Chapter 36: Problem 9
Why is a white-hot object hotter than a red-hot object?
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Chapter 36: Problem 9
Why is a white-hot object hotter than a red-hot object?
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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.
Now 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?
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 \(0.300 \mathrm{~W} / \mathrm{cm}^{2}\).
Consider 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?
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?
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