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2. Consider a classical particle moving in a one-dimensional potential well u(x), as shown The particle is in thermal equilibrium with a reservoir at temperature T, so the probabilities of its various states are determined by Boltzmann statistics.

{a) Show that the average position of the particle is given by

where each integral is over the entire xaxis.

A one-dimensional potential well. The higher the temperature, the farther the particle will stray from the equilibrium point.

(b) If the temperature is reasonably low (but still high enough for classical mechanics to apply), the particle will spend most of its time near the bottom of the potential well. In that case we can expand u(x)in a Taylor series about the equilibrium point x0: u(x)=ux0+x-x0dudxx0+12x-x02d2udx2x0

+13!x-x03d3udx3x0+⋯

Show that the linear term must be zero, and that truncating the series after the quadratic term results in the trivial prediction x=x0.

(c) If we keep the cubic term in the Taylor series as well, the integrals in the formula for xbecome difficult. To simplify them, assume that the cubic term is small, so its exponential can be expanded in a Taylor series (leaving the quadratic term in the exponent). Keeping only the smallest temperature-dependent term, show that in this limit x differs from zo by a term proportional to kT. Express the coefficient of this term in terms of the coefficients of the Taylor series foru(x)

(d) The interaction of noble gas atoms can be modeled using the Lennard Jones potential,

u(x)=u0x0x12-2x0x6

Sketch this function, and show that the minimum of the potential well is at x=x0, with depth u0. For argon, x0=3.9Aand u0=0.010eV. Expand the Lennard-Jones potential in a Taylor series about the equilibrium point, and use the result of part ( c) to predict the linear thermal expansion coefficient of a noble gas crystal in terms of u0. Evaluate the result numerically for argon, and compare to the measured value

α=0.0007K-1(at80K)

Short Answer

Expert verified

For argon factor will be doubled.

Step by step solution

01

part(a) Step 1:Given information

Let the particle be associated with position

02

part(a) Step 2: Simplify

x¯=∑xxP(x)=∑xxe-βu(x)Z

03

part(b) Step 1:Given information

The linear tem in the expansion is zero

04

part(b) Step 2: Simplify

∫xe-β∣ux0+ax-x02dx=e-βux0∫xe-βax-x02dx=e-βux0∫y+x0e-βay2dy

∫e-βux0+ax-x02dx=e-βux0∫e-βax-x02dx=e-βux0∫e-βay2dy,

05

part(c) Step 1:Given information

we use Boltzman factor

06

part(c) Step 2: Simplify

x¯=e-βux0∫y+x0e-βay21-βby3dye-βux0∫e-βay21-βby3dy=∫x0-βby4e-βay2dy∫e-βay2dy

x¯=x0-βb3/4β2a2π/βaπ/βa=x0-34bβa2=x0-34ba2kT.

07

part(d) Step 1:Given information

Lennard-Jones is positive

08

part(d) Step 2: Simplify

d3udx3=u0(-12)(-13)(-14)x012x-15-2(-6)(-7)(-8)x06x-9

α=-34ba2kx0=-34-252u0x03x0236u02kx0=748ku0=1.26×10-5eV/Ku0.

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Most popular questions from this chapter

Apply the result of Problem 6.18 to obtain a formula for the standard deviation of the energy of a system of N identical harmonic oscillators (such as in an Einstein solid), in the high-temperature limit. Divide by the average energy to obtain a measure of the fractional fluctuation in energy. Evaluate this fraction numerically for N = 1, 104, and 1020. Discuss the results briefly.

At room temperature, what fraction of the nitrogen molecules in the air are moving at less than300m/s?

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 starγ UMa, whose surface temperature is approximately 9500 K.

Derive equation 6.92 and 6.93 for the entropy and chemical potential of an ideal gas.

A 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 12hf,32hf,52hf, 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).

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