Exam 38: Photons and Matter Waves

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   (x)is the wave function for a particle moving along the x axis.The probability that the particle is in the interval from x = a to x = b is given by: (x)is the wave function for a particle moving along the x axis.The probability that the particle is in the interval from x = a to x = b is given by:

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In Compton scattering from stationary electrons the largest change in wavelength that can occur is:

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In order to tunnel through a potential barrier a particle must:

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The intensity of a light beam with a wavelength of 500 nm is 2000 W/m2.The photon flux is about:

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An electron with energy E is incident on a potential energy barrier of height Epot and thickness L.The probability of tunneling increases if:

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In a photoelectric effect experiment no electrons are ejected if the frequency of the incident light is less than A/h, where h is the Planck constant and A is:

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Of the following, Compton scattering from electrons is most easily observed for:

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The diagram shows the graphs of the stopping potential as a function of the frequency of the incident light for photoelectric experiments performed on three different materials.Rank the materials according to the values of their work functions, from least to greatest. The diagram shows the graphs of the stopping potential as a function of the frequency of the incident light for photoelectric experiments performed on three different materials.Rank the materials according to the values of their work functions, from least to greatest.

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The quantization of energy, E = nhf, is not important for an ordinary pendulum because:

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Monoenergetic electrons are incident on a single slit barrier.If the energy of each incident electron is increased the central maximum of the diffraction pattern:

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If the kinetic energy of a non-relativistic free electron doubles, the frequency of its wave function changes by the factor:

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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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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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Electromagnetic radiation with a wavelength of 3.5 * 10-12 m is scattered from stationary electrons, and photons that have been scattered through 50° are detected.After a scattering event the magnitude of the photon's momentum is:

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Rank following electromagnetic radiations according to the energies of their photons, from least to greatest. Rank following electromagnetic radiations according to the energies of their photons, from least to greatest.

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The units of the Planck constant h are those of:

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The reflection coefficient R for a certain barrier tunneling problem is 0.80.The corresponding transmission coefficient T is:

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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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Consider the following three particles: Consider the following three particles:   Rank them according to the wavelengths of their matter waves, least to greatest. Rank them according to the wavelengths of their matter waves, least to greatest.

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The wavelength of light beam B is twice the wavelength of light beam B.The energy of a photon in beam A is:

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