1 PHY100 PHY100 ― The Nature of the Physical World Lecture 17 More Particle Physics Arán García-Bellido.

Slides:



Advertisements
Similar presentations
The search for the God Particle
Advertisements

"Now I am become Death, the destroyer of worlds." Robert Oppenheimer after the first test of the atomic bomb.
ATLAS Experiment at CERN. Why Build ATLAS? Before the LHC there was LEP (large electron positron collider) the experiments at LEP had observed the W and.
Tony Liss Saturday Physics for Everyone November 9, 2013 (With debts to Chris Quigg, Leonard Susskind, Hitoshi Murayama)
Nuclear Physics UConn Mentor Connection Mariel Tader.
AAAS 2001 San Francisco1 Supersymmetry The Coming Revolutions in Particle Physics Hitoshi Murayama (UC Berkeley)
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.
Modern Physics LECTURE II.
8/5/2002Ulrich Heintz - Quarknet Particle Physics what do we know? Ulrich Heintz Boston University.
Nuclear Force and Particles
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:
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE 26-Jan pm LRB Intro lecture 28-Jan pm LRBProblem solving.
My Chapter 30 Lecture.
The Dark Side of the Universe What is dark matter? Who cares?
Point 1 activities and perspectives Marzio Nessi ATLAS plenary 2 nd October 2004 Large Hadron Collider (LHC)
Modern Physics We do not Know It All!!.
Jeopardy Jeopardy PHY101 Chapter 12 Review Study of Special Relativity Cheryl Dellai.
The Standard Model of Particles and Interactions Ian Hinchliffe 26 June 2002.
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 of Particle Physics By: Sean Yeager Rutgers, The State University of New Jersey 1 July 2009.
A singularity formed by a previous collapsed Universe? Multiple Universes? We just don’t know… YET What Caused It?
IB Physics Mr. Jean April 16 th, The plan: SL Practice Exam questions HL Particle Physics –Electrons –Protons –Neutrons –Quarks –Gluons –Photos.
The Strong Force.
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
© 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 ? ? ?
Anthropology Series In the Beginning How did the Universe begin? Don’t know!
The Nucleus Nucleons- the particles inside the nucleus: protons & neutrons Total charge of the nucleus: the # of protons (z) times the elementary charge.
What IS Fundamental???  Many new particles were discovered with the advent of particle accelerators …are they ALL fundamental??? Baryons: particles with.
Radioactivity Physics 12 Adv. Radioactivity Radioactive decay is the emission of some particle from a nucleus which is accompanied by a change of state.
The Higgs Boson Observation (probably) Not just another fundamental particle… July 27, 2012Purdue QuarkNet Summer Workshop1 Matthew Jones Purdue University.
A photon with a wavelength of 2
ELECTROWEAK UNIFICATION Ryan Clark, Cong Nguyen, Robert Kruse and Blake Watson PHYS-3313, Fall 2013 University of Texas Arlington December 2, 2013.
Take out hwk & tables. Compare answers to hwk sets.
1 Particle Physics, The Mysteries of the Universe, and The LHC Nhan Tran Johns Hopkins University.
1 The Standard Model of Particle Physics Owen Long U. C. Riverside March 1, 2014.
Particle Detectors January 18, 2011 Kevin Stenson.
Particle Physics Why do we build particle accelerators? The surface is flat Still flat Oh no its not Big balls cannot detect small bumps.
PHY100 ― The Nature of the Physical World November 5th, 2008
Standard Model of Particle Physics
CHAPTER 14 Elementary Particles
Fundamental Particles, Fundamental Questions
The Discovery of THE HIGGS BOSON Why is it Exciting?
The Standard Model of Particle Physics
PHL424: 4 fundamental forces in nature
The Standard Model An Introduction to Particle Physics
From Before… Essay Due Today Discussed the weak interaction
E = mc2 If you can’t explain it simply, you haven’t learned it well enough. Einstein.
Unit 7.3 Review.
The Standard Model strong nuclear force electromagnetic force
The Beginning of Time (Birth Of The Universe)
HCP: Particle Physics Module, Lecture 3
PHL424: 4 fundamental forces in nature
Elementary particles Spring 2005, Physics /24/2018 Lecture XXV.
From Last Time… Discussed the weak interaction
Particle Physics what do we know?
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.
The Color Charge & Bag Model
François PASSEBON & Jack WILLIS
Frontiers of fundamental physics
From Last Time… Discussed the weak interaction
FAMILIAR FORCES Probably the most familiar force is the gravitational force. It does not only pull objects towards the centre of the Earth. The Earth is.
Introduction to Particle Physics
The Standard Model The Standard Model combines the electromagnetic, weak, and strong forces (= interactions). Bosons with spin 1 communicate the force.
Early Universe.
From Last Time… Discussed the weak interaction
Lesson 4: Forces and Bosons
Lesson 4: Forces and Bosons
Presentation transcript:

1 PHY100 PHY100 ― The Nature of the Physical World Lecture 17 More Particle Physics Arán García-Bellido

2 PHY100 News Exam 2: Wednesday March 31 (next week!) Hoyt at pm, instead of class Bring a calculator I will provide a formula sheet Material: lectures 8 – 15 (up to nuclear physics, life of a star), recitations 5-7 I'll be available in my office Monday-Wednesday Come see me if you have questions! No recitations or problems next week

3 PHY100 Last layer in the onion? m

4 PHY100 Quantum field theory Forces are “carried” or “mediated” by particles: exchange force ElectromagneticWeakStrong

5 PHY100 Matter and forces

6 PHY100 Look at the particle “periodic table” It has up and down quarks which make protons and neutrons... Which bind with electrons to make atoms... And a neutrino, partner with electron... So what’s all the stuff to the right? There just appear to be three copies of all the matter that really matters… All that distinguishes the “generations” is their mass Three families -- I.I. Rabi

7 PHY100 Antimatter… is really weird All particles have antiparticles! Antimatter has the same properties as matter Same mass, same spin, same interactions But opposite electric charge Has another weird property… It can annihilate with matter to create pure energy! Or, conversely, energy can create matter and antimatter pairs. E=mc 2 So you might ask: The early Universe had a lot of energy.... where is the antimatter in the Universe?

8 PHY100 Why is the Universe made of matter? Good question: if the Universe started with same amount of matter and antimatter, where is the antimatter? Look for annihilations As far away as we can tell, today there aren’t big matter and antimatter collisions We don't know why this is true yet! Active field of research There must be a basic matter-antimatter asymmetry in one of the forces of Nature

9 PHY100 How weak are Weak Interactions? Weak is, in fact, way weak A 3 MeV neutrino produced in fusion from the sun will travel through water, on average 53 light years, before interacting The 3 MeV positron (anti-matter electron) produced in the same fusion process will travel 3 cm, on average Moral: to find neutrinos, you need a lot of neutrinos and a lot of detector! Super-Kamiokande: confirms the existence of the sun in neutrino image! Masatoshi Koshiba, UR PhD 1955, Nobel 2002 The Sun, imaged in neutrinos, by Super- Kamiokande, and optical

10 PHY100 Where are neutrinos found? Anywhere there are weak interactions! The early Universe The heavy things to the right decay (weakly), leaving a waste trail of 100/cm 3 of each neutrino species They are (now) very cold and slow and hard to detect But if they have even a very small mass, they make up much of the weight of the Universe In the sun Sun shines by fusion, energy reaching Earth in light and in neutrinos is similar 100 billion neutrinos per cm 2 per second rain on us Supernova 1987A (150,000 light years away) When it exploded, it released 100 times the neutrinos the sun will emit in its whole lifetime We observed 11 neutrinos in detectors on Earth!

11 PHY100 More neutrinos! Bananas? We each contain about 20mg of 40 K which is unstable and undergoes β decay So each of us emits 0.3 billion neutrinos/sec For the same reason, the natural radioactivity of the Earth results in 10 million neutrinos per cm 2 per second here Nuclear reactors (6% of energy is anti-neutrinos) Average plant produces anti-neutrinos/sec Cosmic Rays Cosmic rays from galaxy Each particle (mostly protons) has many GeV of energy Collisions in upper atmosphere create particles which decay (weakly) to neutrinos Can use same technique to produce neutrinos at accelerators

12 PHY100

13 PHY100 The Strong Force… This force is so strong that it can effectively be thought of as glue Force carrier is named the “gluon” Gluons connect to “color” Can think of these colors as combining like light “White” (colorless) things don’t feel the strong force

14 PHY100 Fighting the strong force A good model for trying to pull two quarks is like putting energy into a spring When it “breaks” it breaks by creating matter! Separate into two “colorless” objects This is why free or bare quarks have never been observed The further away the strong force binds two quarks, the stronger it is! Why? Because gluons also feel the strong force, so as distance increases, make more and more gluons and quark+antiquark pairs Most of the mass of a proton is actually energy exchanges carried by gluons Most of your mass is strong force dynamics Quantum Chromodynamics (QCD)

15 PHY100 Gluing together protons Asking why two (colorless) protons are attracted by the strong force is analogous to asking how molecules bind together Answer is basically the residual electric force over the size of the atom. Only works if nearby Answer is exactly the same for strong force Residual strong force, but only if nearby…

16 PHY100 Unification of Forces Ever since Maxwell, physicists have dreamed of becoming famous by unifying descriptions of fundamental forces Ha! Beat this! Unfortunately, the history is not encouraging... Einstein spent most of his late career attempting to unify gravity and electromagnetism… The trend is not positive:

17 PHY100 Unification of Forces (cont’d) The one exception to this trend is “electroweak” unification Weak and electromagnetic force share a common description Above ~100 GeV they become one force Below that energy, they are distinct Weak force and electromagnetism are very different because the carriers of the weak force are very massive bosons (W, Z) Can exchange mass over short ranges by the uncertainty principle “Borrow” the energy for a short time How to combine a massless photon and massive W and Z? Answer: The Higgs Mechanism

18 PHY100 Higgs mechanism How does the Higgs work? Envisage the motion of people at a party… Outside the party, they are free to walk Inside, limited by crowd Now imagine a VIP enters the room… A cluster of people forms around the VIP Her motion is more restricted: more inertia (mass) This is what happens to W, Z But not to photon!

19 PHY100 Higgs particles Ok, so the Higgs mechanism explains why particles acquire mass There are also collective excitations of the medium Imagine a rumor spreading… The rumor causes people to cluster This strong interaction is like a mass The mechanism itself has mass! A new particle to discover! This particle has not yet been observed So we still don't know why particles have a mass! It could be a mechanism different from the Higgs mechanism But something does what the Higgs does Build LHC to continue our quest for the origin of mass

20 PHY100 The Rochester connection

21 PHY100 What about gravity? Unifying gravity with all the other forces is the purview of an effort in physics called “string theory” It’s a very beautiful picture, but it shows the unification dynamics happening at very tiny distances Roughly m! We can’t even conceive of how to see something this small! Supersymmetry may get us closer to including gravity, but it is still not a complete theory Like antiparticles but with spin Fermion ↔ Boson