Chapter 36: Problem 28
The threshold wavelength for the photoelectric effect in a specific alloy is \(400 . \mathrm{nm}\). What is the work function in \(\mathrm{eV} ?\)
Chapter 36: Problem 28
The threshold wavelength for the photoelectric effect in a specific alloy is \(400 . \mathrm{nm}\). What is the work function in \(\mathrm{eV} ?\)
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Get started for freeNow consider de Broglie waves for a (relativistic) particle of mass \(m\), momentum \(p=m v \gamma\), and total energy \(E=m c^{2} \gamma\), with \(\gamma=\left[1-(v / c)^{2}\right]^{-1 / 2}\). The waves have wavelength \(\lambda=h / p\) and frequency \(f=E / h\) as before, but with the relativistic momentum and energy. a) Calculate the dispersion relation for these waves. b) Calculate the phase and group velocities of these waves. Now which corresponds to the classical velocity of the particle?
Consider a quantum state of energy \(E\), which can be occupied by any number \(n\) of some bosonic particles, including \(n=0\). At absolute temperature \(T\), the probability of finding \(n\) particles in the state is given by \(P_{n}=N \exp \left(-n E / k_{\mathrm{B}} T\right)\), where \(k_{\mathrm{B}}\) is Boltzmann's constant and the normalization factor \(N\) is determined by the requirement that all the probabilities sum to unity. Calculate the mean or expected value of \(n\), that is, the occupancy, of this state, given this probability distribution.
A free electron in a gas is struck by an \(8.5-\mathrm{nm} \mathrm{X}\) -ray, which experiences an increase in wavelength of \(1.5 \mathrm{pm} .\) How fast is the electron moving after the interaction with the X-ray?
Calculate the peak wavelengths of a) the solar light received by Earth, and b) light emitted by the Earth. Assume the surface temperatures of the Sun and the Earth are \(5800 . \mathrm{K}\) and \(300 . \mathrm{K},\) respectively.
A photovoltaic device uses monochromatic light of wavelength 700 . \(\mathrm{nm}\) that is incident normally on a surface of area \(10.0 \mathrm{~cm}^{2}\). Calculate the photon flux rate if the light intensity is \(0.300 \mathrm{~W} / \mathrm{cm}^{2}\).
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