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Homework assignments (4,5 credits) in Computational Physics

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9 Write a Monte Carlo program to simulate the one<br />

component plasma (OCP)<br />

Instructor: Olle Edholm<br />

Use periodic boundary conditions and make the simulations at fixed N and Γ (see def<strong>in</strong>ition<br />

below). Calculate the energy and heat capacity per particle. Read first the second<br />

(classical) reference below (http://prola.aps.org/abstract/PRA/v8/i6/p3096_1). Try<br />

to reproduce some of the results of that article. You may first start with a cutoff method<br />

but you have to use the Ewald method (see the first reference) <strong>in</strong> the end. (Reference:<br />

Allen and Tildesley, and J.P. Hansen Phys. Rev A. 8 (1973) p. 3096-3109)<br />

The properties of the OCP do not depend separately on density and temperature,<br />

but these can be comb<strong>in</strong>ed <strong>in</strong>to one dimensionless parameter:<br />

Γ = 1<br />

4πɛ 0<br />

(Ze) 2<br />

k B T (4π 3 ρ)1/3<br />

If you use the dimensionless coord<strong>in</strong>ates: y i = x i (4πρ/3) 1/3 , the Coulomb energy between<br />

two particles may be written:<br />

u(r)<br />

k B T = Γ r ,<br />

with r be<strong>in</strong>g the <strong>in</strong>ter particle distance <strong>in</strong> the dimensionless units def<strong>in</strong>ed above. If Z = 1<br />

(protons) and T=300K, Γ = 1 corresponds to a low number density (about 10 21 protons<br />

per m 3 ) while Γ = 200 corresponds to more the k<strong>in</strong>d of densities one has <strong>in</strong> ord<strong>in</strong>ary<br />

matter (10 28 protons per m 3 ). Vary the parameter Γ <strong>in</strong> this range. In a typical plasma<br />

the temperature is usually much higher, but also the density. S<strong>in</strong>ce the density is taken<br />

to the power one third, even typical conditions <strong>in</strong>side a white dwarf star correspond to<br />

quite small values of Γ.<br />

Observe, f<strong>in</strong>ally that you have to <strong>in</strong>clude the attractive <strong>in</strong>teraction with the electrons<br />

as a uniform attractive background. This may be justified s<strong>in</strong>ce at typical plasma conditions<br />

the electrons can be treated as a quantum mechanical highly degenerate Fermi-Dirac<br />

gas. Us<strong>in</strong>g a cutoff, you may add this contribution (which can be calculated analytically)<br />

<strong>in</strong> the end. Us<strong>in</strong>g Ewald summation you have to <strong>in</strong>clude this when you calculate the electrostatic<br />

repulsion between the protons. If you do not do this each part of the <strong>in</strong>teractions<br />

will diverge separately.<br />

6

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