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Trygve Helgaker, Department of Chemistry, University of Oslo, Norway.
Poul Jorgensen and Jeppe Olsen Department of Chemistry, University of Aarhus, Denmark.
Preface xxi
Overview xxv
Programs used in the preparation of this book xxix
1. Second Quantization 1
1.1 The Fock space 1
1.2 Creation and annihilation operators 2
1.3 Number-conserving operators 6
1.4 The representation of one- and two-electron operators 9
1.5 Products of operators in second quantization 14
1.6 First- and second-quantization operators compared 18
1.7 Density matrices 19
1.8 Commutators and anticommutators 25
1.9 Nonorthogonal spin orbitals 27
2. Spin in Second Quantization 34
2.1 Spin functions 34
2.2 Operators in the orbital basis 35
2.3 Spin tensor operators 41
2.4 Spin properties of determinants 46
2.5 Configuration state functions 51
2.6 The genealogical coupling scheme 53
2.7 Density matrices 61
3. Orbital Rotations 80
3.1 Unitary transformations and matrix exponentials 80
3.2 Unitary spin-orbital transformations 86
3.3 Symmetry-restricted unitary transformations 89
3.4 The logarithmic matrix function 93
4. Exact and Approximate Wave Functions 107
4.1 Characteristics of the exact wave function 107
4.2 The variation principle 111
4.3 Size-extensivity 126
4.4 Symmetry constraints 135
5. The Standard Models 142
5.1 One- and N-electron expansions 143
5.2 A model system: the hydrogen molecule in a minimal basis 146
5.3 Exact wave functions in Fock space 162
5.4 The Hartree-Fock approximation 167
5.5 Multiconfigurational self-consistent field theory 176
5.6 Configuration-interaction theory 181
5.7 Coupled-cluster theory 186
5.8 Perturbation theory 192
6. Atomic Basis Functions 201
6.1 Requirements on one-electron basis functions 201
6.2 One- and many-centre expansions 203
6.3 The one-electron central-field system 204
6.4 The angular basis 207
6.5 Exponential radial functions 218
6.6 Gaussian radial functions 229
7. Short-Range Interactions and Orbital Expansions 256
7.1 The Coulomb hole 256
7.2 The Coulomb cusp 259
7.3 Approximate treatments of the ground-state helium atom 262
7.4 The partial-wave expansion of the ground-state helium atom 267
7.5 The principal expansion of the ground-state helium atom 273
7.6 Electron-correlation effects summarized 278
8. Gaussian Basis Sets 287
8.1 Gaussian basis functions 287
8.2 Gaussian basis sets for Hartree-Fock calculations 288
8.3 Gaussian basis sets for correlated calculations 300
8.4 Basis-set convergence 315
8.5 Basis-set superposition error 327
9. Molecular Integral Evaluation 336
9.1 Contracted spherical-harmonic Gaussians 336
9.2 Cartesian Gaussians 338
9.3 The Obara-Saika scheme for simple integrals 344
9.4 Hermite Gaussians 349
9.5 The McMurchie-Davidson scheme for simple integrals 352
9.6 Gaussian quadrature for simple integrals 357
9.7 Coulomb integra;s over spherical Gaussians 361
9.8 The Boys function 365
9.9 The McMurchie-Davidson scheme for Coulomb integrals 372
9.10 The Obara-Saika scheme for Coulomb integrals 381
9.11 Rys quadrature for Coulomb integrals 387
9.12 Scaling properties of the molecular integrals 398
9.13 The multipole method for Coulomb integrals 405
9.14 The multipole method for large systems 417
10. Hartree-Fock Theory 433
10.1 Parametrization of the wave function and the energy 433
10.2 The Hartree-Fock wave function 438
10.3 Canonical Hartree-Fock theory 443
10.4 The RHF total energy and orbital energies 450
10.5 Koopmans' theorem 454
10.6 The Roothaan-Hall self-consistent field equations 458
10.7 Density-based Hartree-Fock theory 465
10.8 Second-order optimization 478
10.9 The SCF method as an approximate second-order method 490
10.10 Singlet and triplet instabilities in RHF theory 496
10.11 Multiple solutions in Hartree-Fock theory 504
11. Configuration-Interaction Theory 523
11.1 The CI model 523
11.2 Size-extensivity and the CI model 527
11.3 A CI model system for noninteracting hydrogen molecules 535
11.4 Parametrization of the CI model 540
11.5 Optimization of the CI wave function 543
11.6 Slater determinants as products of alpha and beta strings 550
11.7 The determinantal representation of the Hamiltonian operator 552
11.8 Direct CI methods 554
11.9 CI orbital transformations 569
11.10 Symmetry-broken CI solutions 573
12. Multiconfigurational Self-Consistent Field Theory 498
12.1 The MCSCF model 498
12.2 The MCSCF energy and wave function 600
12.3 The MCSCF Newton trust-region method 610
12.4 The Newton cigenvector method 616
12.5 Computational considerations 621
12.6 Exponential parametrization of the configuration space 630
12.7 MCSCF theory for several electronic states 637
12.8 Removal of RHF instabilities in MCSCF theory 640
13. Coupled-Cluster Theory 648
13.1 The coupled-cluster model 648
13.2 The coupled-cluster exponential ansatz 654
13.3 Size-extensivity in coupled-cluster theory 665
13.4 Coupled-cluster optimization techniques 670
13.5 The coupled-cluster variational Lagrangian 674
13.6 The equation-of-motion coupled-cluster method 677
13.7 The closed-shell CCSD model 685
13.8 Special treatments of coupled-cluster theory 698
13.9 High-spin open-shell coupled-cluster theory 704
14. Perturbation Theory 724
14.1 Rayleigh-Schrödinger perturbation theory 725
14.2 Møller-Plesset perturbation theory 739
14.3 Coupled-cluster perturbation theory 749
14.4 Møller-Plesset theory for closed-shell systems 759
14.5 Convergence in perturbation theory 769
14.6 Perturbative treatments of coupled-cluster wave functions 783
14.7 Multiconfigurational perturbation theory 796
15. Calibration of the Electronic-Structure Models 817
15.1 The sample molecules 817
15.2 Errors in quantum-chemical calculations 819
15.3 Molecular equilibrium structures: bond distances 821
15.4 Molecular equilibrium structures; bond angles 832
15.5 Molecular dipole moments 836
15.6 Molecular and atomic energies 840
15.7 Atomization energies 854
15.8 Reaction enthalpies 865
15.9 Conformational barriers 874
15.10 Conclusions 879
List of Acronyms 885
Index 887
In the formalism of second quantization as presented in the previous chapter, there is no reference to electron spin – the intrinsic angular momentum of the electron. In nonrelativistic theory, many important simplifications follow by taking spin explicitly into account. In the present chapter, we develop the theory of second quantization further so as to allow for an explicit description of electron spin. Although no fundamentally new concepts of the second-quantization formalism are introduced, the results obtained here are essential for an efficient description of molecular electronic systems in the nonrelativistic limit.
The spin orbitals introduced in Chapter 1 are functions of three continuous spatial coordinates r and one discrete spin coordinate ms. The spin coordinate takes on only two values, representing the two allowed values of the projected spin angular momentum of the electron: . The spin space is accordingly spanned by two functions, which are taken to be the eigenfunctions α(ms) and β(ms) of the projected spin angular-momentum operator
(2.1.1)
(2.1.2)
These spin functions – which we shall generically denote by σ, τ, μ and v – are eigenfunctions of the total-spin angular-momentum operator as well with quantum number s =
(2.1.3)
in accordance with the general theory of angular momentum in quantum mechanics. The functional form of the spin functions is given by the equations
(2.1.4)
(2.1.5)
Completeness of the spin basis leads to the following resolution of the identity
(2.1.6)
as may be verified from relations (2.1.4) and (2.1.5). It should be noted that we have for convenience written the first-quantization spin operators as operating on the spin function of a single electron. The generalization to an N-electron system is simple and requires no comment except to note that, whereas is a true one-electron operator, the operator for the total spin (2.1.3) is a two-electron operator in the sense that it is a linear combination of terms involving two electrons although no physical interactions occur.
We shall occasionally find it convenient to use for the discrete spin functions the same notation as for continuous spatial functions, interpreting integration in spin space as summation over the two discrete values of ms:
(2.1.7)
Thus, we may write the orthonormality conditions of the spin functions in the form
(2.1.8)
Like the resolution of the identity (2.1.6), this relationship is easily verified by reference to (2.1.4) and (2.1.5).
The spin-orbital space is spanned by the direct product of a basis for the orbital space and a basis for the spin space. Thus, a general spin orbital may be written as
(2.1.9)
In nonrelativistic theory, it is common to use spin orbitals of the more restricted form
(2.1.10)
so that a given spin orbital consists of an orbital part multiplied by a spin eigenfunction. This simple product form is acceptable since the nonrelativistic Hamiltonian operator does not involve spin and thus cannot couple the spatial and spin parts of the spin orbitals. We note that spin orbitals (2.1.10) with the same orbital parts but different spins are orthogonal.
We shall in this book use lower-case indices for orbitals, reserving upper-case indices for spin orbitals. For spin orbitals ϕpσ of the form (2.1.10), we shall usually employ a composite index, where the first index p refers to the orbital part and the second index σ to the spin part. The total number of orbitals is denoted by n. Thus, for a basis of n orbitals, there are a total of M = 2n independent spin orbitals of the form (2.1.10). With the necessary elaboration of notation to accommodate composite indices of the spin orbitals, the theory of second quantization presented in Chapter 1 holds unchanged in the product basis (2.1.10). For example, the anticommutator between creation and annihilation operators (1.2.29) now becomes
(2.1.11)
where for example is the creation operator associated with the product spin orbital ϕpσ.
Quantum-mechanical operators may be classified according to how they affect the orbital and spin parts of wave functions. Thus, we classify operators as spin-free or spinless if they work in ordinary space only without affecting the spin part of a function. Conversely, an operator that works in spin space only, without affecting the spatial part of a function, is termed a pure spin operator or simply a spin operator. Finally, an operator is mixed if it affects both the spatial and spin parts of a function. We shall in this section investigate how each of these three classes of operators is represented in second quantization.
Let us first consider one-electron operators. Following the general discussion in Section 1.4.1, a spin-free one-electron operator of the form
(2.2.1)
may in the spin-orbital basis be written as
(2.2.2)
The integrals entering the second-quantization operator vanish for opposite spins since the first-quantization operator fc is spin-free:
(2.2.3)
Here we use the notation
(2.2.4)
for the integrals over spatial coordinates and note that these integrals display the usual Hermitian permutational symmetry:
(2.2.5)
The second-quantization representation of the spin-free one-electron operator (2.2.1) now becomes
(2.2.6)
where we have introduced the singlet excitation operators
(2.2.7)
as a linear combination of the spin-orbital excitation operators of Section 1.3.3. The singlet excitation operator is discussed in detail in Sections 2.3.4 and 2.3.5.
We now turn our attention to spinless two-electron operators. According to the discussion in Section 1.4.2, the second-quantization representation of a general spin-free two-electron operator of the form
(2.2.8)
is given by
(2.2.9)
Most of the terms in this operator vanish because of the orthogonality of the spin functions
(2.2.10)
where we have introduced two-electron integrals in ordinary space
(2.2.11)
Let us consider the permutational symmetries of these integrals. The symmetry
(2.2.12)
follows from the symmetry of the interaction operator in (2.2.8) and is always present in the integrals. The remaining symmetries are different for real and complex orbitals. For complex orbitals, we have the Hermitian symmetry
(2.2.13)
whereas for real orbitals we have the following permutational symmetries
(2.2.14)
For real orbitals, therefore, there are a total of eight permutational symmetries present in the integrals, obtained by combining (2.2.12) with (2.2.14).
Inserting the integrals (2.2.10) in (2.2.9), the second-quantization representation of a spin-free two-electron operator can be written as
(2.2.15)
where for convenience we have introduced the two-electron excitation operator
(2.2.16)
Note the permutational symmetry
(2.2.17)
which follows directly from the last expression in (2.2.16). There are no permutational symmetries analogous to (2.2.14) for the two-electron excitation operator.
We are now in a position to write up the second-quantization representation of the nonrelativistic and spin-free molecular electronic Hamiltonian in the orbital basis:
(2.2.18)
This expression should be compared with the operator in the spin-orbital basis (1.4.39), where each summation index runs over twice the number of orbitals. The one- and two-electron integrals in (2.2.18) are the same as those in (1.4.40) and (1.4.41) except that the integrations are over the spatial coordinates only:
(2.2.19)
(2.2.20)
The scalar nuclear-repulsion term hnuc in (2.2.18) was defined in (1.4.42).
We now consider the representation of first-quantization operators fc that work in spin space only. The associated second-quantization operators may be written in the general form
(2.2.21)
Three important examples of pure spin operators are the raising and lowering operators and (also known as the step-up and step-down operators or as the shift operators) and the operator for the z component of the spin angular momentum . From the effect of these operators on the spin functions (again assuming a one-particle state)
(2.2.22)
(2.2.23)
(2.2.24)
we obtain the following matrix elements
(2.2.25)
(2.2.26)
(2.2.27)
using the same notation for the matrix elements as in Section 1.5.2. Inserting the integrals (2.2.25)–(2.2.27) in the operator (2.2.21), we arrive at the following expressions for the basic spin operators:
(2.2.28)
(2.2.29)
(2.2.30)
The second-quantization lowering operator is readily seen to be the Hermitian adjoint of the raising operator:
(2.2.31)
For the operators for the x and y components of the spin angular momentum
(2.2.32)
(2.2.33)
we obtain from (2.2.28) and (2.2.29) the following expressions for their second-quantization...
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