CHEM699.08 Lecture #9 Calculating Time-dependent Properties June 28, 2001 MM 1 st Ed. Chapter 6 -- 333-342 MM 2 nd Ed. Chapter 7.6 -- 374-382 [ 1 ]

Slides:



Advertisements
Similar presentations
Time averages and ensemble averages
Advertisements

Intermediate Physics for Medicine and Biology Chapter 4 : Transport in an Infinite Medium Professor Yasser M. Kadah Web:
Lecture 15: Capillary motion
Fourier law Conservation of energy The geotherm
Aero-Hydrodynamic Characteristics
Ch 24 pages Lecture 8 – Viscosity of Macromolecular Solutions.
Revision Previous lecture was about Harmonic Oscillator.
Lecture 4 – Kinetic Theory of Ideal Gases
1 Time-Correlation Functions Charusita Chakravarty Indian Institute of Technology Delhi.
Exact results for transport properties of one-dimensional hamiltonian systems Henk van Beijeren Institute for Theoretical Physics Utrecht University.
MASS TRANSPORT OF SOLUTES. I.Basic Processes A. Diffusion B. Advection.
Computational Solid State Physics 計算物性学特論 第2回 2.Interaction between atoms and the lattice properties of crystals.
Incorporating Solvent Effects Into Molecular Dynamics: Potentials of Mean Force (PMF) and Stochastic Dynamics Eva ZurekSection 6.8 of M.M.
Carrier Transport Phenomena
Transport Processes 2005/4/24 Dept. Physics, Tunghai Univ. Biophysics ‧ C. T. Shih.
Lecture 3 The Debye theory. Gases and polar molecules in non-polar solvent. The reaction field of a non-polarizable point dipole The internal and the direction.
Group problem solutions 1.(a) (b). 2. In order to be reversible we need or equivalently Now divide by h and let h go to Assuming (as in Holgate,
Transport Equations and Flux Laws Basic concepts and ideas 1.A concept model of Diffusion 2.The transient Diffusion Equation 3.Examples of Diffusion Fluxes.
Chapter 1 Vector analysis
Fluctuations and Brownian Motion 2  fluorescent spheres in water (left) and DNA solution (right) (Movie Courtesy Professor Eric Weeks, Emory University:
Atkins’ Physical Chemistry Eighth Edition Chapter 21 – Lecture 2 Molecules in Motion Copyright © 2006 by Peter Atkins and Julio de Paula Peter Atkins Julio.
Chapter 4 Fluid Flow, Heat Transfer, and Mass Transfer:
Viscosity. Average Speed The Maxwell-Boltzmann distribution is a function of the particle speed. The average speed follows from integration.  Spherical.
Chapter 21 & 22 Electric Charge Coulomb’s Law This force of repulsion or attraction due to the charge properties of objects is called an electrostatic.
Gravity and Orbits The gravitational force between two objects:
Bioseparation Dr. Kamal E. M. Elkahlout Chapter 3 Mass transfer.
Boundary Conditions Monte Carlo and Molecular Dynamics simulations aim to provide information about the properties of a macroscopic sample (by simulating.
1 April 14 Triple product 6.3 Triple products Triple scalar product: Chapter 6 Vector Analysis A B C + _.
ENE 311 Lecture 2. Diffusion Process The drift current is the transport of carriers when an electric field is applied. There is another important carrier.
© 2012 Eric Pop, UIUCECE 340: Semiconductor Electronics ECE 340 Lectures Diffusion of carriers Remember Brownian motion of electrons & holes! When.
Atkins’ Physical Chemistry Eighth Edition Chapter 21 – Lecture 1 Molecules in Motion Copyright © 2006 by Peter Atkins and Julio de Paula Peter Atkins Julio.
Basics of molecular dynamics. Equations of motion for MD simulations The classical MD simulations boil down to numerically integrating Newton’s equations.
Ch 24 pages Lecture 7 – Diffusion and Molecular Shape and Size.
Chapter 21: Molecules in motion Diffusion: the migration of matter down a concentration gradient. Thermal conduction: the migration of energy down a temperature.
Yoon kichul Department of Mechanical Engineering Seoul National University Multi-scale Heat Conduction.
Introduction 1. Similarity 1.1. Mechanism and mathematical description 1.2. Generalized variables 1.3. Qualitative analysis 1.4. Generalized individual.
Ch 24 pages Lecture 9 – Flexible macromolecules.
Ch 24 pages Lecture 10 – Ultracentrifugation/Sedimentation.
LES of Turbulent Flows: Lecture 2 (ME EN )
Understanding Molecular Simulations Introduction
Cell Biology Core Cell Optimization and Robustness : Countless cycles of replication and death have occurred and the criterion for survival is the passage.
21.4 Transport properties of a perfect gas
Molecular Modelling - Lecture 2 Techniques for Conformational Sampling Uses CHARMM force field Written in C++
Step 1: Derive an expression that shows how the pressure of a gas inside an effusion oven varies with time if the oven is not replenished as the gas escapes.
Ch 24 pages Lecture 11 – Equilibrium centrifugation.
Chapter 21: Molecules in motion Diffusion: the migration of matter down a concentration gradient. Thermal conduction: the migration of energy down a temperature.
1 CE 530 Molecular Simulation Lecture 12 David A. Kofke Department of Chemical Engineering SUNY Buffalo
Interacting Molecules in a Dense Fluid
Chapter 16 Kinetic Theory of Gases. Ideal gas model 2 1. Large number of molecules moving in random directions with random speeds. 2. The average separation.
Transport Phenomena and Diffusion ( ) Net motion of particles occurs when a system is disturbed from equilibrium (e.g., concentration gradients)concentration.
Molecular dynamics (4) Treatment of long-range interactions Computing properties from simulation results.
3/23/2015PHY 752 Spring Lecture 231 PHY 752 Solid State Physics 11-11:50 AM MWF Olin 107 Plan for Lecture 23:  Transport phenomena and Fermi liquid.
Statistical Mechanics of Proteins  Equilibrium and non-equilibrium properties of proteins  Free diffusion of proteins  Coherent motion in proteins:
Conductor, insulator and ground. Force between two point charges:
HW/Tutorial # 1 WRF Chapters 14-15; WWWR Chapters ID Chapters 1-2 Tutorial #1 WRF#14.12, WWWR #15.26, WRF#14.1, WWWR#15.2, WWWR#15.3, WRF#15.1, WWWR.
Particle Tracking for CDC prototype Amangaliyev Temirlan.
Thursday, Sept. 8, 2011PHYS , Fall 2011 Dr. Jaehoon Yu 1 PHYS 1444 – Section 003 Lecture #6 Thursday, Sept. 8, 2011 Dr. Jaehoon Yu Chapter 21 –Electric.
Chapter 22 Electric Fields The Electric Field: The Electric Field is a vector field. The electric field, E, consists of a distribution of vectors,
Transport process In molecular transport processes in general we are concerned with the transfer or movement of a given property or entire by molecular.
Non-local Transport of Strongly Coupled Plasmas Satoshi Hamaguchi, Tomoyasu Saigo, and August Wierling Department of Fundamental Energy Science, Kyoto.
Chapter 6 Vector Analysis
Lecture 34: Diffusion and Chemical Potential
Dynamical correlations & transport coefficients
thermal conductivity of a gas
Chapter 22 Electric Fields.

Chapter 6 Vector Analysis
Stochastic rotation dynamics
Dynamical correlations & transport coefficients
Dynamical correlations & transport coefficients
Presentation transcript:

CHEM Lecture #9 Calculating Time-dependent Properties June 28, 2001 MM 1 st Ed. Chapter MM 2 nd Ed. Chapter [ 1 ]

Calculating Time-dependent Properties [ 2 ] An advantage of a molecular dynamics (MD) simulation over a Monte Carlo simulation is that each successive iteration of the system is connected to the previous state(s) of the system in time. ¤ The evolution of a MD simulation over time allows the data, or some property, at one time (t) to be related to the same or different properties at some other time (t+  t). ¤ A time correlation coefficient is a calculated measurement of the degree of correlation for an observed time-dependent property. ¤

[ 3 ] Calculating Time-dependent Properties Our “simple” 2D MD simulation of a single hard sphere moving through an arbitrarily chosen plane. ¤

[ 3 ] Calculating Time-dependent Properties x y Our “simple” 2D MD simulation of a single hard sphere moving through an arbitrarily chosen plane. ¤

[ 3 ] Calculating Time-dependent Properties Is the movement of the sphere in the x direction related to the motion in the y direction? ¤ x y Our “simple” 2D MD simulation of a single hard sphere moving through an arbitrarily chosen plane. ¤

[ 3 ] Calculating Time-dependent Properties t = 0 x y Our “simple” 2D MD simulation of a single hard sphere moving through an arbitrarily chosen plane. ¤ Is the movement of the sphere in the x direction related to the motion in the y direction? ¤

[ 3 ] Calculating Time-dependent Properties x y t = 0 t = 1 Our “simple” 2D MD simulation of a single hard sphere moving through an arbitrarily chosen plane. ¤ Is the movement of the sphere in the x direction related to the motion in the y direction? ¤

[ 3 ] Calculating Time-dependent Properties x y t = 0 t = 1t = 2 Our “simple” 2D MD simulation of a single hard sphere moving through an arbitrarily chosen plane. ¤ Is the movement of the sphere in the x direction related to the motion in the y direction? ¤

[ 3 ] Calculating Time-dependent Properties x y t = 0 t = 1t = 2t = 3 Our “simple” 2D MD simulation of a single hard sphere moving through an arbitrarily chosen plane. ¤ Is the movement of the sphere in the x direction related to the motion in the y direction? ¤

[ 3 ] Calculating Time-dependent Properties x y t = 0 t = 1t = 2t = 3 t = 4 Our “simple” 2D MD simulation of a single hard sphere moving through an arbitrarily chosen plane. ¤ Is the movement of the sphere in the x direction related to the motion in the y direction? ¤

[ 3 ] Calculating Time-dependent Properties x y t = 0 t = 1t = 2t = 3 t = 4t = 5 Our “simple” 2D MD simulation of a single hard sphere moving through an arbitrarily chosen plane. ¤ Is the movement of the sphere in the x direction related to the motion in the y direction? ¤

[ 4 ] Calculating Time-dependent Properties If there are two sets of data, x and y, the correlation between them (C xy ) can be defined as: ¤ (1)

[ 4 ] Calculating Time-dependent Properties If there are two sets of data, x and y, the correlation between them (C xy ) can be defined as: ¤ This can also be normalized to a value between -1 and +1 by dividing by the rms of x and y: ¤ (1) (2)

[ 5 ] Calculating Time-dependent Properties A value of c xy = 0 would indicate no correlation between the values of x and y, while a value of 1 indicates a high degree of correlation. ¤

[ 5 ] Calculating Time-dependent Properties A value of c xy = 0 would indicate no correlation between the values of x and y, while a value of 1 indicates a high degree of correlation. ¤ If x and y are found to only fluctuate around some average value as would be the case for bond lengths, for example, Equation 2 is commonly expressed only as the fluctuating part of x and y. ¤ (3)

Calculating Time-dependent Properties One drawback to Equation 3 is that the mean values of x and y can’t accurately be known until the MD simulation has completed all M steps. ¤ [ 6 ]

Calculating Time-dependent Properties One drawback to Equation 3 is that the mean values of x and y can’t accurately be known until the MD simulation has completed all M steps. ¤ Tired of waiting for those pesky MD simulations to finish before generating your time-correlation coefficients? ¤ [ 6 ] Well there’s a way around this. ¤

[ 7 ] Calculating Time-dependent Properties Equation 3 can be re-written without the mean values of x and y: ¤ (4) This expression allows for the calculation of c xy on the fly, as the MD simulation progresses! ¤

[ 8 ] Calculating Time-dependent Properties As the MD simulation proceeds the values of one property can be compared to the same, or another property at a later time: ¤ (5)

[ 8 ] Calculating Time-dependent Properties As the MD simulation proceeds the values of one property can be compared to the same, or another property at a later time: ¤ (5) If x and y are different properties, then C xy is referred to as a cross-correlation function. If x and y are the same property, then this is referred to as an autocorrelation function. ¤ The autocorrelation function can be though of as an indication of how long the system retains a “memory” of its previous state. ¤

[ 9 ] Calculating Time-dependent Properties An example is the velocity autocorrelation coefficient which gives an indication of how the velocity at time (t) correlates with the velocity at another time. ¤ (6) (7) We can normalize the velocity autocorrelation coefficient thusly: ¤

[ 10 ] Calculating Time-dependent Properties For properties like velocities, the value of c vv at time t = 0 would be 1, while at loner times c vv would be expected to go to 0. ¤ The time required for the correlation to go to 0 is referred to as the correlation time, or the relaxation time. The MD simulation must be at least long enough to meet the relaxation time, obviously. ¤

Calculating Time-dependent Properties For properties like velocities, the value of c vv at time t = 0 would be 1, while at loner times c vv would be expected to go to 0. ¤ The time required for the correlation to go to 0 is referred to as the correlation time, or the relaxation time. The MD simulation must be at least long enough to meet the relaxation time, obviously. ¤ For long MD simulations the relaxation times can be calculated relative to several starting points in order to reduce the uncertainty. ¤ Fig.1 [ 10 ]

Calculating Time-dependent Properties Shown here are the velocity autocorrelation functions for the MD simulations of argon at two different densities. ¤ Time (ps) c vv (t) At time t = 0 the velocity autocorrelation function is highly correlated as expected, and begins to decrease toward 0. ¤ Fig.2 [ 11 ]

Calculating Time-dependent Properties The long time tail of c vv (t) has been ascribed to “hydrodynamic vortices” which form around the moving particles, giving a small additive contribution to their velocity. ¤ Fig.3 [ 12 ]

[ 13 ] Calculating Time-dependent Properties This slow decay of the time correlation toward 0 can be problematic when trying to establish a time frame for the MD simulation, and also in the derivation of some properties. ¤ Transport coefficients require the correlation function to be integrated between time t = 0 and t =  ¤ In cases where the time correlation has a long time-tail there will be fewer blocks of data over a sufficiently wide time span to reduce the uncertainty in the correlation coefficients. ¤

[ 14 ] Calculating Time-dependent Properties Another example is the net dipole moment of the system. This requires the summation of the individual dipoles (vector quantities) of each molecule in the system -- which will change over time. ¤ (8)

[ 14 ] Calculating Time-dependent Properties Another example is the net dipole moment of the system. This requires the summation of the individual dipoles (vector quantities) of each molecule in the system -- which will change over time. ¤ (8) The total dipole correlation function is expressed as:¤ (9)

[ 15 ] Calculating Time-dependent Properties Transport Properties¤ A mass or concentration gradient will give rise to a flow of material from one region to another until the concentration is even throughout. ¤ Here we will deal with calculating non-equilibrium properties by considering local fluctuations in a system already at equilibrium. ¤ The word “transport” suggests the system is at non-equilibrium.¤ Examples: temperature gradient, mass gradient, velocity gradient, etc. ¤

[ 16 ] Calculating Time-dependent Properties The flux (transport of some quantity) can be expressed by Fick’s first law of diffusion thusly: ¤ (10) J z =  D (d N / dz)

[ 16 ] Calculating Time-dependent Properties The flux (transport of some quantity) can be expressed by Fick’s first law of diffusion thusly: ¤ (10) J z =  D (d N / dz) The time dependence (time-evolution of some distribution) is expressed by Fick’s second law: ¤ (11)  N (z,t)  t  2 N (z,t)  z 2 = D

Calculating Time-dependent Properties [ 17 ] Einstein showed that the diffusion coefficient (D) is related to the mean square of the distance, and in 3-dimensions this is given by: ¤ (12) 3D =

Calculating Time-dependent Properties Einstein showed that the diffusion coefficient (D) is related to the mean square of the distance, and in 3-dimensions this is given by: ¤ (12) It is important to point out that Fick’s law only applies at long time durations, such as the case above. To a good approximation some duration where “t” effectively approaches infinity as far as the simulation is concerned will be sufficient. ¤ [ 17 ] 3D =

Calculating Time-dependent Properties ~ fin ~ [ 18 ]