Study of Pentacene clustering MAE 715 Project Report By: Krishna Iyengar.

Slides:



Advertisements
Similar presentations
Time averages and ensemble averages
Advertisements

Simulazione di Biomolecole: metodi e applicazioni giorgio colombo
I.Dalton’s Law A.The total pressure of a mixture of gases equals the sum of the pressures each gas would exert independently 1.P total = P 1 + P 2 + …
Molecular Dynamics at Constant Temperature and Pressure Section 6.7 in M.M.
Transfer FAS UAS SAINT-PETERSBURG STATE UNIVERSITY COMPUTATIONAL PHYSICS Introduction Physical basis Molecular dynamics Temperature and thermostat Numerical.
Lecture 13: Conformational Sampling: MC and MD Dr. Ronald M. Levy Contributions from Mike Andrec and Daniel Weinstock Statistical Thermodynamics.
Ivan Janeček, Daniel Hrivňák, and René Kalus Department of Physics, University of Ostrava, Ostrava, Czech Republic Supported by the Grant Agency of the.
Incorporating Solvent Effects Into Molecular Dynamics: Potentials of Mean Force (PMF) and Stochastic Dynamics Eva ZurekSection 6.8 of M.M.
Statistical Models of Solvation Eva Zurek Chemistry Final Presentation.
Igls, March Statistical Models What do all the abbreviations mean? What assumptions are behind the various models? What can they tell us? Why do.
Case Studies Class 5. Computational Chemistry Structure of molecules and their reactivities Two major areas –molecular mechanics –electronic structure.
Foundations of College Chemistry, 14 th Ed. Morris Hein and Susan Arena Air in a hot air balloon expands upon heating. Some air escapes from the top, lowering.
Examining the crossover between the hadronic and partonic phases in QCD and the structure of sQGP Xu Mingmei( 许明梅 ), Yu Meiling( 喻梅凌 ), Liu Lianshou( 刘连寿.
Computer Simulations, Nucleation Rate Predictions and Scaling Barbara Hale Physics Department and Cloud and Aerosol Sciences Laboratory, University of.
Polymers PART.2 Soft Condensed Matter Physics Dept. Phys., Tunghai Univ. C. T. Shih.
Computer Simulations, Scaling and the Prediction of Nucleation Rates
Joo Chul Yoon with Prof. Scott T. Dunham Electrical Engineering University of Washington Molecular Dynamics Simulations.
A Monte Carlo discrete sum (MCDS) approach to energies of formation for small methanol clusters Srivatsan Raman*, Barbara Hale and Gerald Wilemski Physics.
Leipzig, 17 May Markov Models of Protein Folding - Application to Molecular Dynamics Simulations Christian Hedegaard Jensen.
Water cluster- silica collision Water cluster, 104 H 2 O Simulation time, 17ps NVE simulations O 1560 Si atoms Molecular mass g/mole.
Avogadro’s Law.
ChE 551 Lecture 19 Transition State Theory Revisited 1.
Chapter 24. Molecular Reaction Dynamics Purpose: Calculation of rate constants for simple elementary reactions. For reactions to take place: 1. Reactant.
Advanced methods of molecular dynamics Monte Carlo methods
12.6 Dalton’s Law of Partial Pressure
Introduction to (Statistical) Thermodynamics
Real gas 1.molecules not always in motion (condense phase can be formed) 2.molecular size is non-negligible (there is molecular repulsion) 3.Molecules.
ChE 452 Lecture 24 Reactions As Collisions 1. According To Collision Theory 2 (Equation 7.10)
Free energies and phase transitions. Condition for phase coexistence in a one-component system:
1 MAE 5310: COMBUSTION FUNDAMENTALS Introduction to Chemical Kinetics September 24, 2012 Mechanical and Aerospace Engineering Department Florida Institute.
Ideal Gas Law PV=nRT Kinetic Molecular Theory 1. Gases have low density 2. Gases have elastic collisions 3. Gases have continuous random motion. 4. Gases.
Prentice Hall © 2003Chapter 10. Prentice Hall © 2003Chapter 10 Look here tomorrow after Period 5 for a link for your class work from the Gas Laws Packet.
Std 4 - Questions Grade: «grade» Subject: Standard 4 - practice q's Date: «date»
The Nature of Gases Kinetic Theory and a Model for Gases.
Section 10.5 The Kinetic Molecular Theory. The Kinetic Molecular Theory In this section… a.Gases and Gas Laws on the Molecular Scale b.Molecular speed,
Rebecca Cantrell MAE Professor Zabaras Atomistic Modeling of Materials Final Project Presentation May 7, 2007.
1 M.Sc. Project of Hanif Bayat Movahed The Phase Transitions of Semiflexible Hard Sphere Chain Liquids Supervisor: Prof. Don Sullivan.
Kinetic Monte Carlo Simulation of Dopant Diffusion in Crystalline CEC, Inha University Chi-Ok Hwang.
ChE 553 Lecture 15 Catalytic Kinetics Continued 1.
Dissipative Particle Dynamics. Molecular Dynamics, why slow? MD solves Newton’s equations of motion for atoms/molecules: Why MD is slow?
Kinetic Molecular Theory. What do we assume about the behavior of an ideal gas?   Gas molecules are in constant, random motion and when they collide.
7. Lecture SS 2005Optimization, Energy Landscapes, Protein Folding1 V7: Diffusional association of proteins and Brownian dynamics simulations Brownian.
Exploring the connection between sampling problems in Bayesian inference and statistical mechanics Andrew Pohorille NASA-Ames Research Center.
© 2014 Carl Lund, all rights reserved A First Course on Kinetics and Reaction Engineering Class 4.
Molecular Modelling - Lecture 2 Techniques for Conformational Sampling Uses CHARMM force field Written in C++
Incremental Integration of Computational Physics into Traditional Undergraduate Courses Kelly R. Roos, Department of Physics, Bradley University Peoria,
ChE 452 Lecture 25 Non-linear Collisions 1. Background: Collision Theory Key equation Method Use molecular dynamics to simulate the collisions Integrate.
حرارة وديناميكا حرارية
Case two for second-order would occur for a reaction involving two reactants: A + B P 241.
Interacting Molecules in a Dense Fluid
An Introduction to Monte Carlo Methods in Statistical Physics Kristen A. Fichthorn The Pennsylvania State University University Park, PA
Monte Carlo in different ensembles Chapter 5
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.
Role of Theory Model and understand catalytic processes at the electronic/atomistic level. This involves proposing atomic structures, suggesting reaction.
Review Session BS123A/MB223 UC-Irvine Ray Luo, MBB, BS.
Generalized van der Waals Partition Function
The Nature of Gases: Part 1 Kinetic Theory and a Model for Gases.
Gas pressure and the ideal gas law Assume specular collisions* *Bold assumption – but more general calculation gives same result. Change in momentum:
HEAT AND THERMAL ENERGY Kinetic Theory of Gases Thermal Expansion Gas Laws.
© 2014 Carl Lund, all rights reserved A First Course on Kinetics and Reaction Engineering Class 4.
Physical Behavior of Matter Review. Matter is classified as a substance or a mixture of substances.
Aim: Explain Kinetic Molecular Theory Notes 12-1.
General Physics 1 Hongqun Zhang The Department of Physics, Beijing Normal University June 2005.
Technological/Societal Impact (1)SEM images of Silicon films deposited in pulsed laser ablation in vacuum Courtesy of A. Perrone Fluence of 3.0 J/cm^2.
CHAPTER 10 – Gases Lecture 1 – KMT, Graham’s & Dalton’s Law
Physical Behavior of Matter Review
Overview of Molecular Dynamics Simulation Theory
Content Heavy ion reactions started fragmenting nuclei in the 1980’s. Its study taught us that nuclear matter has liquid and gaseous phases, phase.
Molecular Modelling - Lecture 3
Gas pressure and the ideal gas law
Presentation transcript:

Study of Pentacene clustering MAE 715 Project Report By: Krishna Iyengar

Motivation  Pentacene - new age applications  Solar Panels  Thin Film Transistors (TFTs)  Organic Light Emitting Diodes (OLEDs)  Experimental study of pentacene deposition to form thin films  Formation of clusters observed

Problem outline  Study the tendency to form clusters  Energetics of clusters  Dynamics of cluster formation  Stochastic simulation

Part I: Tendency to form molecular clusters  MD simulations - as proof of concept  Simulation parameters  MM3 Potential (Tinker)  Partial Pressure of pentacene gas (V = nRT/P)  Volume Å 3  Temperatures K, 573 K, 623 K, 673 K (experimental ~ 320 C)  NVE ensemble (after NVT Thermalization)  Time - 500,000 1 fs time step)

Pentacene Dimers Post processing: Collision causes dimerization Detect collisions / formation of dimers (Cut off distance between CG - 5 Å ) Life time of the formed dimer (Cut off time = 1 pico second )

Normalized Histogram Data  Normalization of the histograms:  523 K K - 70  623 K K - 47  At lower T, larger proportion of stable dimers  At higher T, large # of short life span dimers  Correlation with theory?

Trimers and transition states  Dimer transition state  Stable Trimer  Life time ~200ps  : 380 ps  4-42 : 210 ps  4-30 : 190 ps

Issues with the MD simulations  System size dependence ?  Effect of Pressure / Volume of simulation cell ?  What characterizes a stable clusters?  Formation of N-mers ? (problems with small time scale of simulations)  Does this simulation model the experimental set up?

Part II: Energetics  Why? - Will give an idea of stable structures, energy barriers (if any)  How? :  Ab-initio calculation ( using Gaussian )  Expensive (limited to ~ 200 atoms ~ 4 mol)  Energy minimization using empirical potentials ( MM3 + Tinker)  Range: Dimer - Octamer ---> Bulk

Dimer energetics  2-D configurational space Interaction energy = (Energy of cluster) - (n*Energy of single molecule) E 1 = Kcal/mole 25 ° 3.5 Å

N-mer structures  Take 200 random initial configurations  Energy minimization to obtain structure  At higher cluster size - compare with crystalline pentance : Herring bone structure

Trimer Kcal/mole Interaction Energy : Kcal/mole

Tetramer to Octomer TetramerPentamerHexamer Heptamer Octamer

Trends in cluster formation Bulk Phase Energy of formation ~ -35 Kcal/mole

Part III: Dynamics  Why energetics is required  Rate constant = Prefactor * Energy barrier  -> solve differential equation  -> use KMC to stochastically evolve the system  Assumptions:  Molecules are approximated as spheres  Assume hard sphere collisions  Assume effective radius based on energetics  Ideal gas behavior

Collision Theory Hard Sphere + Energy Barrier Assumption

 Change in opacity factor  Integral from 0 to E* (interaction energy)  Rate Constant based on collision theory Modifications for clustering

Species and Reactions  Each type of cluster is a species  Monomer -> P 1 ; Dimer -> P 2 ; Trimer -> P 3  Cluster formation / dissociation each is modeled as an independent reaction  P 1 + P 1 ---> P 2 ; P 2 ---> P 1 + P 1  P 2 + P 1 ---> P 3 ;P 3 ---> P 2 + P 1 or 3*P 1  Rate Constant for each reaction is found using modified collision theory equations

Further details  Assume effective diameter of pentacene clusters  Monomer Å( 278 amu )  Dimer Å( 556 amu )  Trimer Å ( 834 amu )  Based on geometry of minimized structures  Calculate  Use E * from energetics to find rate contant

Exact Stochastic Simulation  Gillespie algorithm - generates a statistically correct trajectory of a stochastic equation  Useful for simulating chemical or biochemical reaction systems  It is a variety of a dynamic Monte Carlo method and similar to the kinetic Monte Carlo methods

Summary of the steps to run the Gillespie algorithm  Initialization: Initialize the number of molecules in the system, reactions constants, and random number generators.  Monte Carlo Step: Generate random numbers to determine the next reaction to occur as well as the time step.  Update: Increase the time step by the randomly generated time. Update the molecule count based on the reaction that occurred.  Iterate

Test Case  Reactions  P 1 + P 1 --> P 2  P 1 + P 2 --> P 3  Propensity (Rate Constant / Volume )  0.05 (initial # = 300,00 )  (initial # = 30 )

No of P 2 clusters with time

Thank You