Javier Junquera. Statistical mechanics

Similar documents
Basics of Statistical Mechanics

MD Thermodynamics. Lecture 12 3/26/18. Harvard SEAS AP 275 Atomistic Modeling of Materials Boris Kozinsky

Basics of Statistical Mechanics

What is Classical Molecular Dynamics?

Temperature and Pressure Controls

Analysis of MD Results Using Statistical Mechanics Methods. Molecular Modeling

ChE 503 A. Z. Panagiotopoulos 1

REVIEW. Hamilton s principle. based on FW-18. Variational statement of mechanics: (for conservative forces) action Equivalent to Newton s laws!

Gear methods I + 1/18

(# = %(& )(* +,(- Closed system, well-defined energy (or e.g. E± E/2): Microcanonical ensemble

Statistical Mechanics in a Nutshell

Temperature and Pressure Controls

Computer simulation methods (1) Dr. Vania Calandrini

Brief Review of Statistical Mechanics

Appendix C extra - Concepts of statistical physics Cextra1-1

Time-Dependent Statistical Mechanics 5. The classical atomic fluid, classical mechanics, and classical equilibrium statistical mechanics

Computer simulations as concrete models for student reasoning

1. Thermodynamics 1.1. A macroscopic view of matter

Ab initio molecular dynamics and nuclear quantum effects

Statistical Mechanics

Thus, the volume element remains the same as required. With this transformation, the amiltonian becomes = p i m i + U(r 1 ; :::; r N ) = and the canon

G : Statistical Mechanics

Aspects of nonautonomous molecular dynamics

Understanding Molecular Simulation 2009 Monte Carlo and Molecular Dynamics in different ensembles. Srikanth Sastry

G : Statistical Mechanics

Optimization Methods via Simulation

Energy and Forces in DFT

Dissipation and the Relaxation to Equilibrium

Contents. 1 Introduction and guide for this text 1. 2 Equilibrium and entropy 6. 3 Energy and how the microscopic world works 21

fiziks Institute for NET/JRF, GATE, IIT-JAM, JEST, TIFR and GRE in PHYSICAL SCIENCES

Brownian Motion and Langevin Equations

Exercise 2: Solvating the Structure Before you continue, follow these steps: Setting up Periodic Boundary Conditions

Langevin Dynamics in Constant Pressure Extended Systems


A Deeper Look into Phase Space: The Liouville and Boltzmann Equations

LECTURE 6 : BASICS FOR MOLECULAR SIMULATIONS - Historical perspective - Skimming over Statistical Mechanics - General idea of Molecular Dynamics -

Introduction to Computer Simulations of Soft Matter Methodologies and Applications Boulder July, 19-20, 2012

Lecture 19: Calculus of Variations II - Lagrangian

4. The Green Kubo Relations

Molecular Dynamics Simulations. Dr. Noelia Faginas Lago Dipartimento di Chimica,Biologia e Biotecnologie Università di Perugia

Ab initio molecular dynamics. Simone Piccinin CNR-IOM DEMOCRITOS Trieste, Italy. Bangalore, 04 September 2014

in order to insure that the Liouville equation for f(?; t) is still valid. These equations of motion will give rise to a distribution function f(?; t)

Principles of Equilibrium Statistical Mechanics

Classical Molecular Dynamics

III. Kinetic Theory of Gases

The goal of equilibrium statistical mechanics is to calculate the diagonal elements of ˆρ eq so we can evaluate average observables < A >= Tr{Â ˆρ eq

A Study of the Thermal Properties of a One. Dimensional Lennard-Jones System

Constant Pressure Langevin Dynamics: Theory and Application to the Study of Phase Behaviour in Core-Softened Systems.

Nanoscale Energy Transport and Conversion A Parallel Treatment of Electrons, Molecules, Phonons, and Photons

Molecular Dynamics at Constant Pressure: Allowing the System to Control Volume Fluctuations via a Shell Particle

Introduction. Chapter The Purpose of Statistical Mechanics

Introduction to Simulation - Lectures 17, 18. Molecular Dynamics. Nicolas Hadjiconstantinou

Simulations with MM Force Fields. Monte Carlo (MC) and Molecular Dynamics (MD) Video II.vi

Modeling Biological Systems Opportunities for Computer Scientists


Modeling Materials. Continuum, Atomistic and Multiscale Techniques. gg CAMBRIDGE ^0 TADMOR ELLAD B. HHHHM. University of Minnesota, USA

to satisfy the large number approximations, W W sys can be small.

Scientific Computing II

Chapter 4: Going from microcanonical to canonical ensemble, from energy to temperature.

Heat Transport in Glass-Forming Liquids

Energy Landscapes and Accelerated Molecular- Dynamical Techniques for the Study of Protein Folding

4/18/2011. Titus Beu University Babes-Bolyai Department of Theoretical and Computational Physics Cluj-Napoca, Romania

Introduction Statistical Thermodynamics. Monday, January 6, 14

Statistical Mechanics

An Outline of (Classical) Statistical Mechanics and Related Concepts in Machine Learning

510 Subject Index. Hamiltonian 33, 86, 88, 89 Hamilton operator 34, 164, 166

Chapter 4 Molecular Dynamics and Other Dynamics

Statistical Mechanics

A (short) practical introduction to kinetic theory and thermodynamic properties of gases through molecular dynamics

Citation for published version (APA): Hess, B. (2002). Stochastic concepts in molecular simulation Groningen: s.n.

Hydrodynamics. Stefan Flörchinger (Heidelberg) Heidelberg, 3 May 2010

Foundations of Chemical Kinetics. Lecture 19: Unimolecular reactions in the gas phase: RRKM theory

Statistical Thermodynamics and Monte-Carlo Evgenii B. Rudnyi and Jan G. Korvink IMTEK Albert Ludwig University Freiburg, Germany

Declaration. I, Derrick Beckedahl, declare that

UNIVERSITY OF OSLO FACULTY OF MATHEMATICS AND NATURAL SCIENCES

Before we consider two canonical turbulent flows we need a general description of turbulence.

Lecture 1: Historical Overview, Statistical Paradigm, Classical Mechanics

Advanced sampling. fluids of strongly orientation-dependent interactions (e.g., dipoles, hydrogen bonds)

MP203 Statistical and Thermal Physics. Jon-Ivar Skullerud and James Smith

Nanoscale simulation lectures Statistical Mechanics

Introduction to Molecular Dynamics

Grand Canonical Formalism

Concepts in Materials Science I. StatMech Basics. VBS/MRC Stat Mech Basics 0

Statistical Mechanics of Nonequilibrium Liquids

Condensed Matter Physics Prof. G. Rangarajan Department of Physics Indian Institute of Technology, Madras

Molecular Modeling of Matter

HAMILTON S PRINCIPLE

Approach to Thermal Equilibrium in Biomolecular

Concepts of Thermodynamics

Dynamical and Statistical Mechanical Characterization of Temperature Coupling Algorithms

Chapter 9: Statistical Mechanics

Set the initial conditions r i. Update neighborlist. r i. Get new forces F i

Entropy and Ergodic Theory Lecture 12: Introduction to statistical mechanics, I

arxiv: v1 [quant-ph] 1 Jul 2013

2 Canonical quantization

Molecular Simulation Background

ANALYTICAL MECHANICS. LOUIS N. HAND and JANET D. FINCH CAMBRIDGE UNIVERSITY PRESS

Under evolution for a small time δt the area A(t) = q p evolves into an area

In-class exercises Day 1

Dissipative nuclear dynamics

Transcription:

Javier Junquera Statistical mechanics

From the microscopic to the macroscopic level: the realm of statistical mechanics Computer simulations Thermodynamic state Generates information at the microscopic level Defined by a small set of macroscopic parameters Atomic positions Pressure Momenta Temperature Number of particles Can be thought of as coordinates of a multidimensional space of dimensions: the phase space Other thermodynamic properties may be derived through the knowledge of the equation of state and the fundamental equations of thermodynamics

Statistical sampling from ensembles A particular point in phase space A given property (for instance, the potential energy) Instantaneous value of the property when the system is at point It is reasonable to assume that the experimentally observable macroscopic property is really the time average of taken over a long time interval The equations governing this time evolution (Newton's equation of motion in a simple classical system) are well known

Statistical sampling from ensembles The equations governing this time evolution (Newton's equation of motion in a simple classical system) are well known But we can not hope to extend the integration of the dynamical equations: - For a truly macroscopic number 10 23 - To infinite time We might be satisfied to average over: - A system of the order of thousand of atoms (length and size scale) - Over a long but finite time (time scale) That is what we do in MD simulations: The equations of motion is solved step by step a large number of steps

Practical questions regarding the validity of the method Whether or not a sufficient region of phase space is explored by the system trajectory within a feasible amount of computer time Whether thermodynamic consistency can be attained between simulation with identical macroscopic parameters (density, energy, ) but different initial conditions Such simulation runs are within the power of modern computers

Ergodicity In MD we want to replace a full sampling on the appropriate statistical ensemble by a SINGLE very long trajectory. This is OK only if system is ergodic. Ergodic Hypothesis: a phase point for any isolated system passes in succession through every point compatible with the energy of the system before finally returning to its original position in phase space. This journey takes a Poincare cycle. In other words, Ergodic hypothesis: each state consistent with our knowledge is equally likely. Implies the average value does not depend on initial conditions. <A> time = <A> ensemble, so <A time > = (1/N MD ) = t=1,n A t is good estimator. Are systems in nature really ergodic? Not always! Non-ergodic examples are glasses, folding proteins (in practice) and harmonic crystals (in principle).

Ergodicity is the phase space density

Different aspects of ergodicity The system relaxes on a reasonable time scale towards a unique equilibrium state (microcanonical state) Trajectories wander irregularly through the energy surface eventually sampling all of accesible phase space. Trajectories initially close together separate rapidily (Sensitivity to initial conditions). Ergodic behavior makes possible the use of statistical methods on MD of small system. Small round-off errors and other mathematical approximations should not matter.

Particle in a smooth/rough circle From J.M. Haile: MD Simulations

Simple thermodynamic averages: mechanical energy The kinetic, potential, and total energies might be calculated using the phase functions already seen Average of kinetic energy Sum of contribution from individual particle momenta Average of potential energy Sum over all pairs, triplets, depending on the complexity of the potential energy function

Simple thermodynamic averages: virial theorem in the form of generalized equipartition

Simple thermodynamic averages: temperature Applying the previous formula to compute the average kinetic energy in the atomic case Familiar equipartition energy: an average energy of per degree of freedom

Simple thermodynamic averages: instantaneous temperature We can define an instantaneous kinetic energy function from the momenta of the atoms at a given time step (not averaged) whose average is equal to For a system of atoms subject to internal molecular constraints, the number of degrees of freedom will be, where is the total number of independent internal constraints In we should include the fixed bond lengths, angles, or additional global constraints (on the center of mass motion, for instance)

Simple thermodynamic averages: pressure Let us assume that we are using Cartesian coordinates, and we use the Hamilton s equation of motion

Simple thermodynamic averages: pressure Let us assume that we are using Cartesian coordinates, and we use the Hamilton s equation of motion represents the sum of internal molecular forces and external forces

Simple thermodynamic averages: pressure The external forces are related to the external pressure. Considering the effect of the container walls on the system If we define the internal virial, where we now restrict our attention to the intermolecular forces, then So, finally

Simple thermodynamic averages: instantaneous pressure As it happened with the temperature, we can define the instantaneous pressure function as whose average is simply This definition of the instantaneous pressure is not unique. For instance, for a constant temperature ensemble we can define Both definitions of the instantaneous pressure give the same when averaged, but their fluctuations in any ensemble would be different Although the systems simulated we use periodic boundary conditions (and therefore there are no walls), the results are the same

Simple thermodynamic averages: instantaneous pressure For pairwise interaction, we can express in a form that is explicitly independent of the origin of coordinates The indices and are equivalent Newton s third law is used to switch the force indices where

Simple thermodynamic averages: instantaneous pressure In a simulation that uses periodic boundary condition, it is essential to use where the intermolecular pair virial function Like is limited by the range of the interactions, and hence should be a well behaved, ensemble-independent function in most cases

Simple thermodynamic averages: number of molecules and volume Average number of particles Average number of particles Are easily evaluated in the simulation of ensembles in which these quantities vary, and derived functions such as the enthalpy are easily calculated from the above

Constant temperature molecular dynamics: the canonical ensemble A physical picture of a system corresponding to the canonical ensemble Involves weak interactions between molecules of the system and the particles of a heat bath at a specific temperature SYSTEM T Reservoir Simulate an extended system : - the real system - an external (virtual) system, acting as a heat reservoir The energy is allowed to flow dynamically from the reservoir to the system and back. The heat reservoir controls the temperature of the given system, i. e., the temperature fluctuates around a target value. The reservoir is simply included by an extra degree of freedom,, with momentum

Constant temperature molecular dynamics: variables of the Nose-Hoover thermostat SYSTEM T Reservoir The heat bath is considered as an integral part of the system by addition of - an extra degree of freedom, - an extra mometum, - a mass,, [dimensions: (energy) (times) 2 ]. This variable controls the rate of temperature fluctuations

Constant temperature molecular dynamics: variables of the Nose-Hoover thermostat: the artificial variable SYSTEM T Reservoir The extra degree of freedom (artificial parameter) s, plays the role of a time scaling parameter. The time scale in the extended system,, is scaled by the factor s Virtual time in the extended system Real time

Constant temperature molecular dynamics: variables of the Nose-Hoover thermostat: the artificial momentum SYSTEM T Reservoir The atomic coordinates are identical in both systems Atomic coordinates in the extended system Atomic coordinates in the real system Momentum in the extended system Momentum in the real system

Constant temperature molecular dynamics: variables of the Nose-Hoover thermostat: the extended Lagrangian The Lagrangian of the extended system is Kinetic energy minus the potential Kinetic energy of energy of the real system the thermostat Extra potential The extra potential is chosen to ensure that the algorithm produces a canonical ensemble Numbers of degree of freedom: 3N 3N-3 if the total momentum is fixed +1 because of the extra degree of freedom of the thermostat

Constant temperature molecular dynamics: the Lagrangian equations for the Nose-Hoover thermostat The Lagrangian equations of motions are

Constant temperature molecular dynamics: the Lagrangian equations for the Nose-Hoover thermostat The Lagrangian equations of motions are

Constant temperature molecular dynamics: the Lagrangian equations for the Nose-Hoover thermostat The Lagrangian equations of motions are The equations of motion are solved using the standard predictor-corrector method These equations sample a microcanonical ensemble in the extended system. The extended system Hamiltonian is conserved However, the energy of the real system is not constant. Accompanying the fluctuations of s, heat transfers occur between the system and a heat bath, which regulate the system temperature.

Constant temperature molecular dynamics: Choice of Q in the Nose-Hoover thermostat Too high Too low Slow energy flow between the system and the reservoir Long lived weakly damping oscillations of energy occur, resulting in poor equilibration regain conventional Molecular Dynamics