collective dynamics in life sciences
play

Collective dynamics in life sciences Lecture 2: the Vicsek model - PowerPoint PPT Presentation

1 Collective dynamics in life sciences Lecture 2: the Vicsek model Pierre Degond Imperial College London pdegond@imperial.ac.uk (see http://sites.google.com/site/degond/) Joint works with: Amic Frouvelle (Dauphine), Jian-Guo Liu (Duke), S


  1. 1 Collective dynamics in life sciences Lecture 2: the Vicsek model Pierre Degond Imperial College London pdegond@imperial.ac.uk (see http://sites.google.com/site/degond/) Joint works with: Amic Frouvelle (Dauphine), Jian-Guo Liu (Duke), S´ ebastien Motsch (ASU) ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  2. Summary 2 1. The Vicsek model 2. Mean-Field model 3. Self-Organized Hydrodynamics (SOH) 4. Properties of the SOH model and extensions 5. Conclusion ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  3. 3 1. The Vicsek model ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  4. Vicsek model [Vicsek, Czirok, Ben-Jacob, Cohen, Shochet, PRL 95] 4 Individual-Based (aka particle) model self-propelled ⇒ all particles have same constant velocity a align with their neighbours up to a certain noise Time-discrete model k , at t n = n ∆ t k -th particle position X n k , velocity direction V n X n +1 = X n k + aV n | V n k ∆ t, k | = 1 R k V k k = J n � ¯ J n V n V n k X k k = j , |J n k | j, | X n j − X n k |≤ R ) = arg ( ¯ arg ( V n +1 V n k + τ n k ) k τ n k drawn uniformly in [ − τ, τ ] ; R = interaction range J n k = local particle flux in interaction disk ¯ V n k = neighbors’ average direction ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  5. 5 2. Mean-Field model ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  6. Time continuous Vicsek model 6 Passage to time continuous dynamics: requires introduction of new parameter: interaction frequency ν ˙ X k ( t ) = aV k ( t ) √ k ◦ ( ν ¯ 2 τ dB k dV k ( t ) = P V ⊥ V k dt + t ) , P V ⊥ k = Id − V k ⊗ V k V k = J k � ¯ J k = V j , √ 2 τ dB k ν ¯ |J k | V k dt t j, | X j − X k |≤ R V k dV k ¯ V k Recover original Vicsek by: S 1 Time discretization ∆ t s.t. ν ∆ t = 1 Gaussian noise → uniform here ( X k , V k ) ∈ R n × R n , n ≥ 2 Dimension n = 2 ; ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  7. Mean-field model 7 f ( x, v, t ) = particle probability density ν ¯ v f v satisfies a Fokker-Planck equation F f v f ¯ S 1 ∂ t f + av · ∇ x f + ∇ v · ( F f f ) = τ ∆ v f F f ( x, v, t ) = P v ⊥ ( ν ¯ v f ( x, t )) , P v ⊥ = Id − v ⊗ v v f ( x, t ) = J f ( x, t ) � � ¯ |J f ( x, t ) | , J f ( x, t ) = S n − 1 f ( y, w, t ) w dw dy | y − x | <R J f ( x, t ) = particle flux in a neighborhood of x v f ( x, t ) = direction of this flux ¯ F f ( x, v, t )) = projection of the flux direction on v ⊥ ( x, v ) ∈ R n × S n − 1 ; ∇ v · , ∇ v : div and grad on S n − 1 ∆ v Laplace-Beltrami operator on the sphere ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  8. Passage to dimensionless units 8 Highlights important physical scales & small parameters Choose time scale t 0 , space scale x 0 = at 0 Set f scale f 0 = 1 /x n 0 , F scale F 0 = 1 /t 0 τ = τt 0 , ¯ R = R Introduce dimensionless parameters ¯ ν = νt 0 , ¯ x 0 x = x 0 x ′ , t = t 0 t ′ , f = f 0 f ′ , F = F 0 F ′ Change variables Get the scaled Fokker-Planck system (omitting the primes): ∂ t f + v · ∇ x f + ∇ v · ( F f f ) = ¯ τ ∆ v f F f ( x, v, t ) = P v ⊥ (¯ ν ¯ v f ( x, t )) , P v ⊥ = Id − v ⊗ v v f ( x, t ) = J f ( x, t ) � � ¯ |J f ( x, t ) | , J f ( x, t ) = S n − 1 f ( y, w, t ) w dw dy | y − x | < ¯ R ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  9. Macroscoping scaling 9 τ = 1 Choice of t 0 such that ¯ ε , ε ≪ 1 Macroscopic scale: there are many velocity diffusion events within one time unit k := ¯ ν Assumption 1: τ = O (1) ¯ Social interaction and diffusion act at the same scale ν − 1 = O ( ε ) , i.e. mean-free path is microscopic Implies ¯ ¯ Assumption 2: R = ε Interaction range is microscopic ν − 1 and of the same order as mean-free path ¯ R = O ( √ ε ) : interaction range still small Possible variant: ¯ but large compared to mean-free path. To be investigated later ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  10. Fokker-Planck under macroscopic scaling 10 With Assumption 2 ( ¯ R = O ( ε ) ) Interaction is local at leading order: by Taylor expansion: � J f = J f + O ( ε 2 ) , J f ( x, t ) = S n − 1 f ( x, w, t ) w dw J f ( x, t ) = local particle flux. From now on, neglect O ( ε 2 ) term Fokker-Planck eq. in scaled variables ε ( ∂ t f ε + v · ∇ x f ε ) + ∇ v · ( F ε f ε ) = ∆ v f ε F ε ( x, v, t ) = kP v ⊥ u f ε ( x, t ) u f ε ( x, t ) = J f ε � S n − 1 f ε ( x, w, t ) w dw | J f ε | , J f ε ( x, t ) = Hydrodynamic model is obtained in the limit ε → 0 ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  11. 11 3. Self-Organized Hydrodynamics (SOH) ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  12. Collision operator 12 Model can be written ∂ t f ε + v · ∇ x f ε = 1 εQ ( f ε ) with collision operator Q ( f ) = −∇ v · ( F f f ) + ∆ v f F f = kP v ⊥ u f u f = J f � | J f | , J f = S n − 1 f ( x, w, t ) w dw When ε → 0 , f ε → f (formally) such that Q ( f ) = 0 ⇒ importance of the solutions of Q ( f ) = 0 (equilibria) Q acts on v -variable only ( ( x, t ) are just parameters) ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  13. Algebraic preliminaries 13 Force F f can be written: F f ( v ) = k ∇ v ( u f · v ) Note u f independent of v ( ( x, t ) are fixed) Rewrite: � � Q ( f )( v ) = ∇ v · − f k ∇ v ( u f · v ) + ∇ v f � � = ∇ v · f ∇ v ( − k u f · v + ln f ) Let u ∈ S n − 1 be given: Solutions of ∇ v ( − k u · v + ln f ) = 0 are proportional to : e ku · v f ( v ) = M ku ( v ) := � S n − 1 e ku · v dv von Mises-Fisher (VMF) distribution ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  14. VMF distribution 14 Again: e ku · v M ku ( v ) := � S n − 1 e ku · v dv u ∈ S n − 1 : orientation k > 0 : concentration parameter; � Order parameter: c 1 ( k ) = S n − 1 M ku ( v ) u · v dv ր k → c 1 ( k ) , 0 ≤ c 1 ( k ) ≤ 1 � Flux: S n − 1 M ku ( v ) v dv = c 1 ( k ) u Here: concentration parameter k and order parameter c 1 ( k ) are constant ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  15. Equilibria 15 Definition: equilibrium manifold E = { f ( v ) | Q ( f ) = 0 } Theorem: E = { ρM ku for arbitrary ρ ∈ R + and u ∈ S n − 1 } Note: dim mediumblue E = n Proof: follows from entropy inequality: 2 � �� f f � � � H ( f ) = Q ( f ) M kuf dv = − M ku f � ∇ v ≤ 0 � � M kuf � f � � �� follows from Q ( f ) = ∇ v · M ku f ∇ v M kuf f Then, Q ( f ) = 0 implies H ( f ) = 0 and M kuf = Constant and f is of the form ρM ku Reciprocally, if f = ρM ku , then, u f = u and Q ( f ) = 0 ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  16. Use of equilibria 16 f ε → f as ε → 0 with v → f ( x, v, t ) ∈ E for all ( x, t ) Implies that f ( x, v, t ) = ρ ( x, t ) M ku ( x,t ) Need to specify the dependence of ρ and u on ( x, t ) Requires n equations since ( ρ, u ) ∈ R + × S n − 1 are determined by n independent real quantities f satisfies ∂ t f + v · ∇ x f = lim ε → 0 1 ε Q ( f ε ) Problem: lim ε → 0 1 ε Q ( f ε ) is not known Trick: Collision invariant ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  17. Collision invariant 17 � is a function ψ ( v ) such that Q ( f ) ψ dv = 0 , ∀ f Form a linear vector space C Multiply eq. by ψ : ε − 1 term disappears Find a conservation law: � � � � � � ∂ t S n − 1 f ( x, v, t ) ψ ( v ) dv + ∇ x · S n − 1 f ( x, v, t ) ψ ( v ) v dv = 0 � Have used that ∂ t or ∇ x and . . . dv can be interchanged Limit fully determined if dim C = dim E = n C = Span { 1 } . Interaction preserves mass but no other quantity Due to self-propulsion, no momentum conservation dim C = 1 < dim E = n . Is the limit problem ill-posed ? ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

  18. Use of CI: mass conservation eq. 18 Proof that ψ ( v ) = 1 is a CI ? � � Obvious. Q ( f ) = ∇ v · . . . is a divergence � By Stokes theorem on the sphere, Q ( f ) dv = 0 Use of the CI ψ ( v ) = 1 : Get the conservation law � � � � � � ∂ t S n − 1 f ( x, v, t ) dv + ∇ x · S n − 1 f ( x, v, t ) v dv = 0 With f = ρM ku we have � � f ( x, v, t ) dv = ρ ( x, t ) , f ( x, v, t ) v dv = ρc 1 u We end up with the mass conservation eq. ∂ t ρ + c 1 ∇ x · ( ρu ) = 0 ↑ ↓ Pierre Degond - Collective dynamics in life sciences, Lect. # 2 - CIRM, April 2017

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