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Turbulence in the two-dimensional Fourier-truncated Gross–Pitaevskii equation

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Turbulence in the two-dimensional Fourier-truncated Gross–Pitaevskii equation
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We undertake a systematic, direct numerical simulation of the two-dimensional, Fourier-truncated, Gross–Pitaevskii equation to study the turbulent evolutions of its solutions for a variety of initial conditions and a wide range of parameters. We find that the time evolution of this system can be classified into four regimes with qualitatively different statistical properties. Firstly, there are transients that depend on the initial conditions. In the second regime, power-law scaling regions, in the energy and the occupation-number spectra, appear and start to develop; the exponents of these power laws and the extents of the scaling regions change with time and depend on the initial condition. In the third regime, the spectra drop rapidly for modes with wave numbers k > kc and partial thermalization takes place for modes with k < kc; the self-truncation wave number kc(t) depends on the initial conditions and it grows either as a power of t or as log t. Finally, in the fourth regime, complete thermalization is achieved and, if we account for finite-size effects carefully, correlation functions and spectra are consistent with their nontrivial Berezinskii–Kosterlitz–Thouless forms. Our work is a natural generalization of recent studies of thermalization in the Euler and other hydrodynamical equations; it combines ideas from fluid dynamics and turbulence, on the one hand, and equilibrium and nonequilibrium statistical mechanics on the other.
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Transcript: English(auto-generated)
The study of superfluid turbulence is a problem of central importance in non-equilibrium statistical mechanics, turbulence and nonlinear dynamics. One of the equations which is used to study turbulence in superfluids is the Gross-Pilayevsky equation, which
we study here in two dimensions and be studied by the zero-spectral method, therefore it is Fourier truncate. This study has been carried out by Vishwanath Shukla, Margethian Rache and Rahul Pandit. This is the Gross-Pilayevsky equation which comes to this Hamiltonian. Psi here is the wave
function of the Bose gas, G the interaction strengths and A the area of the system. The energy and the number of particles are conserved in the dissipation-less unforced case. The energy can be written as a sum of the kinetic energy, the interaction energy and the quantum pressure energy.
I now give the principal results of our study. We identify four stages in the dynamical evolution of the dissipation-less unforced Fourier truncated Gross-Pilayevsky equation in two dimensions. These are the following. The region of initial transients. This depends on the initial conditions.
The onset of thermalization. Scaling behaviors, for example in spectra change with time in dependent initial conditions. Partial thermalization. There are some universal, that is independent of initial conditions, scaling behaviors in spectra.
Self-truncation occurs in spectra at the wave number KC which can increase either as a power of time or logarithmically in time. Complete thermalization occurs finally and because we are in a two dimensional interacting Bose system, this shows a Berezinski-Koskalit-Salva space.
Some of these results have been obtained in earlier studies but we are not aware of any such comprehensive study of this system which explores a variety of initial conditions. Let me now give a quick overview of our results.
This slide shows the evolution of different energies, for example the compressible energy, the compressible energy and so on. This slide shows how velocity component PDFs change. They have power law forms when there are vortices which eventually annihilate to yield Gaussian PDFs.
Incompressible kinetic energy spectra start which in a way depends on initial conditions but eventually develop power law regions here which have to do with the thermalization of this system which is basically following micro-canonical evolution. Because it's a finite dimensional dynamical system once we have Fourier concatenate.
Here are glass strip plots of compressible kinetic energy spectra. You can see that there is some linearity here. This is the first signature of thermalization but here it does drop off.
This is self-truncation and we do have spectral convergence here. In other parameter regions we get all the way to complete thermalization as shown in these illustrative plots. And in others we have some thermalization but again spectral convergence because of self-truncation.
Let me illustrate all this by a series of animations which show PDFs. So velocity spectra initially power law and then becoming Gaussian as the vorticity decreases by the annihilation of vortices.
This is how the energy spectra evolve in time developing these regions which are the first signatures of thermalization. At the same time occupation number spectra also evolve like this and begin to show power loss.
We have also studied the dependence of this self-truncation wave vector on the interaction strength g. On the number of collocation points in our pseudo-spectral method and on the type of initial condition. These are special initial conditions obtained by solving a Stochastic-Ginzburg-Lendau equation.
In some cases the spectral, the truncation rate number is very short and these evolve very slowly in time. Eventually when the system goes to complete thermalization it should show power loss
as in the Berezinski-Kosner-Staubler space and indeed we find such power loss. This is a summary of the results in our paper. Thank you.