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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 15:45, 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(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 simple to compute and corresponds to a single replica

Z(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:

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=𝒟x1𝒟x2exp[0tdτ12T[(τx1)2+(τx2)2]exp[1T0tdτ1V(x1(τ1),τ1)1T0tdτ2V(x2(τ2),τ2)]
  • Step 2: Use Wick and derive:
Z(x,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(x,t)2=(Z(x,t))2u(0)=0u(t)=0𝒟uexp[0tdτ14T(τu)2DT2δd[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)2DT2δd[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 lnZ(x,t)=lnZ(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^=2T2DT2δd[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 d2 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

lnZ(x,t)lnZ(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
{lnZ(x,t)=lnZ(x,t)forT>TclnZ(x,t)lnZ(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.