Chapter 36: Problem 39
Calculate the wavelength of a) a \(2.00 \mathrm{eV}\) photon, and b) an electron with kinetic energy \(2.00 \mathrm{eV}\).
Chapter 36: Problem 39
Calculate the wavelength of a) a \(2.00 \mathrm{eV}\) photon, and b) an electron with kinetic energy \(2.00 \mathrm{eV}\).
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Get started for freeConsider de Broglie waves for a Newtonian particle of mass \(m,\) momentum \(p=m v,\) and energy \(E=p^{2} /(2 m),\) that is, waves with wavelength \(\lambda=h / p\) and frequency \(f=E / h\). a) Calculate the dispersion relation \(\omega=\omega(k)\) for these waves. b) Calculate the phase and group velocities of these waves. Which of these corresponds to the classical velocity of the particle?
If I look in a mirror while wearing a blue shirt, I see a blue shirt in my reflection, not a red shirt. But according to the Compton effect, the photons that bounce back should have a lower energy and therefore a longer wavelength. Explain why my reflection shows the same color shirt as am wearing.
In a photoelectric effect experiment, a laser beam of unknown wavelength is shined on a cesium cathode (work function \(\phi=2.100 \mathrm{eV}\) ). It is found that a stopping potential of \(0.310 \mathrm{~V}\) is needed to eliminate the current. Next, the same laser is shined on a cathode made of an unknown material, and a stopping potential of \(0.110 \mathrm{~V}\) is found to be needed to eliminate the current. a) What is the work function for the unknown cathode? b) What would be a possible candidate for the material of this unknown cathode?
Calculate the range of temperatures for which the peak emission of the blackbody radiation from a hot filament occurs within the visible range of the electromagnetic spectrum. Take the visible spectrum as extending from \(380 \mathrm{nm}\) to \(780 \mathrm{nm}\). What is the total intensity of the radiation from the filament at these two temperatures?
Scintillation detectors for gamma rays transfer the energy of a gamma-ray photon to an electron within a crystal, via the photoelectric effect or Compton scattering. The electron transfers its energy to atoms in the crystal, which re-emit it as a light flash detected by a photomultiplier tube. The charge pulse produced by the photomultiplier tube is proportional to the energy originally deposited in the crystal; this can be measured so an energy spectrum can be displayed. Gamma rays absorbed by the photoelectric effect are recorded as a photopeak in the spectrum, at the full energy of the gammas. The Compton-scattered electrons are also recorded, at a range of lower energies known as the Compton plateau. The highest-energy of these form the Compton edge of the plateau. Gamma-ray photons scattered \(180 .^{\circ}\) by the Compton effect appear as a backscatter peak in the spectrum. For gamma-ray photons of energy \(511 \mathrm{KeV}\) calculate the energies of the Compton edge and the backscatter peak in the spectrum.
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