L-4: Difference between revisions

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Now the Hamiltonian reads:
Now the Hamiltonian reads:
<center> <math>
<center> <math>
H= -2 T \nabla^2 - \frac{D}{T^2} \delta^d[u]
\hat  H= -2 T \nabla^2 - \frac{D}{T^2} \delta^d[u]
</math></center>
</math></center>


Now the Hamiltonian is time independent:
Now the Hamiltonian is <Strong>time independent </Strong>:
<center> <math>
<center> <math>
W(x,t) = \langle x|\exp\left( - \hat H t\rangle) |0\rangle  
W(x,t) = \langle x|\exp\left( - \hat H t\right) |0\rangle  
</math></center>
</math></center>
At large times the behaviour is dominatate by the low energy part of the spectrum
At large times the behaviour is dominatate by the low energy part of the spectrum

Revision as of 16:45, 11 February 2024

Goal : final lecture on KPZ and directed polymers at finite dimension. We will show that for d>2 a "glass transition" takes place.


KPZ : from d=1 to the Cayley tree

We know a lot about KPZ, but still we have much to understand:

  • In d=1 we found θ=1/3 and a glassy regime present at all temperatures. The stationary solution of the KPZ equation describes, at long times, the fluctions of quantities like Emin[x]Emin[x]. However it does not identify the actual distribution of Emin for a given x. In particular we have no idea from where Tracy Widom comes from.
  • In d=, there is an exact solution for the Cayley tree that predicts a freezing transition to an 1RSB phase (θ=0).
  • In finite dimension, but larger than 1, there are no exact solutions. Numerical simulations find θ>0 in d=2. The case d>2 is very interesting.

Let's do replica!

To make progress in disordered systems we have to go through the moments of the partition function. For simplicity we consider polymers starting in 0 and ending in x. We recall that

  • V(x,τ) is a Gaussian field with
V(x,τ)=0,V(x,τ)V(x,τ)=Dδd(xx)δ(ττ)
  • From the Wick theorem, for a generic Gaussian W field we have
exp(W)=exp[W+12(W2W2)]

The first moment

The first moment of the partition function is

Zt[x,t]=x(0)=0x(t)=x𝒟x(τ)exp[1T0tdτ12(τx)2]exp[1TdτV(x(τ),τ)]

Note that the term T2W2=dτ1dτ2V(x,τ1)V(x,τ2)=Dtδ0 has a short distance divergence due to the delta-function. Hence we can write:

Zt[x]=1(2πtT)d/2exp[12x2tT]exp[Dtδ02T2]

The second moment

Exercise: L-4

  • Step 1: The second moment is
Z[xt,t]2=𝒟x1𝒟x2exp[0tdτ12T[(τx1)2+(τx2)2]exp[1T0tdτ1V(x1(τ1),τ1)1T0tdτ2V(x2(τ2),τ2)]
  • Step 2: Use Wick and derive:
Z[xt,t]2=exp[Dtδ0T2]𝒟x1𝒟x2exp[0tdτ12T[(τx1)2+(τx2)2DT2δd[x1(τ)x2(τ)]]
  • Step 3: Now change coordinate X=(x1+x2)/2;u=x1x2 and get:
Z[xt,t]2=(Z[xt,t])2u(0)=0u(t)=0𝒟uexp[0tdτ14T(τu)2DT2δd[u(τ)]]u(0)=0u(t)=0𝒟uexp[0tdτ14T(τu)2]

Discussion

Hence, the quantity Z[xt,t]2/(Z[xt,t])2 can be computed.

  • The denominator u(0)=0u(t)=0𝒟uexp[0tdτ14T(τu)2] is the free propagator and gives a contribution 4Tt .
  • Let us define the numerator
W(0,t)=u(0)=0u(t)=0𝒟uexp[0tdτ14T(τu)2DT2δd[u(τ)]]

Remark 1: From T-I, remember that if

Z[xt,t]2(Z[xt,t])2=1

the partition function is self-averaging and lnZ[x,t]=lnZ[x,t]. The condition above is sufficient but not necessary. It is enough that Z[xt,t]2/(Z[xt,t])2<const, when t, to have the equivalence between annealed and quenched averages.

Remark II: From L-3, we derive using Feynman-Kac, the following equation

tW(x,t)=H^W(x,t)

Now the Hamiltonian reads:

H^=2T2DT2δd[u]

Now the Hamiltonian is time independent :

W(x,t)=x|exp(H^t)|0

At large times the behaviour is dominatate by the low energy part of the spectrum