Particle Physics and the structure of Space, Time and Matter Tuesday 20 th March Prof.

Slides:



Advertisements
Similar presentations
The search for the God Particle
Advertisements

Chapter 17 The Beginning of Time
ORIGIN OF THE UNIVERSE P In the beginning, God created the heaven and the earth; and the earth was without form and void; and darkness was upon the face.
Cosmology The Origin and Future of the Universe Part 2 From the Big Bang to Today.
Big Bang …..was actually very small and quiet. Atoms are mostly empty space.
Age, Evolution, and Size of the Cosmos Szydagis and Lunin.
Neutrino Physics - Lecture 1 Steve Elliott LANL Staff Member UNM Adjunct Professor ,
Advances in contemporary physics and astronomy --- our current understanding of the Universe Lecture 5: Evolution of Early Universe April 30 th, 2003.
Schlüsselexperimente der Elementarteilchenphysik:.
Particle Physics: Adventures in the Quantum Wonderland Ken Peach (John Adams Institute.
© 2010 Pearson Education, Inc. Chapter 23 The Beginning of Time.
Modern Physics LECTURE II.
Aug 28, 2014 Joao Varela. Outline of the lecture The Higgs field Unsolved mysteries Beyond the Standard Model Dark matter and dark energy What else could.
Background radiation (light) from Big Bang (visible) freely streaming from universe since atoms formed at temperature ~ 3,000 K (cf. sun = 6000 K)
Fundamental Particles (The Standard Model) Nathan Brown June 2007.
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.
The Standard Model and Beyond Harrison B. Prosper 6 July, 2010 Fermilab Summer Lecture Series.
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.
Discovery of the Higgs Boson Gavin Lawes Department of Physics and Astronomy.
ROY, D. (2011). Why Large Hadron Collider?. Pramana: Journal Of Physics, 76(5), doi: /s
My Chapter 30 Lecture.
Hubble’s Law Our goals for learning What is Hubble’s Law?
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.
Quarks, Leptons and the Big Bang particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.
Intro to Cosmology! OR What is our Universe?. The Latest High Resolution Image of the Cosmic Microwave Background Radiation Low Energy RegionHigh Energy.
Happyphysics.com Physics Lecture Resources Prof. Mineesh Gulati Head-Physics Wing Happy Model Hr. Sec. School, Udhampur, J&K Website: happyphysics.com.
The Energy in our Universe Dr. Darrel Smith Department of Physics.
AS2001 / 2101 Chemical Evolution of the Universe Keith Horne Room 315A
The Universe  What do we know about it  age: 14.6 billion years  Evolved from Big Bang  chemical composition  Structures.
Recreating the Big Bang with the World’s Largest Machine Prof Peter Watkins Head of Particle Physics Group The University of Birmingham Admissions Talk.
AS2001 Chemical Evolution of the Universe Keith Horne 315a
Jeopardy Jeopardy PHY101 Chapter 12 Review Study of Special Relativity Cheryl Dellai.
Introduction to CERN David Barney, CERN Introduction to CERN Activities Intro to particle physics Accelerators – the LHC Detectors - CMS.
Fisica Generale - Alan Giambattista, Betty McCarty Richardson Copyright © 2008 – The McGraw-Hill Companies s.r.l. 1 Chapter 30: Particle Physics Fundamental.
Introduction to Particle Physics How to compute the Universe?
SubAtomic Physics & Astrophysics Intimate Connexion between Very Large and Very Small.
The Life of the Universe From Beginning to End.
Chapter 17 The Beginning of Time. Running the Expansion Backward Temperature of the Universe from the Big Bang to the present (10 10 years ~ 3 x
Re-creating the Big Bang Experiments at the Large Hadron Collider Dr Cormac O’ Raifeartaigh (WIT) Albert Einstein Ernest Walton.
The Beginning of Time: Evidence for the Big Bang & the Theory of Inflation.
Introduction to CERN Activities
The Higgs Boson Observation (probably) Not just another fundamental particle… July 27, 2012Purdue QuarkNet Summer Workshop1 Matthew Jones Purdue University.
CERN, 8 February, 2001 Egil Lillestøl, CERN & Univ. of Bergen Lectures recorded at :
Lecture 2: The First Second Baryogenisis: origin of neutrons and protons Hot Big Bang Expanding and cooling “Pair Soup” free particle + anti-particle pairs.
Introduction to Particle Physics Saturday July 3 rd 2010 APPEAL, Oxford Prof. Ken Peach.
Phys 102 – Lecture 28 Life, the universe, and everything 1.
Searching for New Matter with the D0 Experiment Todd Adams Department of Physics Florida State University September 19, 2004.
H. Quarks – “the building blocks of the Universe” The number of quarks increased with discoveries of new particles and have reached 6 For unknown reasons.
1 The Standard Model of Particle Physics Owen Long U. C. Riverside March 1, 2014.
1 LHCb CMS ALICE ATLAS The ATLAS experiment at the LHC 27 km.
CERN Richard Jacobsson 1 Welcome to CERN!. CERN Richard Jacobsson 2 What is CERN? l European Organization for Nuclear Research, founded in 1954 l Currently.
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.
© 2014 Pearson Education, Inc. Building Blocks of the Universe.
Standard Model of Particle Physics
The Standard Model of Particle Physics
Introduction to CERN Activities
Introduction to CERN Activities
Universe! Early Universe.
The Beginning of Time (Birth Of The Universe)
Particle Physics what do we know?
Particle Physics and The Standard Model
SPH4U Elementary Particles.
Ichep.
Lecture 2: The First Second origin of neutrons and protons
Presentation transcript:

Particle Physics and the structure of Space, Time and Matter Tuesday 20 th March Prof. Ken Peach University of Oxford & Royal Holloway University of London

Ken PeachJohn Adams Institute20 March What is ‘Particle Physics’? The Particle Physics (or ‘High Energy Physics’) ‘Mission’ –identify the fundamental constituents of matter –describe the interactions (forces) between them A long and honourable history –Constituents ‘Earth, Fire, Air and Water’ of the Greeks ‘Atoms’ of Democretus and Lucretius –Forces Gravity (Newton) Electricity (Coulomb) A significant achievement of the 20 th century –The electron (JJ Thomson, 1897) –The top quark (CDF & D0, 1995) –QED, QCD, electro-weak (gravity)

Ken PeachJohn Adams Institute20 March Probing Inner Space 3 basic ways Look at it Heat it Smash it Wavelength Temperature TEnergy E h c/ =kTE=

Ken PeachJohn Adams Institute20 March Remarkable comment All three the same fundamental physics! Uses ‘light’ Uses ‘heat’ TUses ‘probe’ E h c/ =kTE= Photons ‘Photons’        

Ken PeachJohn Adams Institute20 March Scattered electronScattered lepton ConstituentsConstituents Particle Hammers proton electron { ProtonfragmentsProtonfragments Scattered ‘parton’ PhotonPhoton, W, Z

Ken PeachJohn Adams Institute20 March HiggsBosonHiggsBoson? Force Carriers Z Z boson W W boson  photon g gluon Generations of matter Generations of matter  tau   -neutrino b bottom t top III  muon   -neutrino s strange c charm II e electron e e-neutrino d down up uI Leptons Quarks Particles and their Interactions Each with its own ‘antiparticle’ © Brian Foster

Ken PeachJohn Adams Institute20 March The Particle Physicists “Periodic Table”

Ken PeachJohn Adams Institute20 March The Particle Physicist’s “Periodic Table” u u d d d u Proton Neutron The Chemist’s Periodic Table

Ken PeachJohn Adams Institute20 March The Standard Model The Parameters 6 quark masses –m u, m c, m t –m d, m s, m b 3 lepton masses –m e, m , m  2 vector boson masses –M w, M Z (m , m g =0) 1 Higgs mass –Mh–Mh 3 coupling constants –G F, ,  s 3 quark mixing angles –  12,  23,  13 1 quark phase – –  Neutrino masses set to 0!

Ken PeachJohn Adams Institute20 March What still remains to be done? The origin of mass –“Hunting the Higgs” The origin of the forces –Strong, electro-weak & gravity, or just one fundamental force The origin of “Dark Matter” (& Dark Energy) –Accounting for most of the mass of the universe The origin of cosmological matter-antimatter asymmetry –Why does the universe today consist only of matter, not equal amounts of matter and antimatter Fundamental questions in particle physics that are equally fundamental questions in cosmology

Ken PeachJohn Adams Institute20 March How do we know all this? © CERN Matter & antimatter annihilate into energy Go to the highest energy See what happens Energy (MeV) ,000 10,000 1, e u,d s  c b  W Z t leptons quarks Weak Bosons Higgs?

Ken PeachJohn Adams Institute20 March CERN from Space

Ken PeachJohn Adams Institute20 March Arial view of the CERN site © CERN

Ken PeachJohn Adams Institute20 March … and what is beneath the surface © CERN

Ken PeachJohn Adams Institute20 March ALEPH A detector for LEP Physics © CERN & PPARC

Ken PeachJohn Adams Institute20 March Some events Ze+e-Ze+e- Z+-Z+- Z   +  - ZqqZqq

Ken PeachJohn Adams Institute20 March More (complicated) events Z   +  -  Z  qqg Z  4 ‘jets’ e+e-W+W-e+e-W+W-

Ken PeachJohn Adams Institute20 March The Large Hadron Collider ATLAS CMS

Ken PeachJohn Adams Institute20 March The problem of mass The Standard Model relies on –Relativity +Quantum mechanics Relativistic Quantum Field Theory –Each particle has an associated all-pervasive ‘field’  (x,t) –Symmetry There is no ‘special place’ in the Universe There are no ‘preferred directions’ in space-time There is ‘local autonomy’ for the particle fields –Produces a beautiful theory –… with all particles massless! Adding mass violates the beautiful symmetries The Higgs Mechanism –Fill space-time with another (Higgs) field  (x,t) A new type of force with special properties –… that give mass to the particles …and leaves a signature behind …– the Higgs Boson!

Ken PeachJohn Adams Institute20 March … but look what we have done to ‘empty space’ It is filled with these ‘fields’

Ken PeachJohn Adams Institute20 March Origin of Mass ? m=0, v = speed of light No Higgs field 00 00H H H H V 0 With Higgs field

Ken PeachJohn Adams Institute20 March From microscopes to telescopes …

Ken PeachJohn Adams Institute20 March The biggest challenge … the Creation of the Universe! The Big Bang

Ken PeachJohn Adams Institute20 March From the Big Bang to today © CERN

Ken PeachJohn Adams Institute20 March Galaxy formation The state of the Universe Time (sec) Temperature ( o K) The Big Bang Biology Solar System forms Atoms form Chemistry begins Today 3 x s 3 o K Neutron lifetime nucleosynthesis Protons, neutrons & nuclei form W & Z production Particle physics

Ken PeachJohn Adams Institute20 March Particle Physics and Cosmology The Higgs potential … Primordial ripples Fundamental mode Geometry Potential wells compression baryons Rarefaction… etc WMAP Data, Verde, LP03 the particle spectrum … and the unknown … Illustrations from Muryama, LP03 should explain

Ken PeachJohn Adams Institute20 March What is the Vacuum? Dictionary Definitions: An entirely (or very nearly) empty space Chambers 20 th Century 1.Emptiness of space; space unoccupied by matter 2.(a) A space entirely empty of matter (b) A space empty of air, esp. one from which the air has been artificially withdrawn 3.An empty space; a portion of space (left) unoccupied or unfilled with the usual or natural contents OED My definition: That which remains when everything else is taken away

Ken PeachJohn Adams Institute20 March New physics scale Note: The vacuum ‘knows’ about particles already found … and all of the particles still to be found!  i -1 Log 10 [Energy Scale (GeV)] No Grand Unification Unification ! “e/m” “weak” “strong” Supersymmetry? Evolution of the strength of the interactions with increasing energy  3 -1  2 -1  1 -1

Ken PeachJohn Adams Institute20 March The Cosmic Recipe 1.The Hubble Constant [H 0 ] expansion rate of the Universe (~7.5  y -1 ) The Age of the Universe [t 0 ] (12-18  10 9 y) 2.The Temperature[ T 0 ] temperature of the cosmic microwave background today (~2.7 o K) 3.The Critical Density[  c ] just prevents eventual collapse (3H 0 2 /8  G N ~ g/cc) The actual density relative to  c [  ] (0.75  1.25) 4.The relative energy density of free space [   ] [aka the Cosmological Constant] (0.6  0.8) ____________… two related numbers________________ a)The relative total matter density [  m ] [all forms of gravitational matter] (0.15  0.45) b)The relative visible matter density [  B ] [normal ‘baryonic’ matter] (0.005  0.012) ____________… and two more numbers______________ I.The ratio of the electron to proton mass [m e /m p ] (1/1896) II.The fine structure constant [  ] (1/137) ___________________… and …_____________________ 5.The number of dimensions of space-time [d] (=3+1)

Ken PeachJohn Adams Institute20 March Dark Matter Prof. Richard Pogge Huge structures in ‘Empty Space’Rotation Curves for Galaxies

Ken PeachJohn Adams Institute20 March Dark Energy – more properties of the vacuum

Ken PeachJohn Adams Institute20 March The Cosmological Budget -  From the ‘flatness’ of space   1 From the observed galaxies & nucleosynthesis  B   0.01 From rotation curves of galaxies & large scale structure  Matter   0.34 Rate of expansion  Space   0.65

Ken PeachJohn Adams Institute20 March Particle Physics Cosmology 1 bb pair qq pairs very early time The Universe 1 bb pair qq pairs quarks intermediate time 1 bb pair 0 qq pairs quarks late time

Ken PeachJohn Adams Institute20 March … but … The matter-antimatter asymmetry in particle physics so far discovered is too small (by 10 orders of magnitude) –although physics beyond the Standard Model has more sources of matter-antimatter asymmetry … but the vacuum knows that there should be such an asymmetry! –Without this, matter, galaxies, the Sun, the Earth cannot be And neither can we! The Big Bang

Ken PeachJohn Adams Institute20 March The vacuum … 1.‘knows’ about all particles that exist …and that can exist 2.‘knows’ about all forces that exist …and that can exist 3.has more energy (x 10) than all normal matter in the universe …we are cosmologically less significant than ‘empty space’ 4.created the Universe …as we know it today 5.made more matter than antimatter … and so created the conditions that allow us to exist! Remember The vacuum is the most complicated thing in the Universe

Ken PeachJohn Adams Institute20 March Summary We have a wonderful “model” to describe the particle world –but it is not a theory it describes but does not explain –and has “missing links” What about gravity? Why 3 forces? Why 3 generations? How does the matter-antimatter asymmetry arise? Why 3 space and 1 time dimension? Are there more dimensions? … (fortunately) still a lot to learn!