations

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

Fundamental Particles

A fantastic experiment

E = mc 2 Opening Windows on the World

Modern experiments - ATLAS

Accelerators. Acceleration mechanism always electromagnetic Start with what s available: e - or p Significant differences between accelerators of

Transcription:

IoP Masterclass The Physics of Flavour at the Large Hadron Collider Tim Gershon University of Warwick March 30th 2011

The Standard Model 2

Some Questions What is antimatter? Why are there three colours of quarks? Why are there so many bosons? These questions have well-understood answers 3

Some More Questions Why are there so many fermions? Why are there three generations of both quarks and leptons? ( flavour ) Why are matter and antimatter different? ( CP violation ) We do not know the answers to these questions! 4

Matter vs. antimatter In the Big Bang, matter and antimatter should have been produced in equal quantities In the Universe today, we observe only matter need CP violation 5

Asymmetry of the Universe Paul Dirac, one of the greatest British physicists of all time, won the 1933 Nobel Prize for his prediction of the existence of antimatter In his Nobel lecture, Dirac concludes:... we must regard it rather as an accident that [the solar system] contains a preponderance of negative electrons and positive protons. It is quite possible that for some of the stars it is the other way about, these stars being built up mainly of positrons and negative protons. In fact, there may be half the stars of each kind. It turns out there are not any antimatter stars Dirac did not know about CP violation! 6

What is CP Violation? Symmetries are powerful tools to understand nature Two important discrete symmetries are C : charge conjugation (exchange particle and antiparticle) P : parity (mirror transform all spatial coordinates) Need violation of combined CP symmetry to distinguish absolutely between matter & antimatter 7

CP Symmetry P CP C Combined CP transformation pictures look the same Illustrated using the images of MC Escher 8

CP Violation P CP C Combined CP transformation pictures look different! Illustrated using the images of MC Escher 9

The CKM Matrix Quark mixing described by Cabibbo-Kobayashi-Maskawa matrix d' s' ' b = V CKM down-type quarks as seen by the weak interaction d s b physical down-type quarks (with well-defined masses) Matrix elements are complex numbers interactions of quarks and antiquarks can be different CP violation! Makoto Kobayashi Nobel Prize in Physics 2008 Toshihide Maskawa 10

B Physics at the LHC CP violation appears to be central to understanding the questions discussed above eg. as shown by Kobayashi & Maskawa (1973), need at least three generations for CP violation to occur Kobayashi-Maskawa mechanism predicts large CP violation effects in particles containing b quarks need dedicated experiments to test KM predictions Exploit copious production of b quarks at the CERN Large Hadron Collider LHCb experiment 11

The LHC at CERN The world's largest machine Located at CERN laboratory near Geneva 26 659 m circumference Emptier (10 13 atm) and colder (1.9 K = 271.3 C) than outer space 1232 superconducting dipole magnets (8.33 T) Total cost ~ 5 billion Main CERN site Geneva LHCb experiment Geneva airport 12

LHC dipole magnets 13

Will the LHC destroy the earth? No! 14

LHC performance Important measures Energy Currently 1/2 design maximum Luminosity Currently ~2/100 design maximum (at the LHCb design luminosity) Still very early days for LHC 2011 performance so far very promising... 15

The LHCb Experiment Searching for new sources of CP violation compare matter and antimatter look for disagreement with Standard Model predictions search for unexpected effects Requires an ultra-high precision detector operated by a collaboration of 700 physicists 16

The LHCb Vertex Locator Need to precisely measure B hadrons decay positions put silicon detectors as close as possible to the beam 42 modules inner radius : 7 mm inside LHC vacuum system 17

Just one result... B 0 K B 0 K red lines signal, i.e. real B decays other colours different types of background processes dark blue lines sum of everything points with error bars events selected from 35/pb of LHCb 2010 data 0 first signs of CP violation at the LHC! We seem to see more B0 than B 18

Summary Studies of B physics provide excellent opportunities to address one of the biggest questions about our Universe By learning more about B physics and CP violation we hope to find clues about the theoretical structure of the Standard Model (and any theories beyond it) What causes the excess of matter over antimatter? Why are there three generations of quarks and leptons? The Warwick group is actively involved in experiments at the forefront of this exciting area of research We hope the LHCb experiment will provide some answers! 19

Can the LHC be used to make antimatter bombs? No! 20