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=== The second moment ===
=== The second moment ===
For the second moment instead the are two replica


* Step 1: The second moment is
* Step 1: The second moment is

Revision as of 14:45, 1 February 2025

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 1d 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(x−x′)δ(τ−τ′)
  • From the Wick theorem, for a generic Gaussian W field we have
exp⁡(W)‾=exp⁡[W‾+12(W2‾−W‾2)]

The first moment

The first moment of the partition function is simple to compute and corresponds to a single replica

Z(x,t)‾=∫x(0)=0x(t)=x𝒟x(τ)exp⁡[−1T∫0tdτ12(∂τx)2]exp⁡[−1T∫dτV(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:

Z(x,t)‾=1(2πtT)d/2exp⁡[−12x2tT]exp⁡[Dtδ02T2]

The second moment

For the second moment instead the are two replica

  • Step 1: The second moment is
Z(x,t)2‾=∫𝒟x1∫𝒟x2exp⁡[−∫0tdτ12T[(∂τx1)2+(∂τx2)2]exp⁡[−1T∫0tdτ1V(x1(τ1),τ1)−1T∫0tdτ2V(x2(τ2),τ2)]‾
  • Step 2: Use Wick and derive:
Z(x,t)2‾=exp⁡[Dtδ0T2]∫𝒟x1∫𝒟x2exp⁡[−∫0tdτ12T[(∂τx1)2+(∂τx2)2−DT2δd[x1(τ)−x2(τ)]]
  • Step 3: Now change coordinate X=(x1+x2)/2;u=x1−x2 and get:
Z(x,t)2‾=(Z(x,t)‾)2∫u(0)=0u(t)=0𝒟uexp⁡[−∫0tdτ14T(∂τu)2−DT2δd[u(τ)]]∫u(0)=0u(t)=0𝒟uexp⁡[−∫0tdτ14T(∂τu)2]

Discussion

Hence, the quantity Z(x,t)2‾/(Z(x,t)‾)2 can be computed.

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

Remark 1: From Valentina's lecture, remember that if

Z(x,t)2‾(Z(x,t)‾)2=1

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

Remark 2: From Feynman-Kac we can write the following equation

∂tW(x,t)=−H^W(x,t)

Here the Hamiltonian reads:

H^=−2T∇2−DT2δd[u]

The single particle potential is time independent and actractive .

W(x,t)=⟨x|exp⁡(−H^t)|0⟩

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

  • In d≤2 an actractive potential always gives a bound state. In particular the ground state has a negative energy E0<0. Hence at large times
W(x,t)=e|E0|t

grows exponentially. This means that at all temperature, when t→∞

ln⁡Z(x,t)‾≪ln⁡Z(x,t)‾
  • For d>2 the low part of the spectrum is controlled by the strength of the prefactor DT2. At high temperature we have a continuum positive spectrum, at low temperature bound states exist. Hence, when t→∞
{ln⁡Z(x,t)‾=ln⁡Z(x,t)‾forT>Tcln⁡Z(x,t)‾≪ln⁡Z(x,t)‾forT<Tc

This transition, in d=3, is between a high temeprature, θ=0 phase and a low temeprature θ>0 no RSB phase.