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Statistical Mechanics - Physics at Oregon State University

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188 CHAPTER 8. MEAN FIELD THEORY: CRITICAL TEMPERATURE.<br />

8.7 Problems for chapter 8<br />

Problem 1.<br />

A model of a binary alloy can be constructed similar to an Ising model.<br />

Assume th<strong>at</strong> the possible <strong>at</strong>omic sites i are fixed and th<strong>at</strong> the actual <strong>at</strong>om on<br />

site i is either type A or type B. The effects of the chemical bond extend only<br />

to nearest neighbors. The energy of an AA-bond is ɛAA, of an AB-bond ɛAB,<br />

and of a BB-bond ɛBB. The parameter ɛ = 1<br />

2ɛAA + 1<br />

2ɛBB − ɛAB is useful. The<br />

concentr<strong>at</strong>ion of A <strong>at</strong>oms is cA = NA/<br />

N and the concentr<strong>at</strong>ion of B <strong>at</strong>oms is<br />

cB = 1 − cA. Introduce variables σi rel<strong>at</strong>ed to the number of A <strong>at</strong>oms nAi on<br />

site i by nAi = 1<br />

2 (1 + σi). Obviously, σi = ±1 and nBi = 1<br />

2 (1 − σi).<br />

A. Calcul<strong>at</strong>e the energy of the binary alloy in a st<strong>at</strong>e {σ1, · · · , σN}.<br />

B. Define variables J and h in such a way th<strong>at</strong> this expression looks like the<br />

Ising model.<br />

C. If J > 0 one finds a critical temper<strong>at</strong>ure Tc. Wh<strong>at</strong> happens below Tc in<br />

this case?<br />

D. Suppose J < 0. Wh<strong>at</strong> is the structure of the alloy <strong>at</strong> low temper<strong>at</strong>ures?<br />

Problem 2.<br />

Consider a one-dimensional Ising model. Assume th<strong>at</strong> J < 0. Introduce new<br />

spin-variables τi rel<strong>at</strong>ed to the σi variables by τi = (−1) i σi.<br />

A. Calcul<strong>at</strong>e Tc for this system.<br />

B. Wh<strong>at</strong> is happening below Tc?<br />

Problem 3.<br />

Consider the Heisenberg model for spin 1<br />

2 particles. The Hamiltonian is<br />

given by<br />

H = −J <br />

<br />

Si • Sj<br />

The spin oper<strong>at</strong>ors <br />

0 1 0 −ı<br />

S are the standard Pauli m<strong>at</strong>rices ,<br />

,<br />

1 0 ı 0<br />

<br />

<br />

1 0<br />

γ<br />

and<br />

. The st<strong>at</strong>e of each individual spin is a two-spinor . The<br />

0 −1<br />

µ<br />

st<strong>at</strong>e of the whole system is now given by the direct product of N spinors |i >,<br />

in the form |1 > |2 > · · · |N >. Assume th<strong>at</strong> the density m<strong>at</strong>rix ρ can be written<br />

as a direct product of 2 × 2 m<strong>at</strong>rices ρ like we did for the Ising model. Use the<br />

same parametriz<strong>at</strong>ion for ρ as for the Ising model.<br />

A. Calcul<strong>at</strong>e the internal energy as a function of a and m. Wh<strong>at</strong> is the<br />

difference compared with the result for the Ising model?

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