Dr. Bill Pezzaglia Particle Physics Updated: 2010May20 Modern Physics Series 1 ROUGH DRAFT.

Slides:



Advertisements
Similar presentations
Modern Physics By Neil Bronks Atoms C 12 6 Mass Number Mass Number - Number of protons + Neutrons. Atomic Number Atomic Number - Number of protons In.
Advertisements

Nuclear Physics UConn Mentor Connection Mariel Tader.
Varan Satchithanandan Mentor: Dr. Richard Jones.  explains what the world is and what holds it together  consists of:  6 quarks  6 leptons  force.
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.
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.
P461 - particles I1 all fundamental with no underlying structure Leptons+quarks spin ½ while photon, W, Z, gluons spin 1 No QM theory for gravity Higher.
University of Birmingham Master class,23rd April 2008 Ravjeet Kour Journey into the heart of matter Introducing Particle Physics.
PH 103 Dr. Cecilia Vogel Lecture 24 From the particle adventure webpage.
Modern Physics LECTURE II.
8/5/2002Ulrich Heintz - Quarknet Particle Physics what do we know? Ulrich Heintz Boston University.
Quantum Electrodynamics Dirac Equation : spin 1/2.
Elementary particles atom Hadrons Leptons Baryons Mesons Nucleons
Particle Physics J1 Particles and Interactions. Particle Physics Description and classification State what is meant by an elementary particle (no internal.
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:
Wednesday, Mar. 23, 2005PHYS 3446, Spring 2005 Jae Yu 1 PHYS 3446 – Lecture #14 Wednesday, Mar. 23, 2005 Dr. Jae Yu Elementary Particle Properties Forces.
Revision Notes - Unit 1 Particles.
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE 26-Jan pm LRB Intro lecture 28-Jan pm LRBProblem solving.
BY: BRETT SLAJUS Particle Physics. Standard Model of Elementary Particles Three Generations of Matter (Fermions)
Particle Physics J4 Leptons and the standard model.
My Chapter 30 Lecture.
2 nd Presentation of Prof. Cho’s Class Hossain Ahmed Introduction to Standard Model.
Yaakov (J) Stein Chief Scientist RAD Data Communications Particle Physics October 2008.
Elementary Particles: Physical Principles Benjamin Schumacher Physics April 2002.
Quarks, Leptons and the Big Bang particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.
Finishing things up. So what’s with that 14 C? Masses of isotopes (not “natural” stuff) truly are multiples of basic hydrogen. Hydrogen is positively.
Jeopardy Jeopardy PHY101 Chapter 12 Review Study of Special Relativity Cheryl Dellai.
The Standard Model of Particles and Interactions Ian Hinchliffe 26 June 2002.
Modern Physics. Answer Me!!! How much energy does a photon have if the light beam has a wavelength of 720 nm?
Fisica Generale - Alan Giambattista, Betty McCarty Richardson Copyright © 2008 – The McGraw-Hill Companies s.r.l. 1 Chapter 30: Particle Physics Fundamental.
The Standard Model Jesse Chvojka University of Rochester PARTICLE Program.
Particles and how they interact
© 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 ? ? ?
Subatomic Particles Lesson 10. Objectives describe the modern model of the proton and neutron as being composed of quarks. compare and contrast the up.
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
Modern Physics. Reinventing Gravity  Einstein’s Theory of Special Relativity  Theorizes the space time fabric.  Describes why matter interacts.  The.
Classification of Particles
A photon with a wavelength of 2
University of Rochester
Modern Physics Chapters Wave-Particle Duality of Light Young’s Double Slit Experiment (diffraction) proves that light has wave properties So does.
PARTICLE PHYSICS Summary Alpha Scattering & Electron Diffraction.
Take out hwk & tables. Compare answers to hwk sets.
What makes up the nucleus? Nucleus is positively charged Different atoms have same electrical properties but different masses Isotopes – same atomic number,
What is the Standard Model of Particle Physics ???? 1. A theory of three of the four known fundamental interactions and the elementary particles that.
More on the Standard Model Particles from quarks Particle interactions Particle decays More conservation laws Quark confinement Spin.
Particle Physics Why do we build particle accelerators? The surface is flat Still flat Oh no its not Big balls cannot detect small bumps.
Phy107 Fall From Last Time… Particles are quanta of a quantum field –Often called excitations of the associated field –Particles can appear and.
The Theory of (Almost) Everything Standard Model.
Particle Physics "three quarks for Muster Mark" -James Joyce (Finnegan’s Wake) Contents: Particle Accelerators Quantum Electrodynamics and Feynman diagrams.
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.
The Standard Model Physics, Not Taxonomy Jesse Chvojka University of Rochester PARTICLE Program.
 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
Lecture 04 - Hadrons Quarks multiplets Hadron decays Resonances
Unit 7.3 Review.
The Standard Model strong nuclear force electromagnetic force
Aim: How can we describe Fundamental Particles?
Search for Order Ancient Greeks: Aristotle Earth Air Fire Water
Particle Physics what do we know?
Particle physics.
Dr. Bill Pezzaglia Nuclear & Particle Physics
ELEMENTARY PARTICLES.
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.
Particle Physics DCC Academic Team Camp 2017.
Introduction to Particle Physics
Modern Studies of the Atom
Physics 4 – April 18, 2019 Agenda:
Particle Physics and The Standard Model
Presentation transcript:

Dr. Bill Pezzaglia Particle Physics Updated: 2010May20 Modern Physics Series 1 ROUGH DRAFT

Particle Physics (aka “high energy physics”) A.Fundamental Forces B.Classical Particles C.Nuclear Force D.Leptons E.More Particles F.Quark Model G.The Standard Model 2

A. Fundamental Forces 1)Gravity 2)Electromagnetism 3)Strong (Nuclear) Force 4)Weak Force (beta decay) 3

1. Gravity & EM Electrical Force is infinite in range, mediated by massless “photon”. Dominates atomic/molecular Gravitational Force is infinite in range, mediated by massless “graviton” (unconfirmed). Dominates in the large (because macroscopic matter is neutral) Einstein attempts to unify these two (Unified Field Theory) 4

B. Classical Particles 1)Classical period (up to 1930) 2)Spin, Pauli Exclusion Principle 3)Antimatter 5

B. Classical Particles 1)Up to 1930, atoms and spectra explained by: Electron(1897) Photon (1905) Proton (1911) Neutron (1932) 6

B1a. The Electron 1891 Stoney proposes “electron” as fundamental electric charge 1897 Thomson discovers the electron. Three experiments on “cathode rays” 1)deflected by magnetic field 2)Deflected by electric field 3)Measures e/m 7

B1b. The Proton 1886 Goldstein discovers “canal rays” which move in opposite direction as “cathode rays” 1918 Rutherford’s experiment demonstrates small size of Hydrogen nucleus, which is 1800x more massive than electron Rutherford calls it the “proton” (greek word “protos” for “first”)

B1c. The Neutron 1920 Rutherford proposes neutral particle in nucleus (thought it was a proton combined with electron) to explain nuclear masses (e.g. helium is mass of 4, but only has charge of +2 protons) 1932 Chadwick discovers neutron (Nobel prize!) Slightly heavier than proton; spin ½ like proton, even though it is neutral, it has a significant magnetic moment! 9

B2. Spin 1922 Stern Gerlach Experiment shows 2 spin states 1924 Pauli introduces “spin” quantum number Pauli Exclusion principle: “fermions” (half integral spin) obey it, but “bosons” (integral spin) do not. 10

B.3. Antimatter Every particle has an “antiparticle”, which is analogous to the particle moving backwards in time 1927 Paul Dirac predicts “anti-electron” 1931 Anderson finds it (“positron”) 1955 Segre & Chamberlain discover the “antiproton” (at UCB !) 1956 the “anti-neutron” is discovered at UCB ! 11

C. Nuclear Force 1)Yukawa Potential 2)Pi Meson Prediction 3)Pion Reactions mediate nuclear force 12

1. Nuclear Force and Yukawa Potential Electromagnetic force is mediated by the massless “photon” and has infinite range “Strong Force” holds the nucleus together, but has range of only about 1.5x meters Yukawa proposes mediated by a massive particle, which limits range 13

2 The Pion (Pi-Meson) Yukawa estimates mass of particle (“meson”) from equating range to its Compton wavelength Mass estimated to be 130 MeV 1947 the “pion” is discovered (140 MeV) Has zero spin (“boson”) Three types:  +  0  - 14

3. Pion Reactions Can change a proton to neutron, etc  + + n  p  - + p  n p  p +  0 n  n +  0 So, a neutron can decay to proton, emits a pi- which is absorbed by a proton, turning into a neutron. This reaction creates an attractive force between the nucleons. 15

D. Leptons and Weak Interaction 1.Three “generations” of the electron (muon, tau) 2.Three types of neutrinos Electroweak Theory (1983 Vector Boson Discovery) 16

E. More Particles 1.“Strange” Mesons 2.More Baryons 3.The 8 fold way 17

1. More Mesons “Strange” Kaon particles 18

2. Strange Baryons 19

Murray Gell-Mann 1969 Nobel Prize (for quark model) 1962 The 8 fold way Predicts a particle that had not yet been found 20

Even More Baryons 21

F. Quark’s Model (1963) 22

2a. Quark model of Baryons 23 All Baryons made of 3 quarks (one of each “color”, so that they can all three be in the same “1s” orbital and not violate pauli exclusion principle) Proton is an “uud”, which adds up to plus charge

2b. The Neutron 24 The neutron is a “udd” combination, which has net zero charge. The “beta” decay of a neutron into a proton is hence due to one of the “d” quarks decaying into an “u” quark

More Quarks “c” Charmed Quark 1977 “b” Bottom (beauty) quark 1995 “t” Top (truth) quark

Charmed Baryons: Spin 1/2 26 C=+2 C=+1 C=0

Charmed Baryons: Spin 3/2 27 C=+2 C=+1 C=0 C=+3

2c. B Baryons (Fermilab) 28

2c. Mesons in quark model 29 All mesons are made of a quark-antiquark pair. Pi plus would be “up” plus “antidown” quark

Charmed Mesons Spin 0 Hexadecimet 30

3. Gluons 1.Gluons mediate the strong force 2.They hold the quarks together 3.i.e. the ‘squiggle” between u and d quarks 31

G. The Standard Model 1. Three generations 3 isospin doublets of quarks Matches 3 generations of lepton doublets Matches (?) 4 fundamental forces? 32

Fundamental Particles and Interactions 33

3. CPT Symmetry 1951 Schwinger suggests that physics is invariant under a CPT transformation Parity: The laws of physics would be the same in a “mirror” universe (weak interactions violate this, neutrinos are only left circularly polarized, antineutrinos are right circularly polarized). Time Reversal: The laws of physics should be valid if we run the movie backwards (problems with entropy) Charge Conjugation: Replace all particles with their antiparticles. Is physics the same? 34

Summary The standard model is an empirical set of rules. There is no theory that yet gives: Masses of quarks Why quarks all decay to u & d the number of generations as being fixed to 3 why there are only 4 forces why only mesons (qq) and baryons (qqq) are allowed. String Theory was our hope to produce this, but so far it has not succeeded. Many feel that this “theory of everything” is actually a “theory of nothing”. 35

References/Notes 36