⚗️Computational Chemistry Unit 12 – Statistical Mechanics in Comp Chemistry
Statistical mechanics bridges the gap between microscopic properties and macroscopic observables in chemical systems. It uses probability distributions and ensemble theory to connect particle-level interactions with measurable quantities like temperature and pressure.
Key concepts include the Boltzmann distribution, partition functions, and various statistical ensembles. These tools enable the calculation of thermodynamic properties and form the basis for computational methods like Monte Carlo and molecular dynamics simulations used in modern chemistry research.
Statistical mechanics provides a framework for understanding macroscopic properties of systems based on their microscopic constituents and interactions
Connects microscopic properties (positions, momenta) to macroscopic observables (temperature, pressure, energy) using probability distributions
Ensemble theory describes a collection of microstates that share common macroscopic properties
Microstate represents a specific configuration of a system (positions and momenta of all particles)
Macrostate corresponds to observable properties (temperature, volume, pressure)
Ergodic hypothesis assumes that given sufficient time, a system will explore all accessible microstates
Boltzmann distribution describes the probability of a system being in a particular microstate based on its energy and temperature
P(Ei)=∑je−Ej/kBTe−Ei/kBT, where Ei is the energy of microstate i, kB is the Boltzmann constant, and T is the temperature
Partition function Z is a sum over all possible microstates, weighted by their Boltzmann factors e−Ei/kBT
Normalizes the probability distribution and connects microscopic properties to macroscopic observables
Statistical Ensembles
Ensembles are collections of microstates that share common macroscopic properties
Microcanonical ensemble (NVE) describes an isolated system with fixed number of particles (N), volume (V), and energy (E)
All accessible microstates have equal probability
Canonical ensemble (NVT) represents a system in contact with a heat bath at constant temperature (T)
Probability of a microstate depends on its energy and temperature through the Boltzmann distribution
Grand canonical ensemble (μVT) allows for exchange of particles with a reservoir at constant chemical potential (μ), volume (V), and temperature (T)
Isothermal-isobaric ensemble (NPT) maintains constant number of particles (N), pressure (P), and temperature (T)
Commonly used in simulations of biological systems and condensed matter
Ensemble averages calculate macroscopic properties as averages over microstates weighted by their probabilities
⟨A⟩=∑iAiP(Ei), where Ai is the value of property A in microstate i
Partition Functions
Partition function Z is a fundamental quantity in statistical mechanics that encodes the statistical properties of a system
Connects microscopic properties to macroscopic observables through ensemble averages
Canonical partition function: Z=∑ie−Ei/kBT, where Ei is the energy of microstate i
Normalizes the Boltzmann distribution and allows calculation of thermodynamic properties
Factorization of partition function into translational, rotational, vibrational, and electronic contributions
Z=ZtransZrotZvibZelec
Simplifies calculations by treating each degree of freedom separately
Translational partition function depends on the mass and temperature of the particles
Rotational partition function depends on the moments of inertia and symmetry of the molecules
Vibrational partition function depends on the frequencies of normal modes
Electronic partition function depends on the electronic energy levels and degeneracies
Thermodynamic Properties
Thermodynamic properties can be derived from the partition function using statistical mechanics
Internal energy: U=−∂β∂lnZ, where β=1/kBT
Average energy of the system over all microstates
Entropy: S=kBlnZ+kBT∂T∂lnZ
Measure of the number of accessible microstates and the disorder of the system
Helmholtz free energy: F=−kBTlnZ
Maximum work that can be extracted from a system at constant temperature and volume
Pressure: P=kBT∂V∂lnZ
Force per unit area exerted by the system on its surroundings
Heat capacity: CV=∂T∂U
Amount of heat required to raise the temperature of the system by one unit at constant volume
Chemical potential: μ=−kBT∂N∂lnZ
Change in free energy when a particle is added to the system
Monte Carlo Methods
Monte Carlo (MC) methods are computational algorithms that use random sampling to estimate properties of systems
Metropolis algorithm is a common MC method for sampling the Boltzmann distribution
Proposes random moves in the configuration space and accepts or rejects them based on the change in energy
Acceptance probability: Pacc=min(1,e−ΔE/kBT), where ΔE is the change in energy
Markov chain Monte Carlo (MCMC) generates a sequence of configurations that converge to the equilibrium distribution
Each new configuration depends only on the previous one (Markov property)
Importance sampling focuses on regions of the configuration space that contribute significantly to the properties of interest
Improves efficiency by avoiding sampling of low-probability regions
Umbrella sampling enhances sampling of rare events by introducing a biasing potential
Helps overcome energy barriers and explore multiple regions of the configuration space
Parallel tempering (replica exchange) simulates multiple replicas of the system at different temperatures
Allows exchange of configurations between replicas to improve sampling efficiency
Molecular Dynamics Simulations
Molecular dynamics (MD) simulations calculate the time evolution of a system by solving Newton's equations of motion
Numerically integrates the equations of motion using finite time steps