Statistical Physics, Second Revised and Enlarged Edition

(Barry) #1

122 Phase transitions


answeris


M=Nμtanh(μB/kkkBT)
=Nμtanh[μ(B 0 +λM)/kkkBT] (11.3)

The spontaneous magnetizationisobtainedbysettingthe appliedfieldB 0 = 0
in (11.3), givinga transcendental equation for M( 0 ). ReplacingM( 0 )bythe
dimensionless order parameterm,(11.1), we obtain


m=tanh(mTC/T) (11.4)

where


TTTC=Nμ^2 λ/kkkB (11.5)

Equation (11.4) canbe readilysolvedgraphically (or numerically) asinFig. 11.2.
Plottedas thex-variableonthegraphisx=mTTTC/T,so that (11.4)becomesxT/TTTC=
tanhx.The solution is simply the intersection of the curvem=tanhxwith the straight
linem=xT/TTTC.Since theslope oftanhxisunity close tox= 0 ,itis at once evident
that:



  1. WhenT>TTTC,(11.4) has onlyone solution, namelym= 0. The spontaneous
    magnetization is zero, and the system is disordered.
    2 .T=TTTCis seen tobeadefinite transition temperature,inthatbelowTTTCother
    solutions arepossible.TTTCdepends linearlyon the mean field parameterλ.It is
    often called (for the ferromagnetic transition) the Curie temperature.
    3 .WhenT<TTTC,theequationhas threepossiblesolutions. We shallseelater that
    them=0 is now an unstable equilibrium. The solutions withm= 0 are the
    stable ones. Hence thesolid developsbelowTTTCaspontaneous magnetization with
    adefinite magnitude,but withanindefinitedirection.


T>TTTcT=TTTc

x

m

T<TTTc
+ 1

1

Fig. 11. 2 Findingthe spontaneous magnetization. The solution of (11.4) formisgiven bythe intersection
of the tanh curve with the straight line. Straight lines are drawn for these different temperatures.

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