* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Download Chapter 30 Quantum Physics
Planck's law wikipedia , lookup
Bremsstrahlung wikipedia , lookup
Elementary particle wikipedia , lookup
Relativistic quantum mechanics wikipedia , lookup
Renormalization wikipedia , lookup
Hydrogen atom wikipedia , lookup
Wheeler's delayed choice experiment wikipedia , lookup
Electron configuration wikipedia , lookup
X-ray photoelectron spectroscopy wikipedia , lookup
Particle in a box wikipedia , lookup
Quantum electrodynamics wikipedia , lookup
Bohr–Einstein debates wikipedia , lookup
Ultrafast laser spectroscopy wikipedia , lookup
Delayed choice quantum eraser wikipedia , lookup
Atomic theory wikipedia , lookup
Double-slit experiment wikipedia , lookup
X-ray fluorescence wikipedia , lookup
Matter wave wikipedia , lookup
Wave–particle duality wikipedia , lookup
Theoretical and experimental justification for the Schrödinger equation wikipedia , lookup
12/7/2011 Units of Chapter 30 Chapter 30 Quantum Physics • 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 Copyright © 2010 Pearson Education, Inc. Copyright © 2010 Pearson Education, Inc. Units of Chapter 30 • The de Broglie Hypothesis and WaveParticle Duality • The Heisenberg Uncertainty Principle • Quantum Tunneling Development of Quantum Physics • Problems remained from classical mechanics that relativity didn’t explain • Blackbody Radiation – The electromagnetic radiation emitted by a heated object • Photoelectric Effect – Emission of electrons by an illuminated metal • Spectral Lines – Emission of sharp spectral lines by gas atoms in an electric discharge tube Copyright © 2010 Pearson Education, Inc. Development of Quantum Physics • 1900 to 1930 – Development of ideas of quantum mechanics Copyright © 2010 Pearson Education, Inc. 30-1 Blackbody Radiation and Planck’s Hypothesis of Quantized Energy An ideal blackbody absorbs all the light that is incident upon it. • Also called wave mechanics • Highly successful in explaining the behavior of atoms, molecules, and nuclei • Quantum Mechanics reduces to classical mechanics when applied to macroscopic systems • Involved a large number of physicists – Planck introduced basic ideas – Mathematical developments and interpretations involved such people as Einstein, Bohr, Schrödinger, de Broglie, Heisenberg, Born and Dirac Copyright © 2010 Pearson Education, Inc. Copyright © 2010 Pearson Education, Inc. 1 12/7/2011 30-1 Blackbody Radiation and Planck’s Hypothesis of Quantized Energy 30-1 Blackbody Radiation and Planck’s Hypothesis of Quantized Energy Classical physics calculations were completely unable to produce this temperature dependence, leading to something called the “ultraviolet catastrophe.” An ideal blackbody is also an ideal radiator. If we measure the intensity of the electromagnetic radiation emitted by an ideal blackbody, we find: Copyright © 2010 Pearson Education, Inc. 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: Rayleigh -Jeans Planck 8π f c3 2 k BT hf 8πf 2 hf (e k BT − 1) −1 c3 Copyright © 2010 Pearson Education, Inc. 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, W0. If the electron is given an energy E by the beam of light, its maximum kinetic energy is: The constant h in this equation is known as Planck’s constant: Copyright © 2010 Pearson Education, Inc. 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. Copyright © 2010 Pearson Education, Inc. Copyright © 2010 Pearson Education, Inc. 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: A more intense beam of light will contain more photons, but the energy of each photon does not change. Example: A laser emits 2.5 W of light energy at the wavelength of 532 nm, determine the number of photons given off by the laser per second. Copyright © 2010 Pearson Education, Inc. 2 12/7/2011 30-2 Photons and the Photoelectric Effect 30-3 The Mass and Momentum of a Photon Explanations: Photons always travel at the speed of light (of course!). What does this tell us about their mass and momentum? 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. The total energy can be written: Example: A sodium surface is illuminated with light of wavelength 300 nm. The work function of solium is 2.46 eV. Calculate (a) the energy of each photon in electron volts, (b) the maximum kinetic energy of the ejected photoelectrons, and (c) the cutoff wavelength for the sodium. Copyright © 2010 Pearson Education, Inc. Since the left side of the equation must be zero for a photon, it follows that the right side must be zero as well. Copyright © 2010 Pearson Education, Inc. 30-3 The Mass and Momentum of a Photon Energy-momentum equation in Relativity: 2 2 2 E = E 0+ p c 2 30-4 Photon Scattering and the Compton Effect The Compton effect occurs when a photon scatters off an atomic electron. With E0 = m0c2 = 0, And finally, Copyright © 2010 Pearson Education, Inc. 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: Copyright © 2010 Pearson Education, Inc. Copyright © 2010 Pearson Education, Inc. 30-5 The de Broglie Hypothesis and WaveParticle 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: Copyright © 2010 Pearson Education, Inc. 3 12/7/2011 30-5 The de Broglie Hypothesis and WaveParticle Duality Indeed, we can even perform Young’s twoslit experiment with particles of the appropriate wavelength and find the same diffraction pattern. 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. Copyright © 2010 Pearson Education, Inc. Copyright © 2010 Pearson Education, Inc. 30-5 The de Broglie Hypothesis and WaveParticle Duality These images show the gradual creation of an electron diffraction pattern. Low Energy Electron Diffraction (LEED) pattern from Silicon (111) surface. Copyright © 2010 Pearson Education, Inc. 30-5 The de Broglie Hypothesis and WaveParticle Duality The same patterns can be observed using either particles or X-rays. Copyright © 2010 Pearson Education, Inc. 30-5 The de Broglie Hypothesis and WaveParticle Duality 30-5 The de Broglie Hypothesis and WaveParticle 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: Example: A beam of neutrons with a de Broglie wavelength of 0.240 nm diffracts from a crystal of table salt, which has an interionic spacing of 0.283 nm. (a) What is the speed of the neutrons? (b) What is the angle of the second interference maximum? Copyright © 2010 Pearson Education, Inc. 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. Copyright © 2010 Pearson Education, Inc. 4 12/7/2011 30-6 The Heisenberg Uncertainty Principle 30-6 The Heisenberg Uncertainty Principle Mathematically, 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. Copyright © 2010 Pearson Education, Inc. Copyright © 2010 Pearson Education, Inc. 30-6 The Heisenberg Uncertainty Principle Thought Experiment – the 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. • • • • A thought experiment for viewing an electron with a powerful microscope In order to see the electron, at least one photon must bounce off it During this interaction, momentum is transferred from the photon to the electron Therefore, the light that allows you to accurately locate the electron changes the momentum of the electron Copyright © 2010 Pearson Education, Inc. 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. Copyright © 2010 Pearson Education, Inc. 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. Copyright © 2010 Pearson Education, Inc. 5 12/7/2011 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: Summary of Chapter 30 • Light is composed of photons, each with energy: • In terms of wavelength: • Photoelectric effect: photons eject electrons from metal surface. • Planck’s hypothesis: • Minimum energy: work function, W0 • Minimum frequency: Copyright © 2010 Pearson Education, Inc. Copyright © 2010 Pearson Education, Inc. Summary of Chapter 30 • Photons have zero rest mass. Summary of Chapter 30 • de Broglie hypothesis: particles have wavelengths, depending on their momentum: • Photon momentum, frequency, and wavelength: • Compton effect: a photon scatters off an atomic electron, and exits with a longer wavelength: Copyright © 2010 Pearson Education, Inc. • Both X-rays and electrons can be diffracted by crystals. • Light and matter display both wavelike and particle-like properties. Copyright © 2010 Pearson Education, Inc. 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. Copyright © 2010 Pearson Education, Inc. 6