Chapter 38: Q82P (page 1185)
Derive Eq. 38-11, the equation for the Compton shift, from Eqs. 38-8, 38-9, and 38-10 by eliminating v and .
Short Answer
The equation 38-11 is derived as follows:
Chapter 38: Q82P (page 1185)
Derive Eq. 38-11, the equation for the Compton shift, from Eqs. 38-8, 38-9, and 38-10 by eliminating v and .
The equation 38-11 is derived as follows:
All the tools & learning materials you need for study success - in one app.
Get started for freeLight strikes a sodium surface, causing photoelectric emission. The stopping potential for the ejected electrons is 50 V, and the work function of sodium is 2.2 eV. What is the wavelength of the incident light?
If 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 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?
Question: You will find in Chapter 39 that electrons cannot move in definite orbits within atoms, like the planets in our solar system. To see why, let us try to “observe” such an orbiting electron by using a light microscope to measure the electron’s presumed orbital position with a precision of, say, (a typical atom has a radius of about localid="1663132292844" ). The wavelength of the light used in the microscope must then be about . (a) What would be the photon energy of this light? (b) How much energy would such a photon impart to an electron in a head-on collision? (c) What do these results tell you about the possibility of “viewing” an atomic electron at two or more points along its presumed orbital path? (Hint:The outer electrons of atomsare bound to the atom by energies of only a few electron-volts.)
In a photoelectric experiment using a sodium surface, you find a stopping potential of 1.85 V for a wavelength of and a stopping potential of 0.820 V for a wavelength of 400 nm. From these data find (a) a value for the Planck constant, (b) the work function for sodium, and (c) the cutoff wavelength for sodium?
What do you think about this solution?
We value your feedback to improve our textbook solutions.