Lecture Outline Chapter 30. Physics, 4 th Edition James S. Walker. Copyright 2010 Pearson Education, Inc.

Similar documents
Announcements. Lecture 8 Chapter. 3 Wave & Particles I. EM- Waves behaving like Particles. The Compton effect (Arthur Compton 1927) Hypothesis:

Quantum Theory of Light

Planck s Quantum Hypothesis Blackbody Radiation

Chapter 37 Early Quantum Theory and Models of the Atom. Copyright 2009 Pearson Education, Inc.

General Physics (PHY 2140)

Explain how Planck resolved the ultraviolet catastrophe in blackbody radiation. Calculate energy of quanta using Planck s equation.

Supplemental Activities. Module: Atomic Theory. Section: Electromagnetic Radiation and Matter

Chapter 28: Quantum Physics. Don t Copy This. Quantum Physics 3/16/13

Learning Objectives and Worksheet I. Chemistry 1B-AL Fall 2016

Physics 1C. Lecture 27A

Chapter 27 Quantum Physics

Chapter 30 Quantum Physics 30.1 Blackbody Radiation and Planck s Hypothesis of Quantum Energy 30.2 Photons and the Photoelectric Effect 30.

Class 21. Early Quantum Mechanics and the Wave Nature of Matter. Physics 106. Winter Press CTRL-L to view as a slide show. Class 21.

Physics 1161: Lecture 22

Light Quanta. Particle-Wave History 11/2/2008. Particle-Wave Nature Continued s

Lecture 16 Quantum Physics Chapter 28

Chapter 27. Quantum Physics

Early Quantum Theory & Models of the Atom (Ch 27) Discovery of electron. Blackbody Radiation. Blackbody Radiation. J. J. Thomson ( )

Lecture 36 Chapter 31 Light Quanta Matter Waves Uncertainty Principle

Physics 1C Lecture 28C. "For those who are not shocked when they first come across quantum theory cannot possibly have understood it.

Chapter 10: Wave Properties of Particles

Title / paragraph example Topic: Quantum Computers. Course Essay. Photoelectric effect summary. From Last Time. Compton scattering

Supplemental Activities. Module: Atomic Theory. Section: Electromagnetic Radiation and Matter - Key

Alan Mortimer PhD. Ideas of Modern Physics

Problems with Classical Physics. Blackbody Radiation Photoelectric Effect Compton Effect Bohr Model of Atom

CHAPTER 27 Quantum Physics

RED. BLUE Light. Light-Matter

CHE3935. Lecture 2. Introduction to Quantum Mechanics

c = λν 10/23/13 What gives gas-filled lights their colors? Chapter 5 Electrons In Atoms

We also find the development of famous Schrodinger equation to describe the quantization of energy levels of atoms.

Chapter 38. Photons Light Waves Behaving as Particles

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS

5.111 Lecture Summary #3 Monday, September 8, 2014

PHY202 Quantum Mechanics. Topic 1. Introduction to Quantum Physics

Title / paragraph example Topic: Quantum Computers. Course essay. Photoelectric effect summary. From Last Time. Photon interference?

Quantum Mechanics. Particle in a box All were partial answers, leading Schrödinger to wave mechanics

It s a wave. It s a particle It s an electron It s a photon. It s light!

Preview. Atomic Physics Section 1. Section 1 Quantization of Energy. Section 2 Models of the Atom. Section 3 Quantum Mechanics

Physics 1C. Chapter 28 !!!!

Chapter 37 Early Quantum Theory and Models of the Atom

4/14/2015. Models of the Atom. Quantum Physics versus Classical Physics The Thirty-Year War ( ) Classical Model of Atom

Early Quantum Theory and Models of the Atom

General Physics (PHY 2140) Lecture 14

Lecture PowerPoints. Chapter 27 Physics: Principles with Applications, 7th edition Giancoli

Chapter 7. The Quantum Mechanical Model of the Atom

Accounts for certain objects being colored. Used in medicine (examples?) Allows us to learn about structure of the atom

QUANTUM MECHANICS Chapter 12

Lecture 6 - Atomic Structure. Chem 103, Section F0F Unit II - Quantum Theory and Atomic Structure Lecture 6. Lecture 6 - Introduction

12/04/2012. Models of the Atom. Quantum Physics versus Classical Physics The Thirty-Year War ( )

is the minimum stopping potential for which the current between the plates reduces to zero.

Particles and Waves Particles Waves

Semiconductor Physics and Devices

Chapter 27 Early Quantum Theory and Models of the Atom Discovery and Properties of the electron

Atomic Spectra. if you pass white light through a gas dark narrow lines on a bright continuum "Absorption spectrum"

Welcome back to PHY 3305

PARTICLES AND WAVES CHAPTER 29 CONCEPTUAL QUESTIONS

Particle nature of light & Quantization

The Photoelectric Effect

Physics 102: Lecture 23

Chapter 5 Electrons In Atoms

27-1 Planck Solves the Ultraviolet Catastrophe

Chapter 27. Quantum Physics

Wave function and Quantum Physics

Conceptual Physics Fundamentals

Blackbody Radiation. Rayleigh-Jeans law was an attempt to explain blackbody radiation based on classical ideas:

General Physics (PHY 2140) Lecture 15

Table of Contents Electrons in Atoms > Light and Quantized Energy > Quantum Theory and the Atom > Electron Configuration

Energy levels and atomic structures lectures chapter one

Quantum Mechanics Tutorial

CHAPTER 5 Wave Properties of Matter and Quantum Mechanics I

( ) # velocity. Wavelengths of massive objects. From Last Time. Wavelength of electron. Wavelength of 1 ev electron. A little complicated ( ) " = h mv

Chapter 28 Quantum Theory Lecture 24

MIDTERM 3 REVIEW SESSION. Dr. Flera Rizatdinova

Light was recognised as a wave phenomenon well before its electromagnetic character became known.

Today: Finish Color (Ch. 27) Intro to Quantum Theory (Ch.31)

Physics 102: Lecture 23

Einstein. Quantum Physics at a glance. Planck s Hypothesis (blackbody radiation) (ultraviolet catastrophe) Quantized Energy

Introduction. Electromagnetic Waves. Electromagnetic Waves

Historical Background of Quantum Mechanics

AP Physics Study Guide Modern Physics I. Atomic Physics and Quantum Effects 1. Who is generally credited with the discovery of the electron?

Chapter 1 Early Quantum Phenomena

Quantum Physics and Atomic Models Chapter Questions. 1. How was it determined that cathode rays possessed a negative charge?

Physics 1302, Exam 4 Review

Chapter 7. The Quantum- Mechanical Model of the Atom. Chapter 7 Lecture Lecture Presentation. Sherril Soman Grand Valley State University

Entering the 2009 Raab Contest Steve Brehmer

PSI AP Physics How was it determined that cathode rays possessed a negative charge?

Chapter 38. Photons and Matter Waves

Physics. Light Quanta

Chap. 3. Elementary Quantum Physics

Chapter 1. From Classical to Quantum Mechanics

CHAPTER I Review of Modern Physics. A. Review of Important Experiments

End-of-Chapter Exercises

Chapter 6 - Electronic Structure of Atoms

Physics 116. Nov 21, Session 31 De Broglie, duality, and uncertainty. R. J. Wilkes

Chapter 6: The Electronic Structure of the Atom Electromagnetic Spectrum. All EM radiation travels at the speed of light, c = 3 x 10 8 m/s

Chapter 27 Lecture Notes

Dual Nature of Radiation and Matter GLIMPSES 1. Electron. It is an elementary particle having a negative charge of 1.6x C and mass 9.1x kg

λ = h = h p mv λ = h mv FXA 2008 Candidates should be able to :

WAVE PARTICLE DUALITY

FI 3103 Quantum Physics

Transcription:

Lecture Outline Chapter 30 Physics, 4 th Edition James S. Walker

Chapter 30 Quantum Physics

Units of Chapter 30 Blackbody Radiation and Planck s Hypothesis of Quantized Energy Photons and the Photoelectric Effect The Mass and Momentum of a Photon Photon Scattering and the Compton Effect

Units of Chapter 30 The de Broglie Hypothesis and Wave- Particle Duality The Heisenberg Uncertainty Principle Quantum Tunneling

30-1 Blackbody Radiation and Planck s Hypothesis of Quantized Energy An ideal blackbody absorbs all the light that is incident upon it.

30-1 Blackbody Radiation and Planck s Hypothesis of Quantized Energy An ideal blackbody is also an ideal radiator. If we measure the intensity of the electromagnetic radiation emitted by an ideal blackbody, we find:

30-1 Blackbody Radiation and Planck s Hypothesis of Quantized Energy This illustrates a remarkable experimental finding: The distribution of energy in blackbody radiation is independent of the material from which the blackbody is constructed it depends only on the temperature, T. The peak frequency is given by:

30-1 Blackbody Radiation and Planck s Hypothesis of Quantized Energy The peak wavelength increases linearly with the temperature. This means that the temperature of a blackbody can be determined by its color. Classical physics calculations were completely unable to produce this temperature dependence, leading to something called the ultraviolet catastrophe.

30-1 Blackbody Radiation and Planck s Hypothesis of Quantized Energy Classical predictions were that the intensity increased rapidly with frequency, hence the ultraviolet catastrophe.

30-1 Blackbody Radiation and Planck s Hypothesis of Quantized Energy Planck discovered that he could reproduce the experimental curve by assuming that the radiation in a blackbody came in quantized energy packets, depending on the frequency: The constant h in this equation is known as Planck s constant:

30-1 Blackbody Radiation and Planck s Hypothesis of Quantized Energy Planck s constant is a very tiny number; this means that the quantization of the energy of blackbody radiation is imperceptible in most macroscopic situations. It was, however, a most unsatisfactory solution, as it appeared to make no sense.

30-2 Photons and the Photoelectric Effect Einstein suggested that the quantization of light was real; that light came in small packets, now called photons, of energy:

30-2 Photons and the Photoelectric Effect Therefore, a more intense beam of light will contain more photons, but the energy of each photon does not change.

30-2 Photons and the Photoelectric Effect The photoelectric effect occurs when a beam of light strikes a metal, and electrons are ejected. Each metal has a minimum amount of energy required to eject an electron, called the work function, W 0. If the electron is given an energy E by the beam of light, its maximum kinetic energy is:

30-2 Photons and the Photoelectric Effect This diagram shows the basic layout of a photoelectric effect experiment.

30-2 Photons and the Photoelectric Effect Classical predictions: 1. Any beam of light of any color can eject electrons if it is intense enough. 2. The maximum kinetic energy of an ejected electron should increase as the intensity increases. Observations: 1. Light must have a certain minimum frequency in order to eject electrons. 2. More intensity results in more electrons of the same energy.

30-2 Photons and the Photoelectric Effect Explanations: 1. Each photon s energy is determined by its frequency. If it is less than the work function, electrons will not be ejected, no matter how intense the beam.

30-2 Photons and the Photoelectric Effect 2. A more intense beam means more photons, and therefore more ejected electrons.

30-3 The Mass and Momentum of a Photon Photons always travel at the speed of light (of course!). What does this tell us about their mass and momentum? The total energy can be written: Since the left side of the equation must be zero for a photon, it follows that the right side must be zero as well.

30-3 The Mass and Momentum of a Photon The momentum of a photon can be written: Dividing the momentum by the energy and substituting, we find:

30-3 The Mass and Momentum of a Photon Finally, we can write the momentum of a photon in the following way:

30-4 Photon Scattering and the Compton Effect The Compton effect occurs when a photon scatters off an atomic electron.

30-4 Photon Scattering and the Compton Effect In order for energy to be conserved, the energy of the scattered photon plus the energy of the electron must equal the energy of the incoming photon. This means the wavelength of the outgoing photon is longer than the wavelength of the incoming one:

30-5 The de Broglie Hypothesis and Wave- Particle Duality In 1923, de Broglie proposed that, as waves can exhibit particle-like behavior, particles should exhibit wave-like behavior as well. He proposed that the same relationship between wavelength and momentum should apply to massive particles as well as photons:

30-5 The de Broglie Hypothesis and Wave- Particle Duality The correctness of this assumption has been verified many times over. One way is by observing diffraction. We already know that X- rays can diffract from crystal planes:

30-5 The de Broglie Hypothesis and Wave- Particle Duality The same patterns can be observed using either particles or X-rays.

30-5 The de Broglie Hypothesis and Wave- Particle Duality Indeed, we can even perform Young s twoslit experiment with particles of the appropriate wavelength and find the same diffraction pattern.

30-5 The de Broglie Hypothesis and Wave- Particle Duality This is even true if we have a particle beam so weak that only one particle is present at a time we still see the diffraction pattern produced by constructive and destructive interference. Also, as the diffraction pattern builds, we cannot predict where any particular particle will land, although we can predict the final appearance of the pattern.

30-5 The de Broglie Hypothesis and Wave- Particle Duality These images show the gradual creation of an electron diffraction pattern.

30-6 The Heisenberg Uncertainty Principle The uncertainty just mentioned that we cannot know where any individual electron will hit the screen is inherent in quantum physics, and is due to the wavelike properties of matter.

30-6 The Heisenberg Uncertainty Principle The width of the central maximum is given by: Therefore, it would be possible to have a narrower central peak by using light of a shorter wavelength. However, from the de Broglie relation, as the wavelength goes down, the momentum goes up:

30-6 The Heisenberg Uncertainty Principle When the electrons diffract through the slit, they acquire a y-component of momentum that they had not had before. This leads to the uncertainty principle: If we know the position of a particle with greater precision, its momentum is more uncertain; if we know the momentum of a particle with greater precision, its position is more uncertain.

30-6 The Heisenberg Uncertainty Principle Mathematically,

30-6 The Heisenberg Uncertainty Principle The uncertainty principle can be cast in terms of energy and time rather than position and momentum: The effects of the uncertainty principle are generally not noticeable in macroscopic situations due to the smallness of Planck s constant, h.

30-7 Quantum Tunneling Waves can tunnel through narrow gaps of material that they otherwise would not be able to traverse. As the gap widens, the intensity of the transmitted wave decreases exponentially.

30-7 Quantum Tunneling Given their wavelike properties, it is not surprising that particles can tunnel as well. A practical application is the scanning tunneling microscope, which can image single atoms using the tunneling of electrons.

Summary of Chapter 30 An ideal blackbody absorbs all light incident on it. The distribution of energy within it as a function of frequency depends only on its temperature. Frequency of maximum radiation: Planck s hypothesis:

Summary of Chapter 30 Light is composed of photons, each with energy: In terms of wavelength: Photoelectric effect: photons eject electrons from metal surface. Minimum energy: work function, W 0 Minimum frequency:

Summary of Chapter 30 Photons have zero rest mass. Photon momentum, frequency, and wavelength: Compton effect: a photon scatters off an atomic electron, and exits with a longer wavelength:

Summary of Chapter 30 de Broglie hypothesis: particles have wavelengths, depending on their momentum: Both X-rays and electrons can be diffracted by crystals. Light and matter display both wavelike and particle-like properties.

Summary of Chapter 30 The position and momentum of waves and particles cannot both be determined simultaneously with arbitrary precision: Nor can the energy and time: Particles can tunnel through a region that classically would be forbidden to them.