Exam 38: Photons and Matter Waves
Exam 1: Measurement37 Questions
Exam 2: Motion Along a Straight Line90 Questions
Exam 3: Vector32 Questions
Exam 4: Motion in Two and Three Dimensions53 Questions
Exam 5: Force and Motion I73 Questions
Exam 6: Force and Motion II74 Questions
Exam 7: Kinetic Energy and Work72 Questions
Exam 8: Potential Energy and Conservation of Energy62 Questions
Exam 9: Center of Mass and Linear Momentum98 Questions
Exam 10: Rotation99 Questions
Exam 11: Rolling, Torque, and Angular Momentum65 Questions
Exam 12: Equilibrium and Elasticity57 Questions
Exam 13: Gravitation54 Questions
Exam 14: Fluids87 Questions
Exam 15: Oscillations75 Questions
Exam 16: Waves I80 Questions
Exam 17: Waves II70 Questions
Exam 18: Temperature, Heat, and the First Law of Thermodynamics96 Questions
Exam 19: The Kinetic Theory of Gases111 Questions
Exam 20: Entropy and the Second Law of Thermodynamics61 Questions
Exam 21: Electric Charge51 Questions
Exam 22: Electric Fields52 Questions
Exam 23: Gauss Law39 Questions
Exam 24: Electric Potential50 Questions
Exam 25: Capacitance59 Questions
Exam 26: Current and Resistance54 Questions
Exam 27: Circuits73 Questions
Exam 28: Magnetic Fields51 Questions
Exam 29: Magnetic Fields Due to Currents48 Questions
Exam 30: Induction and Inductance90 Questions
Exam 31: Electromagnetic Oscillations and Alternating Current86 Questions
Exam 32: Maxwells Equations; Magnetism of Matter81 Questions
Exam 33: Electromagnetic Waves81 Questions
Exam 34: Images78 Questions
Exam 35: Interference45 Questions
Exam 36: Diffraction77 Questions
Exam 37: Relativity68 Questions
Exam 38: Photons and Matter Waves57 Questions
Exam 39: More About Matter Waves41 Questions
Exam 40: All About Atoms76 Questions
Exam 41: Conduction of Electricity in Solids49 Questions
Exam 42: Nuclear Physics68 Questions
Exam 43: Energy From the Nucleus50 Questions
Exam 44: Quarks, Leptons, and the Big Bang55 Questions
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The quantization of energy, E = nhf, is not important for an ordinary pendulum because:
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B
The concentration of photons in a uniform light beam with a wavelength of 500 nm is 1.7*1013 m - 3.The intensity of the beam is:
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D
The frequency of light beam A is twice that of light beam B.The ratio EA/EB of photon energies is:
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D
Light beams A and B have the same intensity but the wavelength associated with beam A is longer than that associated with beam B.The photon flux (number crossing a unit area per unit time)is:
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The main problem that physicists had in understanding blackbody radiation before Planck's work was:
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Consider the following: I.A photoelectric process in which all emitted electrons have energy less than hf, where f is the frequency of the incident light.
II.A photoelectric process in which some emitted electrons have kinetic energy greater than hf.
III.Compton scattering from stationary electrons for which the emitted light has a frequency that is greater than that of the incident light.
IV.Compton scattering from stationary electrons for which the emitted light has a frequency that is less than that of the incident light.
The only possible processes are:
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The surface of the Sun is at a temperature of approximately 5800 K, and radiates a peak wavelength of 500 nm.According to the Planck radiation law, what is its emitted intensity per unit wavelength at the peak?
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In Compton scattering from stationary electrons the largest change in wavelength that can occur is:
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Consider the following three particles:
Rank them according to the wavelengths of their waves, least to greatest.

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An electron with energy E is incident upon a potential energy barrier of height Epot < E and thickness L.The reflection coefficient R:
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A free electron in motion along the x axis has a localized wave function.The uncertainty in its momentum is decreased if:
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An electron with energy E is incident upon a potential energy barrier of height Epot > E and thickness L.The transmission coefficient T:
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Rank following electromagnetic radiations according to the energies of their photons, from least to greatest. 

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In Compton scattering from stationary particles the maximum change in wavelength can be made smaller by using:
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A non-relativistic free electron has kinetic energy K.If its wavelength doubles, its kinetic energy is:
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The work function for a certain sample is 2.3 eV.The stopping potential for electrons ejected from the sample by 7.0 * 1014-Hz electromagnetic radiation is:
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A free electron has a momentum of 5.0 *10-24 kg .m/s.Its wavelength, as given by its wave function, is:
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Maxwell's equations are to electric and magnetic fields as __________ equation is to the wave function of the particle.
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In order to tunnel through a potential barrier a particle must:
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