with p l krapivsky and arkady vilenkin prof giulio racah
play

with P.L. Krapivsky and Arkady Vilenkin Prof. Giulio Racah - PowerPoint PPT Presentation

Survival of a target in a gas of diffusing particles with exclusion Racah Institute of Physics, Baruch Meerson Hebrew University of Jerusalem with P.L. Krapivsky and Arkady Vilenkin Prof. Giulio Racah 1909-1965 He was born in Firenze, and


  1. Survival of a target in a gas of diffusing particles with exclusion Racah Institute of Physics, Baruch Meerson Hebrew University of Jerusalem with P.L. Krapivsky and Arkady Vilenkin Prof. Giulio Racah 1909-1965 He was born in Firenze, and died here Advances in Nonequilibrium Statistical Mechanics, GGI, Firenze, July 4 2014

  2. Plan  Macroscopic Fluctuation Theory of diffusive lattice gases  MFT in non-stationary settings: examples  Survival of a target against “searchers” a. Stationary fluctuations: d>2, long times b. Non-stationary fluctuations: d=1, and any d for intermediate times  Extensions and summary

  3. Diffusive lattice gases SSEP: simple symmetric exclusion process RWs, ZRP: a = a (n i ) random walkers; zero-range process Large-scale behavior: fluctuating hydrodynamics   , x: Gaussian noise,            ξ D ( ) ( ) ( , t ) delta-correlated in x and t x t Spohn 1991, Kipnis and Landim 1999 Diffusive lattice gases are fully characterized, at large scales, by the diffusivity D (  ) and mobility  (  )

  4.              ξ D ( ) ( ) ( , t ) x t D (  ) and  (  ) are related to the equilibrium free energy density F (  ):   2 d F ( ) 2 D ( )     2 d ( ) When noise is ignored: diffusion equation           D ( ) t

  5. Macroscopic Fluctuation Theory (MFT) Bertini, De Sole, Gabrielli, Jona-Lasinio and Landim (2001 , …) Large parameter: number of particles in a relevant region of space. Generalizes the weak-noise WKB theory of Freidlin and Wentzel to fields Similar in spirit: Elgart and Kamenev (2004), M and Sasorov (2010) – WKB approximation to master equation for random walk on lattice and on-site reactions . Large parameter: number of particles on a single site MFT can be derived from fluctuating hydrodynamics via saddle-point expansion of a proper path integral (Tailleur, Kurchan, Lecomte 2007). This leads to a minimization problem that can be cast into a classical Hamiltonian field theory for the particle density q(x,t) and conjugate “momentum” density p(x,t):         q [ D ( q ) q ( q ) p )]     t q H / p , t 1             p H / q , 2 2 p D ( q ) p ' ( q )( p ) t t 2   H, H [ q ( , t ), p ( , t )] d x x x 1         H 2 D ( q ) q p ( q )( p ) 2

  6.         q [ D ( q ) q ( q ) p )] t 1        2 2 p D ( q ) p ' ( q )( p ) t 2 Boundary conditions, in x and t, are determined by specific problem. Mean-field (noiseless) limit: p( x ,t)=0: downhill trajectories        q D ( q ) q t Fluctuations: p( x ,t )≠ 0: uphill trajectories, the optimal density history The probability density of a large deviation is given by the mechanical action along a proper uphill trajectory: T          P H ln S d dt p ( , t ) q ( , t ) x x x t 0 T 1      2 d dt ( q )( p ) x 2 0 If the initial condition is random, one should also find the optimal initial density profile and add to S the Boltzmann- Gibbs free energy “cost” of creating it

  7. MFT emerged in the context of non-equilibrium steady states of lattice gases ρ - ρ + L Expected density profile solves the steady-state mean-field problem    D ( ) d / dx const         (x 0) (x L)         Density fluctuations P [ ( x )] ~ exp L F [ ( x / L )] L 1 F  large deviation functional [ ( x / L )] Reviews: Derrida 2007, Jona-Lasinio 2010, Bertini et al 2014

  8. MFT emerged in the context of non-equilibrium steady states of lattice gases ρ - ρ + L   A ( , ) Average current    J L     P Fluctuations of current ( J ) ~ exp[ L S ( J , , )], L 1      large deviation function S ( J , , )  What is the most probable density profile for given J ? Reviews: Derrida 2007, Jona-Lasinio 2010, Bertini et al. 2014

  9. MFT emerged in the context of non-equilibrium steady states of lattice gases ρ - ρ + L • Non-locality: long range correlations • Uphill trajectory is different from time-reversed downhill trajectory • Non-smooth parameter dependence of large deviation function/functional: “phase transitions” Reviews: Derrida 2007, Jona-Lasinio 2010, Bertini et al. 2014

  10. Non-stationary settings are also interesting Example 1: Formation of void of size L at time T in an initially uniform gas Krapivsky, M and Sasorov 2012 n L    P d / 2 ( L , T ) ~ exp[ T S ( , n )], T 1 , L 1 d T d: dimension of space L large deviation function; Most probable density history S d ( , n ) T

  11. Non-stationary settings are also interesting Example 2: Fluctuations of mass/energy transfer in finite time Derrida and Gerschenfeld 2009a,2009b, Sethuraman and Varadhan 2011, Krapivsky and M 2012, M and Sasorov 2013, 2014, Vilenkin, M and Sasorov 2014           M T [ ( x , T ) ( x , 0 )] dx 0    for Random Walkers     M T T , T 1 (RWs), SSEP and KMP  M     P T ( M ) ~ exp[ T S ( , , )], T 1   T T M         Large deviation function Even is nontrivial T S ( , , ) ?   T What is the most probable history of the density field conditional on M T ?

  12. Non-stationary settings Example 3 (this talk): Target survival problem n 0 Diffusion-controlled reactions R Smoluchowski 1917 What is the probability that no particle hit the target until t=T? What is the most probable density history of the gas conditional on the non-hitting? For a given lattice gas, the answers depend on three parameters: R l  , d , n 0 DT

  13. The T → ∞ asymptotic of the target survival probability is known for ideal gas (RWs), see references in Bray, Majumdar and Schehr, Adv. Phys. 62 , 225 (2013) Most probable density histories have not been found even for ideal gas. For non-ideal gases such as SSEP there are no previous results, except for some bounds.

  14. MFT formulation is similar to that for the mass transfer:         q [ D ( q ) q ( q ) p )] + spherical symmetry t 1        2 2 p D ( q ) p ' ( q )( p ) t 2   Boundary condition: q ( r R , t ) 0 The process is conditional on N absorbed particles by time T:   d / 2 2     d 1 M and Redner 2014 dr r [ n q ( r , T )] N  0 ( d / 2 ) R This integral constraint calls for a Lagrangian multiplier  and leads to additional boundary condition (in time) coming from the minimization of action:     p ( r , t T ) ( r R ) The parameter  is ultimately fixed by N=0

  15.    Deterministic, or quenched, initial condition q ( r R , t 0 ) n 0 Once q(r,t) and p(r,t) found:   T d / 2         P d 1 2 ln S(N) dt dr r ( q )( p )  r ( d / 2 ) 0 R Random, or annealed initial condition introduces two changes: • the initial condition becomes p-dependent: q ( r , 0 ) D ( q )      1 p ( r , 0 ) 2 dq ( r R ) ( 1 )  1 ( q ) 1 n 0 (Derrida and Gerschenfeld 2009) • when evaluating the probability, one should add to S the Boltzmann-Gibbs free energy “cost” of creating the optimal initial density profile q(r,0) described by Eq. (1)

  16. Dynamic scaling of the absorption probability MFT equations are invariant under rescaling   t / T t , / DT x x  The radius of absorber becomes l R / DT   N    P d / 2 ln S ( DT ) s  l , , n  , 0 d / 2   ( DT ) We are interested in the limit N->0   1 d / 2       d 1 2 s dt dr r ( q )( p )  r ( d / 2 ) 0 l d=1: S is independent of R, so s doesn’t depend on l leading to survival probability   P 1 / 2 for all diffusive lattice gases ln ( DT ) s ( n ) 1 0 The T 1/2 scaling signals that the 1d-problem is non-stationary. An important consequence is that s 1 (n 0 ) depends on whether the initial condition is deterministic or random.

  17. Long-time asymptotics for d>2: stationary fluctuations dq     D ( q ) ( q ) v 0 zero flux at all times dr   D ( q ) d 1      d 1 2 r v ' ( q ) v 0 , v dp / dr  d 1 r dr 2 This leads to a single nonlinear ODE for q(r):  2     D ' ' dq         2 q 0, where  r     D 2 dr   1 d d      2 d 1 q r  r   d 1 r dr dr

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