Chapter 40: Q1P (page 1247)
An electron in a hydrogen atom is in a state with . What is the minimum possible value of the semi-classical angle between and ?
Short Answer
The possible value of the semi-classical angle between and is .
Chapter 40: Q1P (page 1247)
An electron in a hydrogen atom is in a state with . What is the minimum possible value of the semi-classical angle between and ?
The possible value of the semi-classical angle between and is .
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Get started for freeA rectangular corral of widths and contains seven electrons. What multiple of gives the energy of the ground state of the system? Assume that the electrons do not interact with one another, and do not neglect spin.
The active medium in a particular laser generates laser light at a wavelength of 694nm is 6.00 cm long and 1.00 cm in diameter. (a) Treat the medium as an optical resonance cavity analogous to a closed organ pipe. How many standing-wave nodes are there along the laser axis? (b) By what amountwould the beam frequency have to shift to increase this number by one? (c) Show that is just the inverse of the travel time of laser light for one round trip back and forth along the laser axis. (d) What is the corresponding fractional frequency shift ? The appropriate index of refraction of the lasing medium (a ruby crystal) is 1.75.
Comet stimulated emission.When a comet approaches the Sun, the increased warmth evaporates water from the ice on the surface of the comet nucleus, producing a thin atmosphere of water vapor around the nucleus. Sunlight can then dissociate molecules in the vapor to H atoms and OH molecules. The sunlight can also excite the OH molecules to higher energy levels.
When the comet is still relatively far from the Sun, the sunlight causes equal excitation to the and levels (Fig. 40-28a). Hence, there is no population inversion between the two levels. However, as the comet approaches the Sun, the excitation to thelevel decreases and population inversion occurs. The reason has to do with one of the many wavelengths—said to be Fraunhofer lines—that are missing in sunlight because, as the light travels outward through the Sun’s atmosphere, those particular wavelengths are absorbed by the atmosphere.
As a comet approaches the Sun, the Doppler Effect due to the comet’s speed relative to the Sun shifts the Fraunhofer lines in wavelength, apparently overlapping one of them with the wavelength required for excitation to the level in OH molecules. Population inversion then occurs in those molecules, and they radiate stimulated emission (Fig. 40 28b). For example, as comet Kouhoutek approached the Sun in December 1973 and January 1974, it radiated stimulated emission at about during mid-January. (a) What was the energy difference for that emission? (b) In what region of the electromagnetic spectrum was the emission?
When electrons bombard a molybdenum target, they produce both continuous and characteristic x-rays as shown in Fig. 40-13. In that figure the kinetic energy of the incident electrons is 35.0 keV. If the accelerating potential is increased to 50.0 keV, (a) what is the value of , and (b) do the wavelengths of the role="math" localid="1661497027757" and lines increase, decrease, or remain the same?
X-rays are produced in an x-ray tube by electrons accelerated through an electric potential difference of 50 kV. Let be the kinetic energy of an electron at the end of the acceleration. The electron collides with a target nucleus (assume the nucleus remains stationary) and then has kinetic energy . (a) What wavelength is associated with the photon that is emitted? The electron collides with another target nucleus (assume it, too, remains stationary) and then has kinetic energy . (b) What wavelength is associated with the photon that is emitted?
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