Presentation is loading. Please wait.

Presentation is loading. Please wait.

Computer Simulation of Colloids Jürgen Horbach Institut für Materialphysik im Weltraum, Deutsches Zentrum für Luft- und Raumfahrt, Linder Höhe, 51147 Köln.

Similar presentations


Presentation on theme: "Computer Simulation of Colloids Jürgen Horbach Institut für Materialphysik im Weltraum, Deutsches Zentrum für Luft- und Raumfahrt, Linder Höhe, 51147 Köln."— Presentation transcript:

1 Computer Simulation of Colloids Jürgen Horbach Institut für Materialphysik im Weltraum, Deutsches Zentrum für Luft- und Raumfahrt, Linder Höhe, Köln

2  lecture 1 introduction  lecture 2 introduction to the Molecular Dynamics (MD) simulation method  lecture 3 case study: a glassforming Yukawa mixture under shear  lecture 4 introduction to the Monte Carlo (MC) method  lecture 5 case study: phase behavior of colloid-polymer mixtures studied by grandcanonical MC  lecture 6 modelling of hydrodynamic interactions using a hybrid MD-Lattice Boltzmann method

3 Computer Simulations of Colloids Introduction

4 (1) colloids as model systems: different interaction potentials and hydrodynamic interactions (2) correlation functions: describe the structure and dynamics of colloidal fluids (3) outline of the forthcoming lectures

5 (1) colloids as model systems: different interaction potentials and hydrodynamic interactions (2) correlation functions: describe the structure and dynamics of colloidal fluids (3) outline of the forthcoming lectures

6 colloids as model systems size: 10nm – 1µm, dispersed in solvent of viscosity   large, slow, diffusive → optical access  can be described classically  tunable interactions, analytically tractable → theoretical guidance  soft → shear melting phenomena studied via colloidal systems: glass transition, crystallisation in 2d and 3d, systems under shear, sedimentation, phase transitions and dynamics in confinement, etc.

7 hard sphere colloids  confirmed theoretically predicted crystallization (of pure entropic origin)  study of nucleation and crystal growth  test of the mode coupling theory of the glass transition

8 hard spheres soft spheres volume fraction  volume fraction, hair length and density tunable interactions I

9 charged spheres super-paramagnetic spheres magnetic field number density, salt concentration, charge tunable interactions II

10 entropic attraction in colloid-polymer mixtures volume fraction of colloidal particles, number of polymers, colloid/polymer size ratio tunable interactions III  colloid-polymer mixtures may exhibit a demixing transition which is similar to liquid-gas transition in atomistic fluids  transition is of purely entropic origin

11 interaction between colloids due to the momentum transport through the solvent (with viscosity η) hydrodynamic interactions  D ij : hydrodynamic diffusion tensor  decays to leading order ~ r -1 (long-range interactions!)

12  choose some effective interaction between the colloidal particles  but what do we do with the solvent? simulation of a colloidal system simulate the solvent explicitly describe the solvent on a coarse-grained level as a hydrodynamic medium Brownian dynamics (ignores hydrodynamic interactions) ignore the solvent: not important for dynamic properties (glass transition in hard spheres), phase behavior only depends on configurational degrees of freedom

13 (1) colloids as model systems: different interaction potentials and hydrodynamic interactions (2) correlation functions: describe the structure and dynamics of colloidal fluids (3) outline of the forthcoming lectures

14 pair correlation function r Δr small i n p (r) = number of pairs (i,j) with ideal gas: fluid with structural correlations:

15 pair correlation function: hard spheres vs. soft spheres soft sphere fluid: hard sphere fluid:

16 static structure factor microscopic density variable: static structure factor: low q limit: homogeneous fluid: large q:

17 typical structure factor for a liquid  1st peak at ~2π/r p where r p measures the periodicity in g(r)  dense liquid → low compressibility and therefore small value of S(q→0)  in general S(q) appropriate quantity to extract information about intermediate and large length scales  S(q) can be measured in scattering experiments

18 van Hove correlation function  generalization of the pair correlation function to a time-dependent correlation function  self part: proportional to the probability that a particle k at time t is separated by a distance |r k (t) - r l (0)| from a particle l at time 0

19 intermediate scattering functions coherent intermediate scattering function: incoherent intermediate scattering function: can one relate these quantities to transport processes?

20 F(q,t) for a glassforming colloidal system Eckert, Bartsch, Faraday Discuss. 123, 51 (2003)

21 diffusion constants diffusion process self-diffusioninterdiffusion tagged atoms in I concentration differences in I and II homogeneous distribution of tagged particles in I+II homogeneous distribution of red and blue atoms in I+II ↓↓

22 calculation of the self-diffusion constant Einstein relation: Green-Kubo relation: v tag (t): velocity of tagged particle at time t the two relations are strictly equivalent!

23 Computer Simulations of Colloids Molecular Dynamics I: How does it work?

24 Outline MD – how does it work?  numerical integration of the equations of motion  periodic boundary conditions, neighbor lists  MD in NVT ensemble: thermostatting of the system  MD simulation of a 2d Lennard-Jones fluid: structure and dynamics

25 Newton‘s equations of motion  classical system of N particles at positions  U pot : potential function, describes interactions between the particles  simplest case: pairwise additive interaction between point particles  solution of equations of motion yield trajectories of the particles, i.e. positions and velocities of all the particles as a function of time

26 microcanonical ensemble  consider closed system with periodic boundary conditions, no coupling to external degrees of freedom (e.g. a heat bath, shear, electric fields)  particle number N and volume V fixed → microcanonical ensemble  momentum conserved, set initial conditions such that total momentum is zero  total energy conserved:

27 simple observables and ergodicity hypothesis  potential energy :  kinetic energy:  pressure: here is the ensemble average; we assume the ergodicity hypothesis: time average = ensemble average

28 a simple model potential for soft spheres WCA potential:  σ=1, ε=1  cut off at r cut =2 1/6 σ, corresponds to minimum of the Lennard-Jones potential

29 a simple problem N = 144 particles in 2 dimensions:  starting configuration: particles sit on square lattice  velocities from Maxwell-Boltzmann distribution (T = 1.0)  potential energy U = 0 due to d > r cut how do we integrate the equations of motion for this system? L=14.0 d>r cut

30 the Euler algorithm Taylor expansion with respect to discrete time step δt bad algorithm: does not recover time reversibility property of Newton‘s equations of motion → unstable due to strong energy drift, very small time step required

31 the Verlet algorithm consider the following Taylor expansions: equations (1) and (2): velocity form of the Verlet algorithm symplectic algorithm: time reversible and conserves phase space volume addition of Eqs. (1) and (2) yields:

32 implementation of velocity Verlet algorithm do i=1,3*N ! update positions displa=hstep*vel(i)+hstep**2*acc(i)/2 pos(i)=pos(i)+displa fold(i)=acc(i) enddo do i=1,3*N ! apply periodic boundary conditions if(pos(i).lt.0) then pos(i)=pos(i)+lbox else if(pos(i).gt.lbox) pos(i)=pos(i)-lbox endif enddo call force(pos,acc) ! compute forces on the particles do i=1,3*N ! update velocities vel(i)=vel(i)+hstep*(fold(i)+acc(i))/2 enddo

33 neighbor lists force calculation is the most time-consuming part in a MD simulation → save CPU time by using neighbor lists  Verlet list: update when a particle has made a displacement > (r skin -r cut )/2  cell list: most efficient is a combination of Verlet and cell list

34 simulation results I initial configuration with u=0: after 10 5 time steps:

35 energies as a function of time → determine histogramm P(u) for the potential energy for different N

36 pressure

37 fluctuations of the potential energy  dotted lines: fits with Gaussians  width of peaks is directly related to specific heat c V per particle at constant volume V  compare to canonical ensemble

38 simulations at constant temperature: a simple thermostat idea: with a frequency ν assign new velocities to randomly selected particles according to a Maxwell-Boltzmann (MB) distribution with the desired temperature simple version: assign periodically new velocities to all the particles (typically every 150 time steps) algorithm: (i)take new velocities from distribution (ii)total momentum should be zero (iii)scale velocities to desired temperature

39 energies for the simulation at constant temperature

40 pair correlation function  pair correlation function very similar to 3d  no finite size effects visible

41 static structure factor  S(q) also similar to 3d  no finite size effects  low compressibility indicated by small value of S(q) for q→0

42 mean squared displacement diffusion constant increases with increasing system size !?

43 long time tails in 3d Green-Kubo relation for diffusion constant: → power law decay of velocity autocorrelation function (VACF) at long times low density high density Alder, Wainwright, PRA 1, 18 (1970) Levesque, Verlet, PRA 2, 2514 (1970) cage effect in dense liquid:

44 Alder‘s argument Stokes equation describes momentum diffusion: consider momentum in volume element δV at t=0 volume at time t: amount of momentum in original volume element at time t →  d=2:  refined theoretical prediction backflow pattern around particle:

45 effective diffusion constants → larger system sizes required to check theoretical prediction !

46 literature  M. Allen, D. J. Tildesley, Computer Simulation of Liquids (Clarendon Press, Oxford, 1987)  D. Rapaport, The Art of Molecular Dynamics (Cambridge University Press, Cambridge, 1995)  D. Frenkel, B. Smit, Understanding Molecular Simulation: From Algorithms to Applications (Academic Press, San Diego, 1996)  K. Binder, G. Ciccotti (eds.), Monte Carlo and Molecular Dynamics of Condensed Matter Systems (Societa Italiana di Fisica, Bologna, 1996)

47 Computer Simulations of Colloids Molecular Dynamics II: Application to Systems Under Shear with Jochen Zausch (Universität Mainz)

48 shear viscosity of glassforming liquids Poise → Poise → dramatic slowing down of dynamics in a relatively small temperature range

49 F(q,t) for a glassforming colloidal system Eckert, Bartsch, Faraday Discuss. 123, 51 (2003)

50 glassforming fluids under shear apply constant shear rate Weissenberg number: τ(T): relaxation time in equilibrium hard sphere colloid glass: confocal microscopy Besseling et al., PRL (2007)  central question: transient dynamics towards steady state for W >>1  problem amenable to experiment, mode coupling theory and simulation drastic acceleration of dynamics

51 outline  simulation details: interaction model, thermostat, boundary conditions  dynamics from equilibrium to steady state?  dynamics from steady state back to equilibrium?

52 technical requirements (1) model potential (2) external shear field produces heat: thermostat necessary (3) can we model the colloid dynamics realistically? (4) how can we shear the system without using walls?

53 model potential: a binary Yukawa mixture requirements: → binary mixture (no crystallization or phase separation) → colloidal system (more convenient for experiments) → possible coupling to solvent: density not too high

54 equations of motion and thermostat  use of thermostat necessary + colloid dynamics → solve Langevin equation  equations of motion:  dissipative particle dynamics (DPD): → Galilean invariant, local momentum conservation, no bias on shear profile  low ξ (ξ=12): Newtonian dynamics, high ξ (ξ=1200): Brownian dynamics

55 Lees-Edwards boundary conditions  no walls, instead modified periodic boundary conditions  shear flow in x direction, velocity gradient in y direction, “free“ z direction  shear rate: linear shear profile

56 further simulation details  generalized velocity Verlet algorithm, time step  system size: equimolar AB mixture of 1600 particles (N A =N B =800)  L=13.3, density ρ=0.675, volume fraction Φ≈48%  at each temperature at least 30 independent runs  temperature range 1.0 ≥ T ≥ 0.14 (40 million time steps for production runs at T=0.14)

57 self diffusion  B particles slower than A particles  weak temperature dependence of D for sheared systems if  along T = 0.14: W ~

58 shear stress: equilibrium to steady state definition:  maximum around marks transition to plastic flow regime  steady state reached on time scale  time scale on which linear profile evolves? averaging over 250 independent runs

59 shear profile  velocity profile becomes almost linear in the elastic regime  maximum in stress not related to evolution of linear profile

60 structural changes: pair correlation function pair correlation function not very sensitive to structural changes → consider projections of g(r) onto spherical harmonics

61 structure and stresses how is the stress overshoot reflected in dynamic correlations?

62 mean squared displacement  occurrence of superdiffusive regime in the transient plastic flow regime  superdiffusion less pronounced in hard sphere experiment (→ Joe Brader)

63 EQ to SS: superdiffusive transient regime  y: gradient direction z: free direction  measure effective exponent:

64 EQ to SS: Incoherent intermediate scattering function  transients can be described by compressed exponential decay: t w =0: β ≈ 1.8 → different for Brownian dynamics?

65 EQ to SS: Newtonian vs. overdamped dynamics → same compressed exponential decay also for overdamped dynamics change friction coefficient in DPD forces:

66 shear stress: from steady state back to equilibrium  decay can be well described by stretched exponential with β ≈0.7  stressed have completely decayed at

67 SS to EQ: mean squared displacement  stresses relax on time scale of the order of 300 (“crossover“ in t w =0 curve)  then slow aging dynamics toward equilibrium

68 conclusions phenomenology of transient dynamics in glassforming liquids under shear:  binary Yukawa mixture: model for system of charged colloids, using a DPD thermostat and Lees-Edwards boundary conditions  EQ→SS: superdiffusion on time scales between the occurrence of the maximum in the stress and the steady state  SS→EQ: stresses relax on time scale 1/, followed by slow aging dynamics

69 Computer Simulations of Colloids Monte Carlo Simulation I: How does it work?

70 Outline MC – how does it work?  calculation of π via simple sampling and Markov chain sampling  Metropolis algorithm for the canonical ensemble  MC at constant pressure  MC in the grandcanonical ensemble

71 calculation of π  first method: integrate over unit circle  second method: use uniform random numbers → direct sampling → Markov chain sampling Werner Krauth, Statistical Mechanics: Algorithms and Computations (Oxford University Press, Oxford, 2006)

72 calculation of π : direct sampling  estimate π from  algorithm: N hits =0 do i=1,N x=ran(-1,1) y=ran(-1,1) if(x 2 +y 2 <1) N hits =N hits +1 enddo  estimate of π from ratio N hits /N

73 calculation of π : Markov chain sampling  algorithm: N hits =0; x=0.8; y=0.9 do i=1,N Δx=ran(-δ,δ) Δy=ran(-δ,δ) if(|x+Δx|<1.and.|y+Δy|<1) then x=x+Δx; y=y+Δy endif if(x 2 +y 2 <1) N hits =N hits +1 enddo  optimal choice for δ range: not too small and not too large  here good choice δ max =0.3

74 calculation of π with simple and Markov chain sampling simple sampling (N = 4000): run N hits estimate of π run N hits estimate of π Markov chain sampling (N = 4000, δ max = 0.3)

75 simple sampling vs. Markov chain sampling probability density: observable:  simple sampling: A sampled directly through π  Markov sampling: acceptance probability p(old→new) given by

76 more on Markov chain sampling  Markov chain: probability of generating configuration i+1 depends only on the preceding configuration i  important: loose memory of initial condition  consequence of algorithm: points pile up at the boundaries δ max shaded region: piles of sampling points

77 detailed balance  consider discrete system: configurations a, b, c should be generated with equal probability  detailed balance condition holds

78 detailed balance in the calculation of π  one can easiliy show that detailed balance: analog to the time-reversibility property of Newton‘s equations of motion  acceptance probability for a trial move

79 a priori probabilities  generalized acceptance criterion:  moves Δx and Δy in square of linear size δ defines a priori probability p ap (old→new)  different choices possible

80 canonical ensemble  problem: compute expectation value  simple sampling: sample random configurations samples mostly states in the tails of the Boltzmann distribution  direct evaluation of the integrals: does not work!

81 idea of importance sampling  sample configurations according to probability  choose  this can be realized by Markov chain sampling: random walk through regions in phase space where the Boltzmann factor is large, then

82 importance sampling  choose transition probability such that  to achieve this use detailed balance condition  possible choice  yields no information about the partition sum

83 Metropolis algorithm N. Metropolis, A.W. Rosenbluth, M.N. Rosenbluth, A.H. Teller, E. Teller, JCP 21, 1087 (1953) old configuration trial configuration ΔE = E(trial) - E(old) ΔE ≤ 0 ? new config. = trial config. r < exp[-ΔE/(k B T)] ? new config. = old config. yes no  r uniform random number 0 < r < 1  displacement move  acceptance probability

84 implementation of the Metropolis algorithm do icycl=1,ncycl old=int[ran(0,1)*N]+1 ! select a particle at random call energy(x(old),en_old) ! energy of old conf. xn=x(old)+(ran(0,1)-0.5)*disp_x ! random displacement call energy(x(new),en_new) ! energy of new conf. if(ran(0,1).lt.exp[ -beta*(en_new-en_old) ] ) x(old)=x(new) if( mod(icycl,nsamp).eq.0) call sample ! sample averages enddo

85 dynamic interpretation of the Metropolis precedure probability that at time t a configuration r (N) occurs during the Monte Carlo simulation rate equation (or master equation): equilibrium: detailed balance condition one possible solution:

86 remarks  Monte Carlo measurements: first equilibration of the system (until P eq is reached), before measurement of physical properties  random numbers: real random numbers are generated by a deterministic algorithm and thus they are never really random (be aware of correlation effects)  a priori probability: can be used to get efficient Monte Carlo moves!

87 Monte Carlo at constant pressure system of volume V in contact with an ideal gas reservoir via a piston V V 0 - V acceptance probability for volume moves: trial move:

88 grand-canonical Monte Carlo system of volume V in contact with an ideal gas reservoir with fugacity V V 0 - V insertion: removal:

89 textbooks on the Monte Carlo simulation method  D. P. Landau, K. Binder, A Guide to Monte Carlo Simulations in Statistical Physics (Cambridge University Press, Cambridge, 2000)  W. Krauth, Statistical Mechanics: Algorithms and Computations (Oxford University Press, Oxford, 2006)  M. Allen, D. J. Tildesley, Computer Simulation of Liquids (Clarendon Press, Oxford, 1987)  D. Frenkel, B. Smit, Understanding Molecular Simulation: From Algorithms to Applications (Academic Press, San Diego, 1996)  K. Binder, G. Ciccotti (eds.), Monte Carlo and Molecular Dynamics of Condensed Matter Systems (Societa Italiana di Fisica, Bologna, 1996)

90 Computer Simulations of Colloids Monte Carlo II: Phase Behaviour of Colloid-Polymer Mixtures collaborations: Richard Vink, Andres De Virgiliis, Kurt Binder

91 depletion interactions in colloid-polymer mixtures → demixing transition possible into colloid-rich phase (liquid) and colloid-poor phase (gas) polymers cannot move into depletion zones of colloids with their center of mass  gain of free volume if there is overlap of the depletion zones of two colloids  effective attraction between colloids (of entropic origin)

92 Asakura-Oosawa (AO) model in the following AO model for R p /R c = 0.8: → exhibits demixing transition into a colloid-poor phase (gas) and a colloid-rich phase (liquid) → temperature not relevant; what is the corresponding variable here?

93 Outline phase diagram: AO model for R P /R C = 0.8:  binodal  critical point (FSS)  interfacial tension  interfacial width  capillary waves

94  volume V, polymer fugacity z P and colloid fugacity z C fixed → removal and insertion of particles  problem 1: high free energy barrier between coexisting phases in the two-phase region (far away from the critical point) → use successive umbrella sampling  problem 2: low acceptance rate for trial insertion of colloidal particle, high probability that it overlaps with a polymer particles → use cluster move grandcanonical MC for the AO model

95 problem: high free energy barrier between coexisting phases successive umbrella sampling

96 cluster move try to replace n r ≤ n P polymers (A) by a colloid (B): reverse move (C+D): sphere of radius δ and volume V δ around randomly selected point problem: low acceptance rate for trial insertion of a colloid → cluster move R.L.C. Vink, J. H., JCP 121, 3253 (2004)

97 phase diagram → estimate interfacial tension by γ = ΔF/(2A) (Binder 1982) critical point from finite size scaling → 3D Ising universality class

98 finite size scaling cumulant ratio → critical value η r P,cr ≈0.766

99 interfacial tension γ*≡(2R C ) 2 γ as a function of the difference in the colloid packing fraction of the liquid (L) and the vapor (V) phase at coexistence → DFT (M. Schmidt et al.) yields accurate result

100 interfacial profile mean field result: → strong finite size effects (not due to critical fluctuations), L x,y =31.3, L x,y =23.1

101 capillary wave theory  free energy cost of spatial interfacial fluctuations (long wavelength limit)  result for mean square amplitude of the interfacial thickness  combination with mean-field result by convolution approximation → determination of intrinsic width w 0 by simulation not possible

102 is CWT valid? logarithmic divergence? lateral dimension L x = L y large enough?

103 finite size scaling II  map on universal 3D Ising distribution  account for field mixing → AO model belongs to 3D Ising universality class

104 conclusions discrepancies to mean-field results  AO model belongs to 3D Ising universality class  interfacial broadening by capillary waves much more on the AO model in R.L.C. Vink, J.H., JCP 121, 3253 (2004); R.L.C. Vink, J.H., JPCM 16, S3807 (2004); R.L.C. Vink, J.H., K. Binder, JCP 122, (2005); R.L.C. Vink, J.H., K. Binder, PRE 71, (2005); R.L.C. Vink, M. Schmidt, PRE 71, (2005); R.L.C. Vink, K. Binder, J.H., Phys. Rev. E 73, (2006); R.L.C. Vink, K. Binder, H. Löwen, PRL 97, (2006); R.L.C. Vink, A. De Virgiliis, J.H. K. Binder, PRE 74, (2006); A. De Virgiliis, R.L.C. Vink, J.H., K. Binder, Europhys. Lett. 77, (2007); K. Binder, J.H., R.L.C. Vink, A. De Virgiliis, Softmatter (2008).

105 Computer Simulations of Colloids Modelling of hydrodynamic interactions collaboration: Apratim Chatterji (FZ Jülich)

106 simulation of colloids colloids:  size 10 nm – 1 μm  mesoscopic time scales solvent:  atomistic time (~ 1 ps) and length scales (~ Å) simulation difficult due to different time and length scales → coarse graining of solvent‘s degrees of freedom

107 Langevin equation Brownian particles of mass M : f r,i uncorrelated random force with zero mean: fluctuation-dissipation theorem:  many collisions with solvent particles on typical time scale of colloid  systematic friction force on colloid

108 decay of velocity correlations consider single Brownian particle of mass M : → exponential decay of velocity autocorrelation function (VACF) correct behavior: power law decay of VACF due to local momentum conservation

109 generalized Langevin equation  idea: couple velocity of colloid to the local fluid velocity field via frictional force  point particle: problems:  determination of hydrodynamic velocity field from solution of Navier-Stokes equation  rotational degrees of freedom → colloid-fluid coupling?

110 lattice Boltzmann method I  : number of particles at a lattice node, at a time t, with a velocity  discrete analogue of kinetic equation: Δ i : collision operator  velocity space from projection of 4D FCHC lattice onto 3D (isotropy)  moments of n i :

111 lattice Boltzmann method II  linearized collision operator:  equilibrium distr.:  recover linearized Navier-Stokes equations:  thermal fluctuations: add noise terms to stress tensor

112 lattice Boltzmann algorithm III  collision step: compute  propagation step: compute

113 colloid fluid momentum exchange sphere represented by (66) uniformly distributed points on its surface each point exchanges momentum with surrounding fluid nodes

114 velocity correlations at short times give particle a kick and determine decay of its velocity blue curves: red curves: fluid velocity at the surface of the sphere

115 C v (t) and C ω (t) independent of R and ξ 0 I: moment of inertia

116 thermal fluctuations ok? linear response theory: velocity relaxation of kicked particle in a fluid at rest = velocity autocorrelation function of particle in a thermal bath

117 charged colloids

118 colloids in electric field


Download ppt "Computer Simulation of Colloids Jürgen Horbach Institut für Materialphysik im Weltraum, Deutsches Zentrum für Luft- und Raumfahrt, Linder Höhe, 51147 Köln."

Similar presentations


Ads by Google