Hauptseminar Moderne Simulationsmethoden WS 2009/Fortgeschrittene Molekulardynamik I

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<setdata> date=t.b.a. topic=Fortgeschrittene Molekulardynamik I: Wie man die freie Energie berechnet speaker= tutor=Shervin Rafatnia </setdata>

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Chapter 7

  • D. A. Kofke and P. T. Cummings.
"Quantitative comparison and optimization of methods for evaluating the chemical potential by molecular simulation."
Mol. Phys., 92:973-996, 1997.

Kurz zum Inhalt

The aim of this seminar would be to give a short introduction to free energy and to discuss some methods of calculating this energy in a MC or MD simulation.

In thermodynamics, the term free energy refers to the amount of work that can be extracted from a system. It is a subtraction of the entropy of a system multiplied by a reference temperature (giving the "unusable energy") from the total energy, yielding a thermodynamic state function which represents the "useful energy".

Free energy governs thermodynamic processes; all systems minimize their free energy to reach equilibrium. Therefore, calculating the free energy of a system is of great importance. But doing so in a simulation is not always easy. There are different methods to calculate the free energy of a system in MD or MC simulations. One can mention the thermodynamic integration method, the particle insertion method, overlapping distribution method, umbrella sampling and a few others.


1. Einleitung
2. Thermodynamische Integration
3. Widom's Teilcheneinsetzungsmethode
4. Histogramm-Methoden