Chapter 6: Q. 6.35 (page 246)
Verify from Maxwell speed distribution that the most likely speed of a molecule is.
Short Answer
The most likely speed of a molecule is.
Chapter 6: Q. 6.35 (page 246)
Verify from Maxwell speed distribution that the most likely speed of a molecule is.
The most likely speed of a molecule is.
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Get started for freeA water molecule can vibrate in various ways, but the easiest type of vibration to excite is the "flexing' mode in which the hydrogen atoms move toward and away from each other but the HO bonds do not stretch. The oscillations of this mode are approximately harmonic, with a frequency of 4.8 x 1013Hz. As for any quantum harmonic oscillator, the energy levels are , and so on. None of these levels are degenerate.
(a) state and in each of the first two excited states, assuming that it is in equilibrium with a reservoir (say the atmosphere) at 300 K. (Hint: Calculate 2 by adding up the first few Boltzmann factors, until the rest are negligible.) Calculate the probability of a water molecule being in its flexing ground
(b) Repeat the calculation for a water molecule in equilibrium with a reservoir at 700 K (perhaps in a steam turbine).
For a mole nitrogen gas at room temperature and atmospheric pressure, compute the following and . (The electronic ground state of nitrogen is not degenerate.)
Consider an ideal gas of highly relativistic particles ( such as photons or fast-moving electrons) whose energy-momentum relation is instead of . Assume that these particles live in a one-dimensional universe. By following the same logic as above, derive a formula for the single particle partition function,, for one particle in the gas.
The dissociation of molecular hydrogen into atomic hydrogen, can be treated as an ideal gas reaction using the techniques of Section 5.6. The equilibrium constant K for this reaction is defined as
whereis a reference pressure conventionally taken to beand the other P's are the partial pressures of the two species at equilibrium. Now, using the methods of Boltzmann statistics developed in this chapter, you are ready to calculate K from first principles. Do so. That is, derive a formula for K in terms of more basic quantities such as the energy needed to dissociate one molecule (see Problem 1.53) and the internal partition function for molecular hydrogen. This internal partition function is a product of rotational and vibrational contributions, which you can estimate using the methods and data in Section 6.2. (An molecule doesn't have any electronic spin degeneracy, but an H atom does-the electron can be in two different spin states. Neglect electronic excited states, which are important only at very high temperatures. The degeneracy due to nuclear spin alignments cancels, but include it if you wish.) Calculate K numerically at Discuss the implications, working out a couple of numerical examples to show when hydrogen is mostly dissociated and when it is not.
Estimate the probability that a hydrogen atom at room temperature is in one of its first excited states (relative to the probability of being in the ground state). Don't forget to take degeneracy into account. Then repeat the calculation for a hydrogen atom in the atmosphere of the star UMa, whose surface temperature is approximately 9500 K.
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