SPP: Statistical Physics of Particles
SPF: Statistical Physics of Fields
What actually is a field??? Kardar defines an "average deformation field" u(x) as an alternative to the interacting particle model of phonons, with a corresponding velocity field ∂u/∂t.
- Locality gives us short range interactions between particles, such that we can define a potential energy density Φ for every x, where V[u]=∫dxΦ(u(x),∂u/∂x,⋯)
- Translational Symmetry For a 1-d chain, uniform translation does not change the energy, so the energy density satisfies a periodic Φ(u(x)+c)=Φ(u(x)). This removes the dependence of Φ on u itself and only on its derivatives.
- Stability Looking at equilibrium, we don't want linear terms in u (linearizing everything should mean all particles are stable). Then, quadratic term of V should be pos-definite.
What potential does this give us? The most general one is of the form
V(u)=∫dx[2K(∂x∂u)2+2L(∂x2∂2u)2+⋯]
Update: A better answer may be in Zee
2. (SPF) Ising model of magnetism: Hamiltonian for configuration {σi} of spins is
H=21i,j=1∑NJijσiσj−hi∑σi- Suppose Jij=−J/N, so H=−2NJ∑i,j=1Nσiσj−h∑iσi. Take the magnetization to be m=∑i=1Nσi/N=M/N (average spin direction), so
E(M,h)=⟨H⟩=⟨−2NJi,j=1∑Nσiσj−hi∑σi⟩=−N(Jm2/2+hm)- The partition function is Z(h,T)=∑(σi)exp(−βH), where our sum is over all spin configurations (σi). However, our Hamiltonian is invariant to specific spin values and only depends on the total net spin, so we can alter our sum to be over the number of positive spins Np, which also fixes a magnetization M such that H=E(M,h):
Z(h,T)=Np=0∑N( number of configs with Np up spins )×exp(−βE(M,h))=Np=0∑N(NpN)exp(−βE(M,h))=Np=0∑Nexp(−β(−1/βln(NpN)))exp(−βE(M,h))=Np=0∑Nexp(−β(E(M,h)−1/βln(NpN)))But having Np up spins forces N−Np down spins, so we might as well just sum over M=2Np−N instead, which gives us
Z(h,T)=M∑exp(−β(E(M,h)−kBTln((M+N)/2N)))=M∑exp(−βF(M,h))F(m,h)=E(M,h)−kBTln((M+N)/2N)- Free energy F(h,T)=−kBTlnZ(h,T)=minm(F(m,h))