Introduction to CERN David Barney, CERN Introduction to CERN Activities Intro to particle physics Accelerators – the LHC Detectors - CMS.

Slides:



Advertisements
Similar presentations
Bruce Kennedy, RAL PPD Particle Physics 2 Bruce Kennedy RAL PPD.
Advertisements

The search for the God Particle
Bruce Kennedy, RAL PPD Particle Physics 2 Bruce Kennedy RAL PPD.
Feb 6, 2003M. Fincke-Keeler, Univ. of Victoria Motivation A little bit of history Orders of magnitude Elementary particles Tools: Accelerators and Detectors.
Nuclear Physics Part 1: The Standard Model
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE  5-Feb pm Physics LRA Dr M Burleigh Intro lecture  9-Feb-04.
Laura Gilbert How We Study Particles. The basics of particle physics! Matter is all made up of particles… Fundamental particle: LEPTON Fundamental particles:
27 km ring Large Hadron Collider went online on Sept
Schlüsselexperimente der Elementarteilchenphysik:.
PH 103 Dr. Cecilia Vogel Lecture 24 From the particle adventure webpage.
8/5/2002Ulrich Heintz - Quarknet Particle Physics what do we know? Ulrich Heintz Boston University.
Elementary particles atom Hadrons Leptons Baryons Mesons Nucleons
Fundamental Particles (The Standard Model) Nathan Brown June 2007.
Particle Physics Intro. What’s Stuff Made Of…Really? All particles can be grouped into two categories: Fermions and Bosons Things to know about Fermions:
The Big Bang, the LHC and the Higgs Boson Dr Cormac O’ Raifeartaigh (WIT)
Christina Markert Physics Workshop UT Austin November Christina Markert The ‘Little Bang in the Laboratory’ – Accelorator Physics. Big Bang Quarks.
 Stable and unstable particles  How to observe them?  How to find their mass?  How to calculate their lifetime? 6/9/
Particle Physics at the Energy Frontier Tevatron → LHC & The Very Early Universe Tony LissAir Force Institute of TechnologyApril 10, 2008.
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE 26-Jan pm LRB Intro lecture 28-Jan pm LRBProblem solving.
ROY, D. (2011). Why Large Hadron Collider?. Pramana: Journal Of Physics, 76(5), doi: /s
Particle Physics J4 Leptons and the standard model.
The Higgs Boson: without the maths and jargon David Hall Graduate Seminar Series St Catherine’s College MCR 11 th May 2011.
My Chapter 30 Lecture.
Point 1 activities and perspectives Marzio Nessi ATLAS plenary 2 nd October 2004 Large Hadron Collider (LHC)
August 22, 2002UCI Quarknet The Higgs Particle Sarah D. Johnson University of La Verne August 22, 2002.
School of Arts & Sciences Dean’s Coffee Presentation SUNY Institute of Technology, February 4, 2005 High Energy Physics: An Overview of Objectives, Challenges.
LHC and Search for Higgs Boson Farhang Amiri Physics Department Weber State University Farhang Amiri Physics Department Weber State University.
From Luigi DiLella, Summer Student Program
Quarks, Leptons and the Big Bang particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.
Particle Physics Quiz EPPOG Hands on Particle Physics Masterclasses 2011.
Jeopardy Jeopardy PHY101 Chapter 12 Review Study of Special Relativity Cheryl Dellai.
Fisica Generale - Alan Giambattista, Betty McCarty Richardson Copyright © 2008 – The McGraw-Hill Companies s.r.l. 1 Chapter 30: Particle Physics Fundamental.
A singularity formed by a previous collapsed Universe? Multiple Universes? We just don’t know… YET What Caused It?
ATLAS experiment at the CERN Large Hadron Collider Peter Watkins, Head of Particle Physics Group, University of Birmingham, UK
Aim: How can we explain the four fundamental forces and the standard model? Do Now: List all the subatomic particles that you can think of.
P ARTICLE D ETECTORS Mojtaba Mohammadi IPM-CMPP- February
© John Parkinson 1 e+e+ e-e- ANNIHILATION © John Parkinson 2 Atom 1x m n n n n Nucleus 1x m U Quarks 1x m U D ? ? ?
The Nucleus Nucleons- the particles inside the nucleus: protons & neutrons Total charge of the nucleus: the # of protons (z) times the elementary charge.
Modern Physics. Reinventing Gravity  Einstein’s Theory of Special Relativity  Theorizes the space time fabric.  Describes why matter interacts.  The.
Introduction to CERN Activities
1 Methods of Experimental Particle Physics Alexei Safonov Lecture #15.
CERN, 8 February, 2001 Egil Lillestøl, CERN & Univ. of Bergen Lectures recorded at :
SYNTHESIS The Standard Model 1.Elementary particles 2.Strong nuclear force 3.Weak nuclear force 4.The Standard Model.
1 Particle Physics, The Mysteries of the Universe, and The LHC Nhan Tran Johns Hopkins University.
What is the Standard Model of Particle Physics ???? 1. A theory of three of the four known fundamental interactions and the elementary particles that.
Particle Detectors January 18, 2011 Kevin Stenson.
1 LHCb CMS ALICE ATLAS The ATLAS experiment at the LHC 27 km.
1 Experimental Particle Physics PHYS6011 Fergus Wilson, RAL 1.Introduction & Accelerators 2.Particle Interactions and Detectors (2) 3.Collider Experiments.
Phy107 Fall From Last Time… Particles are quanta of a quantum field –Often called excitations of the associated field –Particles can appear and.
10/29/2007Julia VelkovskaPHY 340a Lecture 4: Last time we talked about deep- inelastic scattering and the evidence of quarks Next time we will talk about.
Higgs in the Large Hadron Collider Joe Mitchell Advisor: Dr. Chung Kao.
LHC LARGE HADRON COLLIDER World’s largest and highest-energy particle accelerator. Built by the European Organization for Nuclear Research(CERN). To study.
 All elementary particles in physics are classified as either fermions or bosons. Quantum physics demonstrates the particles may have an intrinsic non-zero.
The Standard Model of Particle Physics
Introduction to CERN Activities
Introduction to CERN Activities
The Standard Model strong nuclear force electromagnetic force
Aim: How can we describe Fundamental Particles?
Exploration and Challenges at the Large Hadron Collider
Elementary particles Spring 2005, Physics /24/2018 Lecture XXV.
Particle Physics what do we know?
Particle physics.
SPH4U Elementary Particles.
Subatomic Particles and Quantum Theory
Do Now An electron in a hydrogen atoms drops from n=5 to n=4 energy level. What is the energy of the photon in eV? What is the frequency of the emitted.
Experimental Particle Physics PHYS6011 Putting it all together Lecture 4 6th May 2009 Fergus Wilson, RAL.
CMS Masterclass 2017.
Experimental Particle Physics PHYS6011 Putting it all together Lecture 4 28th April 2008 Fergus Wilson. RAL.
Modern Studies of the Atom
Physics 4 – April 18, 2019 Agenda:
Presentation transcript:

Introduction to CERN David Barney, CERN Introduction to CERN Activities Intro to particle physics Accelerators – the LHC Detectors - CMS

Introduction to CERN David Barney, CERN From atoms to quarks I

Introduction to CERN David Barney, CERN From atoms to quarks II Hadrons are made of quarks, e.g. p = uud  0 = uds  0 b = udb  + = ud  = cc  = bb Baryons Mesons Leptons are fundamental e.g. electron muon neutrinos

Introduction to CERN David Barney, CERN The structure of the Proton Proton is not, in fact, simply made from three quarks (uud) There are actually 3 “valence” quarks (uud) + a “sea” of gluons and short-lived quark-antiquark pairs

Introduction to CERN David Barney, CERN Matter and Force Particles Gluons (8) Quarks Mesons Baryons Nuclei Graviton ? Bosons (W,Z) Atoms Light Chemistry Electronics Solar system Galaxies Black holes Neutron decay Beta radioactivity Neutrino interactions Burning of the sun Strong Photon Gravitational Weak The particle drawings are simple artistic representations Electromagnetic Tau Muon Electron Tau Neutrino Muon Neutrino Electron Neutrino Bottom Strange Down Top Charm Up 2/3 -1/3 each quark: R, B, G 3 colours Quarks Electric Charge Leptons Electric Charge

Introduction to CERN David Barney, CERN Characteristics of the 4 forces Ratio of electrical to gravitational force between two protons is ~ !! Can such different forces have the same origin ?? Interaction Exchanged Range Relative Examples quantum(m)Strengthin nature (source ch) Stronggluon proton (quarks) colour Electromagneticphoton<10 -2 atoms electric WeakW, Z< radioactivity hypercharge Gravitygraviton ? solar system mass What characterizes a force ? Strength, range and source charge of the field.

Introduction to CERN David Barney, CERN Unification of fundamental forces

Introduction to CERN David Barney, CERN Unanswered questions in Particle Physics a. Can gravity be included in a theory with the other three interactions ? b. What is the origin of mass?  LHC c. How many space-time dimensions do we live in ? d. Are the particles fundamental or do they possess structure ? e. Why is the charge on the electron equal and opposite to that on the proton? f. Why are there three generations of quark and lepton ? g. Why is there overwhelmingly more matter than anti-matter in the Universe ? h. Are protons unstable ? i. What is the nature of the dark matter that pervades our galaxy ? j. Are there new states of matter at exceedingly high density and temperature? k. Do the neutrinos have mass, and if so why are they so light ?

Introduction to CERN David Barney, CERN The Standard Model Where is Gravity? M e ~ 0.5 MeV M ~ 0 M t ~ 175,000 MeV! M  = 0 M Z ~ 100,000 MeV Why ?

Introduction to CERN David Barney, CERN Mathematical consistency of the SM

Introduction to CERN David Barney, CERN What is wrong with the SM?

Introduction to CERN David Barney, CERN Origin of mass and the Higgs mechanism Simplest theory – all particles are massless !! A field pervades the universe Particles interacting with this field acquire mass – stronger the interaction larger the mass The field is a quantum field – the quantum is the Higgs boson Finding the Higgs establishes the presence of the field

Introduction to CERN David Barney, CERN CERN Site LHC CERN Site (Meyrin) SPS

Introduction to CERN David Barney, CERN CERN Member States

Introduction to CERN David Barney, CERN CERN Users

Introduction to CERN David Barney, CERN Particle Collider

Introduction to CERN David Barney, CERN Types of Particle Collider Electron-Positron Collider (e.g. LEP) e-e- e+e+ E collision = E e- + E e+ = 2 E beam e.g. in LEP, E collision ~ 90 GeV = m Z i.e. can tune beam energy so that you always produce a desired particle! Electrons are elementary particles, so Proton-Proton Collider (e.g. LHC) u u d u u d E proton1 = E d1 + E u1 + E u2 + E gluons1 E proton2 = E d2 + E u3 + E u4 + E gluons2 Collision could be between quarks or gluons, so 0 < E collision < (E proton1 + E proton2 ) i.e. with a single beam energy you can “search” for particles of unknown mass!

Introduction to CERN David Barney, CERN CERN Accelerator Complex

Introduction to CERN David Barney, CERN Collisions at the Large Hadron Collider Bunch Crossing 4x10 7 Hz 7x10 12 eV Beam Energy cm -2 s -1 Luminosity 2835Bunches/Beam Protons/Bunch 7 TeV Proton colliding beams Proton Collisions 10 9 Hz Parton Collisions New Particle Production 10 5 Hz (Higgs, SUSY,....) p p H µ + µ - µ + µ - Z Z pp e - e     q q q q  1 - g ~ ~  2 0 ~ q ~  1 0 ~ 7.5 m (25 ns)

Introduction to CERN David Barney, CERN LHC Detectors B-physics CP Violation Heavy Ions Quark-gluon plasma General-purpose Higgs SUSY ?? General-purpose Higgs SUSY ??

Introduction to CERN David Barney, CERN The two Giants!

Introduction to CERN David Barney, CERN Particle Detectors I Cannot directly “see” the collisions/decays –Interaction rate is too high –Lifetimes of particles of interest are too small Even moving at the speed of light, some particles (e.g. Higgs) may only travel a few mm (or less) Must infer what happened by observing long-lived particles –Need to identify the visible long-lived particles Measure their momenta Energy (speed) –Infer the presence of neutrinos and other invisible particles Conservation laws – measure missing energy

Introduction to CERN David Barney, CERN Particle Momentum Measurement Electrically charged particles moving in a magnetic field curve Radius of curvature is related to the particle momentum –R = p/0.3B Should not disturb the passage of the particles Low-mass detectors sensitive to the passage of charged particles Many layers – join the dots! E.g. CMS silicon tracker Electron In CMS

Introduction to CERN David Barney, CERN Energy Measurement - Calorimeters Idea is to “stop” the particles and measure energy deposit Particles stop via energy loss processes that produce a “shower” of many charged and neutral particles – pair-production, bremstrahlung etc. Detector can be to measure either hadrons or electrons/photons Two main types of calorimeter: –Homogeneous: shower medium is also used to produce the “signal” that is measured – e.g. CMS electromagnetic calorimeter –Sampling: the shower develops in one medium, whilst another is used to produce a signal proportional to the incident particle energy – e.g. CMS Hadron Calorimeter

Introduction to CERN David Barney, CERN Particle interactions in detectors

Introduction to CERN David Barney, CERN CMS – Compact Muon Solenoid

Introduction to CERN David Barney, CERN CMS – Compact Muon Solenoid

Introduction to CERN David Barney, CERN Puzzle

Introduction to CERN David Barney, CERN Answer Make a “cut” on the Transverse momentum Of the tracks: p T >2 GeV