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Physical Chemistry II: Quantum Chemistry Lecture 20: Introduction to Computational Quantum Chemistry Yuan-Chung Cheng yuanchung@ntu.edu.tw 5/14/2019 Tutorial Information n https://ceiba.ntu.edu.tw/1063NCHUCompChem01 n Books: Computational


  1. Physical Chemistry II: Quantum Chemistry Lecture 20: Introduction to Computational Quantum Chemistry Yuan-Chung Cheng yuanchung@ntu.edu.tw 5/14/2019

  2. Tutorial Information n https://ceiba.ntu.edu.tw/1063NCHUCompChem01 n Books:

  3. Computational Chemistry Overview

  4. Quantum Chemistry The general theory of quantum mechanics is now complete... The underlying physical laws necessary for the mathematical theory of a large part of physics and the whole of chemistry are thus completely known – Paul Dirac, 1929. Right: QM is the foundation of Chemistry Wrong: Not so fast - complexities necessitate approximations Nowadays we have powerful Paul Dirac computers!!

  5. The Nobel Prize in Chemistry 1998 John A. Pople "for his development of computational methods in quantum chemistry" Walter Kohn "for his development of the density- functional theory”

  6. The Nobel Prize in Chemistry 2013 2013 Nobel Chemistry Prize jointly to Martin Karplus, Michael Levitt and Arieh Warshel "for the development of multiscale models for complex chemical systems" . Martin Karplus Michael Levitt Arieh Warshel

  7. Computational Chemistry Methods n Molecular mechanics n Semiempirical molecular orbital methods n Ab initio molecular orbital methods n Density functional method n Quantum Monte Carlo method n … Yields Energy, Structure, and Properties

  8. Molecular Mechanics n Simplest type of calculation ¨ Used when systems are very large and approaches that are more accurate become to costly (in time and memory) n Does not use any quantum mechanics instead uses parameters derived from experimental or ab initio data ¨ Uses information like bond stretching, bond bending, torsions, electrostatic interactions, van der Waals forces and hydrogen bonding to predict the energetics of a system ¨ The energy associated with a certain type of bond is applied throughout the molecule. This leads to a great simplification of the equation n It should be clarified that the energies obtained from molecular mechanics do not have any physical meaning, but instead describe the difference between varying conformations (type of isomer). Molecular mechanics can supply results in heat of formation if the zero of energy is taken into account. Courtesy of Shalayna Lair, University of Texas at El Paso

  9. Semiempirical n Semiempirical methods use experimental data to parameterize equations n Like the ab initio methods, a Hamiltonian and wave function are used ¨ much of the equation is approximated or eliminated n Less accurate than ab initio methods but also much faster n The equations are parameterized to reproduce specific results, usually the geometry and heat of formation, but these methods can be used to find other data. Courtesy of Shalayna Lair, University of Texas at El Paso

  10. Ab Initio Methods n “Ab initio” – Latin, means “from the beginning” or “from first principles.” n No experimental input is used and calculations are based on fundamental laws of physics. n Various levels of ab initio calculations (jargons): ¨ Hartree-Fock Self-Consistent Field (HF-SCF) n simplest ab initio MO calculation n electron correlation is not taken into consideration. ¨ Configuration Interaction (CI) ¨ Coupled-Cluster (CC) ¨ The Møller-Plesset Perturbation Theory (MP) ¨ Density Functional Theory (DFT) Include electron correlation Courtesy of Shalayna Lair, University of Texas at El Paso

  11. Quantum Chemistry Courtesy of Donald G Truhlar

  12. Hartree-Fock SCF Review Slides from Hai Lin

  13. Schrödinger Equation H Ψ = E Ψ H = T n + T e + V nn + V ee + V ne e 1 N 1 = å n e 2 - M Ñ 2 T Kinetic energy of nuclei n a 2 n 1 n 2 a a N 1 e å = - Ñ 2 T Kinetic energy of electrons e i 2 m i e N N Z Z n n åå = V a b Coulombic energy between nuclei nn r > a b a ab e 1 N N e åå = V Coulombic energy between electrons ee r > i i j ij N N Z åå n e = Coulombic energy between nuclei and electrons V a ne r a i ai The “electronic structure problem” Courtesy of Hai Lin

  14. Approximations To solve the Schrödinger equation approximately, assumptions are made to simplify the equation: • Born-Oppenheimer approximation allows separate treatment of nuclei and electrons. ( m a >> m e ) • Hartree-Fock independent electron approximation allows each electron to be considered as being affected by the sum (field) of all other electrons. • LCAO Approximation represents molecular orbitals as linear combinations of atomic orbitals (basis functions). Courtesy of Hai Lin

  15. Born-Oppenheimer Approximation •Nuclei are much heavier than electrons ( m a / m e > 1836) and move much slower. •Effectively, electrons adjust themselves instantaneously to nuclear configurations. •Electron and nuclear motions are uncoupled, thus the energies of the two are separable. Energy 1. For a given nuclear configuration, one calculates Internuclear electronic energy. Distance 2. As nuclei move continuously, the points of electronic energy joint to form a potential energy surface on which nuclei move. Elec. Schrodinger equation: H ( R ) Ψ ( R ) = E ( R ) Ψ ( R )

  16. Basic Quantum Mechanics H Ψ = E Ψ Schrodinger equation: Variational principle: E = Ψ ˆ H Ψ ≥ E exact Ψ = Ψ ( x 1 , x 2 ..., x N ) The N-electron wave function is a function with 3N dimensions, this is too complicated to even “think about” practically for systems with > 3 electrons à must simplify the functional form of the wave function.

  17. Many-electron Wave function Hartree product: All electrons are independent, each in its own orbital. ψ HP ( x 1 , x 2 ,..., x N ) = f 1 ( x 1 ) f 2 ( x 2 )  f N ( x N ) Pauli principle: Two electrons can not have all quantum number equal. e 1 e 2 This requires that the total (many-electron) wave function e i is anti-symmetric whenever one exchanges two electrons’ … coordinates. ψ ( x 1 , x 2 ,..., x N ) = − ψ ( x 2 , x 1 ,..., x N ) e N Slater determinant satisfies the Pauli exclusion principle.  f 1 ( x 1 ) f 2 ( x 1 ) f N ( x 1 )  1 f 1 ( x 2 ) f 2 ( x 2 ) f N ( x 2 ) ψ ( x 1 , x 2 , … x N ) =     N !  f 1 ( x N ) f 2 ( x N ) f N ( x N ) Courtesy of Hai Lin

  18. Many-electron Wave function (2) Example: A two-electron system. Hartree product: Both electrons are independent. ψ HP ( x 1 , x 2 ) = f 1 ( x 1 ) f 2 ( x 2 ) Slater determinant satisfies the Pauli principle. e 1 f 1 ( x 1 ) f 2 ( x 1 ) ψ ( x 1 , x 2 ) = 1 e 2 f 1 ( x 2 ) f 2 ( x 2 ) 2 [ ] ψ ( x 1 , x 2 ) = (1/ 2) 1/2 f 1 ( x 1 ) f 2 ( x 2 ) − f 2 ( x 1 ) f 1 ( x 2 ) [ ] = − ψ ( x 1 , x 2 ) ψ ( x 2 , x 1 ) = (1/ 2) 1/2 f 1 ( x 2 ) f 2 ( x 1 ) − f 2 ( x 2 ) f 1 ( x 1 ) The total (many-electron) wavefuntion is anti-symmetric when one exchanges two electrons’ coordinates x 1 and x 2 . Courtesy of Hai Lin

  19. Hartree-Fock Approximation •Assume the wave function is a single Slater determinant. • Each electron “feels” all other electrons as a whole (field of charge), .i.e., an electron moves in a mean-field generated by all other electrons. à variational ground state composed of “optimal” single electron wavefunctions (orbitals) • A Fock operator F is introduced for a given electron in the i -th orbital: F i f i = e i f i e 1 potential energy kinetic energy + F i = e 2 term due to fixed term of the e i nuclei given electron … averaged potential e N + energy term due to the other electrons f i is the i -th molecular orbital, and e i is the corresponding orbital energy. Note: The total energy is NOT the sum of orbital energies. If you sum them up, you count the electron-electron interactions twice. Courtesy of Hai Lin

  20. The Fock Operator N å = + - F h ( J K ) i i j j j Exchange Coulomb Core-Hamiltonian operator operator operator Exchange energy due Coulombic energy Kinetic energy to another electron term for the given term and nuclear (A pure quantum electron due to attraction for the mechanical term due to another electron given electron the Pauli principle, no classical interpretation) Courtesy of Hai Lin

  21. Self-consistency •Each electron “feels” all the other electrons as a whole (field of charge), .i.e., an electron moves in a mean-field generated by all the other electrons. •The Fock equation for an electron in e k e j the i -th orbital contains information of all the other electrons (in an averaged e i fashion), i.e., the Fock equations for all electrons are coupled with each other. •All equations must be solved together (iteratively until self-consistency is obtained). — Self-consistent field (SCF) method. Courtesy of Hai Lin

  22. Molecular Orbital & Slater Determinant Single-electron wavefunction (orbital!!): χ i (x 1 ) : spin orbital x 1 : electron variable virtual N-electron wavefunction: Slater determinants orbitals χ i (x 1 ) χ j (x 1 ) χ k (x 1 )  χ i (x 2 ) χ j (x 2 ) χ k (x N )  Ψ (x 1 ,...,x N ) = ( N !) 1/ 2    occupied orbitals χ i (x N ) χ j (x N ) χ k (x N )  Given a basis, Hartree-Fock theory provides a variational groundstate & molecular orbitals within the single determinant approximation è mean-field, no electron correlations

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