Chapter 6: Q. 6.33 (page 246)
Calculate the most probable speed, average speed and rms speed for Oxygenmolecules at room temperature.
Short Answer
The most probable speed is, the average speed isand the rms speed is.
Chapter 6: Q. 6.33 (page 246)
Calculate the most probable speed, average speed and rms speed for Oxygenmolecules at room temperature.
The most probable speed is, the average speed isand the rms speed is.
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Get started for freeIn problem 6.20 you computed the partition function for a quantum harmonic oscillator :, where is the spacing between energy levels.
(a) Find an expression for the Helmholtz free energy of a system of harmonic oscillators.
(b) Find an expression for the entropy of this system as a function of temperature. (Don't worry, the result is fairly complicated.)
In this problem you will investigate the behavior of ordinary hydrogen, , at low temperatures. The constant is. As noted in the text, only half of the terms in the rotational partition function, , contribute for any given molecule. More precisely, the set of allowed values is determined by the spin configuration of the two atomic nuclei. There are four independent spin configurations, classified as a single "singlet" state and three "triplet" states. The time required for a molecule to convert between the singlet and triplet configurations is ordinarily quite long, so the properties of the two types of molecules can be studied independently. The singlet molecules are known as parahydrogen while the triplet molecules are known as orthohydrogen.
(a) For parahydrogen, only the rotational states with even values of j are allowed.Use a computer (as in ) to calculate the rotational partition function, average energy, and heat capacity of a parahydrogen molecule. Plot the heat capacity as a function of
(b) For orthohydrogen, only the rotational states with odd values of are allowed. Repeat part (a) for orthohydrogen.
(c) At high temperature, where the number of accessible even-j states is essentially the same as the number of accessible odd-j states, a sample of hydrogen gas will ordinarily consist of a mixture of parahydrogen and orthohydrogen. A mixture with these proportions is called normal hydrogen. Suppose that normal hydrogen is cooled to low temperature without allowing the spin configurations of the molecules to change. Plot the rotational heat capacity of this mixture as a function of temperature. At what temperature does the rotational heat capacity fall to half its hightemperature value (i.e., to per molecule)?
(d) Suppose now that some hydrogen is cooled in the presence of a catalyst that allows the nuclear spins to frequently change alignment. In this case all terms in the original partition function are allowed, but the odd-j terms should be counted three times each because of the nuclear spin degeneracy. Calculate the rotational partition function, average energy, and heat capacity of this system, and plot the heat capacity as a function of .
(e) A deuterium molecule, , has nine independent nuclear spin configurations, of which six are "symmetric" and three are "antisymmetric." The rule for nomenclature is that the variety with more independent states gets called "ortho-," while the other gets called "para-." For orthodeuterium only even-j rotational states are allowed, while for paradeuterium only oddj states are allowed. Suppose, then, that a sample of gas, consisting of a normal equilibrium mixture of ortho and para, is cooled without allowing the nuclear spin configurations to change. Calculate and plot the rotational heat capacity of this system as a function of temperature.*
Cold interstellar molecular clouds often contain the molecule cyanogen (CN), whose first rotational excited states have an energy of 4.7x 10-4 eV (above the ground state). There are actually three such excited states, all with the same energy. In 1941, studies of the absorption spectrum of starlight that passes | through these molecular clouds showed that for every ten CN molecules that are in the ground state, approximately three others are in the three first excited states (that is, an average of one in each of these states). To account for this data, astronomers suggested that the molecules might be in thermal equilibrium with some "reservoir" with a well-defined temperature. What is that temperature?
Use Boltzmann factors to derive the exponential formula for the density of an isothermal atmosphere, already derived in Problems 1.16 and 3.37. (Hint: Let the system be a single air molecule, let s1 be a state with the molecule at sea level, and let s2 be a state with the molecule at height z.)
In the low-temperature limit , each term in the rotational partition function is much smaller than the one before. Since the first term is independent of , cut off the sum after the second term and compute the average energy and the heat capacity in this approximation. Keep only the largest T-dependent term at each stage of the calculation. Is your result consistent with the third law of thermodynamics? Sketch the behavior of the heat capacity at all temperature, interpolating between the high-temperature and low- temperature expressions.
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