C.T.R. Wilson. Charles Wilson is 2nd from right in the front row. Can you find Paul Langevin and O.W. Richardson?

Slides:



Advertisements
Similar presentations
Radioactive Decay. - Alpha Decay The emission of an particle from the nucleus of an atom is called alpha decay An alpha particle is just a helium nucleus.
Advertisements

Early Quantum Theory and Models of the Atom
APHY201 4/29/ The Electron   Cathode rays are light waves or particles?
1 Chapter 38 Light Waves Behaving as Particles February 25, 27 Photoelectric effect 38.1 Light absorbed as photons: The photoelectric effect Photoelectric.
2. The Particle-like Properties Of Electromagnetic Radiation
Copyright © 2012 Pearson Education Inc. PowerPoint ® Lectures for University Physics, Thirteenth Edition – Hugh D. Young and Roger A. Freedman Chapter.
Chapter 27 Quantum Physics.  Understand the relationship between wavelength and intensity for blackbody radiation  Understand how Planck’s Hypothesis.
 The nucleus of the atom is composed of protons and neutrons  Some nuclei are stable, some are unstable  Larger nucleus = more unstable  Smaller nucleus.
ATOM Chapter 14. I CAN IDENTIFY THE PROPERTIES OF THE THREE SUBATOMIC PARTICLES OF ATOMS. I CAN USE A MODEL TO REPRESENT THE STRUCTURE OF AN ATOM AND.
INTERACTION OF IONISING RADIATION WITH MATTER
Techniques for detecting X-rays and gamma-rays Pair production Creation of elementary particle and its antiparticle from a photon. Occurs only if enough.
Positron. Pair Production  Photons above twice the electron rest mass energy can create a electron positron pair. Minimum = ÅMinimum = Å.
Ionizing Radiation radioactivity measurements
Radiation L.O: Describe an isotope understand properties of alpha, beta and gamma radiation Explain background radiation.
Stopping Power The linear stopping power S for charged particles in a given absorber is simply defined as the differential energy loss for that particle.
Discovering Particles
The development of Particle Physics Adapted from webnotes by Dr Vitaly Kudryavtsev, Sheffield University.
Discovery of Radiation Roentgen (1895) Discovered a mysterious form of radiation was given off even without electron beam. This radiation could pass through.
Chapter 30: Nuclear Physics and Radioactivity. Radioactivity Radioactivity is the discentigration of an unstable nuclei. when the nuclei decays the nucleus.
the photoelectric effect. line spectra emitted by hydrogen gas
Melanie Carter and Jamie Hegarty. CLOUD CHAMBER OUTLINE Introduction: Cloud Chamber Principles All About Ionizing Radiation –Types of Radiation, why it’s.
Space Instrumentation. Definition How do we measure these particles? h p+p+ e-e- Device Signal Source.
Photo of Particles Interacting within a Bubble Chamber Fermilab bubble chamber: 4.6 m in diameter in a 3 T magnetic field How does a bubble chamber work.
Quantum Physics. Quantum Theory Max Planck, examining heat radiation (ir light) proposes energy is quantized, or occurring in discrete small packets with.
Discovery of cosmic rays In 1909 Theodor Wulf developed an electrometer, a device to measure the rate of ion production inside a hermetically.
Calorimeters  A calorimeter is a detector that measures “energy” of the particles that pass through. Ideally it stops all particles of interest.  Usually.
The nucleus consists of protons and neutrons, collectively called nucleons. The number of protons is the atomic number. Protons plus neutrons is the atomic.
LIGHT and MATTER Chapters 12 and 13. Originally performed by Young (1801) to demonstrate the wave-nature of light. Has now been done with electrons, neutrons,
Seeing the Subatomic Stephen Miller Saturday Morning Physics October 11, 2003.
Section 19.1 Radioactivity 1.To learn the types of radioactive decay 2.To learn to write nuclear equations for radioactive decay 3.To learn how one element.
Classical ConceptsEquations Newton’s Law Kinetic Energy Momentum Momentum and Energy Speed of light Velocity of a wave Angular Frequency Einstein’s Mass-Energy.
Ch. 25 Nuclear Changes Begins on p. 35 of your PACKET.
Review of Special Relativity S and S’ system: S and S’ system: For a particle with velocity in S: For a particle with velocity in S: The Doppler effect:
Physics 2170 – Spring X-rays and Compton effect Next weeks homework will be available late this afternoon.
Electromagnetic radiation behaves as particles 1. Notes of the problem discussed Tuesday. 2. Quiz 9.11 and a few comments on quiz Topics in EM.
Section 19.1 Radioactivity 1.Students will be able to describe the factors that lead to nuclear stability. 2.Students will be able to describe types of.
PHYSICS 225, 2 ND YEAR LAB NUCLEAR RADIATION DETECTORS G.F. West Thurs, Jan. 19.
Gamma and X ray interactions
Edexcel A2 Physics Unit 4 : Chapter 3 : Particle Physics 3.1: Probing Matter Prepared By: Shakil Raiman.
LIGHT and MATTER Chapters 11 & 12. Originally performed by Young (1801) to demonstrate the wave-nature of light. Has now been done with electrons, neutrons,
1 2. Atoms and Electrons How to describe a new physical phenomenon? New natural phenomenon Previously existing theory Not explained Explained New theoryPredicts.
Nuclear Changes Objectives: Students will:
Wilson cloud chamber.
INTERACTIONS OF RADIATION WITH MATTER. twCshttp:// twCs
Measurement devices Cloud chamber Geiger counter Bubble chamber Nuclear emulsion 2.
STATION 1 Light and Waves 1.According to Einstein’s view of matter and energy, what is the common link between light and matter? 2.How does diffraction.
3.1 Discovery of the X-Ray and the Electron 3.2Determination of Electron Charge 3.3Line Spectra 3.4Quantization 3.5Blackbody Radiation 3.6Photoelectric.
DISCOVERY OF THE NUCLEUS: PROTONS AND NEUTRONS. ERNEST RUTHERFORD Determined the structure of the atom First to split the atom.
Compton Effect X-Ray Scattering Classical Theory (cont’d): c) The scattered radiation should have the same frequency as the incident radiation d) Because.
EMR 2 The Compton Effect. Review of Photoelectric Effect: Intensity Matters - the greater the intensity/brightness, the greater the photoelectric current.
Compton Effect Objective:
Photoelectric Effect. Lenard 1902: Studied energy of the photoelectrons with intensity of light. He could increase the intensity thousand fold. 1.Noticed.
Jan 13 th Posters due Friday Interactions of Photons with matter.
Chapter 9 – Radioactivity and Nuclear Reactions
Chapter 38 Photons: Light Waves Behaving as Particles
Photons: Light Waves Behaving as Particles
Objectives To learn the types of radioactive decay
Quiz_14 Previous material – Compton scattering, pair production New material – Wave-Particle duality, probability, Uncertainty Principle Physics 274 9/30/2016.
Photoelectric Effect.
Chapter 38 Photons: Light Waves Behaving as Particles
Photon-Matter Interactions
Pair Production and photon-matter interactions
Interaction of Electromagnetic Radiation with Matter
THE ATOMIC MODEL Learning Challenges
Quantization of light, charge and energy Chapter 2-Class5
Technician’s Notes Activity 10S Software Based 'Bubble chamber photographs'
P2 - Physics Radiation.
4.6 NOTES Atomic Emission Spectra
Chapter 38 Photons: Light Waves Behaving as Particles
Objectives To learn the types of radioactive decay
Presentation transcript:

C.T.R. Wilson

Charles Wilson is 2nd from right in the front row. Can you find Paul Langevin and O.W. Richardson?

First cloud chamber “the most original and wonderful instrument in scientific history.” - Rutherford

Diagram

ALPHA broad, straight track BETA thin, bending track GAMMA no tracks as too few ions are produced in the air

1911 photo

1912 photo 1912 Wilson photo

Compton Scattering : What? X-ray photons collide with electrons in carbon atoms. The scattered photons are shifted to longer wavelengths (lower energies).

Compton Scattering : So What? The particle theory of light was still controversial in the 1920’s, despite Einstein’s photoelectric effect. Compton used a particle model of the photon, and classical conservation of momentum, to explain the shift in wavelength of the observed scattered x-rays.

evidence of Compton Effect (Nobel Prize Compton & Wilson 1927) evidence of transmutation of elements (Rutherford’s N +  -> O + p) discovery of positron and the pair creation- annihilation of electrons & positrons (Nobel Prize Anderson 1936) discovery of muon

P. BLACKETT “counter controlled cloud chamber” (Nobel Prize 1948) added a Geiger Counter above & below the c.c. Cosmic rays triggered gas expansion and their own photos when impulses hit both counters simultaneously. D.A. GLASER “bubble chamber” replaced the c.c. in 1952, using liquid He or H 2. Higher density medium allowed photos of high-E particles that were too fast for the c.c. Beyond the Cloud Chamber

Web Resources how to make a cloud chamberhttp://home.houston.rr.com/molerat/cloud.htm ss.html Wilson’s Nobel addresshttp:// ss.html astr.gsu.edu/hbase/quantum/comptint.html#c1 Compton Effecthttp://hyperphysics.phy- astr.gsu.edu/hbase/quantum/comptint.html#c1 ng_physics.htm lightning physicshttp:// ng_physics.htm