 9.1: How relevant is the Heisenberg uncertainty principlein frustrating ...
 9.2: Why might the measured molar heat capacity of Cl2not match the pred...
 9.3: In a diatomic gas why should it be more diffi cult toexcite the vib...
 9.4: What is the physical signifi cance of the rootmeansquarespeed in a...
 9.5: An insulated container fi lled with an ideal gas movesthrough fi el...
 9.6: Maxwell conceived of a device (later called Maxwellsdemon) that cou...
 9.7: If the distribution function f(q) for some physicalproperty q is ev...
 9.8: If a collection of particles are identical, how can theybe distingu...
 9.9: Which of the following act as fermions and which asbosons: hydrogen...
 9.10: Theorists tend to believe that free quarks (with charge 23e and 13e...
 9.11: Explain why you expect E to be greater than 12EF[Equation (9.45)].
 9.12: Why doesnt the total energy of a collection of fermionsapproach zer...
 9.13: How would the behavior of metals be different if electronswere boso...
 9.14: What would happen to the Planck distribution andthe behavior of liq...
 9.15: If only the superfl uid component of liquid heliumfl ows through a ...
 9.16: Why is BBE 1 the minimum allowed value in theintegral in Equation (...
 9.17: Discuss similarities and differences between an atomlaser and an op...
 9.18: One way to decide whether MaxwellBoltzmann statisticsare valid is ...
 9.19: Use Equation (9.24) to turn the Maxwell speed distribution,Equation...
 9.20: Consider an atom with a magnetic moment and atotal spin 1/2. The at...
 9.21: The Fermi energy can be defi ned as the energy atwhich the Fermi fa...
 9.22: At T 0, what fraction of electrons have energyE E?
 9.23: Silver has exactly one conduction electron per atom.(a) Use the den...
 9.24: What fraction of the electrons in a good conductorhave energies bet...
 9.25: Use the data in to compute (a) EF and (b)uF for silver.
 9.26: The Fermi energy for gold is 5.51 eV at T 293 K.(a) Find the averag...
 9.27: The density of pure copper is 8.92 103 kg/m3, and itsmolar mass is ...
 9.28: Aluminum has a density of 2.70 103 kg/m3 at atemperature of 293 K, ...
 9.29: Compute the Fermi speed for (a) Ca (EF 4.69 eV)and (b) Be (EF 14.3 ...
 9.30: Verify that Equation (9.35) is valid in the limit T S 0.
 9.31: Show that in general (that is, T 0) the energy distributionof N ele...
 9.32: Use the result of with copper (EF 7.0 eV)to sketch n(E) at (a) T 0,...
 9.33: Use numerical integration of the function given in to verify that q...
 9.34: Use numerical integration of the function given in to fi nd the fra...
 9.35: In a neutron star the entire stars mass has collapsedessentially to...
 9.36: Consider a collection of fermions at T 293 K. Findthe probability t...
 9.37: Suppose you have an ideal gas of fermions at roomtemperature (293 K...
 9.38: Gold is a dense metal, with a density of 1.93 104 kg/m3 at T 300 K....
 9.39: Next to helium, the lightest noble gas is neon. (a) Estimatethe tem...
 9.40: Consider the problem of photons in a spherical cavityat temperature...
 9.41: Use numerical integration on a computer to verify theoutput of the ...
 9.42: Show that the wave functions in Equations (9.67) satisfythe require...
 9.43: Assume that air is an ideal gas under a uniform gravitationalfi eld...
 9.44: Use the law of atmospheres ( 43) to comparethe air densities at sea...
 9.45: Consider the law of atmospheres ( 43). Firstshow that the pressure ...
 9.46: Consider a thinwalled, fi xedvolume container ofvolume V that hol...
 9.47: For the situation described in 46, show thatthe speed distribution ...
 9.48: Escape speed from near Earths surface is 1.1 104m/s. (a) Find the t...
 9.49: The escape speed of a particle near the suns surfaceis 6.2 105 m/s....
 9.50: (a) What density of conduction electrons in copper isneeded in orde...
 9.51: Starting with the Fermi energy given in Table 9.4, estimatethe numb...
 9.52: Use the method described in Appendix 6 to evaluatethe integral q0 x...
 9.53: For a (classical) simple harmonic oscillator with fi xedtotal energ...
 9.54: Stars similar to our sun eventually become whitedwarfs, in which th...
 9.55: An atoms nucleus is a collection of fermionsprotons and neutrons. (...
 9.56: During World War II, physicists developed methods toseparate the ur...
 9.57: Find the number density N/V for BoseEinstein condensationto occur ...
 9.58: BoseEinstein condensates of rubidium have reachedtemperatures of 2...
 9.59: The 40Ar isotope of argon (its most common form) isa boson, like 4H...
 9.60: In one experiment done by Cornell and Wieman, aBoseEinstein conden...
Solutions for Chapter 9: Statistical Physics
Full solutions for Modern Physics for Scientists and Engineers  4th Edition
ISBN: 9781133103721
Solutions for Chapter 9: Statistical Physics
Get Full SolutionsThis textbook survival guide was created for the textbook: Modern Physics for Scientists and Engineers, edition: 4. Chapter 9: Statistical Physics includes 60 full stepbystep solutions. This expansive textbook survival guide covers the following chapters and their solutions. Since 60 problems in chapter 9: Statistical Physics have been answered, more than 7290 students have viewed full stepbystep solutions from this chapter. Modern Physics for Scientists and Engineers was written by and is associated to the ISBN: 9781133103721.

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