Observing the Universe by Going Underground ZOOMING OUT by ZOOMING IN HAIM HARARI Years of Physics at the Weizmann Institute of Science May 12 th, 2004.

Slides:



Advertisements
Similar presentations
The Big Bang, the LHC and the Higgs Boson Dr Cormac O’ Raifeartaigh (WIT)
Advertisements

Neutrino Masses, Leptogenesis and Beyond The Incredible Foresight of ETTORE MAJORANA Haim Harari Erice, August 31, 2006.
Particles in the Standard Model John Charters
Leptons: There are 6 leptons (and their corresponding anti-leptons). One 1st generation lepton is the electron previously discussed. The electron.
Sub-Atomic Particles Another building block of matter?? Richard Lasky – Summer 2010.
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.
UNIT 2: OUTLINE SYLLABUS: 1st Lecture Introduction Hadrons and Leptons Spin & Anti-Particles The conservation laws: Lepton Number Baryon number Strangeness.
8/5/2002Ulrich Heintz - Quarknet Particle Physics what do we know? Ulrich Heintz Boston University.
5.3.2 Fundamental Particles. (a) explain that since protons and neutrons contain charged constituents called quarks they are, therefore, not fundamental.
Nuclear Force and Particles
Elementary particles atom Hadrons Leptons Baryons Mesons Nucleons
The Big Bang, the LHC and the Higgs Boson Dr Cormac O’ Raifeartaigh (WIT)
THE STANDARD MODEL  What’s fundamental  What’s in a name.
The Particle Zoo. Too Many Particles Far from just finding Protons Neutrons Electrons Neutrinos and their antiparticles, during the 20 th century many.
Review Game Eureeka! Get a board, marker, wipey thing, and partner.
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.
Point 1 activities and perspectives Marzio Nessi ATLAS plenary 2 nd October 2004 Large Hadron Collider (LHC)
Lecture 29 Elementary Particles and Quarks
Nuclear Energy Nuclear fission is when a heavy nucleus splits into two smaller nuclei. The total mass of the products is less than the original mass. The.
Atomic Structure Basic and Beyond. What are the 3 major parts of an atom? Protons Electrons Neutrons.
Overview of Astroparticle Physics 4 th Winter School on Astroparticle Physics Mayapuri, Darjeeling Rajarshi Ray Center for Astroparticle Physics & Space.
Quarks, Leptons and the Big Bang particle physics  Study of fundamental interactions of fundamental particles in Nature  Fundamental interactions.
Happyphysics.com Physics Lecture Resources Prof. Mineesh Gulati Head-Physics Wing Happy Model Hr. Sec. School, Udhampur, J&K Website: happyphysics.com.
基本粒子. 2 The Periodic Table Mendeleev (1869) introduced the periodic table.
Option 212: UNIT 2 Elementary Particles Department of Physics and Astronomy SCHEDULE 26-Jan pm LRB Intro lecture 28-Jan pm LRBProblem solving.
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.
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.
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.
What IS Fundamental???  Many new particles were discovered with the advent of particle accelerators …are they ALL fundamental??? Baryons: particles with.
Quarks and Leptons Announcements 1.Recitation this week in lab. BRING QUESTIONS ! 2.See my by Wed. if you have any grading issues with your exam. 3.Reading.
Re-creating the Big Bang Experiments at the Large Hadron Collider Dr Cormac O’ Raifeartaigh (WIT) Albert Einstein Ernest Walton.
Modern Physics. Reinventing Gravity  Einstein’s Theory of Special Relativity  Theorizes the space time fabric.  Describes why matter interacts.  The.
Introduction to CERN Activities
Particles & Waves The Standard Model. Orders of Magnitude Human Scale Distance10 -3 ~ 10 2 m Measurable without additional technology Time10 0 ~ 10 2.
What’s Hot in High Energy Particle Physics Study of the fundamental constituents & interactions of matter. What is the universe made of and by what rules.
Chapter 30: Nuclear Energy and Elementary Particles
Seeing the Sky Underground The Birth of Neutrino Astronomy Chiaki Yanagisawa Stony Brook University October 13, 2007 Custer Institute.
Lecture 2: The First Second Baryogenisis: origin of neutrons and protons Hot Big Bang Expanding and cooling “Pair Soup” free particle + anti-particle pairs.
Phys 102 – Lecture 28 Life, the universe, and everything 1.
High Energy Accelerators Dennis Silverman Physics and Astronomy U. C. Irvine.
Introduction to Particle Physics (for non physics students) 2. PARTICLES (from atoms to quarks and leptons)
SYNTHESIS The Standard Model 1.Elementary particles 2.Strong nuclear force 3.Weak nuclear force 4.The Standard Model.
PARTICLE PHYSICS Summary Alpha Scattering & Electron Diffraction.
The cosmic connection There is a very close connection between particle physics and astrophysics. I’m going to show two examples: Type II supernovas Dark.
1 The Standard Model of Particle Physics Owen Long U. C. Riverside March 1, 2014.
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.
Particle Physics Why do we build particle accelerators? The surface is flat Still flat Oh no its not Big balls cannot detect small bumps.
The Theory of (Almost) Everything Standard Model.
What is Matter? 1.Sequencing the content 2.Challenges 3.Assessment tasks.
Introduction to CERN Activities
The Standard Model.
Introduction to CERN Activities
The Standard Model strong nuclear force electromagnetic force
Particle Physics.
Aim: How can we describe Fundamental Particles?
The Quarks Inside Baryons
Particle Physics what do we know?
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.
Quarks Remember the family of ordinary matter consists of only 4 particles, (not counting their antiparticles) quark u d lepton (electron) e Lepton (electron.
Early Universe.
Lecture 2: The First Second origin of neutrons and protons
Modern Studies of the Atom
Atomic Structure.
Quarks Types Up Down Charmed Strange Top Bottom Formations Hadrons
Presentation transcript:

Observing the Universe by Going Underground ZOOMING OUT by ZOOMING IN HAIM HARARI Years of Physics at the Weizmann Institute of Science May 12 th,

“ZOOMING IN” Matter Chemical Elements Atoms ~

Galaxies Stars Life NOW 13.7G yr ~100M yr 300K yr 3 min sec sec sec sec 1 sec 10 2 sec sec sec sec “ZOOMING OUT” Atoms

“ZOOMING IN” Into the ATOM Matter Chemical Elements Atoms Nucleus ~

Radioactive  -Decay e-e- A 1  A 2 + e -

“ZOOMING IN” Into the ATOM Matter Chemical Elements Atoms Nucleus e ~ Systematics: “Periodic Table” Mendeleyev Collisions and Interactions Chemistry “Smashing” Experiments Rutherford

Radioactive  -Decay e-e- e-e- e-e- e-e- N 1  N 2 + e -

Radioactive  -Decay e-e- e-e- e-e- e-e- N 1  N 2 + e - +

“ZOOMING IN” Into the NUCLEUS Matter Chemical Elements Atoms Nucleus p, n e ~100 ~

Radioactive  -Decay n p n p e-e- e-e- e-e- e-e- e-e- n  p + e - +

Light Nuclei Heavy Nuclei Atoms Galaxies Stars Life NOW 13.7G yr ~100M yr 300K yr 3 min sec sec sec sec 1 sec 10 2 sec sec sec sec “ZOOMING OUT”

Antiparticles p n e p n e Equal Numbers of Particles and Antiparticles? Why p and e Have Equal and Opposite Charge? THE BIG BANG Only  -decay Can Convert n  p Nuclear Reactions: The Dream of the Alchemists Mass Converted to Energy Energy of the Sun Creation of Heavy Elements

“ZOOMING IN” Into the PROTON & NEUTRON Matter Chemical Elements Atoms Nucleus p, n  … Antiparticles e ~100 ~ 4  Hadrons ~100

e -- e-e- Electric Charge

Baryons Electric Charge “Strangeness” p n

Baryons Electric Charge “Strangeness” Mesons Electric Charge +1 0 “Strangeness” p n       

Baryons Electric Charge “Strangeness” Mesons Electric Charge +1 0 “Strangeness” p n u ds _+_ Quarks       

Mesons Electric Charge +1 0 “Strangeness” Electric Charge “Strangeness” uuu uud udd ddd uus uds dds uss dsssss p n u ds _+_ Quarks Baryons       

Mesons Electric Charge +1 0 “Strangeness” Electric Charge “Strangeness” uuu uud udd ddd uus uds dds uss dsssss p n u ds _+_ sd u _+_ QuarksAnti-Quarks Baryons       

Electric Charge “Strangeness” uuu uud udd ddd uus uds dds uss dsssss u ds _+_ p n Mesons Electric Charge +1 0 “Strangeness” us ds ud uu dd ss du sd su sd u _+_ QuarksAnti-Quarks       

“ZOOMING IN” Into the PROTON & NEUTRON Matter Chemical Elements Atoms Nucleus Hadrons Quarks p, n  … Antiparticles e ~100 ~ 4 ~100 ~ 7  

u s d e -- e-e- Electric Charge LeptonsQuarks

LeptonsQuarks u s d  e -- e-e- Electric Charge

Baryon-Mesons Collisions Time B1B1 M1M1 M2M2 B2B2 B*

Baryon-Mesons Collisions B1B1 M1M1 M2M2 B2B2 B* Time B1B1 M1M1 M2M2 B2B2 M*

Baryon-Mesons Collisions B1B1 M1M1 M2M2 B2B2 B* Time B1B1 M1M1 M2M2 B2B2 M* B1B1 M1M1 M2M2 B2B2 Duality Diagram

Baryon-Mesons Collisions B1B1 M1M1 M2M2 B2B2 B* Time B1B1 M1M1 M2M2 B2B2 M* B1B1 M1M1 M2M2 B2B2 Duality Diagram B*

Baryon-Mesons Collisions B1B1 M1M1 M2M2 B2B2 B* Time B1B1 M1M1 M2M2 B2B2 M* B1B1 M1M1 M2M2 B2B2 Duality Diagram M*

Baryon-Mesons Collisions B1B1 M1M1 M2M2 B2B2 B* Time B1B1 M1M1 M2M2 B2B2 M* B1B1 M1M1 M2M2 B2B2 Duality Diagram B* M* Meson Is a “String” Can Split Into Two

Deep Inelastic Scattering e e P Hadrons All Hadrons Made of Quarks Free Quarks Do Not Exist Only at Very Short Distance They Can Be Detected Early Universe - Soup of Quarks and Antiquarks

Stanford Linear Accelerator

Radioactive  -Decay d  u + e - + n p n p e-e- e-e- e-e- e-e- e-e- e-e- d

“ZOOMING IN” Into the PROTON & NEUTRON Matter Chemical Elements Atoms Nucleus Hadrons Quarks p, n  … Antiparticles e ~100 ~ 4 ~100 ~ 7   Systematics: “Periodic Table” Eightfold Way Collisions and Interactions Duality+Quark Counting “Smashing” Experiments Deep Inelstic

LeptonsQuarks u s d  e -- e-e- Electric Charge c

LeptonsQuarks u s d  e -- e-e- Electric Charge c t b  --

Matter Chemical Elements Atoms Nucleus Hadrons Quarks p, n  … c b t Antiparticles e ~100 ~ 4 ~100 ~ 7 ~ 20     “ZOOMING IN” Into the QUARK & LEPTON

LeptonsQuarks u s d  e -- e-e- Electric Charge c t b  --

Quark Mixing Heavy Quarks decay fast Heavy Quarks are Short-Lived Three Generations of Quarks & Leptons Do Heavy Quarks Matter? Violation of Symmetry between Particle and Antiparticle? 6 Quarks Masses 3 Mixing Parameters

CERN OPAL

Particle Masses Generated “Quark Soup” Protons & Neutrons Light Nuclei Heavy Nuclei Atoms Galaxies Stars Life NOW 13.7G yr ~100M yr 300K yr 3 min sec sec sec sec 1 sec 10 2 sec sec sec sec “ZOOMING OUT”

is Massless ? Is Different from ? Are e     Really Different ? Nuclear Reactions Neutrinos Solar Neutrinos Cosmic Ray Neutrinos Supernova Neutrinos - ASTRONOMY Neutrinos Have Masses They Are Extremely Light Masses of e     Are Different e     Mix Conclusions:

Kamiokande Japan

LeptonsQuarks Electric Charge u s d c t b  e -- e-e-  --

LeptonsQuarks Electric Charge u s d c t b  e -- e-e-  -- 4M 150M7M 1.3G170G 5G 8m<8m 100M500K 30m 1.8G

LeptonsQuarks Electric Charge u s d c t b  e -- e-e-  --

LeptonsQuarks Electric Charge u s d c t b  e -- e-e-  -- Leptons & Quarks

Electric Charge u s d c t b  e ++ e+e+  ++ Antiparticles  e -- e-e-  -- u s d c t b

Leptons & Quarks Electric Charge u s d c t b  e ++ e+e+  ++ Antiparticles Electric Charge  e -- e-e-  -- u s d c t b

OPEN QUESTIONS Why Are We Here (“Baryogenesis”)? What Is the Dark Matter? What Is the Dark Energy? Connection to Gravity? Why Three Generation? Do the 2nd and 3rd Generation Make a Difference? Quarks – Lepton relation? ?,,, Why only 20 Building Blocks? 20 Arbitrary Parameters? Origin of Masses?

A New Ingenious Theoretical Framework STRING THEORY Grand Unified Theories (GUT) Supersymmetry (SUSY) Sub-particles (“Rishons”?) Options

BIG BANG Gravity Connection Inflation Particle Masses Generated “Quark Soup” Protons & Neutrons Light Nuclei Heavy Nuclei Atoms Galaxies Stars Life NOW 13.7G yr ~100M yr 300K yr 3 min sec sec sec sec 1 sec 10 2 sec sec sec sec Grand Unification ? Baryogenesis ? Subparticles ? Strings ? “ZOOMING OUT”

50 HAPPY BIRTHDAY WEIZMANN-PHYSICS