Chapter 38: Q3P (page 1181)
At what rate does the Sun emit photons? For simplicity, assume that the Sun’s entire emission at the rate of is at the single wavelength of 550 nm.
Short Answer
The rate of emitted protons from the Sun is
Chapter 38: Q3P (page 1181)
At what rate does the Sun emit photons? For simplicity, assume that the Sun’s entire emission at the rate of is at the single wavelength of 550 nm.
The rate of emitted protons from the Sun is
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Get started for freeIf the de Broglie wavelength of a proton is , (a) what is the speed of the proton and (b) through what electric potential would the proton have to be accelerated to acquire this speed?
The meter was once defined as 1650763.73 wavelengths of the orange light emitted by a source containing krypton-86 atoms. What is the photon energy of that light?
Calculate the percentage change in photon energy during collision like that in Fig. 38-5 for and for radiation in
(a) the microwave range, with ;
(b) the visible range, with ;
(c) the x-ray range, with ; and
(d) the gamma-ray range, with a gamma photon energy of 1.0 MeV.
(e) What are your conclusions about the feasibility of detecting the Compton shift in these various regions of the electromagnetic spectrum, judging solely by the criterion of energy loss in a single photon-electron encounter?
The Sun is approximately an ideal blackbody radiator with surface temperature of 5800 K.
(a) Find the wavelength at which its spectral radiancy is maximum and
(b) identify the type of magnetic wave corresponding to that wavelength.
(c) As we shall discuss in chapter 44, the universe is approximately an ideal blackbody radiator with radiation emitted when atoms first formed. Today the spectral radiancy of that radiation peaks at a wavelength of 1.06 mm (in the microwave region). What is the corresponding temperature of the universe?
Through what angle must aphoton be scattered by a free electron so that the photon loses of its energy?
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