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.

Short Answer

Expert verified

Hence,

s¯=tanh(β(ϵns¯+μB))

Step by step solution

01

Given information

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 (where μB is the dipole's magnetic moment).

02

Explanation

Assume we have dipoles on an external magnetic field, and the energy of the interaction between the dipole and the external magnetic field is:

ϵ=μB

Where,

μis the dipole moment and it has two allowed magnetic orientation, hence:

ϵ=±μB

The total energy of the system resulting from all interactions with its nearest neighbours is:

U=-ϵsisj±μB

Consider a lsing model with two dipoles. This system has four alignments, which are as follows:

:-ϵ:ϵ:ϵ:-ϵ

where si =-1 when the dipole pointing down and si= l when the dipole pointing up, for two dipoles in an external magnetic field, we have two energies, that are:

E=-ϵns¯-μBE=ϵns¯+μB

03

Explanation

The partition function is:

Z=e-βEZ=e-βE+eβE

Thus,

Z=eβ(ϵns¯+μB)+e-β(ϵns¯+μB)Z=2cosh(β(ϵns¯+μB))(1)

The average expected value for the spin alignment is given by (from equation 8.49):

s¯=1Zeβ(ϵns¯+μB)-e-β(ϵns¯+μB)

Using sinh(x)=ex-e-x/2

s¯=2sinh(β(ϵns¯+μB))Z

Substitute from (1):

s¯=2sinh(β(ϵns¯+μB))2cosh(β(ϵns¯+μB))s¯=tanh(β(ϵns¯+μB))

When magnetic field is zero, the equation will be:

s¯=tanh(βϵns¯)

To plot this function, we substitute with: β=1/kTcandt=kT/nϵ

s¯=tanhs¯t

we have two cases the first one when t = kT/nε> 1, in this case we have only one solution and when t = kT/nε<l we have three solutions, two of them are stable and the third one is unstable, as shown in the following figure (the first figure is when t>1 and the second one is when t < 1)

04

Explanation

The following codes were used to plot the graph:

When we have a non zero magnetic field, then we modify the code as follows to have the following graph:

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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?

Consider a gas of "hard spheres," which do not interact at all unless their separation distance is less than r0, in which case their interaction energy is infinite. Sketch the Mayer f-function for this gas, and compute the second virial coefficient. Discuss the result briefly.

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.

Modify the ising program to simulate a one-dimensional Ising model.

(a) For a lattice size of 100, observe the sequence of states generated at various temperatures and discuss the results. According to the exact solution (for an infinite lattice), we expect this system to magnetise only as the temperature goes to zero; is the behaviour of your program consistent with this prediction? How does the typical cluster size depend on temperature?

(b) Modify your program to compute the average energy as in Problem 8.27. Plot the energy and heat capacity vs. temperature and compare to the exact result for an infinite lattice.

(c) Modify your program to compute the magnetisation as in Problem 8.28. Determine the most likely magnetisation for various temperatures and sketch a graph of this quantity. Discuss.

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.

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