non equilibrium condensation in wt gp models
play

Non-equilibrium condensation in WT & GP models Sergey Nazarenko - PowerPoint PPT Presentation

Non-equilibrium condensation in WT & GP models Sergey Nazarenko INPHYNI (Insitute de Physique de Nice) In past and present collaboration with Yu. Lvov, S. Medvedev, M. Onorato, D. Proment, B. Semisalov, V. Shukla, S. Thalabard, R. West


  1. Non-equilibrium condensation in WT & GP models Sergey Nazarenko INPHYNI (Insitute de Physique de Nice) In past and present collaboration with Yu. Lvov, S. Medvedev, M. Onorato, D. Proment, B. Semisalov, V. Shukla, S. Thalabard, R. West Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 1 / 28

  2. BEC turbulence. BEC is described by Gross-Pitaevskii equation: i ∂ψ ∂ t + ∇ 2 ψ − | ψ | 2 ψ = 0 . (1) where ψ is a complex scalar field. GP equation (1) conserves two quantities with positive quadratic parts—the energy and the total number of particles, � | ψ ( x , t ) | 2 d x , N = (2) and the total energy, � � |∇ ψ ( x , t ) | 2 + 1 � 2 | ψ ( x , t ) | 4 H = d x , (3) Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 2 / 28

  3. Weak wave turbulence Weak wave turbulence (WWT) refers to systems with random weakly nonlinear waves. In WWT, waveaction spectrum n k = ( L / 2 π ) d �| ψ k | 2 � evolves according to the wave-kinetic equation (WKE): � 1 + 1 − 1 − 1 � � | n k 1 n k 2 n k 3 n k × ∂ t n k = 4 π n k n k 3 n k 1 n k 2 δ ( k + k 3 − k 1 − k 2 ) δ ( ω k + ω k 3 − ω k 1 − ω k 2 ) d k 1 d k 2 d k 3 , (4) where ω k = k 2 . � � k 2 n k d k . Now the invariants are: N = n k d k and E = Such wave fields contain a lot of vortices but they are all ghosts! Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 3 / 28

  4. Dual cascades 2D turbulence Weak wave turbulence Standard (Fjortoft’1953) argument in 2D turbulence predicts a dual cascade behaviour: energy cascades to low wavenumbers while enstrophy cascades to high wavenumbers. Similar argument in WT predicts a forward cascade of energy and an inverse cascade of waveaction (particles in the GP model. Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 4 / 28

  5. Dual cascades in BEC Navon et al.’2018. Direct E-cascade: “evaporation”. Inverse N-cascade: Non-equilibrium condensation. Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 5 / 28

  6. Kolmogorov-Zakharov spectra in the GP model Stationary Kolmogorov-Zakharov (KZ) spectra n k ∼ k ν are solutions of WKE corresponding to the energy and the particle cascades: ν E = − d , ��� and ν N = − d + 2 / 3 , ��� . KZ spectra are only meaningful if they are local , i.e. when the collision integral in the original kinetic equation converges. In 3D ( d = 3) the inverse N -cascade spectrum is local, whereas the the direct E -cascade spectrum is log-divergent at the infrared (IR) limit (i.e. at k → 0). As usual, the log-divergence can be remedied by a log-correction, n k ∼ [ln( k / k f )] − 1 / 3 k ν E , where k f is an IR cutoff provided by the forcing scale. Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 6 / 28

  7. KZ solutions of the GP system cont’d The 2D case ( d = 2) appears to be even more tricky. It turns out that formally the N -cascade spectrum is local, but the N -flux appears to be positive, in contradiction with the Fjørtoft’s argument. Further, for the E -cascade spectrum, the exponent ν E coincides with the one of the thermodynamic E -equipartition spectrum. As a results, the KZ spectra are not realisable in the 2D GP turbulence. Instead, “warm cascade” states are observed where the E and N k-space fluxes are on background of a thermalised background. Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 7 / 28

  8. Direct and inverse cascades in 2d GPE Figure: SN & M. Onorato (2006) Both direct and inverse cascades are “warm”: their spectra are thermal equipartition of energy with small corrections to accommodate E and N fluxes. Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 8 / 28

  9. Evolving 2d GP turbulence Figure: SN & M. Onorato (2007) Evolution scenario: 4-wave WT of de-Broglie waves → hydrodynamics of point vortices → 3-wave WT of Bogoliubov sound Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 9 / 28

  10. Direct and inverse cascades in 3d GPE Figure: Proment, SN & M. Onorato (2012) The spectrum is very sensitive to the type of IR dissipation: KZ for friction and Critical Balance for hypo-viscosity Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 10 / 28

  11. Evolving weak 3D BEC turbulence Isotropic WKE is � √ ω, √ ω 1 , √ ω 2 , √ ω 3 d � ω − 1 / 2 � = min (5) dt n ω n ω n 1 n 2 n 3 n − 1 ω + n − 1 − n − 1 − n − 1 � � δ ( ω + ω 1 − ω 2 − ω 3 ) d ω 1 d ω 2 d ω 3 . 1 2 3 where ω = k 2 is the wave frequency and n ω ( t ) ∼ �| ψ k | 2 � is the spectrum. Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 11 / 28

  12. Self-similar evolution in the inverse cascade range Non-equilibrium condensation process. ( Semikoz and Tkachev 1995, Lacaze et al 2001 ) Solution ”blows up” in finite time t ∗ . Shortly before t ∗ they reported n = ω − x ∗ x ∗ = 1 . 23 > 1 . 16 = x KZ . Thermodynamic n = 1 /ω is observed after t ∗ . Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 12 / 28

  13. Self-similar formulation in the inverse cascade range Boris Semisalov, Vladimir Grebenev, Sergey Medvedev and SN are currently working on finding the self-similar solution of WKE. Let us search the solution of the WKE in a similarity form n ω = τ a f ( η ), where η = ωτ − b , b = a − 1 / 2 > 0 , τ = t ∗ − t . If we denote x = a b , WKE can be rewritten as xf + η f ′ = 1 bSt [ f ] (6) Self-similarity of the second type (Zeldovich): a and b cannot be found from a conservation law (e.g. energy), but are solutions of a nonlinear eigenvalue problem. Boundary conditions: (1) f ( η ) → η x for η → ∞ . (2) f ( η ) → ? for η → 0. Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 13 / 28

  14. Nonlocal interaction in the low-frequency range For power spectrum solution n ω = ω − x , the collision integral integral converges in the range 1 < x < 3 / 2. Simulations of Semikoz and Tkachev indicate x ≈ 0 at low ω . For such spectra the integral is divergent at infinity. Thus, the leading contribution comes from non-local interactions with ω 1 , 2 , 3 ≫ ω , so the WKE becomes d � n 1 n 2 n 3 δ ( ω 1 − ω 2 − ω 3 ) d ω 1 d ω 2 d ω 3 + dt n ω = (7) � n − 1 − n − 1 − n − 1 � � n ω n 1 n 2 n 3 δ ( ω 1 − ω 2 − ω 3 ) d ω 1 d ω 2 d ω 3 , 1 2 3 where the integrals in RHS are independent of ω and n ω . Denoting the first integral by A ( t ) and the second – by B ( t ), we can write (7) as d dt n ω = A ( t ) + B ( t ) n ω , (8) which can be easily integrated for any A ( t ) and B ( t ). Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 14 / 28

  15. Self-similar solution for small η For the similarity form n ω = τ a f ( η ), equation (8) can be rewritten as ˜ ˜ A B xf + η f ′ = b + (9) b f where ˜ A and ˜ B present similarity counterpart of the integrals A ( t ) and B ( t ). Equation (9) can be easily integrated: ˜ A + C η ( ˜ B / b ) − x . f ( η ) = (10) b ( x − ˜ B / b ) Taking into account that ˜ A ≥ 0 for f ≥ 0 and b > 0 for 1 < x < 3 / 2, it is easy to see that in the vicinity of η = 0 there is only one non-negative bounded solution ˜ A f ( η ) → , η → 0 . (11) ( bx − ˜ B ) This is the second BC for the nonlinear eigenvalue problem. Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 15 / 28

  16. Self-similar solution of WKE xf + η f ′ = 1 bSt [ f ] (12) Nonlinear eigenvalue problem: find x for which the following boundary conditions are satisfied simultaneously. (1) f ( η ) → η x for η → ∞ . (2) f ( η ) → const for η → 0. It is much harder to solve the equation for f ( η ) than to solve WKE for evolving n ( k , t ). Relaxation of iterations. No theory or developed numerical algorythms. Ongoing work with B. Semisalov, V. Grebenev and S. Medvedev. Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 16 / 28

  17. Computing the collision integral For computation of the integrals over ∆ η we also need the values of f ( η ) for η > η max and η < η min . We assume that ∀ η > η max f ( η ) = C η − x and ∀ η ∈ [0 , η min ] f ( η ) ≡ f ( η min ). � � � 3 ��� max � max � � min � min � � max ��� � 2 max Figure: Domain of integration ∆ η (shadowed). Solid lines show the borders η min , η max . Dashed lines show the discontinuity of integrand’s derivative due to presence of function “min”. Red lines along the boundary show the singularity of integrand near zero values of η 2 , η 3 and η 2 + η 3 − η Sergey Nazarenko INPHYNI Non-equilibrium condensation in WT & GP models (Insitute de Physique de Nice) 17 / 28

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend