Landau Free Energy & Ising Model at T=0

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SUMMARY

The discussion centers on the Landau free energy and the Ising model at absolute zero temperature (T=0). The total energy of the Ising model is defined as ##E = −J \sum_{} S_iS_j##, where ##S_i = \pm 1## and the ground state is antiferromagnetic for ##J < 0##. The Landau free energy is expressed as $$F = at\psi^2 + b\psi^4 + ...$$, with ##t = (T − T_c)/T_c##, where ##a, b > 0## are constants. The discussion emphasizes the symmetry of the order parameter ##\psi ≡ m_1−m_2## and the conditions for equilibrium, leading to the conclusion that ##\psi = 0## at critical temperature and two minima for ##T < T_c##.

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  • Understanding of the Ising model and its energy formulation
  • Familiarity with Landau theory and free energy concepts
  • Knowledge of phase transitions and order parameters
  • Basic mathematical skills for polynomial expansions and derivatives
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Students and researchers in condensed matter physics, particularly those focusing on statistical mechanics, phase transitions, and the Ising model. This discussion is beneficial for anyone seeking to deepen their understanding of Landau theory and its applications in physical systems.

CAF123
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Homework Statement


The total energy of the Ising model is ##E = −J \sum_{<ij>} S_iS_j ##, where ##S_i = \pm 1## and ##< ij >## implies sum over nearest neighbours. For ##J < 0## explain why the ground state of this system at ##T = 0## is antiferromagnetic.

Let ##m_{1,2}## be the magnetisations in the two sublattices of an antiferromagnetic Ising model. Define the order parameter ##\psi ≡ m_1−m_2##. Argue why the Landau free energy for this system should have the form, $$F = at\psi^2 + b\psi^4 + ...,$$ where ##t \equiv (T − T_c)/T_c ## and ##a, b > 0## are constants.

Homework Equations


[/B]
F some polynomial expansion in order parameter ##\psi##.

The Attempt at a Solution


So as far as I understand from the Landau theory, we construct a function F for the free energy based solely on the symmetries of the system, particularly that obeyed by the order parameter. ##m_i \rightarrow -m_i## can be viewed as a rotation of the system by ##\pi## so F should be invariant under ##m_i \rightarrow -m_i## which is to say ##\psi \rightarrow -\psi## is a symmetry. So we construct ##F = c + a(T)\psi^2 + b(T)\psi^4 + ...##, where c is a constant, can be set to 0. I am just a bit confused as to how we solve for a(T) and b(T). Imposing that at equilibrium, ##\partial F/\partial \psi = 0## then this means $$2\psi(a(T) + 2b(T) \psi^2) = 0$$ ie ##\psi = 0## or ##\psi^2 = -a(T)/2b(T)##. But how should I progress? The case ##\psi = 0## corresponds to the case when ##m_1 = m_2## so that this could be realized in the ground state. Thanks!
 
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Ok I guess I can work with what is given and try to justify it. At the critical temperature (or temperature at which we reach criticality) the first term vanishes which implies the equilibrium situation is one in which we have ##\psi=0.## Similarly for the case ##T>T_c##. (We must choose ##\psi=0## otherwise we get an imaginary solution for ##\psi## which is unphysical.) For ##T<T_c## we get two minima, with ##\psi=0## a maximum. Is this correct understanding? It seems that this is the same analysis for the case ##J>0##.
 

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