Chapter 36: Problem 9
Why is a white-hot object hotter than a red-hot object?
Chapter 36: Problem 9
Why is a white-hot object hotter than a red-hot object?
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Get started for freeAn X-ray photon with an energy of \(50.0 \mathrm{keV}\) strikes an electron that is initially at rest inside a metal. The photon is scattered at an angle of \(45^{\circ} .\) What is the kinetic energy and momentum (magnitude and direction) of the electron after the collision? You may use the nonrelativistic relationship connecting the kinetic energy and momentum of the electron.
The Solar Constant measured by Earth satellites is roughly \(1400 . \mathrm{W} / \mathrm{m}^{2}\). Though the Sun emits light of different wavelengths, the peak of the wavelength spectrum is at \(500 . \mathrm{nm}\) a) Find the corresponding photon frequency. b) Find the corresponding photon energy. c) Find the number flux of photons arriving at Earth, assuming that all light emitted by the Sun has the same peak wavelength.
Ultra-high-energy gamma rays are found to come from the Equator of our galaxy, with energies up to \(3.5 \cdot 10^{12} \mathrm{eV}\). What is the wavelength of this light? How does the energy of this light compare to the rest mass of a proton?
Given that the work function of tungsten is \(4.55 \mathrm{eV}\) what is the stopping potential in an experiment using tungsten cathodes at \(360 \mathrm{nm} ?\)
Consider the equivalent of Compton scattering, but the case in which a photon scatters off of a free proton. a) If \(140 .-\mathrm{keV} \mathrm{X}\) -rays bounce off of a proton at \(90.0^{\circ},\) what is their fractional change in energy \(\left(E_{0}-E\right) / E_{0} ?\) b) What energy of photon would be necessary to cause a \(1.00 \%\) change in energy at \(90.0^{\circ}\) scattering?
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