Consider a gas of molecules whose interaction energy u(r)u is infinite for r<r0and negative for r>r0, with a minimum value of -u0. Suppose further that kTu0, so you can approximate the Boltzmann factor forr>r0using ex1+x. Show that under these conditions the second virial coefficient has the form B(T)=b-(a/kT), the same as what you found for a van der Waals gas in Problem 1.17. Write the van der Waals constants aand b in terms of r0and u(r), and discuss the results briefly.

Short Answer

Expert verified

The van der waals constants are:

akT=2πv0r2u(r)kTdr

b=2πr033

Step by step solution

01

Step 1. Given information

Equation for Mayer's f-function

f(r)=e-βu(r)-1

here the factor β=

β=1kTc

Here,

Tc= Critical temperature

k=Bolztmann constant

Rewriting the Mayer's equation:

f(r)=eM(r)kT-1

Here,u(r)=potential energy due to interaction of any pair of molecules.

Considering the gaseous molecules as hard hemispheres.

If the separation between them is ris more than the intermolecular separationr0then potential is

r<r0forr>r0

Ifr<r0, then the potential energy is,

u(r)

The second viral coefficient:

B(T)=-12d3rf(r)

Using the spherical coordination, the volume element is,

d3r=(dr)(rdθ)(rsinθdϕ)

The integralf(r)is independent of the anglesθ&ϕ. sod3r=4πr2dr

02

Step 2.  The second viral coefficient is expressed as 

we have,

B(T)=-120f(r)4πr2dr

=-2π0r2f(r)dr

=-2π0r0r2f(r)dr

=-2π0r0r2e-u(r)kT-1dr-2πs0r2eu(r)kT-1drB(T)=-2π0r0r2e-u(r)kT-1dr-2π0r2e-u(r)kT-1dr

=-2π0r2e-kTdr+2π0r0r2dr-2π0r21-u(r)kT-1dr

=0+2πr033-2πKT50r2u(r)dr

On comparing,

B(T)=2πr033+2πv0r2u(r)kTdr

=b-akT

and,

akT=2πs0r2u(r)kTdr

The second and third viral coefficient from van der waal model is,

B=b-aRT&C=b2

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Most popular questions from this chapter

Implement the ising program on your favourite computer, using your favourite programming language. Run it for various lattice sizes and temperatures and observe the results. In particular:

(a) Run the program with a 20 x 20 lattice at T = 10, 5, 4, 3, and 2.5, for at least 100 iterations per dipole per run. At each temperature make a rough estimate of the size of the largest clusters.

(b) Repeat part (a) for a 40 x 40 lattice. Are the cluster sizes any different? Explain. (c) Run the program with a 20 x 20 lattice at T = 2, 1.5, and 1. Estimate the average magnetisation (as a percentage of total saturation) at each of these temperatures. Disregard runs in which the system gets stuck in a metastable state with two domains.

(d) Run the program with a 10x 10 lattice at T = 2.5. Watch it run for 100,000 iterations or so. Describe and explain the behaviour.

(e) Use successively larger lattices to estimate the typical cluster size at temperatures from 2.5 down to 2.27 (the critical temperature). The closer you are to the critical temperature, the larger a lattice you'll need and the longer the program will have to run. Quit when you realise that there are better ways to spend your time. Is it plausible that the cluster size goes to infinity as the temperature approaches the critical temperature?

Problem 8.13. Use the cluster expansion to write the total energy of a monatomic nonideal gas in terms of a sum of diagrams. Keeping only the first diagram, show that the energy is approximately
U32NkT+N2V·2π0r2u(r)e-βu(r)dr
Use a computer to evaluate this integral numerically, as a function of T, for the Lennard-Jones potential. Plot the temperature-dependent part of the correction term, and explain the shape of the graph physically. Discuss the correction to the heat capacity at constant volume, and compute this correction numerically for argon at room temperature and atmospheric pressure.

Show that, if you don't make too many approximations, the exponential series in equation 8.22 includes the three-dot diagram in equation 8.18. There will be some leftover terms; show that these vanish in the thermodynamic limit.

For each of the diagrams shown in equation 8.20, write down the corresponding formula in terms of f-functions, and explain why the symmetry factor gives the correct overall coefficient.

Consider an Ising model in the presence of an external magnetic field B, which gives each dipole an additional energy of -μBB if it points up and +μBB if it points down (whereμB is the dipole's magnetic moment). Analyse this system using the mean field approximation to find the analogue of equation 8.50. Study the solutions of the equation graphically, and discuss the magnetisation of this system as a function of both the external field strength and the temperature. Sketch the region in the T-B plane for which the equation has three solutions.

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