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Molecular Simulation I Quantum Chemistry Classical Mechanics E = Ψ H Ψ ΨΨ U = E bond +E angle +E torsion +E non-bond Jeffry D. Madura Department of Chemistry & Biochemistry Center for Computational Sciences Duquesne University

Quantum Chemistry Molecular Orbital Theory Based on a wave function approach Schrödinger equation Density Functional Theory Based on the total electron density Hohenberg Kohn theorem Semi-empirical Some to most integrals parameterized MNDO, AM1, EHT Empirical All integrals are parameterized Huckel method

The Beginning... Schrödinger equation H Ψ = Hamiltonian operator EΨ 2 2 2 2 2 h h H = + + V r V r 2 2 2 + = + 2m x y z 2m Wave function ( ) Ψ characterizes the particles motion ( ) 2 ( ) various properties of the particle can be derived

Quantum Chemistry Start with Schrödinger s equation HΨ = EΨ Make some assumptions Born-Oppenheimer approximation Linear combination of atomic orbitals Ψ = c ϕ + cϕ a a b b Apply the variational method E Ψ * HΨdτ * ΨΨ dτ

LCAO A practical and common approach to solving the Hartree-Fock equations is to write each spin orbital as a linear combination of single electron orbitals (LCAO) K ψ i = ν = 1 c ν i the φ v are commonly called basis functions and often correspond to atomic orbitals K basis functions lead to K molecular orbitals the point at which the energy is not reduced by the addition of basis functions is known as the Hartree- Fock limit φ ν

Basis Sets Slater type orbitals (STO) Gaussian type orbitals (GTO) functional form n+ 1/2 1/2 n 1 r R ( ) ( 2 ) ( 2 ) nl r = ζ n! r e ζ x y z e a a b c - r zeroth-order Gaussian function 2 3/4 2α r gs ( α, r) = e α π 2

Property of Gaussian functions is that the product of two Gaussians can be expressed as a single Gaussian, located along the line joining the centers of the two Gaussians a a -a - a = a + a -a m n 2 2 2 - rmn 2 mrm nrn m n rc e e e e 1 0.8 fx ( ) 0.6 g( x) fx ( ). g( x) 0.4 0.2 0 0 6 4 2 0 2 4 6 6 x 6

STO vs. GTO

Gaussian expansion the coefficient the exponent uncontratcted or primitive and contracted s and p exponents in the same shell are equal Minimal basis set STO-NG Double zeta basis set linear combination of a contracted function and a diffuse function. Split valence 3-21G, 4-31G, 6-31G φ L = d ( ) φ α µ iµ i iµ i= 1

Polarization to solve the problem of non-isotropic charge distribution. 6-31G*, 6-31G** Diffuse functions fulfill as deficiency of the basis sets to describe significant amounts of electron density away from the nuclear centers. (e.g. anions, lone pairs, etc.) 3-21+G, 6-31++G

Roothaan-Hall equations The recasting of the integro-differential equations into matrix form. The Hartree-Fock equation is written as This is transformed to give a Fock matrix (for closedshell systems) where K () 1 φ () 1 = ε φ () 1 F c c i νi ν i νi ν ν= 1 ν= 1 K K K core Fµν = Hµν + Pλσ λ= 1 σ= 1 P N /2 λσ = 2 cλicσi i= 1 1 2 ( µν λσ ) ( µλ νσ)

The energy is K K 1 core E = P H + F 2 µ = 1 ν= 1 the electron density is expressed as K K ( ) µν ν µν ( r) P ( r) ( r) ρ φ φ = µ = 1 ν= 1 µν µ ν In matrix form the Roothaan-Hall equation is written as FC = SCE

Solving the Roothaan-Hall Equation Common scheme for solving the Roothaan-Hall equations is calculate the integrals to form the Fock matrix, F calculate the overlap matrix, S diagonalize S form S -1/2 guess or calculate an initial density matrix, P Form the Fock matrix using the integrals and density matrix solve the secular equation F -EI =0 to give the eigenvalues E and the eigenvectors C by diagonalizing F calculate the molecular orbital coefficients, C, from C=S -1/2 C calculate a new density matrix, P, from matrix C check for convergence

RHF vs. UHF Restricted Hartree-Fock (RHF) closed-shell molecules Restricted Open-shell Hartree-Fock (ROHF) combination of singly and doubly occupied molecular orbitals. Unrestricted Hartree-Fock (UHF) open-shell molecules Pople and Nesbet: one set of molecular orbitals for α spin and another for the β spin.

UHF and RHF Dissociation Curves for H 2 0.2 0.1 E(H 2 )-2E(H) a.u. 0.0-0.1-0.2 0.2 1.2 2.2 3.2 4.2 R (a.u.)

Electron Correlation The most significant drawback to HF theory is that it fails to adequately represent electron correlation. NR E = E E corr Configuration Interactions HF excited states are included in the description of an electronic state Many Body Perturbation Theory based upon Rayleigh-Schrödinger perturbation theory

Configuration Interaction The CI wavefunction is written as Ψ= c0ψ 0 + c1ψ 1+ c2ψ 2 +L where Ψ 0 is the HF single determinant where Ψ 1 is the configuration derived by replacing one of the occupied spin orbitals by a virtual spin orbital where Ψ 2 is the configuration derived by replacing one of the occupied spin orbitals by a virtual spin orbital The system energy is minimized in order to determine the coefficients, c 0, c 1, etc., using a linear variational approach

Many Body Peturbation Theory Based upon perturbation concepts The correction to the energies are ( 0) ( 0) ( 0) E = Ψ H Ψ dτ i i 0 i ( 1) ( 0) ( 0) E = Ψ VΨ dτ i i i ( 2) ( 0) ( 1) E = Ψ VΨ dτ i i i ( 3) ( 0) ( 2) E = Ψ VΨ dτ i i i Perturbation methods are size independent these methods are not variational H = H0 + V

Geometry Optimization Derivatives of the energy ( ) ( ) ( ) ( ) ( ) 2 E x 1 E x ( )( ) L E xf = E x + xif xi + xif xi xj xj + x 2 x x i i i j i j the first term is set to zero the second term can be shown to be equivalent to a force the third term can be shown to be equivalent to a force constant

Internal coordinate, Cartesian coordinate, and redundant coordinate optimization choice of coordinate set can determine whether a structure reaches a minimum/maximum and the speed of this convergence. Internal coordinates are defined as bond lengths, bond angles, and torsions. There are 3N-6 (3N-5) such degrees of freedom for each molecule. Chemists work in this world. Z-matrix... Cartesian coordinates are the standard x, y, z coordinates. Programs often work in this world. Redundant coordinates are defined as the number of coordinates larger than 3N-6.

Frequency Calculation The second derivatives of the energy with respect to the displacement of coordinate yields the force constants. These force constants in turn can be used to calculate frequencies. All real frequencies (positive force constants): local minimum One imaginary frequency (one negative force constant): saddle point, a.k.a. transition state. From vibrational analysis can compute thermodynamic data

Charges Molecular Properties Mulliken Löwdin electrostatic fitted (ESP) Bond orders Bonding Natural Bond Analysis Bader s AIM method Molecular orbitals and total electron density Dipole Moment Energies ionization and electron affinity

Energies Koopman s theorem equating the energy of an electron in an orbital to the energy required to remove the electron to the corresponding ion. frozen orbitals lack of electron correlation effects

Dipole Moments The electric multipole moments of a molecule reflect the distribution of charge. Simplest is the dipole moment nuclear component electronic µ M = Z R nuclear A A A= 1 K K µ = 1 ν= 1 µ = qr ( ) µ electronic = P dτφ r φ µν µ ν i i i

Molecular Orbitals and Total Electron Density Electron density at a point r 2 ( r) = 2 ( r) = P ( r) ( r) + 2 P ( r) ( r) Number of electrons is Molecular orbitals HOMO LUMO N /2 K K K ρ ψ φ φ φ φ i µµ µ µ µν µ ν i= 1 µ = 1 µ = 1ν = µ + 1 N /2 2 K K K ( ) N = 2 drψ r = P + 2 P S i µµ µν µν i= 1 µ = 1 µ = 1ν = µ + 1

Natural Bond Analysis Bonding a way to describe N-electron wave functions in terms of localized orbitals that are closely tied to chemical concepts. Bader F. W. Bader s theory of atoms in molecules. This method provides an alternative way to partition the electrons among the atoms in a molecule. Gradient vector path bond critical points charges are relatively invariant to the basis set

Bond Orders Wiberg Mayer WAB P µν µ on Aνon B = B PS PS AB = µ on Aνon B Bond orders can be computed for intermediate structures which can be useful way to describe similarity of the TS to the reactants or to the products. 2 ( ) ( ) µν νµ

Mulliken A Löwdin A Charges K K K q = Z P P S µµ µν µν µ = 1; on A µ = 1; on Aν= 1; ν µ atomic orbitals are transformed to an orthogonal set, along with the mo coefficients φ K ' ( 1/2 S ) µ = φ νµ ν ν = 1 A A K ( 1/2 1/2 ) q = Z S P µ = 1; µ on A µµ

Electrostatic potentials the electrostatic potential at a point r, φ(r), is defined as the work done to bring a unit positive charge from infinity to the point. the electrostatic interaction energy between a point charge q located at r and the molecule equals qφ(r). there is a nuclear part and electronic part φ nucl r ( ) = M A= 1 r Z A R A φ r = elec ( ) dr r ' ρ ' r ( ) r φ r = φ r + φ r ( ) ( ) ( ) nucl elec

Water Example Geometry ------------------------------------------------------------------------ Z-MATRIX (ANGSTROMS AND DEGREES) CD Cent Atom N1 Length/X N2 Alpha/Y N3 Beta/Z J ------------------------------------------------------------------------ 1 1 H 2 2 O 1 0.989400( 1) 3 3 H 2 0.989400( 2) 1 100.028( 3) ------------------------------------------------------------------------ Population Analysis Energy E(RHF) = -74.9658952265 A.U. ********************************************************************** Population analysis using the SCF density. ********************************************************************** Alpha occ. eigenvalues -- -20.25226-1.25780-0.59411-0.45987-0.39297 Alpha virt. eigenvalues -- 0.58175 0.69242 Condensed to atoms (all electrons): 1 2 3 1 H 0.626190 0.253760-0.045250 2 O 0.253760 7.823081 0.253760 3 H -0.045250 0.253760 0.626190 Total atomic charges: 1 1 H 0.165300 2 O -0.330601 3 H 0.165300

Limitations, Strengths & Reliability Limitations Requires more CPU time Can treat smaller molecules Calculations are more complex Have to worry about electronic configuration Strengths No experimental bias Can improve a calculation in a logical manner (e.g. basis set, level of theory, ) Provides information on intermediate species, including spectroscopic data Can calculate novel structures Can calculate any electronic state Reliability The mean deviation between experiment and theory for heavy-atom bond lengths in twoheavy-atom hydrides drops from 0.082 A for the RHF/STO-3G level of theory to just 0.019 A for MP2/6-31G(d). Heats of hydrogenation of a range of saturated and unsaturated systems are calculated sufficiently well at the Hartree-Fock level of theory with a moderate basis set (increasing the basis set from 6-31G(d) to 6-31G(d,p) has little effect on the accuracy of these numbers). Inclusion of electron correlation is mandatory in order to get good agreement between experiment and theory for bond dissociation energies (MP2/6-31G(d,p) does very well for the one-heavy-atom hydrides). http://www.chem.swin.edu.au/modules/mod5/limits.html