L-4: Difference between revisions

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</center>
</center>


==Discussion==
===The two replica propagator===
Hence, the quantity <math>\overline{Z(x,t)^2}/ (\overline{Z(x,t)})^2</math> can be computed.  
Hence, the quantity <math>\frac{\overline{Z(x,t)^2}}{ (\overline{Z(x,t)})^2}</math> can be computed.   
* The denominator <math>\int_{u(0)=0}^{u(t)=0} {\cal D} u  \exp\left[-  \int_0^t d \tau  \frac{1}{4T}(\partial_\tau u)^2\right]  </math> is the free propagator and gives a contribution <math> \sim (4 T  t)^{d/2}</math> .
* Let us define  the numerator
<center> <math>
W(0,t)= \int_{u(0)=0}^{u(t)=0} {\cal D} u  \exp\left[-  \int_0^t d \tau  \frac{1}{4T}(\partial_\tau u)^2- \frac{D}{T^2} \delta^d[u(\tau)]\right]
</math></center>


* The denominator 
  <center> 
  <math> 
  \int_{u(0)=0}^{u(t)=0} {\cal D} u  \exp\left[-  \int_0^t d \tau  \frac{1}{4T}(\partial_\tau u)^2\right] 
  </math> 
  </center> 
  is the free propagator and contributes as <math>\sim (4 T t)^{d/2}</math>. 


* Let us define the numerator: 
  <center> 
  <math> 
  W(0,t)= \int_{u(0)=0}^{u(t)=0} {\cal D} u  \exp\left[-  \int_0^t d \tau  \frac{1}{4T}(\partial_\tau u)^2- \frac{D}{T^2} \delta^d[u(\tau)]\right] 
  </math> 
  </center> 


<Strong>Remark 2:</Strong> From Feynman-Kac we can write the following equation
Using the Feynman-Kac formula, we can write the following equation
<center> <math>
<center>
\partial_t W(x,t) =- \hat H W(x,t)  
<math>
</math></center>
\partial_t W(x,t) = - \hat H W(x,t)
Here the Hamiltonian reads:
</math>   
<center> <math>
</center>   
\hat H= -2 T \nabla^2 - \frac{D}{T^2} \delta^d[u]
</math></center>
The single particle potential  is <Strong> time independent and actractive </Strong>.
<center> <math>
W(x,t) = \langle x|\exp\left( - \hat H t\right) |0\rangle
</math></center>
At large times the behaviour is dominatated by the low energy part of the spectrum.


* In <math> d\le 2</math> an actractive potential always gives a bound state. In particular the ground state has a negative energy <math> E_0 <0</math>. Hence at large times
Here, the Hamiltonian is given by: 
<center> <math>
<center>
W(x,t) = e^{ |E_0| t}
<math>
</math></center>
\hat H = -2 T \nabla^2 - \frac{D}{T^2} \delta^d[u] 
grows exponentially. This means that at all temperature, when  <math>  t\to \infty</math>
</math>
<center><math> \overline{\ln Z(x,t)} \ll \ln\overline{Z(x,t)}
</center>
</math></center>


* For <math> d > 2</math> the low part of the spectrum is controlled by the strength of the prefactor <math>\frac{D}{T^2} </math>. At high temperature we have a continuum positive spectrum, at low temperature bound states exist. Hence,   when  <math> t\to \infty</math>  
=== The Spectrum of the Two-Replica Hamiltonian ===
<center><math> \begin{cases}
 
\overline{\ln Z(x,t)} = \ln\overline{Z(x,t)} \quad \text{for} \; T>T_c \\
The single-particle potential is '''time-independent and attractive'''. Since it is time-independent, we can use the spectral decomposition of the propagator. The long-time behavior is controlled by the low-energy part of the spectrum. In the presence of an attractive potential, we may have: 
\\
 
\overline{\ln Z(x,t)} \ll \ln\overline{Z(x,t)} \quad \text{for} \; T<T_c
* A discrete set of eigenvalues corresponding to bound states, followed by a continuous spectrum. 
\end{cases}  
* Only a continuous spectrum. 
</math></center>
 
This transition, in <math> d =3 </math>, is between a high temeprature, <math> \theta=0</math> phase and a low temeprature <math> \theta>0</math> <Strong> no RSB </Strong> phase.
* For <math>d \leq 2</math>: 
** An attractive potential always leads to the formation of a bound state. 
** The ground state has a negative energy <math>E_0 < 0</math>. 
** At long times, the propagator behaves as: 
<center> 
<math> 
W(x,t) \sim e^{ |E_0| t} 
</math> 
</center> 
** This implies that at all temperatures, in the limit <math>t \to \infty</math>: 
<center> 
<math> 
\overline{\ln Z(x,t)}  \ll \ln\overline{Z(x,t)} 
</math> 
</center> 
 
* For <math>d > 2</math>
** The low-energy part of the spectrum is controlled by the prefactor <math>\frac{D}{T^2}</math>.
** At high temperatures, the spectrum remains continuous and positive
** At low temperatures, bound states appear.
** Thus, in the limit <math>t \to \infty</math>
<center>
<math>
\begin{cases}
\overline{\ln Z(x,t)} = \ln\overline{Z(x,t)} \quad \text{for} \quad T > T_c \\
\\
\overline{\ln Z(x,t)} \ll \ln\overline{Z(x,t)} \quad \text{for} \quad T < T_c
\end{cases}
</math>
</center>
** This transition, in <math>d = 3</math>, separates: 
*** A high-temperature phase with <math>\theta = 0</math>
*** A low-temperature phase with <math>\theta > 0</math> and '''no RSB'''.

Revision as of 10:49, 2 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 there is still much to understand:

  • In d=1, we have found θ=1/3 and a glassy regime present at all temperatures. The stationary solution of the KPZ equation describes, at long times, the fluctuations of quantities such as Emin[x]Emin[x]. However, it does not determine the actual distribution of Emin for a given x. In particular, we have no clear understanding of the origin of the Tracy-Widom distribution.
  • In d=, an exact solution exists for the Cayley tree, predicting a freezing transition to a 1RSB phase (θ=0).
  • In finite dimensions greater than one, no exact solutions are available. Numerical simulations indicate θ>0 in d=2. The case d>2 remains particularly intriguing.

Let's do replica!

To make progress in disordered systems, we need to analyze the moments of the partition function. From Valentina's lecture, recall that if

Z(x,t)2(Z(x,t))2=1

then 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 ensure the equivalence between annealed and quenched averages.

In the following, we compute this quantity, which corresponds to a two-replica calculation. For simplicity, we consider polymers starting at 0 and ending at 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 Wick's theorem, for a generic Gaussian field W, we have
exp(W)=exp[W+12(W2W2)]

The first moment

The first moment of the partition function is straightforward 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 exhibits 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, there are two replicas:

  • 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: Using Wick's theorem, we obtain

Z(x,t)2=exp[Dtδ0T2]𝒟x1𝒟x2exp[0tdτ12T[(τx1)2+(τx2)2DT2δd[x1(τ)x2(τ)]]

  • Step 3: Changing coordinates** X=(x1+x2)/2;u=x1x2, we 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]

The two replica propagator

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 contributes as (4Tt)d/2.  
  • Let us define the numerator:
 W(0,t)=u(0)=0u(t)=0𝒟uexp[0tdτ14T(τu)2DT2δd[u(τ)]]  

Using the Feynman-Kac formula, we can write the following equation:

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

Here, the Hamiltonian is given by:

H^=2T2DT2δd[u]

The Spectrum of the Two-Replica Hamiltonian

The single-particle potential is time-independent and attractive. Since it is time-independent, we can use the spectral decomposition of the propagator. The long-time behavior is controlled by the low-energy part of the spectrum. In the presence of an attractive potential, we may have:

  • A discrete set of eigenvalues corresponding to bound states, followed by a continuous spectrum.
  • Only a continuous spectrum.
  • For d2:
    • An attractive potential always leads to the formation of a bound state.
    • The ground state has a negative energy E0<0.
    • At long times, the propagator behaves as:

W(x,t)e|E0|t

    • This implies that at all temperatures, in the limit t:

lnZ(x,t)lnZ(x,t)

  • For d>2:
    • The low-energy part of the spectrum is controlled by the prefactor DT2.
    • At high temperatures, the spectrum remains continuous and positive.
    • At low temperatures, bound states appear.
    • Thus, in the limit t:

{lnZ(x,t)=lnZ(x,t)forT>TclnZ(x,t)lnZ(x,t)forT<Tc

    • This transition, in d=3, separates:
      • A high-temperature phase with θ=0.
      • A low-temperature phase with θ>0 and no RSB.