Transcript Basis sets
Hartree-Fock Theory 1 The orbitalar approach Slater Mulliken Y(1,….N) = Pi fi(i) Pauli principle spin Combination of Slater determinants Solutions for S2 2 MO approach A MO is a wavefunction associated with a single electron. The use of the term "orbital" was first used by Mulliken in 1925. We are looking for wavefunctions for a system that contains several particules. We assume that H can be written as a sum of one-particle Hi operator acting on one particle each. H = Si Hi Y(1,….N) = Pi fi(i) E = Si Ei Robert Sanderson Mulliken 1996-1986 Nobel 1966 3 Approximation of independent particles Hartree Fock 1927 Fi = Ti + Sk Zik/dik+ Sj Rij Each one electron operator is the sum of one electron terms + bielectronic repulsions Rij is the average repulsion of the electron j upon i. The self consistency consists in iterating up to convergence to find agreement between the postulated repulsion and that calculated from the electron density. 4 This ignores the real position of j vs. i at any given time. Self-consistency Given a set of orbitals Yi, we calculate the electronic distribution of j and its repulsion with i. This allows expressing Fi = Ti + Sk Zik/dik+ Sj Rij and solving the equation to find new Y1i allowing to recalculate Rij. The process is iterated up to convergence. Since we get closer to a real solution, the energy decreases. 5 Assuming Y= Y1Y2 Jij, Coulombic integral for 2 e Let consider 2 electrons, one in orbital Y1, the other in orbital Y2, and calculate the repulsion <1/r12>. Assuming Y= Y1Y2 This may be written Jij = Dirac notation used in physics = < Y1Y2IY1Y2> = (Y1Y1IY2Y2) Notation for 6 Quantum chemists Assuming Y= Y1Y2 Jij, Coulombic integral for 2 e Jij = < Y1Y2IY1Y2> = (Y1Y1IY2Y2) means the product of two electronic density Coulombic integral. This integral is positive (it is a repulsion). It is large when dij is small. When Y1 are developed on atomic orbitals f1, bilectronic integrals appear involving 4 AOs (pqIrs) 7 Assuming Y= Y1Y2 Jij, Coulombic integral involved in two electron pairs electron 1: Y1 or Y1 interacting with electron 2: Y2 or Y2 When electrons 1 have different spins (or electrons 2 have different spins) the integral = 0. <aIb>=dij. Only 4 terms are 0 and equal to Jij. The total repulsion between two electron pairs is equal to 4Jij. 8 Particles are electrons! Pauli Principle Wolfgang Ernst Pauli Austrian 1900 1950 electrons are indistinguishable: |Y(1,2,...)|2 does not depend on the ordering of particles 1,2...: | Y (1,2,...)|2 = | Y (2,1,...)|2 Thus either Y (1,2,...)= Y (2,1,...) S bosons or Y (1,2,...)= -Y (2,1,...) A fermions The Pauli principle states that electrons are fermions. 9 Particles are fermions! Pauli Principle The antisymmetric function is: YA = Y (1,2,3,...)-Y (2,1,3...)-Y (3,2,1,...)+Y (2,3,1,...)+... which is the determinant Such expression does not allow two electrons to be in the same state the determinant is nil when two lines (or columns) are equal; "No two electrons can have the same set of quantum numbers". One electron per spinorbital; two electrons per orbital. “Exclusion principle” 10 Two-particle case The simplest way to approximate the wave function of a many-particle system is to take the product of properly chosen wave functions of the individual particles. For the two-particle case, we have This expression is a Hartree product. This function is not antisymmetric. An antisymmetric wave function can be mathematically described as follows: Therefore the Hartree product does not satisfy the Pauli principle. This problem can be overcome by taking a linear combination of both Hartree products where the coefficient is the normalization factor. This wave function is antisymmetric and no longer distinguishes between fermions. Moreover, it also goes to zero if any two wave functions or two fermions are the same. This is equivalent to satisfying the Pauli 11 exclusion principle. Generalization: Slater determinant . The expression can be generalized to any number of fermions by writing it as a determinant. John Clarke Slater 1900-1976 12 Obeying Pauli principleY= 1/√ IY1Y2I Slater determinant Kij, Exchange integral for 2 e Let consider 2 electrons, one in orbital Y1, the other in orbital Y2, and calculate the repulsion <1/r12>. Assuming Y= 1/√ IY1Y2I Kij is a direct consequence of the Pauli principle Dirac notation used in physics Kij = = < Y1Y2IY2Y1A> = (Y1Y2IY1Y2) Notation for 13 Quantum chemists Obeying Pauli principleY= 1/√ IY1Y2I Slater determinant Kij, Exchange integral It is also a positive integral (-K12 is negative and corresponds to a decrease of repulsion overestimated when exchange is ignored). two electron pairs 14 Obeying Pauli principleY= 1/√ IY1Y2I Slater determinant Interactions of 2 electrons 15 Unpaired electrons: sgsu Singlet and triplet states bielectronic terms │YiYj│+ │YiYj│ Jij+Kij │YiYj│ Jij Kij │YiYj│ Jij-Kij │YiYj│ │YiYj│ │YiYj│- │YiYj│ 16 a(1)a() is solution of S2 a(1) (Sz2+Sz+S-S+) a(2) [1/2]2 + 1/2 + 0 0.75 a(2) (Sz2+Sz+S-S+) a(1) [1/2]2 + 1/2 + 0 0.75 2½½ 0.5 S-a(1)S+a(2) 0 0 S+a(1)S-a(2) 0 0 2Sza(1)Sza(2) total S2 a(1) a() = 2 a(1) a() 2 17 a(1)b() is not a solution of S2 a(1) (Sz2+Sz+S-S+) b(2) [1/2]2 - 1/2 + 1 0.75 b(2) (Sz2+Sz+S-S+) a(1) [1/2]2 + 1/2 + 0 0.75 2 ½ (-½) -.5 S-a(1)S+b(2) b(1) a(2) b(1) a(2) S+a(1)S-b(2) 0 0 2Sza(1)Szb(2) total S2 a(1) b() = a(1) b() + b(1) a() 2 18 A combination of Slater determinant then may be an eigenfunction of S2 IabI± IbaI = a(1)b(2) a(1)b() - b(1)a(2) a()b(1) ± b(1)a(2) a(1)b() +- a(1)b(2) a()b(1) IabI+ IbaI = [a(1)b(2) + b(1)a(2)] (a(1)b() - a()b(1)) IabI- IbaI = [a(1)b(2) - b(1)a(2)] (a(1)b() + a()b(1)) are a eigenfunction of S2 The separation of spatial and spin functions is possible If the spatial function (a or b) is associated with opposite spins 19 UHF: Variational solutions are not eigenfunctions of S2 Iab’I+ Iba’I = a(1)b’(2) a(1)b() - b’ (1)a (2) a()b(1) + b(1)a’(2) a(1)b() – a’(1)b(2) a()b(1) =[a(1)b’(2) + b(1)a’(2)](a(1)b() - [a’(1)b(2) + b’(1)a(2)] a()b(1)) Not equal The separation of spatial and spin functions is not possible If 2 spatial functions (a a’; b b’) are associated with opposite spins 20 Electronic correlation • VB method and polyelectronic functions • IC • DFT The charge or spin interaction between 2 electrons is sensitive to the real relative position of the electrons that is not described using an average distribution. A large part of the correlation is then not available at the HF level. One has to use polyelectronic functions (VB method), post Hartree-Fock methods (CI) or estimation of the correlation contribution, DFT. 21 Electronic correlation A of the correlation refers to HF: it is the “missing energy” for SCF convergence: Ecorr= E – ESCF Ecorr< 0 ( variational principle) Ecorr~ -(N-1) eV 22 Energy (kcal/mol) Importance of correlation effects on Energy RHF in blue, Exact in red. 23 Valence Bond 24 Heitler-London 1927 Electrons are indiscernible: If f1(1).f() is a valid solution Walter Heinrich Heitler German 1904 –1981 f1().f(1) also is. The polyelectronic function is therefore: [f1(1).f() + f1().f(1)] Fritz Wolfgang London German 1900–1954 To satisfy Pauli principle this symmetric expression is associated with an antisymmetric spin function: a (1).b() - a().b(1) this represents a singlet state! Each atomic orbital is occupied by one electron: for a bond, this represents a covalent bonding. 25 The resonance, ionic functions - H1 -H2 + Other polyelectronic functions : - + + H1 -H2 ↔ H1 -H2 - f1(1).f1() [f1(1).f1() + f().f(1)] f().f(1) [f1(1).f1() -f().f(1)] + H1 -H2 - symmetric antisymmetric According to Pauli principle, these functions necessarily correspond to the singlet state: a (1).b() - a().b(1) 26 H2 dissociation The cleavage is whether homolytic, H2 → H• + H• or heterolytic: H2 → H+ + H- H+ + H- E = 2 √(1-s)3/p = -0.472 a.u. with s=0.31 H+H E = -1 a.u; 27 MO behavior of H2 dissociation The cleavage is whether homolytic, H2 → H• + H• or heterolytic: H2 → H+ + H- Energy Energie Yu distance A-B internucdistance léa ire Yg sg2 = (fA +fB)2 = [(fA(1) fA(2) + fB(1) fB(2)] + [(fA(1) fB(2) + fB(1) fA(2)] 50% ionic + 50% covalent The MO description fails to describe correctly the dissociation! su2 = (fA -fB)2 = [(fA(1) fA(2) + fB(1) fB(2)] - [(fA(1) fB(2) + fB(1) f28A(2)] 50% ionic 50% covalent The Valence-Bond method It consists in describing electronic states of a molecule from AOs by eigenfunctions of S2, Sz and symmetry operators. There behavior for dissociation is then correct. These functions are polyelectronic. To satisfy the Pauli principle, functions are determinants or linear combinations of determinants build from spinorbitals. 29 Covalent function for electron pairs Ordered on spins a (1) b(1) or Y = IabI + IbaI Ordered on electrons IabI = a (2) b(2) Y = IabI - IabI Y = [a(1).b(2) +a(2). b(1)].[a(1).b(2) - a(2).b(1)] Y = [a(1).a(1)b (2)b(2) - b(1).b(1). a(2).a(2)] + [b(1).a(1) a(2)b(2) - a(1).b(1).b (2).a(2)] Y = IabI + IbaI This is the Heitler-London expression 30 Interaction Configuration OM/IC: In general the OM are those calculated in an initial HF calculation. Usually they are those for the ground state. MCSCF: The OM are optimized simultaneously with the IC (each one adapted to the state). 31 Interaction Configuration: mono, di, tri, tetra excitations… Monexcitation: promotion of i to k k I ki> j i Diexcitation promotion of i and j to k and l l kl Ij I > k j i 32 IC: increasing the space of configuration 4x4 2x2 Exact energy levels 3x3 33 Density Functional Theory What is a functional? A function of another function: In mathematics, a functional is traditionally a map from a vector space to the field underlying the vector space, which is usually the real numbers. In other words, it is a function that takes a vector as its argument or input and returns a scalar. Its use goes back to the calculus of variations where one searches for a function which minimizes a certain functional. E = E[r(r)] E(r) = T(r) + VN-e(r) + Ve-e(r) 34 Thomas-Fermi model (1927): The kinetic energy for an electron gas may be represented as a functional of the density. It is postulated that electrons are uniformely distributed in space. We fill out a sphere of momentum space up to the Fermi value, 4/3 p pFermi3 . Equating #of electrons in coordinate space to that in phase space gives: n(r) = 8p/(3h3) pFermi3 and T(n)=c ∫ n(r)5/3 dr T is a functional of n(r). Llewellen Hilleth Thomas 1903-1992 Enrico Fermi 1901-1954 Italian nobel 1938 35 DFT Pierre C Hohenberg Kohn 1923, german-born american Two Hohenberg and Kohn theorems : The existence of a unique functional. The variational principle. Walter Kohn 1923, Austrian-born American nobel 1998 36 First theorem: on existence The first H-K theorem demonstrates that the ground state properties of a many-electron system are uniquely determined by an electron density. It lays the groundwork for reducing the many-body problem of N electrons with 3N spatial coordinates to only 3 spatial coordinates, through the use of functional of the electron density. This theorem can be extended to the time-dependent domain to develop timedependent density functional theory (TDDFT), which can be used to describe excited states. The external potential, and hence the total energy, is a unique functional of the electron density. 37 First theorem on Existence : demonstration The external potential, and hence the total energy, is a unique functional of the electron density. The proof of the first theorem is remarkably simple and proceeds by reductio ad absurdum. Let there be two different external potentials, V1 and V2 , that give rise to the same density r. The associated Hamiltonians,H1 and H2, will therefore have different ground state wavefunctions, Y1 and Y2, that each yield r. E1 < < Y2 IH 1I Y2 > = < Y2 IH 2I Y2 > + < Y2 IH1 -H 2I Y2 > = E2 + ∫ r(r)(V1(r)- V2(r))dr E2 < < Y1 IH 2I Y1 > = E1 + ∫ r(r)(V2(r)- V1(r))dr E1 + E2 < E1 + E2 Therefore ∫ r(r)(V1(r)- V2(r))dr=0 and V1(r) = V2(r) The electronic energy of a system is function of a single electronic density only. 38 Second theorem: Variational principle The second H-K theorem defines an energy functional for the system and proves that the correct ground state electron density minimizes this energy functional : If r(r) is the exact density, E[r(r)] is minimum and we search for r by minimizing E[r(r)] with ∫ r(r)dr = N r(r) is a priori unknown As for HF, the bielectronic terms should depend on two densities ri(r) and rj(r) : the approximation r2e(ri,rj) = ri(ri) rj(rj) assumes no coupling. 39 Kohn-Sham equations 3 equations in their canonical form: Lu Jeu Sham San Diego Born in Hong-Kong member of the National Academy of Sciences and of the Academia Sinica of the Republic of China 40 Kohn-Sham equations Equation 1: This reintroduces orbitals: the density is defined from the square of the amplitudes. This is needed to calculate the kinetic energy. 41 Kohn-Sham equations Equation 2: Using an effective potential, one has a one-body expression. The intractable many-body problem of interacting electrons in a static external potential is reduced to a tractable problem of non-interacting electrons moving in an effective potential. The effective potential includes the external potential and the effects of the Coulomb interactions between the electrons, e.g., the exchange and correlation interactions. 42 Kohn-Sham equations Equation 3: the writing of an effective single-particle potential Eeff(r) = <Y│Teff+Veff │ Y > Teff+Veff = T + Vmono + RepBi Veff = Vmono + RepBi + T – Teff Aslo a mono electronic expression Unknown except for free electron gas Veff(r) = V(r) + ∫e2r(r’)/(r-r’) dr’ + VXC[r(r)] as in HF 43 Exchange correlation functionals VXC[r(r)] This term is not known except for free electron gas: LDA EXC[r(r)] = ∫r(r) EXC(r) dr EXC[r(r)] = VXC[r(r)]/ r(r) = EXC( r) + r(r) EXC( r)/ r EXC( r) = EX( r) + EC( r) = -3/4(3/p)1/3 r(r) + EC( r) determined from Monte-Carlo 44 and approximated by analytic expressions Exchange correlation functionals SCF-Xa The introduction of an approximate term for the exchange part of the potential is known as the Xa method. VXa () = -6a(3/4 pr )1/3 r is the local density of spin up electrons and a is a variable parameter. with a similar expression for r↓ 45 Exchange correlation functionals VXC[r(r)] EXC = EXC( r) LDA or LSDA (spin polarization) EXC = EXC( r,r) GGA or GGSDA - Perdew-Wang - PBE: J. P. Perdew, K. Burke, and M. Ernzerhof EXC = EXC( r,r,Dr) metaGGA 46 Hybrid methods: B3-LYP (Becke, three-parameters, Lee-Yang-Parr) Incorporating a portion of exact exchange from HF theory with exchange and correlation from other sources : a0=0.20 ax=0.72 aC=0.80 List of hybrid methods: B1B95 B1LYP MPW1PW91 B97 B98 B971 B972 PBE1PBE O3LYP BH&H BH&HLYP BMK 47 Axel D. Becke german 1953 Robert G. Parr Chicago 1921 Chengteh Lee received his Ph.D. from Carolina in 1987 for his work on DFT and is now a senior scientist at the supercomputer company Cray, Inc. Weitao Yang Duke university USA Born 1961 in Chaozhou, China got his undergraduate degree at the University of Peking 48 DFT Advantages : much less expensive than IC or VB. adapted to solides, metal-metal bonds. Disadvantages: less reliable than IC or VB. One can not compare results using different functionals*. In a strict sense, semi-empical,not abinitio since an approximate (fitted) term is introduced in the hamiltonian. * The variational priciples applies within a given functional and not to compare them. The only test for validity is comparison with experiment, not a global energy minimum! 49 DFT good for IPs IP for Au (eV) Without f With f functions SCF 7.44 7.44 SCF+MP2 8.00 8.91 B3LYP 9.08 9.08 Experiment 9.22 Electron affinity H Exp. SCF IC B3LYP Same basis set 0.735 -0.528 0.382 0.635 50 DFT good for Bond Energies Bond energies (eV); dissociation are better than in HF Exp. HF LDA GGA B2 3.1 0.9 3.9 3.2 C2 6.3 0.8 7.3 6.0 N2 9.9 5.7 11.6 10.3 O2 5.2 1.3 7.6 6.1 F2 1.7 -1.4 3.4 2.2 51 DFT good for distances Distances (Å) Exp. HF LDA GGA B2 1.59 1.53 1.60 1.62 C2 1.24 0.8 7.3 6.0 N2 1.10 1.06 1.09 1.10 O2 1.21 1.15 1.20 1.22 F2 1.41 1.32 1.38 1.41 52 DFT polarisabilities (H2O) Distances (Å) Exp. HF LDA m 0.728 0.787 0.721 axx 9.26 7.83 9.40 axx 10.01 9.10 10.15 axx 9.62 8.36 9.75 53 DFT dipole moments (D) Distances (Å) Exp. HF LDA GGA CO -0.11 0.33 -0.17 -0.15 CS 1.98 1.26 2.11 2.01 LiH 5.83 5.55 5.65 5.74 HF 1.82 1.98 1.86 1.80 54 Jacobs’scale, increasing progress according Perdew Steps Paradise = exactitude Method Example 5th step Fully non local - Hybrid Meta GGA B1B95 Hybrid GGA B3LYP 3rd step Meta GGA BB95 2nd step GGA BLYP 1st step LDA SPWL th 4 step Earth = Hartree-Fock Theory 55 Basis sets There is no general solution for the Schrödinger except for hydrogenoids. It is however natural to search for solutions resembling them. There is strictly no requirement to start by searching functions close to hydrogenoids. We can use any function not necessarily localized on atoms: for solids, plane waves are useful. We can use functions localized on bonds, on vacancies… 56 Large basis sets What is stronger than a turkishman? Turkishmen What is better than a function? Several ones. Minimizing parameters combing several functions is generally an improvement (at the most, it is useless). Basis set associated with hydrogenoids: minimum basis set. more: extended basis set. 57 SCF limit Increasing the number of (independent) functions leads to improve the energy (variational principle). This improvement saturates. The limit is called SCF limit. This limit can be estimated by interpolation. 58 SCF convergence for H+ H2+ d a0 (Ả) E diss eV exp 2.0 (1.06 ) 2.791 1sH z=1 2.5 (1.32) 1.76 1sH z opt 2.0 (1.06) 2.25 + 2p 2.0 (1.06) 2.71 + more 2.0 (1.06) 2.791 59 H2 d a0 (Ả) E diss eV 1.40 (0.74) 4.746 1sH z=1 1.61 2.695 1sH z = 1.197 SCF Limit VB 1sH z=1.166 1.38 3.488 1.40 3.636 1.41 3.782 VB + p (93%s 7%p) A hundred of functions 1.41 4.122 1.40 D = 0.5 10-4 4.746 D = 10-6 exp 60 Variation of the Slater exponent • Hydrogen z=1.24 or z=1.30 smaller than z=1.0 • Diffuse orbitals: z small “soft” • contracted orbitals: z large “hard” z =Z/na0 < r> = a0 n(n+1/2)/Z = (n+1/2)/Z 61 Incomplete Basis sets DZ: E(H2)=-1.128720 a.u. TZ+0.31(TZ-DZ): E(H2)=-1.134308 a.u. The term “ab initio” suggest no subjectivity. However the choice of the functions is arbitrary; The variational principle allows comparing several choices for quantitative results (not always desirable for understanding). Some functions may be redundant. Therefore, it is better to express the functions on a basis set of orthogonal and normalized functions. 63 Basis set superposition error, BSSE Since basis sets are incomplete, there is an error when calculating A + B → C. Indeed, it seems fair to use the same basis set for A, B and C. However in C, the orbitals of B contribute to stabilize A if it the basis set to describe A is incomplete. The same is true the other way round. Each monomer "borrows" functions from other nearby components, effectively increasing its basis set and improving the calculation of derived properties such as energy Thus A and B should be better described using the orbitals centered on the other fragment than alone. It follows that A+B is underestimated relative to C. 64 Basis set superposition error, BSSE (counterpoise method). The energy gain for the reaction is therefore overestimated. • For a diatomic formation, the solution is to calculate A and B using the full basis set for A+B. (B being a dummy atom when A is calculated). Ghost orbitals are orbitals localized where there is no nucleus (no potential). • For an interaction between 2 large fragments, there is a problem of choosing the geometry for A: that of lowest energy for A or that in the fragment A-B. The method is estimating the BSSE correction in the fragment of A-B and assuming that it is the correction for A. 65 Basis set superposition error, BSSE (Chemical Hamiltonian approach) The (CHA) replaces the conventional Hamiltonian with one designed to prevent basis set mixing a priori, by removing all the projector-containing terms which would allow basis set extension. Though conceptually different from the counterpoise method, it leads to similar results. 66 Basis set transformation, orthogonalization Starting from scratch, a set of functions is not necessarily orthogonal. Orthogonalization uses matrix transformations. There are 3 main orthogonalization processes: depends on the ordering; this may be useful a' 2 a' 2 a2 a2 a1 a1 a' 1 Löwdin S ch midt a' 1 a' 2 a2 Insensitive to the ordering. a' 1 a1 C anon iqu e 67 hydrogenoids Solving Schrödinger equation for hydrogenoids leads to spatial functions: Y(r,q,f)= Nn,l rl Pn,l(r) exp(-Zr/n) R(q,f) • Nn,l is a normalization function (it contains the dimension a0-3/2) • rl is a power of r and Pn,l(r) a polynom of degree n-l-1 • exp(-Zr/n) makes the summation in the universe finite. • R(q,f) is an spherical harmonic function. 69 Slater-type orbitals (STOs ) 1930 The radial part appears as a simplification of that of the hydrogenoid. Y(r)= Nn,l rl exp(- z r/n*) Where John Clarke Slater 1900-1976 Nn,l is a normalization constant, z is a constant related to the effective charge of the nucleus, the nuclear charge being partly shielded by electrons. n* plays the role of principal quantum number, n = 1,2,..., The normalization constant is computed from the integral Hence There is no node for the radial part! 70 Slater-type orbital Why this simplification? In LCAO, we make combinations of AOs. It is therefore useless to start by imposing the polynoms. What changes? The hydrogenoids are orthogonal <1sI2s>=0. (eigenfunctions associated with different quantum numbers). The Slater orbitals are not orthogonal. 1s+2s resembles the hydrogenoid 1s (no node) and 2s-1s resembles the 2s orbital (the combination makes the nodal surface appear. 72 Double zeta Using several Slater functions allows representing better different oxidation states. When there is an electron transfer, an atom could be A+, A° or A-. For a metal, often several atomic configurations are close in energy: s2d8, s1d9 or d10. This correspond to different exponents for the s and d AOs. Double and triple zeta functions 2 or 3 AOs adapted to one oxidation state each and allowing variation in a linear combination and flexibility. As soon as the reference to oxidation states disappears (Gaussian contractions) the terminology becomes less justified and just qualify the number of independent functions. 73 Gaussian functions rn-1 2 -ar e with N= (2a/p)0.75 have expressions close to Gaussians, N Slater. They are decreasing exponentials (more rapidly than Slaters), with different slope at r=0*. Close to r=req, differences are small. Gaussians are not as appropriate than Slaters but not so different to prevent considering them. The reason to use Gaussians is a computing facility. In the H-F method, many integrals (N4) involve the product of 4 orbitals. The product of two Gaussian is easily calculated; it is another Gaussian: * 74 Gaussian functions fitting Slater functions with z=1 A Gaussian orbital is a combination (contraction) of several individual Gaussian functions called primitive. A STO-NG orbital is a linear combination of N Gaussian fitting closely a Slater orbital. Minimal basis set: Sir John Anthony Pople 1925-2004 Nobel 1998 STO-1G e-0.27095 r2 STO-2G .678914 e-0.151623 r2 STO- 3G 0.444635. 0.535328 e-0.109818 r2 e-0.405771 r2 0.430129 e0.9518195 r2 0.154329 e-2.22766 r2 75 Fit of a Slater-type orbital by STO-NG 0,6 Slater Amplitude Amplitude 0,5 STO3G 0,4 0,3 0,2 STO1G 0,1 -0,0 0 1 2 3 4 rayon (bohr) Radius (a.u.) 76 density Radiale probability RadialDensité de Probalibilté Fit of a Slater-type orbital by STO-NG 0,05 ST O1G 0,04 ST O3G 0,03 SLATER 0,02 0,01 0,00 0 1 2 3 rayon (bohr) Radius (a.u.) 4 77 Correspondance for z≠1 There is scaling factor: r →z/z1 r When the Slater exponent is multiplied by z/z1, the Gaussian exponent is multiplied by (z/z1)2. e-zr = -ar e = -[√ar] e → (z/z1) = (a/a1)0.5 For H, the Slater exponent is multiplied by 1.24; those of the gaussian function are multiplied by 1.242= 1.5376 For C, the Slater exponent is multiplied by 1.625; those of the gaussian function are multiplied by 1.6252= 2.640625 78 Minimal basis set and split valence basis set. STO-3G has been a long time used; with improvement of computing facilities, this is not the case nowadays in spite of the simplicity of using minimal basis. One way to improve accuracy is taking more functions. Releasing all contractions (N functions instead of 1 linear combination) is expensive. We can split the Gaussian into two sets. The partition may make groups or isolate the outermost primitive. The first procedure perhaps involves larger energy contribution but the second one is more chemical. The flexibility in reaction is necessary for the electron participating to the transformation (chemical reaction). If only the outermost primitive is isolated, we have the split-valence basis set named N-X1G by Pople. 79 Split valence basis set; N-X1G Core orbitals are represented by a single orbital with N primitives. Valence orbitals are represented by 2 orbitals: one orbital with X primitives and one diffuse orbital. Sir John Anthony Pople 1925-2004 Nobel 1998 basis 3-21G 4-31G 6-31G core 3 4 6 valence valence 2 1 3 1 3 1 80 Forget about Slater : Minimal basis set Huzinaga and Dunning One way to obtain contraction is making a full calculation with no contraction and using the MO coefficients for contraction. Basis set for O 81 Alternative partitioning for extended basis sets; Huzinaga and Dunning The basis set for O [9s5p/3s2p] by Dunning means that there are 3 s orbitals (using 1, 2 and 6 primitives) and 2 p orbitals (using 4 and 1 primitives). The “1s” orbital is represented by the first orbital (1 primitive). The basis set for O2- [13s7p/5s3p] by Pacchioni and Bagus means that there are 5 s orbitals (using 6, 2, 1, 2 and 1 primitives) and 2 p orbitals (using 4, 2 and 1 primitives). The “1s” orbital is represented by the first orbital (6 primitives). DZHD Double-Zeta Huzinaga-Dunning DTZHD Double-triple-Zeta Huzinaga-Dunning: The contraction generates several orbitals and is qualified a N zeta even if this is more mathematics than physics: the relation with Slater orbitals and oxidation states desappears. 82 Polarized Basis sets For H2, 7% of p improved the total energy from 3.782 eV to 4.122 eV. The molecular potential is not spherical around each atom. The directionality is provided by p-type orbitals. Polarization functions consists to add “l+1” functions: External valence shell s p d polarization p d f Pople’s notation 6-31G**: first asterisk “heavy atoms”; second asterisk: p-type on H 84 6-21G(df) add d and f functions and He Basis sets for anions, 6-31++G** Anions require diffuse orbitals and are more difficult to calculate “in gas phase” than neutral or cationic species. Usually one can use more diffuse (smaller) exponents. The addition of diffuse functions, denoted in Pople-type sets by a plus sign, +, and in Dunning-type sets by "aug" (from "augmented"). Two plus signs indicate that diffuse functions are also added to light atoms (hydrogen and helium). 85 Pseudopotentials Core orbitals do not participate to much to chemistry and it is more useful and simpler to calculate only the valence. Then core electron interactions are replaced by a pseudopotential. The pseudopotential is an effective potential constructed to replace the atomic allelectron potential such that core states are eliminated and the valence electrons are described by nodeless pseudowavefunctions. Only the chemically active valence electrons are dealt with explicitly, while the core electrons are 'frozen' Motivation: Reduction of basis set size Reduction of number of electrons Inclusion of relativistic and other effects 87 88 Step calculations To save calculation efforts, on can use different accuracy for optimization of geometry and calculation of properties on the optimized geometry. UHF/3-21G(d) means that the geometry was optimized using UHF/3-21G(d) and the final result was calculated using UB3LYP/6-31G(d) 91 How many AOs? How many occupied MOs? How many vacant MOs? For C2H4 # MOs # occ # vac EHT STO-3G 3-21G 4-31G 6-31-G** PS-31G 93 How many AOs? How many occupied MOs? How many vacant MOs? For C2H4 EHT # MOs 12 # occ 6 # vac 6 STO-3G 14 8 6 3-21G 20 8 12 4-31G 20 8 12 6-31-G** 42 8 34 PS-31G 6 12 18 94