(and why it may one day save your life!)

Slides:



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

Garfield Graphics included with kind permission from PAWS Inc. All Rights Reserved. Strange Particles AS level Notes.
HEP Experiments Detectors and their Technologies Sascha Marc Schmeling CERN.
Antimatter: Past, Present & Future Presentation By Paramita Barai In Course Phys 6410: Introductory Nuclear and Particle Physics Instructor: Dr. Xiaochun.
The Asymmetry between Matter and Antimatter Besma M’charek FEW, Vrije Universiteit Amsterdam.
Laura Gilbert How We Study Particles. The basics of particle physics! Matter is all made up of particles… Fundamental particle: LEPTON Fundamental particles:
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE 3-Feb pm Physics LRA Dr Matt Burleigh Intro lecture 7-Feb-05.
Antimatter  The mass of a p is 938MeV/c 2 and its charge is +e. The mass of a  p is __ and its charge is ___ a ) 938MeV/c 2, +e b ) - 938MeV/c 2, +e.
PH 103 Dr. Cecilia Vogel Lecture 24 Review Outline  Nuclei  decay rate and number of nuclei  Matter Particles  leptons & quarks  More Particles.
Recreating the Big Bang with the Large Hadron Collider at CERN 1 Public Lecture – Jammu September 2013 Professor David Evans The University of Birmingham,
Particles energy states
Particles & Antiparticles
1 Oct 8 th, 2003Gerhard Raven CP violation: The difference between matter and antimatter Gerhard Raven Vrije Universiteit Amsterdam, Subatomic Physics.
The Production of Cold Antihydrogen w. A Brief History of Antimatter In 1928, Paul Dirac proposes antimatter with his work in relativistic quantum mechanics.
Elementary Particles: Physical Principles Benjamin Schumacher Physics April 2002.
Antimatter Mysteries 1 Rolf Landua Research physicist CERN.
Recreating the Big Bang with the World’s Largest Machine Prof Peter Watkins Head of Particle Physics Group The University of Birmingham Admissions Talk.
Jeopardy Jeopardy PHY101 Chapter 12 Review Study of Special Relativity Cheryl Dellai.
The BTeV Project at Fermilab Talk to DOE/Fermi Group Jan. 11, 2001 Introduction – Joel Butler Tracking detectors – David Christian Particle Identification.
Physics 6.5.
The Nucleus Nucleons- the particles inside the nucleus: protons & neutrons Total charge of the nucleus: the # of protons (z) times the elementary charge.
Atomic Physics – Part 3 Ongoing Theory Development To accompany Pearson Physics PowerPoint presentation by R. Schultz
SYNTHESIS Space-Time Revisited 1.Antimatter 2.Feynman Diagrams 3.Quantum Electrodynamics.
Introduction to CERN Activities
DISCOVERY OF THE NEUTRON
A photon with a wavelength of 2
High Energy Accelerators Dennis Silverman Physics and Astronomy U. C. Irvine.
ANTIMATTER Didsbury Scibar May 25 th 2009 Roger Barlow.
What are the Elementary Constituents of Matter? What are the forces that control their behaviour at the most basic level?
Antimatter Mysteries 1 Rolf Landua Research physicist - Head of Education CERN.
IoP Masterclass The Physics of Flavour at the Large Hadron Collider Tim Gershon University of Warwick March 30 th 2011.
IoP Masterclass The Physics of Flavour at the Large Hadron Collider Tim Gershon University of Warwick April 14 th 2010.
Overview. In Search of Giants Documentary Splitting the Atom Cockcroft and Walton shared the Nobel Prize for their work in splitting the atom.
IoP Masterclass B PHYSICS Tim Gershon University of Warwick March 18 th 2009.
NUCLEAR CHANGE.
Standard Model of Particle Physics
High Energy Particle Physics
Announcements Please fill out ECAFE online evaluations !!!
The Standard Model of Particle Physics
PHL424: 4 fundamental forces in nature
Introduction to CERN Activities
Particle Physics Lesson 6
Cold Antimatter at CERN
Introduction to CERN Activities
G. Arnison et al., UA1 Collaboration
A –Level Physics: Nuclear Physics Particle Classification
Particle Physics.
PHL424: Feynman diagrams 1. In this case a neutron decays to a proton, an electron and an anti-neutrino via the weak interaction.
The Beginning of Time (Birth Of The Universe)
PHL424: 4 fundamental forces in nature
Elementary particles Spring 2005, Physics /24/2018 Lecture XXV.
Search for Order Ancient Greeks: Aristotle Earth Air Fire Water
Particle Physics what do we know?
Particle Physics Part 1 -James Joyce Contents: Particle Accelerators
Particle physics.
Chapter 10 Radioactivity and Nuclear reactions
Subatomic Particles and Quantum Theory
What’s the matter with antimatter?
Dirac and Antimatter In 1927 Paul Dirac was working on the problem of combining the theory of the very small (quantum mechanics) with Einstein’s special.
Matter & Forces Matter Hadrons Leptons Forces
CMS Masterclass 2017.
RADIOACTIVITY B.Sc. 5th sem.
SEMINAR ON ANTI-MATTER
Early Universe.
Technician’s Notes Activity 10S Software Based 'Bubble chamber photographs'
Particle Physics Lesson 6
Modern Studies of the Atom
Fundamental Particles
Lesson 4: Forces and Bosons
Lesson 4: Forces and Bosons
Presentation transcript:

(and why it may one day save your life!) Matter ? Antimatter ? .… how to tell an alien from an anti-alien (and why it may one day save your life!) Richard Batley Particle Physics Masterclass Cavendish Lab, 21 - 22 April 2005

Antiparticles Cambridge, 1928 : The Dirac Equation Quantum Mechanics Special Relativity The Dirac Equation

the positron, e+ e- e+ Dirac’s equation predicted the existence of Same mass but opposite charge to e- e- e+

Discovery of the Positron Anderson, 1933 Cosmic ray track in cloud chamber: (trail of water droplets)

g + N  e+ + e- + N

e+e- pair creation is commonplace :

e+e- annihilation Use g  e+ + e- to produce positron beams e.g. LEP e+e- Collider at CERN Collide ~1011 e+ with ~1011 e- ( ~10-12 kg of e+ in lifetime of LEP )

OPAL experiment at LEP Collider e+ + e-  g + g OPAL experiment at LEP Collider Eg = 45 GeV

(e.g. fluorine doped glucose) The PET Scanner Inject a positron-emitting radioactive isotope : (e.g. fluorine doped glucose) study metabolic activity

e+ + e-  g + g Eg = mec2 = 511 keV

e+ + e-  m+ + m-

e+ + e-  W+ + W-

UA1 experiment at CERN SppS Collider p + p  Z0 + stuff e+ + e- UA1 experiment at CERN SppS Collider (1984)

Particle Antiparticle e- e+ ne ne p p u u u u d d p- p+ u u d d

Antiparticles Particles and antiparticles have : the same mass opposite charge and, if they are unstable : the same lifetime e.g. muons : Particles and antiparticles coexist on an equal footing in the Standard Model

Matter e- p n Antimatter e+ p n … but where is it ?

Neutral Kaons Neutral particles containing a strange quark or antiquark : K0 K0 s s d d “K-zero” “K-zero bar” Size : ~ 10-15 m Mass :

Discovery of K0 1946 Butler and Rochester Manchester K0  p+ + p-

KS and KL K0 K0 KS KL The neutral kaons can “mix” : s s d d The particles we see decaying are : KS KL “K-short” “K-long” Quantum mechanical mixtures of K0 and K0

A mechanical analogy …. K0 K0 KS KL

K0 K0

KS and KL have very different lifetimes : e.g. for a beam of energy 100 GeV : Average distance travelled before decay is KS : 5.4 m KL : 3.1 km The beam starts out as an equal mix of KS and KL Eventually: only K-long’s are left

DAPHNE “phi factory”, Frascati, Italy KS and KL in KLOE DAPHNE “phi factory”, Frascati, Italy

The NA48 Experiment K0 K0 K0 K0 KS KL + - Create a beam of neutral kaons …. proton beam B + secondary particles K0 target K0 - B (mixture) Let them decay …. K0 K0 (vacuum) (mixture) KS KL NA48 detector

The NA48 Detector

A different experiment The NA48 Experiment A different experiment (NA50)

Magnetic Spectrometer Detects charged particles Consists of 4 drift chambers …. …. and a magnet

LKr Electromagnetic Calorimeter Mainly for photons and electrons 10 m3 liquid krypton

More e+ than e- in K-long decays CP Violation The K-Long has revealed subtle differences between matter and antimatter For example, the decay occurs slightly (0.3%) more often than More e+ than e- in K-long decays  allows unambiguous definition of matter and antimatter

Contact is made with aliens …. The President of the World is sent to greet them ….

e+ + e-  g + g p + p  g + g, p + p, ... n + n  g + g, p + p, ... But are they aliens or anti-aliens ?? e+ + e-  g + g p + p  g + g, p + p, ... n + n  g + g, p + p, ... E = mc2 : D.Beckham + anti-alien  1019 Joules (1 Megaton of TNT = 4.2 x 1015 Joules)

In an Anti-world : In the NA48 experiment at CERN …. The neutral kaon beams starts out with opposite amounts of K0 and K0 But, just as in our world : the neutral kaon beam still starts out as an equal mix of KS and KL and eventually becomes pure K-long And, the decay still occurs slightly (0.3%) more often than

Our World An Anti-world p n e- more e+ than e- in K-long decays p n e+ DIFFERENT more e+ than e- in K-long decays An Anti-world p n e+ SAME more e+ than e- in K-long decays

~ 109 photons for every proton The Universe ~ 1080 protons ~ 0 antiprotons ~ 109 photons for every proton

The Big Bang the Universe was born with equal amounts of matter and antimatter (and B violation and phase transitions) CP violation : the Universe contains slightly more matter than antimatter Particles and anti- particles annihilate : the Universe contains only matter (and lots of photons)

and ~ 109 photons for every proton t ~ 1 msec : A hot, expanding “particle soup” : e+ , e- , g , p, p, n, n T ~ 1013 K with a small excess of particles : 109 + 1 protons 109 antiprotons After particle - antiparticle annihilation : p + p  g + g 1 proton antiprotons 2 x 109 photons Today : the Universe contains ~ 1080 protons and ~ 109 photons for every proton

Open Questions What is the origin of CP violation ? ( NA48, LHCb, …. ) Is the CP violation we see what is needed in the Big Bang ? Do aliens exist ? (or even anti-aliens ?)