PHYS 3313 – Section 001 Lecture #12

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PHYS 3313 – Section 001 Lecture #12 Monday, Feb. 27, 2017 Dr. Jaehoon Yu Photoelectric Effect Compton Effect Pair production/Pair annihilation Rutherford Scattering Experiment and Rutherford Atomic Model Monday, Feb. 27, 2017 PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu

PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu Announcements Midterm Exam In class Wednesday, March. 8 Covers from CH1.1 through what we learn March 6 plus the math refresher in the appendices Mid-term exam constitutes 20% of the total Please do NOT miss the exam! You will get an F if you miss it. BYOF: You may bring a one 8.5x11.5 sheet (front and back) of handwritten formulae and values of constants for the exam No derivations, word definitions or solutions of any problems! Eg., Lorentz velocity transformation NOT allowed! No additional formulae or values of constants will be provided! Quiz 2 results Class Average: 34.5/60 Equivalent to : 57.5/100 Previous result: 20.8/100 Class top score: 60/60 Monday, Feb. 27, 2017 PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu

Experimental Observations KE proportional to frequency!! The same V0 but higher current The same current!! Number of photoelectrons proportional to light intensity!! Wednesday, Feb. 22, 2017 PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu

Summary of Experimental Observations Light intensity does not affect the KE of the photoelectrons The max KE of the photoelectrons for a given emitter material depends only on the frequency of the light The smaller the work function φ of the emitter material, the smaller is the threshold frequency of the light that can eject photoelectrons. When the photoelectrons are produced, their number is proportional to the intensity of light. The photoelectrons are emitted almost instantly following the illumination of the photocathode, independent of the intensity of the light.  Totally unexplained by classical physics Wednesday, Feb. 22, 2017 PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu

Einstein’s Theory of Photoelectric Effect Einstein suggested that the electromagnetic radiation of the light is quantized into particles called photons. Each photon has the energy quantum: where f is the frequency of the light and h is Planck’s constant. The photon travels at the speed of light in vacuum, and its wavelength is given by Monday, Feb. 27, 2017 PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu

Experimental Observations The same current!! Number of photoelectrons proportional to light intensity!! Wednesday, Feb. 22, 2017 PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu

PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu Einstein’s Theory Conservation of energy yields: where φ is the work function of the metal The photon energy can then be written The retarding potentials measure the KE of the most energetic photoelectrons. Monday, Feb. 27, 2017 PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu

Quantum Interpretation KE of the electron depends only on the light frequency and the work function φ of the material not the light intensity at all Einstein in 1905 predicted that the stopping potential was linearly proportional to the light frequency, with the slope h, the same constant found by Planck. From this, Einstein concluded that light is a particle with energy: Was he already thinking about particle/wave duality? Monday, Feb. 27, 2017 PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu

Ex 3.11: Photoelectric Effect Light of wavelength 400nm is incident upon lithium (φ=2.93eV). Calculate (a) the photon energy (eV) and (b) the stopping potential V0. Since the wavelength is known, we use plank’s formula: The stopping potential can be obtained using Einstein’s formula for photoelectron energy Monday, Feb. 27, 2017 PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu

PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu X-Ray Production Bremsstrahlung (German word for braking radiation): Radiation of a photon from an energetic electron passing through matter due to an acceleration Since linear momentum must be conserved, the nucleus absorbs very little energy, and it is ignored. The final energy of the electron is determined from the conservation of energy An electron that loses a large amount of energy will produce an X-ray photon. Current passing through a filament produces copious numbers of electrons by thermionic emission. These electrons are focused by the cathode structure into a beam and are accelerated by potential differences of thousands of volts until they impinge on a metal anode surface, producing x rays by bremsstrahlung as they stop in the anode material X-ray wavelengths range 0.01 – 10nm. What is the minimum energy of an electron to produce X-ray? Monday, Feb. 27, 2017 PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu

Inverse Photoelectric Effect. Conservation of energy requires that the electron KE equals the maximum photon energy Work function neglected since it’s small compared to the potential energy of the electron. This is the Duane-Hunt limit The photon wavelength depends only on the accelerating voltage The same for all targets. Monday, Feb. 27, 2017 PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu

PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu Compton Effect When a photon enters matter, it is likely to interact with one of the atomic electrons. The photon is scattered from only one electron The laws of conservation of energy and momentum apply as in any elastic collision between two particles. The momentum of a particle moving at the speed of light is The electron energy can be written as Change of the scattered photon wavelength is known as the Compton effect: Monday, Feb. 27, 2017 PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu

Pair Production and Annihilation If a photon can create an electron, it must also create a positive charge to balance charge conservation. In 1932, C. D. Anderson observed a positively charged electron (e+) in cosmic radiation. This particle, called a positron, had been predicted to exist several years earlier by P. A. M. Dirac. A photon’s energy can be converted entirely into an electron and a positron in a process called pair production. Can only happen inside a material How much energy do you think is needed? Monday, Feb. 27, 2017 PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu

Pair Production in Empty Space? Energy conservation for pair production in empty space Momentum conservation yields Thus max momentum exchange Recall that the total energy for a particle can be written as However this yields a contradiction: and hence the conversion of energy in empty space is impossible and thus pair production cannot happen in empty space Monday, Feb. 27, 2017 PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu

Pair Production in Matter Since the relations and contradict each other, a photon can not produce an electron and a positron in empty space. In the presence of matter, however, the nucleus absorbs some energy and momentum. The photon energy required for pair production in the presence of matter is Monday, Feb. 27, 2017 PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu

PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu Pair Annihilation A positron going through matter will likely annihilate with an electron. A positron is drawn to an electron and form an atom-like configuration called positronium. Pair annihilation in empty space will produce two photons to conserve momentum. Annihilation near a nucleus can result in a single photon. Conservation of energy: Conservation of momentum: The two photons will be almost identical, so that The two photons from a positronium annihilation will move in the opposite directions with an energy of: Monday, Feb. 27, 2017 PHYS 3313-001, Spring 2017 Dr. Jaehoon Yu