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Advanced Review Dirac-exact relativistic methods: the normalized elimination of the small component method† Dieter Cremer,∗ Wenli Zou and Michael Filatov

Dirac-exact relativistic methods, i.e., 2- or 1-component methods which exactly reproduce the one- energies of the original 4-component Dirac method, have established a standard for reliable relativistic quantum chemical calculations targeting medium- and large-sized molecules. Their development was initiated and facilitated in the late 1990s by Dyall’s development of the normalized elimination of the small component (NESC). Dyall’s work has fostered the conversion of NESC and related (later developed) methods into routinely used, multipurpose Dirac- exact methods by which energies, first-order, and second-order properties can be calculated at computational costs, which are only slightly higher than those of nonrelativistic methods. This review summarizes the development of a generally applicable 1-component NESC algorithm leading to the calculation of reliable energies, geometries, electron distributions, electric moments, electric field gradients, hyperfine structure constants, contact and Mossbauer¨ isomer shifts, nuclear quadrupole coupling constants, vibrational frequencies, infrared intensities, and static electric dipole polarizabilities. In addition, the derivation and computational possibilities of 2-component NESC methods are discussed and their use for the calculation of -orbit coupling (SOC) effects in connection with spin-orbit splittings and SOC-corrected energies are demonstrated. The impact of scalar relativistic and spin-orbit effects on molecular properties is presented. © 2014 John Wiley & Sons, Ltd.

How to cite this article: WIREs Comput Mol Sci 2014. doi: 10.1002/wcms.1181

IMPORTANCE OF RELATIVISTIC mass-velocity effect originally discovered by Einstein16 EFFECTS IN CHEMISTRY when developing the theory of special relativity:

he identification and understanding of relativistic m0 m0 me =  =  (1) effects is essential for an expert analysis of the − 2 T 1 − (v/c)2 1 β chemistry of heavy and superheavy elements.1–15 For a long time, relativistic effects were not considered to According to the mass-velocity effect, the mass of be important for chemistry because chemical processes an electron at rest, m , increases with its velocity v and chemical properties are largely determined by 0 to the effective mass m (c = 137.035 999 074(44) the valence of an atom. This belief was e atomic units: speed of light17) and this will to a based on a misleading interpretation of the so-called decrease of the Bohr radius rB of an electron because the latter is proportional to 1/m .18 The shortening ∗ e Correspondence to: [email protected] of the Bohr radius of an electron orbit to an Computational and Theoretical Chemistry (CATCO), increase of nucleus–electron attraction and relates in Department of Chemistry, Southern Methodist University, Dallas, TX, USA the quantum mechanical description to a contraction †This article is dedicated to Kenneth G. Dyall of the 1s-orbital. Conflict of interest: The authors have declared no conflicts of interest Using the virial theorem E =−T (the total for this article. energy of an atom or molecule is equal to the negative

© 2014 John Wiley & Sons, Ltd. Advanced Review wires.wiley.com/wcms of its kinetic energy), the energy of The mass-velocity effect leads to a bond a -like ion with Z can be shortening, for which it seems logical to relate expressed according to this effect to the relativistic orbital contraction. Extended relativistic studies, however, have clarified 1 1 − Z2 =− v2 (2) that these are independent phenomena because the 2 2 bond contraction is due to a kinetic energy decrease in the bonding region as a result of the relativistic where atomic units are used. Hence, v2 = Z2 follows effects.21–23 and by this the ratio β = v/c = Z/c can be predicted to The contraction of s- or p-orbitals and the adopt significant values only for the 1s-electrons of expansion of d- or f-orbitals are the result of scalar heavy atoms (large Z). Following this argument, the relativistic effects. A third, nonscalar relativistic effect general expectation was that only for the 1s electrons of atoms with Z ≥ 80 does the mass-velocity become is spin-orbit coupling (SOC), i.e., electrons with > important, and therefore relativity is a physics rather the angular momentum l 0(p, ... than a chemistry problem. d, f, ) are described by that are eigen- functions of j2 and j where j, defined by the However, this interpretation of the mass-velocity z  relationships j = l + s and j2 = l2 +s2 + 2l· s,isthe effect overlooked the fact that the higher s-orbital  states including the valence s-orbital also show strong total angular momentum operator (l and l:orbital relativistic effects according to the exact solution of the angular momentum operator and corresponding  . Often this is explained in a rather sim- vector; s and s: spin angular momentum operator plified way that the s-orbitals with principal quantum and corresponding vector). Hence, the total angular = ± number n > 1 have to be orthogonal to the contracted momentum quantum number of a is j l 1/2 1s-orbital, which leads to a propagation of the thus leading to the well-known splitting of s, p, d, orbital contraction into the valence shell and by this ... levels into s1/2,p1/2,p3/2,d3/2,d5/2, ... levels. becomes chemically relevant. The contracted orbitals The splitting caused by SOC increases with the atomic adopt lower energies compared to the nonrelativistic number and adopts values as large as 1 eV, for example 2 − 2 situation and this has far-reaching consequences for in the energy difference E( P3/2) E( P1/2)ofTl(for the chemistry of the corresponding atom. a discussion of SOC, see Refs 10 and 24). Besides the contraction of the s-orbitals, there is Scalar relativistic and SOC effects influence also a (smaller) contraction of the p-orbitals because literally all physical and chemical properties of their relativistic counterparts have a finite amplitude relativistic elements (i.e., elements from the fifth at the position of the nuclei. Specifically, this is on in the ) and molecules true for the p1/2 spinor (for the counterpart of the containing these atoms. For example, relativistic nonrelativistic or scalar relativistic spin-orbital, see effects influence the value of ionization potentials below) that experiences comparable relativistic effects and electron affinities. Excitation spectra of molecules as the s1/2 spinor, at least for H-like systems. The with heavier atoms are characteristically changed. The contraction of the s- and p-orbitals leads to a second, yellow color of is directly related to a relativistic generally observed, relativistic effect: the nuclei are decrease of the 5d − 6s orbital energy gap.25 The more shielded by the s- and p-electron density so relativistic effects on the optical properties of gold that the electron–nucleus attraction of the d- and f- were recently reconsidered and quantified.26,27 The electrons is reduced; their energies are increased; their relativistic bond contraction leads to a change in bond orbitals expanded; and the d- and f-densities become strength where bond shortening is often accompanied more diffuse than in the nonrelativistic case. by a weakening of the bond.28,29 This in turn causes The relativistic changes in the orbital energies changes in molecular stability and reactivity. Hence, are reflected by the electron configurations of the all aspects of the chemical behavior of molecules transition metal atoms. For example, molybdenum containing relativistic atoms are changed due to scalar prefers a [Kr] 4d55s1 electron configuration, whereas and/or SOC relativistic effects. tungsten a [Xe] 5d46s2 configuration, thus reflecting Relativistic effects are especially strong for the lowering of the energy of the 6s orbital and the gold (Au-maximum of relativity in period 6) and increase of the 5d-orbital energy due to relativity. the neighboring elements platinum and mercury. Similar changes are found for the pairs Nb–Ta, In period 7, the maximum of relativistic effects is Ru–Os, Rh–Ir, and Pd–Pt, for which the element with shifted to eka-mercury (, Z = 112). This the higher atomic number and the stronger relativistic becomes obvious when calculating the relativistic effects has a higher s-orbital occupation in its ground contraction of the 6s and 7s shell for periods 6 and state.19,20 7.30,31

© 2014 John Wiley & Sons, Ltd. WIREs Computational Molecular Science Dirac-exact relativistic methods

In this connection it is interesting that also the nonrelativistic spin orbitals. The Dirac-Coulomb liquid state of elemental mercury is directly influenced (DC) Hamiltonian contains a fully relativistic one- by relativistic effects. The 6s − 6p gap is increased electron part as given by the D-Hamiltonian combined by the mass-velocity effect thus effectively reducing with the nonrelativistic Coulomb potential, 1/r12, the p-orbital (spinor) participation in bonding as well in the two-electron part,39,40 thus neglecting some as the strength of the van der Waals interactions subtle relativistic corrections to the electron–electron between Hg atoms. The latter effect is the cause for interaction.1 the liquid state of Hg. The peculiar properties of Hg, The relativistic correction of the two-electron which are different from those of Zn and Cd, are part of the Hamiltonian was first derived by convincing manifestations of relativity. Recently, a Breit using perturbational procedures.41 It contains, detailed discussion of this topic was given by Calvo besides the nonrelativistic Coulomb term, two rel- et al.32 ativistic corrections where the former represents a There are other relativistic effects such as the current–current interaction and the latter represents a Lamb shift in the spectrum of the H atom,33 which gage term originating from choosing a specific gage can no longer be explained using the theory of (Coulomb gage) for electron–electron interactions.1 special relativity as it presents an interaction of Although the Coulomb-Breit electron–electron inter- the H electron with the vacuum. Instead, the Lamb action is not fully Lorentz invariant (correct to shift requires a theoretical description employing the the order of O(c− 2)), it represents a sufficiently theory of (QED) developed accurate approximation to the interaction between by Schwinger et al.. QED provides the theoretical electrons moving with relatively low velocities. The basis for special relativity and thereby the description Dirac–Coulomb–Breit (DCB) Hamiltonian requires of relativistic effects in chemistry.34 However, QED however a large load of additional calculations effects (Lamb shift, vacuum polarization, etc.) are very for the determination of the two-electron part. small (1% of the Dirac description of the relativistic The DCB-Hamiltonian written in the presence of effects for the ns binding energies of ns1 atomic states an external field includes as relativistic corrections with Z > 41) and therefore they are of little interest in orbit–orbit, spin-other orbit, dipole spin–spin, contact chemistry.35,36 spin–spin, and the two electron Darwin interaction, of which especially the latter term may become important. In general, one can say that the two- SHORT HISTORICAL OVERVIEW electron relativistic corrections are rather small (with OF RELATIVISTIC METHODS the exclusion of superheavy elements) and therefore chemically relevant results can be obtained with the From the 1970s on, an increasing number of quantum DC-Hamiltonian. chemical investigations pointed out the importance of Dirac-Coulomb Hartree-Fock, or Dirac- relativity for heavy-atom chemistry. In this connection Hartree-Fock (DHF) for brevity, calculations of large the pioneering work of Desclaux (Grenoble), Grant molecules become expensive because they require a (Cambridge), and Pyykko¨ (Helsinki) has to be 4-component description of the wave function (split mentioned. The work of these theoreticians and that up into a large and a small component each with α- of many others, which followed in the last 40 years, and β-spin part) and lead to positive eigenvalues for is summarized in textbooks, review articles, and electrons and negative ones (shifted by the amount the references cited therein.1–15 In this time span, − 2mc2) for positrons (see Figure 1). The coupling relativistic quantum chemical methods were developed between the positive and negative eigenstates leads which made a reliable calculation of relativistic effects to the small component and therefore is a direct for atoms and molecules possible. A way of describing reflection of the positronic eigenstates. The large these developments is by referring to the relativistic component converges for c →∞to the nonrelativistic Hamiltonian (i.e., the energy operator) used by electronic wave function. The terms, small and large quantum chemists. component, result from the fact that the amplitudes The Dirac (D) Hamiltonian37,38 includes of the former are much smaller than those of the Einstein’s mass velocity effect in its Lorentz latter, as seen by invariant and quantized form and the corresponding eigenvalue equation for an H-like ion leads to Z S ≈ L (3) eigenfunctions in the form of 4-component vectors, 2mc which are called bi-spinors, that is functions comprising two spinors (2-component vectors) with In the case of one-electron atoms, the hydrogen wave the latter being the relativistic counterparts of the function, L ≈ exp(−Zr) can be used. One of the

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Continuum states Here, σ collects the Pauli matrices and p is the linear momentum vector. The kinetic balance condition (4)

Electrons guarantees that the kinetic energy is properly described 42,43 2 in the nonrelativistic limit. The momentum mc 0 Discrete states operator p on the right side of Eq. (4) implies that the small component basis set must contain functions Relativistic Non-relativistic which are derivatives of the large-component basis 0 functions. Basis sets which do not fulfill the kinetic balance condition can lead in a variational DHF −mc2 −2mc2 calculation to energies below the boundary condition Positrons and thereby to a variational collapse. Continuum states Another problem of the DHF method is that with the use of finite basis sets, positronic eigenvalues significantly above the limit − 2mc2 can be obtained, | FIGURE 1 Schematic illustration of positive and negative thus causing an inverse variational collapse and an eigenvalues obtained by DHF calculations. Besides the discrete unreliable total energy.44,45 Contrary to variational electronic energy levels for bound states, there is a negative (positronic) collapse, which has to do with the kinetic balance and positive (electronic) continuum at −mc2 and +mc2, respectively (left side). To simplify a comparison with nonrelativistic calculations, the problem, inverse variational collapse results from the rest mass of the electron is subtracted in the D-Hamiltonian, which finite precision of computer algorithms in the case of corresponds to a shift by mc2 so that the discrete electron energies basis functions that are very steep in the vicinity of a become negative (right side). nucleus. This problem can be solved by increasing the precision of computer algorithms.44 Apart from these effects of the small component is that the relativistic problems, it is typical of relativistic descriptions that spinors differ significantly from the nonrelativistic they require more often (than nonrelativistic ones) a spin-orbitals as they do not have nodal surfaces. multireference treatment, which is a result of SOC Since the DHF equations are solved for both included into the DC-Hamiltonian. the electronic and the positronic eigenstates, the Hence, solving the DHF equations (or similarly energy of the former no longer corresponds to a the Dirac-Kohn-Sham equations of relativistic density global minimum. Numerical problems in the form functional theory (DFT)) leads to a number of of variational or inverse variational collapse may computational problems, which are enhanced by the occur. The D-Hamiltonian37,38 is not bounded from need for complex computer algebra caused by the spin below, and therefore a variational procedure of a 4- terms in the D-Hamiltonian. Apart from this, a post- component wave function can lead to a variational DHF treatment for electron correlation may suffer collapse, i.e., E →−∞. In atomic calculations at from the Brown-Ravenhall disease,46 which originates the single-configuration DHF level using numerical from the fact that for any perturbational solution methods for the radial functions,2,30 no particular one must include the negative energy eigenstates. problems arise. The boundary conditions at the origin Hence, all two-electron states with one electron at 2 and at infinity keep the solutions electron-like. As E1 < − 2mc and the other having a positive energy E2 soon as electron correlation is introduced, e.g., by are degenerate (because of the large gap of 2mc2) thus employing a multiconfigurational DHF approach, causing a breakdown of perturbation theory. Sucher47 projection operators onto the electronic states have has described this problem as continuum dissolution to be used to avoid dissolution into the negative because in the two-electron system a transition energy-continuum. At the DHF level, provided that becomes possible which ejects one electron into the prerequisites of the kinetic balance are fulfilled, a the positive continuum. The continuum dissolution boundary can be established via the nonrelativistic applies to both the DC and the DCB Hamiltonian. energy and the first-order relativistic perturbation When solving chemical problems, only the correction to the energy evaluated with the large- positive (electronic) eigenstates and the positive component wave function.1 This implies the use of continuum of the DC-Hamiltonian are of relevance, a kinetically balanced basis set42,43 where the small- and therefore modern relativistic quantum chemistry component basis functions must be chosen according is based on no-pair Hamiltonians, i.e., a relativistic to the requirement (4) description that excludes electron–positron pair-   creations that become possible when the negative σ · p 1 χ S = χ L (4) eigenstates are included. This is in line with μ 2mc μ the necessity of simplifying the Dirac 4-component

© 2014 John Wiley & Sons, Ltd. WIREs Computational Molecular Science Dirac-exact relativistic methods calculations so that larger molecules can be normalization of the wave function is carried out investigated. Already early attempts focused on at infinite order and which therefore was dubbed eliminating the small component S,causedbythe (rather misleading) IORA (Infinite Order Regular positronic states, from the wave function. This can be Approximation).60 Hence, ZORA and IORA are done in an exact way for a free electron utilizing based on the same Hamiltonian but use different the Foldy-Wouthuysen transformation, which is wave function metrics. Originally, ZORA and IORA based on a series of unitary transformations suffered from three serious shortcomings: (1) The of the D-Hamiltonian.48 For bound electrons in relativistic one-electron integrals of ZORA (IORA) atoms or molecules, however, the Foldy-Wouthuysen could only be obtained using numeric quadratures, transformation can only be approximated or replaced which hampered an extension of these methods by other techniques. In the 1980s and 1990s, beyond the DFT realm; (2) ZORA (IORA) results perturbation theory was preferentially employed to suffered from an electrostatic gage-dependence, i.e., obtain quasi-relativistic approximations with two- or they depended on where the zero of the potential is just one-component wave functions, where the latter chosen; and (3) it was not clear how in a simple and corresponded to a spin-free description.1 economical way the RA methods could be improved The basic idea of the quasi-relativistic methods so that a Dirac-exact relativistic result would become is to approximate the Foldy-Wouthuysen transforma- available. tion by expanding it in powers of V (nucleus–electron Some of the shortcomings of ZORA and attraction potential) or in powers of IORA were overcome by Filatov and Cremer, who developed matrix representations of the ZORA and  61–64 (5) IORA Hamiltonians, derived their relationship 2 − 2mc V to an exact quasi-relativistic Hamiltonian,65 and solved the gage-dependence problem of ZORA and where  is the energy of the one-particle Dirac IORA.66 Although only low orders of the RA were equation. The former approach was pursued by implemented, the development of the latter had an Douglas and Kroll in 197449 and, later in the important impact on the derivation of a Dirac- 1980s and 1990s, extended by Hess so that low exact relativistic method applicable to large molecules orders n of the so-called Douglas-Kroll-Hess (DKH) containing relativistic atoms.65,67 Other approximate method could be developed.50–53 As in the case quasi-relativistic methods were developed, which are of the Foldy-Wouthuysen transformation, the DKH described in the relevant literature.1–3,9,10,12–14 transformation cannot be given in closed form and accordingly requires a number of transformations ··· U0, U1, thus leading to a decoupling of the DIRAC-EXACT RELATIVISTIC electronic from the positronic states and with each METHODS transformation to increasing accuracy. When however higher orders of the DKH method54,55 are worked By definition a Dirac-exact relativistic method is a out, it becomes obvious that the DKHn theory quasi-relativistic 2- or 1-component method which (DKH of order n) suffers from slow convergence and exactly reproduces the one-electron energies of the mathematical complexity. original 4-component Dirac method,37,38 where the These convergence problems are not experienced starting wave function can be of the HF or KS when using a perturbation expansion in terms type. In the following, we will speak of Dirac- of expression (5), which is the basis of the so- exact methods without emphasizing always their called Regular Approximation (RA) to the relativistic quasi-relativistic nature. It is desirable to develop a Hamiltonian and which provides rapid convergence Dirac-exact relativistic method in such a way that to the Dirac one-electron energy.56 However, the it can be smoothly integrated in the toolbox of RA suffers from technical problems due to the nonrelativistic theory. This concerns the use of (1) fact that the potential energy V appears in the correlation methods for determining dynamic and denominator of (5). Originally, the methods based nondynamic electron correlation; (2) methods and on the RA were formulated by Baerends and co- techniques of calculating response properties; and (3) workers57–59 on numeric quadratures in connection methods to describe excited states. with density functional theory (DFT) in the form As pointed out in the previous section, one of the of the zero-order regular approximation (ZORA) major objectives pursued during the last 15 years in and the first-order regular approximation (FORA) relativistic quantum chemistry was the derivation of method. An improvement of ZORA was obtained Dirac-exact relativistic methods which do not require by developing an approach for which the relativistic the solution of Dirac’s 4-component equation.37,38

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This objective was first achieved by Dyall,68 who this regard an important improvement of DKH developed the NESC method as the first Dirac- and represented a Dirac-exact method. exact 2-component relativistic approach. With NESC, • In the years 2005–2007, Kutzelnigg and Liu Dyall accomplished two objectives. First, he projected classified quasi-relativistic methods as being 37 the exact relativistic one-electron D-Hamiltonian operator-based or matrix-based and pointed onto the positive-energy (electronic) states to get a out in this connection that the latter lead in Dirac-exact 2-component representation. Second, he a much easier way to Dirac-exact relativistic separated the spin part of the D-Hamiltonian to obtain descriptions.45,76,77 These authors established a 1-component, spin-free representation. the basic requirements for exact 2-component NESC requires just one transformation matrix relativistic methods, for which the term X2C U to eliminate the small component and accordingly was coined.78 only one Fock matrix F, which however was originally • In the same time period, the Infinite-Order calculated in an iterative manner where for each  Two-Component (IOTC) method, which was iteration step a new relativistic metric S hadtobe originally developed by Barysz et al.79 using determined (because of its dependence on U,see operator algebra and which had already been below). In his 1997 publication, Dyall calculated 80 83 + extensively used, – was converted into matrix only the one-electron Ne9 ion, however, the algebra by Iliasˇ and co-workers.84 Iliasandˇ corresponding results revealed already the advantages Saue85 and Barysz et al.86 demonstrated that of the NESC method compared to perturbative IOTC also provides Dirac-exact energies. approaches such as DKHn or ZORA (IORA).68 • 87 Dyall based his development on two-important In 2006, Filatov emphasized that Dyall’s 2- 68 innovations: (1) He introduced a matrix representa- component NESC method fulfills the criteria tion of the Dirac equation. This was a novel approach of an exact X2C method and therefore its because most previous development work had focused practical realization, accomplished in the year on an operator presentation of the effects of relativity. 2007 by introducing a new iterative algorithm for 88 By switching to a matrix presentation, he implicitly solving the NESC equations, was considered introduced a description of the relativistic problem by as making X2C calculations generally available. 89 a finite basis set with all the problems accompany- Kutzelnigg and Liu identified NESC also as ing such a step (basis set truncation error, singularity an X2C method, but criticized the unnormalized problem at the point-nucleus, etc.). However, writ- version of NESC (UESC), which had also been 68 ing the Dirac equation in matrix form proved to be discussed in Dyall’s original NESC paper. This essential for an elimination of the small component. was relevant in connection with ZORA, which (2) He rewrote the Dirac equation and obtained what can be considered as an UESC-ZORA method, is known today as the modified Dirac equation.1,68 whereas IORA corresponds to a NESC-ZORA Steps (1) and (2) were important for deriving the method as had been pointed out by Filatov and NESC equations. Cremer.67 Dyall’s work triggered in the following years a • In 2011, the computational difficulties still number of developments, which led to a number of accompanying the solution of the NESC Dirac-exact relativistic methods that could routinely equations were finally solved by Zou, Filatov and be applied for the relativistic quantum chemical Cremer (ZFC),44 which made obsolete the atom- description of large molecules and their properties: centered approximation to NESC developed by Dyall and Enevoldsen,69 the iterative approach • In the years 1999–2002, Dyall simplified the by Filatov and Dyall,88 and the early low- solution of the NESC equations by fixing the order NESC approximations of Filatov and ratio of the large to the small component Cremer.90,91 Part of the success of ZFC44 was (and thereby matrix U) in atomic calculations, based on the use of IORA as a convenient thus yielding approximate NESC energies but starting point for an iterative solution of the effectively reducing the calculational load of the NESC equations.67 69,70 NESC description for molecules. • In the following years, ZFC converted NESC to • From 2002 on, Wolf et al. mastered the a generally applicable method44 that can be used problems of high-order DKHn calculations by for the routine calculation of first-order response developing an infinite order DKHn theory, properties (molecular geometries,92–94 electric which reproduced exact 4-component Dirac dipole moment,95 electric field gradients,96 energies.71–75 The infinite order theory offered in hyperfine structure constants,97 contact densities

© 2014 John Wiley & Sons, Ltd. WIREs Computational Molecular Science Dirac-exact relativistic methods

98 and Mossbauer¨ shifts, etc.) and second-order Here, matrices A and B collect the eigenvectors 95,99 response properties (vibrational frequencies, of the large and pseudo-large component (with 95 95 electric polarizabilities, infrared intensities, subscript p: positronic; without: electronic). They are etc.) related via the matrix U according to Eq. (8.68) • Parallel and independently, Gauss and Cheng developed methods to calculate molecular B = UA (8) geometries, vibrational frequencies, and mag- netic properties at the level of Dirac-exact In Eq. (7), Ep and E denote the positronic (negative) methods.100–102 and electronic (positive) eigenvalues, respectively. • In 2013, Filatov, Zou, and Cremer (FZC) Matrices T, V,andS correspond to the nonrelativistic extended the spin-free 1-component NESC kinetic energy, potential energy (nucleus–electron method to a 2-component method to calculate attraction), and overlap matrix, respectively. W SOC effects.103 is the negative definite matrix of the operator (1/4m2c2)σ · pV(r)σ · p, which simplifies in the scalar relativistic approximation to (1/4m2c2)∇V(r) ·∇ and In the following, we will focus on the description which can be easily derived from the derivatives of the of these last steps and in this way present an potential energy integrals. updated account on the applicability of Dirac-exact The elimination of the small component via the methods such as NESC. In this connection, we will pseudo-large component is the key for deriving the consider first the spin-free approach, which includes NESC equation, which can be written in the simple only scalar relativistic effects and in a later section form68 also the 2-component NESC method. In view of the accomplishments of Dyall in connection with Dirac-  LA = SA (9) exact relativistic methods, we stick to the acronym NESC rather than using the acronym X2C (for an Here, L is the matrix of the NESC Hamiltonian,  exact 2-component method), which is preferred by is the diagonal matrix of the NESC eigenvalues, A some authors, however, sometimes indiscriminately has been defined in connection with Eq. (7), and the for 1- and 2-component methods.  relativistic metric S is given by

THE NESC EIGENVALUE PROBLEM  = + 1 † S S 2 U TU (10) AND ITS SOLUTION 2mc Dyall’s derivation of a spin-free NESC equation68 The eigenvectors of the large component are is based on the no-pair approximation (which normalized on the relativistic metric according to guarantees that negative eigenstates do not intrude the † = space of the positive eigenstates1,3) and the definition A SA I (11) of a pseudo-large component of the wave function, L, The NESC Hamiltonian matrix is given by for the purpose of eliminating the small component:    = + † − † ( − ) + 2mcS = σ · p L (6) L TU U T U T W U V (12)   Equation 6 is not unique, but has the advantage which shows that both L and S depend on matrix U,  of making the relativistic metric S spin-free.1 This i.e., the matrix of the small component elimination simplifies the partitioning of the D-Hamiltonian operator. The calculation of U is the key problem of 68 into spin-free and a spin-dependent part (the latter solving the NESC equation. Work by Dyall, Filatov 67 88 44 describing the SOC effects), which was first discussed and Cremer, Filatov and Dyall, and ZFC has by Kutzelnigg104 and later by Dyall.105 stepwise improved the solution of this problem where 60,67 The modified Dirac equation in matrix notation in all cases the IORA solution is taken as the takes the form starting point for the calculation of U.   IORA IORA IORA IORA IORA VT Ap A L A = S A  (13) TW− T Bp B    S0 Ap A Ep 0 IORA =  − (7) Here, the matrix of the IORA Hamiltonian L 2 1  0 2mc T Bp B 0E and the IORA metric SIORA are obtained with

© 2014 John Wiley & Sons, Ltd. Advanced Review wires.wiley.com/wcms the help of Eq. (14,67) = −1 − − Z SS L V (19) UIORA = (T − W) 1 T (14)  1 − S = S + Z†T 1Z, (20) and by inserting UIORA into the IORA-equivalent of 2mc2 Eqs (12) and (10). Because W is a negative definite matrix (see above), Eq. (14) does not diverge. It has By applying a fixed-point iteration with a damping 44 been shown by ZFC that matrix U can be expressed parameter α according to IORA 44 via U as − − − Z(n) = f Z(n 1) − α f Z(n 1) − Z(n 1) (21) 1 − U = UIORA I − US 1 (TU + V) (15) 2mc2 first the product TU and then, with the help of the known matrix T, U was determined. Convergence This is the key equation for determining U by either a was monitored by comparing the absolute differences one-step or an iterative method. in the diagonal elements of the NESC Hamiltonian matrix (18) from successive iterations. Solution of the NESC Equation Via Comparison of the one-step and iterative method the Riccati Equation: The One-Step Method revealed that the former is of advantage in energy calculations with less than 1000 basis functions, The one-step method was first suggested by Dyall68 45,81,85 whereas the latter reduces computational costs for and later used by other authors. The method is large basis set calculations, geometry optimizations, based on the fact that Eq. (15) can be rewritten in the and reaction path calculations.44 form  − 1 − 1 U S 1T U + UIORA U Renormalization of the Wave Function: The 2mc2  Picture-Change 1 − The NESC equation provides the Dirac-exact solution + U S 1V − I = 0 (16) 2mc2 of the one-electron problem. In the context of the DC- Hamiltonian for many-electron systems, the NESC which corresponds to a nonsymmetric algebraic one-electron Hamiltonian can be combined with Riccati equation:106 the nonrelativistic two-electron part, which leads to the so-called one-electron approximation.70,107 UαU + βU + Uγ + δ = 0 (17) This implies, however, that the one-electron NESC Hamiltonian is renormalized on the nonrelativistic where α, β, γ ,andδ are known matrices. Using metric with the help of a renormalization matrix standard procedures, the unknown matrix U can G:70,107 be determined.106 This implies the transformation † of the M-dimensional quadratic equation into the H1−e = G LG (22) 2 M-dimensional matrices of the Dirac equation (7). Solving Eq. (7) by diagonalization provides all needed Equation (22) guarantees that H1 − e (set up in the eigenvalues and eigenvectors. Then, the matrix U is relativistic picture) can be applied in connection with directly determined with the help of Eq. (8). Once U the HF or KS equations (defined in a nonrelativistic   is known, the NESC matrices S and L can be obtained picture). This picture-change caused by switching from Eqs. (10) and (12). from the relativistic Dirac–Pauli representation to the nonrelativistic Newton–Wigner representation is Iterative Solution of the NESC Equation: correctly handled by a renormalization matrix G derived by Liu and Peng,78 The TU Algorithm  Since the calculation of matrix L depends on U − − 1/2 G = S 1/2 S1/2S 1S1/2 S1/2 (23) and that of U on L, an iterative determination of the former becomes obvious. Starting from Eq. (15), ZFC44 expanded L in terms of Z = TU thus yielding Picture change effects may not be large for relative energies (dominated by the properties of the − − − valence electrons), but become large when properties L = Z + Z† − Z† T 1 − T 1WT 1 Z + V (18) depending on a close distance from the nucleus have

© 2014 John Wiley & Sons, Ltd. WIREs Computational Molecular Science Dirac-exact relativistic methods to be determined. The total electronic energy at the a spherically symmetric charge distribution, which HF level is given by Eq. (24), can be represented by a Gaussian-type function110,111 according to = + 1 −  E tr [PH1−e] tr [P (J K)] (24) 3/2 2 1 − 2 2 ρ (r) = Z e r /ζ (25) A A πζ2 where J and K are the Coulomb and the exchange parts of the Fock matrix and P is the density Using the function of Eq. (25), the electron-nuclear matrix calculated as P = CnC† with C collecting the interaction potential v(r − RK)(RK: position vector of eigenvectors of the Fock matrix and n being the nucleus K) is given by Eq. (26) diagonal matrix of the orbital occupation numbers.  | − | − =− 1 r RK v (r RK) | − |erf (26) First-Diagonalize-Then-Contract Strategy r RK ζK When using a basis with a sufficiently large number where erf is the error function and ζ K is introduced as of primitive Gaussian functions Mp,theexact a parameter, which can be derived from the measured solutions of the Dirac equation for one electron can 1/2 root mean square (rms) charge radius R2 of be reproduced with sufficient accuracy.44,68,107 For K nucleus K using Eq. (27): many-electron systems, use of a large number of primitive basis functions leads to an M4 increase    p 1/2 = 2 2 in the number of two-electron integrals and high ζK RK (27) computational cost. Cost reduction is achieved in 3 these cases by using contracted basis sets (Mc basis The Coulomb potential of a point-charge model of << functions with Mc Mp). For the purpose of the nucleus used in nonrelativistic quantum chemistry solving this dichotomy, the following procedure was is recovered by setting ζ = 0. New molecular used by ZFC:44 The NESC one-electron equations K integrals of the type χ μ|v(r − RK)|χ ν have to were solved in the basis set of Mp primitive be calculated, which however does not pose any basis functions and the renormalized one-electron problem.44 Hamiltonian (22) was converted to a contracted Of course, the assumption of a Gaussian charge basis set with Mc functions. This First-Diagonalize- 44 distribution and the determination of the exponent of then-Contract strategy has some advantages: (1) the corresponding Gaussian function via the measured The completeness requirement is better fulfilled; (2) root-mean square radius of the nucleus110,111 can Computational costs are not significantly increased only be considered as an approximation since the to those of a nonrelativistic HF or KS calculation; exact charge distribution in the nucleus is not known. (3) variational collapse that can emerge when using 112 108 For example, the Zemach radius of a nucleus, strongly contracted basis functions no longer i.e., the magnetic nuclear radius, is more appropriate occurs; and (4) inverse variational collapse problems, when calculating magnetic properties. In any case, which may occur when using uncontracted basis sets use of a finite nuclear model leads to relatively with very steep basis functions, can easily be handled large changes in the total energy, whereas properties by using a finite nucleus model. depending preferentially on the valence electrons (e.g., bond lengths, vibrational frequencies) do not 92,99 The Finite Nucleus Model change significantly. In the case of a nonrelativistic treatment, the orbitals have a cusp at the position of a point Comparison of NESC Energies charge nucleus, which for a relativistic treatment with 4-Component Dirac Results converts into a singularity. The latter is difficult In Table 1, NESC Hartree-Fock (HF) energies of to describe with a basis set comprising Gaussian- hydrogen-like ions with atomic numbers Z = 20, 40, type functions. By introducing a nuclear model ..., 120 are compared with those of 4-component with a finite size of the nucleus, the singularity is DHF and quasi-relativistic calculations.44 NESC removed, thus leading to a better description of reproduces the 4-component DHF atomic energies in the region close to the nucleus. Although the finite all cases, which confirms that NESC is a Dirac-exact size nucleus has a charge distribution closer to a relativistic method. Fermi-Dirac distribution (a liquid drop with a diffuse Perturbational approaches such as DKHn or surface),109 one assumes, because of practical reasons, RA-based methods, which do not provide an upper

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TABLE 1 Ground State Energies (in Hartree) of Hydrogen-Like Ions Calculated with Different 4-Component (4c) and 1-Component Relativistic Methods Method Z = 20 40 60 80 100 120 Point charge nuclear model with 50 s-functions1 4c-DHF(UKB) −201.076522 −817.807491 −1895.68234 −3532.19213 −5939.19514 −9710.71531 NESC −201.076522 −817.807491 −1895.68234 −3532.19213 −5939.19514 −9710.71531 Approximate methods ZORA67 −202.158829 −836.011368 −1996.45087 −3898.86916 −7054.8079 −13096.9617 IORA67 −201.082194 −818.171957 −1899.90000 −3536.90102 −6042.5850 −10089.4142 NESC-SORA67 −201.076522 −817.807633 −1895.68972 −3532.31224 −5940.2749 −9718.0099 DKH274 −201.072540 −817.615780 −1893.89769 −3523.32490 −5906.1919 −9594.1000 DKH374 −201.076662 −817.820117 −1895.84407 −3533.11958 −5942.3695 −9712.9340 DKH1474 −201.076523 −817.807497 −1895.68235 −3532.19184 −5939.1821 −9710.2510 Finite nuclear model with 50 s-functions2 4c-DHF(UKB) −201.076001 −817.788172 −1895.45071 −3530.19419 −5922.78995 −9545.87512 NESC −201.076001 −817.788172 −1895.45071 −3530.19419 −5922.78995 −9545.87512

1UKB: unrestricted kinetic balance. See Ref 44. 2Ref 44. Mass number of was taken from Ref 111. For Z = 120, mass number = 2.556 × Z = 306.72. bound to the correct DHF energy, approach the exact FIRST-ORDER RESPONSE PROPERTIES results in an oscillatory manner, overestimating or The usefulness of a new quantum chemical method is underestimating exact atomic energies. This is also measured by its accuracy and general applicability. reflected by the data in Table 1. For Z ≤ 60, DKHn General applicability implies the possibility of atomic energies with n = 14 are close to the exact routinely calculating molecular properties such values, whereas for Z > 60, one has to apply DKHn as geometries, vibrational frequencies, electric or with n > 20 to obtain accurate values. Infinite order magnetic quantities, excitation energies, etc. A large DKH theory correctly reproduces DHF (and NESC) number of molecular properties needed by chemists energies. However, it becomes also obvious that to analyze and characterize structure, stability, and convergence of the DKHn energies to the correct 44 reactivity of a chemical compound are response result is rather slow. properties, which can be effectively calculated with the Methods based on the RA converge much faster, help of analytical energy derivatives.113 Accordingly, but largely overshoot exact results at the ZORA and the usefulness of a quantum mechanical method IORA levels of theory. The development of a matrix increases substantially when its applicability range formulation for the methods based on the RA by is extended by the introduction of analytical energy Filatov and Cremer made it possible to consider derivatives. second- and third-order IORA methods65 and to connect the RA directly to NESC, for example, via the NESC-SORA (second-order regular approximation) Derivation of the NESC Gradient method. NESC-SORA provides exact results for small The first derivative of the total energy, Z, whereas for larger Z its energies again overshoot Eq. (24), with respect to a parameter λ, exact DHF energies. which can correspond to a nuclear coordi- As mentioned before, the relativistic calculations nate or a component of the electric field benefit from a finite nucleus model rather than a or another external perurbation, is given by 1,44,111 0-radius (point charge) model. For example, Eq. (28)114 the singularity of the Dirac equation at the position of the nucleus caused by the point charge model is ∂E ∂S ∂H − 1 ∂ avoided. The increase in energy as described by the = tr  + tr P 1 e + tr P (J − K) 4-component DHF method is correctly reproduced ∂λ ∂λ ∂λ 2 ∂λ by the NESC method (Table 1). (28)

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Here, matrix  is defined by  =−CnC†,andthe the partial derivative of U with regard to λ is obtained prime at ∂ /∂λ implies that only the two-electron as integrals rather than the density matrix need to be ∂U ∂UIORA −1 1 differentiated. The first and the last term on the = UIORA U − UIORA ∂λ ∂λ 2mc2 right hand side (r.h.s.) are calculated utilizing the −1 nonrelativistic methodology. Only the second term ∂U − ∂S × S 1 (TU + V) + U (TU + V) has to be determined in a NESC gradient calculation. ∂λ ∂λ This was first done by ZFC92 and somewhat later by  100 − ∂T ∂U ∂V Cheng and Gauss. +US 1 U + T + (33) The second term in Eq. (28) has the form92 ∂λ ∂λ ∂λ    † ∂H1−e ∂L ∂G ∂G This equation can be brought in the form of the tr P = tr P + tr D + tr D† ∂λ ∂λ ∂λ ∂λ Sylvester equation.92,99 (29) Solution of the Gradient Problem Via  = † =  where the new matrices P GPG and D LGP the Sylvester Equation: The One-Step are introduced. Hence, the derivative of the NESC Hamiltonian matrix L and the renormalization Method 99 matrix G are required for calculating the NESC The Sylvester equation has the form energy gradient. For the first term in Eq. (29), one + = obtains: AX XB C (34)   99 ∂L ∂T If matrix X contains the derivatives ∂U/∂λ,then tr P = tr UP +PU† − UPU† ∂λ ∂λ − 1 − A = I − T 1W + US 1T (35) ∂W ∂V 2mc2 + tr UPU† + tr P ∂λ ∂λ 1 − † ∂U† ∂U B = S 1 (TU + V) (36) + tr PL + PL (30) 2mc2 ∂λ ∂λ

  − ∂T − − ∂W where PL = P T − U† (T − W) . The calculation of C =−T 1 T 1WU + T 1 U ∂λ ∂λ the first three terms on the r.h.s. of Eq. (30) 1 − ∂S − ∂T ∂V is straightforward because the one-electron integral + US 1 S 1 (TU + V) − U − derivatives are directly available from nonrelativistic 2mc2 ∂λ ∂λ ∂λ quantum chemical methods. The major difficulty (37) results from term four, which contains the derivatives ∂U/∂λ.TheU derivatives also appear in ∂G/∂λbecause Depending on what response properties are required,   G depends on S and S on U (see Eqs 23 and the Sylvester equation can be solved in a one-step 10). procedure or by an iterative procedure according to By collecting all contributions ∂U/∂λ from L and − − 92 = 1 − 1 G, one obtains a relatively simple equation: Xn+1 A C A XnB (38)   ∂U † ∂U† ∂U† ∂U The latter is the method of choice, e.g., for geom- tr PL + PL +tr PG U+PGU† ∂λ ∂λ ∂λ ∂λ etry optimizations. However, for higher accuracy,  especially in the case of very steep basis functions † ∂U † ∂U (exponents |ζ| > 1012) and a point-nucleus model the = tr P0 + P (31) ∂λ 0 ∂λ eigenvalue decomposition method is preferable, which is more costly, but numerically more stable. The latter where matrices PG and PL have been defined in the method has been used by several authors63,101,115 and original literature.92 By writing Eq. (15) in the form was also applied by ZFC.99 For high accuracy calculations which are 1 − U = UIORA − UIORAUS 1 (TU + V) (32) required, e.g., when determining contact densities 2mc2 (see below), a more efficient method is based on

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response theory. For this purpose, ZFC rewrote the of Be = UAe, one obtains Dirac equation in the following form:99 ∂ U = λ − λ † ˜ BpOpe UApOpe Ae S (50) D˜ = S˜  (39) ∂λ which can be directly calculated. Cheng and Gauss101 with neglected the contributions of the positronic wave  function and kept only the last part of Eqs. (48) ˜ = VT D − (40) and (49). ZFC correctly included the positronic TW T contributions and derived the full equation of the  matrix Uλ.99 ˜ S0  Another important improvement of the calcula- S = −1 (41) 0 2mc2 T tion of the NESC gradient according to the procedure 92,99  given by ZFC resulted from the fact that these authors formulated the NESC first derivatives exclu- = Ap A (42) sively via traces of matrix products, in which the Bp B matrices of integral derivatives are contracted with  precomputed square matrices. This saves time and E 0  = p (43) disc space, as one does not need to recalculate the 0E molecular integral derivatives or store them on disk. In particular, all terms of the first derivative of G Differentiation with respect to λ leads to and U were expressed in the form of traces of matrix products, which is more efficient compared to a term- D˜ λ + D˜ λ = S˜ λ + S˜λ  + S˜ λ (44) by-term calculation and a final contraction of these terms with the respective integral derivatives. which can be simplified by multiplication with † from the left and using the normalization condition NESC Calculations of Atomic Forces: † ˜ S = I to obtain Molecular Geometries ZFC92 used the analytical NESC energy gradient † ˜ λ + † ˜ λ = † ˜ λ + † ˜λ + λ D D S  S   . (45) to determine molecular geometries. These authors found that only in the case of bond lengths between λ Introducing the matrix O that describes the first- relativistic atoms an accurate account of the gradient order orbital response with respect to perturbation of matrix U based on response theory is required, λ whereas in other cases an approximate calculation of ∂U/∂λ is sufficient.44 These authors calculated λ = λ O , (46) NESC/CCSD geometries for Hg-containing molecules and NESC/CCSD(T) bond dissociation energies (BDE) and performing some mathematical rearrangements, at NESC/CCSD geometries. 99 one obtains NESC/CCSD geometries were found to be reasonably close to experimental geometries (see HgCl λ − λ + λ = † ˜ λ − † ˜λ O  O  D S  (47) and HgBr in Table 2). However, a final judgment on the accuracy of the NESC calculations could not be λ from which the matrix elements of O can be derived. made because the influence of SOC on the bond ZFC showed that the response of the large and small length was not considered in their work.44 Compared components of the electronic states causes a mixing to other calculated values, NESC HgX bond lengths with the positronic states according to turned out to be closer to the experimental ones with deviations being smaller than 0.1 A.˚ 44 The λ = λ + λ = λ + λ A ApO2 AO4 ApOpe AeOee (48) agreement between NESC/CCSD(T) and experimental bond dissociation enthalpies (BDH) D0 for mercury halides was excellent in view of a mean deviation of λ = λ + λ = λ + λ −1 92 B BpO2 BO4 BpOpe BeOee (49) just 0.3 kcal mol . A number of studies have been published since where the subscripts e (electronic) and p (positronic) then, which confirm the reliability of NESC geometries have been used to simplify the identification of mixed either in connection with DFT or coupled cluster positronic–electronic contributions. By differentiation theory.93–99

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1 TABLE 2 NESC/CCSD Geometries and NESC/CCSD(T) Bond Dissociation Energies De (Enthalpies D0) of Mercury Molecules

Molecule Symmetry State Method Geometry Parameters De (D0) Reference 2 + HgF C∞v  NESC/CCSD(T)//NESC/CCSD 2.024 33.0 (32.3) 92 Expt. 32.9 116 2 + HgCl C∞v  NESC/CCSD(T)//NESC/CCSD 2.402 23.8 (23.4) 92 SOC/ECP/CCSD(T) 2.354 22.9 117 Expt. 2.395, 2.42 23.4, 24.6 118–120 2 + HgBr C∞v  NESC/CCSD(T)//NESC/CCSD 2.546 20.0 (17.5) 92 SOC/ECP/CCSD(T) 2.498 16.3 117 Expt. 2.62 17.2, 18.4 121–123 2 + HgI C∞v  NESC/CCSD(T)//NESC/CCSD 2.709 12.9 (7.6) 92 SOC/ECP/CCSD(T) 2.708 8.6 117 Expt. 2.81 7.8, 8.1, 8.9 119, 120, 124 2 + HgCN C∞v  NESC/CCSD(T)//NESC/CCSD Hg–C: 2.118, C–N: 1.161 36.1 92 IORA/QCISD Hg–C: 2.114, C–N: 1.179 28, 125 2 + HgNC C∞v  NESC/CCSD(T)//NESC/CCSD Hg–N: 2.077, N–C: 1.176 22.4 92 2 HgCH3 C3v A 1 NESC/CCSD(T)//NESC/CCSD Hg–C: 2.344, H–C: 1.084 3.2 92 Hg–C–H: 104.3

1From Ref 92. NESC/CCSD(T)//NESC/CCSD denotes NESC/CCSD(T) energies calculated at NESC/CCSD geometries. For HgX (X = F, Cl, Br, I), BDE values De include SOC corrections and are corrected by ZPE (zero-point energies) to yield D0 values. In the calculations of HgCH3, HgOCH3, and HgCF3,the − fourteen 4f-electrons of Hg were frozen. D values in kcal mol 1, bond lengths in A,˚ and angles in deg.

NESC Description of Molecular Density reveals how scalar relativistic effects lead to a change Distributions and Dipole Moments in the electron density distribution. For example, in The total electron density distribution ρ(r) at a point Figure 2 the NESC difference density distribution of the molecule HAt is shown. Around the astatine rP is the result of the response of a molecule to a perturbation λ that corresponds to the one-electron atom a somewhat distorted pattern of spherical  shells with density increase (red contour lines) and operator δ (rP − r), i.e., the Dirac delta operator. By using the Hellmann-Feynman theorem,126,127 one gets density depletion (blue lines) is recognizable. The  shell structure is a result of the s,p-orbital contraction    dE (λ) = | − | = and d,f-orbital expansion, which propagates from the   δ (rP r)  ρ (rP) (51) innermost core to the valence shell and which leads to dλ λ=0 a charge transfer from H to At. Because of the scalar When ρ(r) is expanded in terms of basis functions, Eq. relativistic effects the of At increases. (51) describes the response density: The NESC density matrix has to be available  when calculating NESC-based first-order response = ˜ ρ (rP) Pμνχμ (rP) χν (rP) (52) properties such as the molecular dipole moment μν or other electric multipole moments. In a static homogeneous electric field F , the potential V’(r) Using the definition of the NESC gradient, the NESC adopts the form response density matrix is given by P˜ = GPG† (see Eq. 29). Hence, the NESC electron density distribution ( ) = ( ) + · can be written in terms of a renormalized matrix P˜ V r V r F r (54) depending on P = CnC† where C is the matrix of the NESC orbital coefficients in the spin-free (scalar and the total molecular energy can be expressed in the relativistic) 1-component representation. Once P˜ is form of a Taylor expansion according to determined, the NESC electron density distribution ∂E (F ) can be calculated according to Eq. (52). E (F ) = E (0) + |F =0· F The difference density distribution ∂F 1 ∂2E (F ) NESC = NESC − non-relat + F · |F =0· F +··· (55) ρ (r) ρ (r) ρ (r) (53) 2 ∂F ∂F

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2 TABLE 3 NESC/CCSD(T) and NESC/PBE0 Dipole Moments of Diatomic Molecules in Their Ground State Compared with Other Theoretical Values.95 ˚ 1 Molecule State Method Re (A) μ (Debye) At AuF 1+ NESC/CCSD(T) 1 4.32 RECP/CCSD(T)/CBS128 1 4.37 0 H Expt.129,130 1.918 4.13 AuCl 1+ NESC/CCSD(T) 1 3.81 RECP/CCSD(T)/CBS128 1 3.90 −1 Expt.131 2.199 AuBr 1+ NESC/CCSD(T) 1 3.50 RECP/CCSD(T)/CBS128 1 3.48 −2 Unit: Å Expt.131 2.318 −2 −1 0 1 2 AuI 1+ NESC/CCSD(T) 1 3.16 FIGURE 2| Contourline diagram of the NESC difference density RECP/CCSD(T)/CBS128 1 2.94 distribution of the HAt molecule. red (dashed blue) contour lines Expt.131 2.506 indicate an increase (decrease) of the density because of scalar AuH 1+ NESC/PBE0 1.530 1.47 relativistic effects. The difference density adopts a shell structure at the 132 At atom, which is caused by sp contraction. The outer red sphere RECP/MP2 1.51 1.03 corresponds to the 6s6p shell and and the most inner red sphere to the Expt.116 1.524 overlapping 3s3p and 2s2p shells. The 1 s region cannot be seen HgH 2+ NESC/PBE0 1.747 0.37 because it is just 0.1 A˚ outside the At nucleus. NESC/PBE0 calculations. Expt. 133,134 1.741 0.47 HgF 2+ NESC/PBE0 2.039 3.69 The first-order term of the expansion gives the electric HgCl 2+ NESC/PBE0 2.403 3.84 dipole moment Expt.118 2.395

1Calculated at the experimental . The NESC/CCSD(T) bond ∂E (F ) = ˚ μ =− | = (56) lengths for AuX are: 1.922 (X F); 2.219 (Cl); 2.333 (Br); 2.482 A(I). ∂F F 0 where the scalar dipole moment is defined as the norm of the dipole moment vector μ =||μ||. Equation (58) reveals that the NESC dipole Hence, the derivative of the electronic energy moment can reliably be calculated by combining (24) has to be taken with regard to the components the nonrelativistic formula with the NESC density ˜ F α(α = x, y, z) of the electric field. The only matrix P. nonrelativistic contributions arise from V; however, In Table 3, NESC bond lengths and NESC for NESC contributions from W, G,andU (since G dipole moments of some diatomic Au- and Hg- depends on U,andU depends on V and W)alsoresult. containing molecules are listed together with the For component μα of the dipole moment one obtains: available experimental values. For the gold halides, NESC/CCSD(T) dipole moments (calculated at ∂ − ∂ =− H1 e =− † ˜ CCSD(T) and experimental bond lengths) are close to μα tr P tr P G LG 128 ∂Fα ∂Fα RECP/ CCSD(T)/CBS values, which were obtained   at the CCSD(T) level using experimental bond ∂L˜ ∂G† ∂G =−tr P˜ + tr D + D† (57) lengths, numerical derivatives, relativistic effective ∂Fα ∂Fα ∂Fα core potentials (RECPs), and aug-cc-pVnZ (n = 4,5) basis sets to extrapolate to the complete basis set ZFC95 analyzed the individual terms of Eq. (57) and (CBS) limit. NESC/CCSD(T) reproduces the results showed that, by eliminating small terms, it can be of the latter calculations within 0.1–0.2 Debye while simplified to requiring less than 10% of the computer time needed   for the RECP/CCSD(T)/CBS calculations. For a larger ˜ set of calculated dipole moments, ZFC95 found ˜ ∂L ˜ ∂V μα =−tr P =−tr P (58) that NESC predicts the experimental values with an ∂F ∂F α α accuracy of 0.2 Debye or better.

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NESC Hyperfine Structure Constants reliable values; and (3) relativity has to be taken into Atoms and molecules possessing unpaired electrons, account. i.e., radicals, are recognized by the hyperfine structure Filatov and Cremer125 demonstrated that useful (HFS) of their electron spin resonance (ESR) and HFS constants could be obtained with an open-shell optical spectra.135,136 The hyperfine structure of IORA formalism (for related relativistic investigations, the spectra arises from the interaction between the see also the work of the Baerends group or Malkin’s unpaired electrons and the magnetic field generated work137,138). In extension of their work, FZC97 by the magnetic moments of the nuclei with nonzero derived an approach for calculating HFS constants spin. A nonuniform magnetic field characterized by with the Dirac-exact NESC method starting either the magnetic induction B(r) and its associated vector from an unrestricted HF or unrestricted KS wave func- iso potential A (r) according to B (r) =∇×A (r) result tion. They obtained for AK the following equation: from the magnetic nuclei in the molecule. The vector iso =−  −1 potential is given by AK gegKμBμK Sz    ˜ σ FC 3 ˜ σ −1 FC FC −1 1 μ × (r − RK) × tr P H + P WT H +H T W ( ) = K T K,z W K,z K,z A r 2 3 (59) 4 c |r − RK| σ K −1 =−gegKμBμK Sz  where μK is the magnetic moment of the nucleus K at × ˜ s FC + 3 ˜ s −1 FC + FC −1 position RK. tr PTHK,z PW WT HK,z HK,zT W For radicals, the magnitude of the HFS constants 4 (62) AK obtained from the ESR spectra is related to the spin density distribution and therefore characteristic of the 135,136 FC electronic structure of a radical. These HFS In Eq. (62), HK,α is the matrix of the operator (60). constants can be quantum mechanically determined The constants ge, gK, μB,andμK are the electron and via the hyperfine tensor AK, which is given by the nuclear g-factors as well as the Bohr and nuclear derivative of the total energy with respect to the magnetons, respectively. The quantity Sz is the nuclear magnetic moment μK. Two contributions expectation value of the z-component of the electron ˜ σ ˜ σ result, which are determined by the so-called Fermi- spin. Matrices PT and PW are similarly defined as in contact operator and the spin-dipole operator: the closed shell case44 only that they refer in the open- ˜ s shell calculation to a specific spin σ. The matrices PT π ˜ s ˆ FC = 4 − and P are calculated by substituting the spin-density hK (r) δ (r RK) σˆα (60) W α 3c2 matrix Ps = Pα − Pβ in the respective expressions.97 The calculated relativistic corrections of the ˆ SD mercury HFS values can be as large as 15,000 MHz hK (r) α (HgF97) or, as in the case of the mercury cation, more · − − = 1 (σˆ (r RK)) (r RK)α − σˆα than 30,000 MHz (13,734 MHz at UHF compared 2 3 5 3 97 2c |r − RK| |r − RK| with 43,400 MHz obtained with NESC/UHF ). (61) Equally important is the inclusion of correlation effects, which is reflected by the NESC/QCISD and where α again denotes the Cartesian components of NESC/CCSD values given in Table 4.97 At this iso a vector. As a result of the molecular motion in the level of theory, AHg values are in good agreement gas and in solution, the anisotropic spin-dipole with experiment. With the exception of HgH and contribution averages to zero so that the isotropic HFS HgF molecules, the deviation of the calculated HFS iso constants AK are determined by the Fermi-contact constants from the corresponding experimental contributions associated with operators (60). value is within a few percent. Inclusion of electron For organic molecules, the measurement of HFS correlation leads to a contraction of the atomic inner constants is routine whereas it is still a challenge for shell electron spin-density toward the nucleus, thus radicals containing relativistic atoms. In the latter case, increasing the HFS constant.125 ForHgF,thisincrease the quantum chemical calculation of HFS constants is is counterbalanced by the increasing bond polarity, an important option provided three prerequisites are which withdraws spin-density from the 6 s-orbital fulfilled: (1) The wave function used must satisfy the of Hg, thus reducing the value of the HFS constant. Hellmann-Feynman theorem;126,127 (2) Correlation A delicate balance between these effects can only corrected ab initio methods or at least well-tuned be achieved by using correlated methods including XC-functionals of DFT methods are required to get connected 3-electron correlation effects.

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iso TABLE 4 Isotropic Hyperfine Structure Constants AHg (in MHz) of The interaction of the nuclear quadrupole the Mercury Atom in Hg-Containing Molecules Calculated at the moment (NQM) Qαβ with the EFG Vαβ at the site NESC/CCSD and NESC/QCISD Levels of Theory Compared with the of the nucleus is described by Eq. (63),144,152 97 Corresponding Experimental Values  ˆ int Molecule Exp. NESC/QCISD NESC/CCSD H = Qαβ Vαβ (63) HgH 68591;71982 7446 7463 α,β 3 HgF 22,163 20,929 20,558 where the summation is carried out with respect to HgCN 15,9604 15,948 16,135 the Cartesian components α, β. The NQM tensor 5 HgCH3 4921 5299 5428 components are given by:

HgCH2CH3 3504 3623  6 eQ 1     1 HgAg 2723 2967 2962 Qαβ = IαIβ + Iβ Iα − δαβ I (I + 1) 2I (2I − 1) 2 3 1Ref 139; measurement in Ne matrix. (64) 2Ref 139; Ar matrix. 3 Ref 140; Ar matrix. ˆ 4Ref 141; Ar matrix. where I and Iα are the nuclear spin and the nuclear 5Ref 142; Ne matrix. spin operator, respectively, and e is the elementary 6Ref 143. charge. For nuclei with I = 1/2, all components Qαβ of the NQM tensor vanish. Problematic in this connection is that measured For a given nucleus, the EFG operator is values are often obtained for molecules embedded defined as a second derivative of the electron–nucleus in inert gas matrices (see Table 4). As was pointed attraction operator V with regard to the Cartesian 125 out by Filatov and Cremer, the effect of the inert coordinates, gas matrix can change the HFS constant as much  as 6–10%. Reliable NESC constants obtained with ∂ ∂ 1 2  Vˆ αβ = − δαβ ∇ V (65) highly correlated methods and large basis sets could ∂xα ∂xβ 3 make it possible to determine these matrix effects. which describes the interactions of the nucleus in NESC Electric Field Gradients question with electrons and other nuclei in the molecule. It is convenient to define the principal An electric field gradient (EFG) at an axis system (by diagonalization of the Vαβ tensor), exists only if the charges surrounding the nucleus in which the axes a, b,andc are labeled in in question (i.e., the electron density distribution a way that the diagonal components Vaa, Vbb, and the other nuclei in a molecule) generate an | |≤| |≤| | and Vcc satisfy the relation Vaa Vbb Vcc . inhomogeneous electric field, which via its electric Then, the EFG tensor can be characterized by the field gradient provides a sensitive measure of the = 144 principal value Vcc and the asymmetry parameter η local electronic structure. The EFG can be accessed − (Vaa Vbb) /Vcc. In practice, the nuclear quadrupole via the nuclear quadrupole interaction that can be coupling constant (NQCC) ν 144,146,153 is used to measured by various experimental techniques includ- Q 145 interpret nuclear quadrupole resonance (NQR) and ing Mossbauer¨ spectroscopy, nuclear quadrupole Mossbauer¨ spectra:145,147 resonance spectroscopy,146,147 or perturbed angular correlations (PAC) of γ -ray spectroscopy.148 The eQ V ν = cc (66) interpretation of the experimental spectroscopic data Q h often requires high-level theoretical calculations to reveal the relationship between electronic structure Here, Vcc is the expectation value of the component 149 and measured nuclear quadrupole interactions. In Vcc in the ground state of the molecule. this connection, the same requirements apply as those The elements of the EFG tensor can be directly mentioned in connection with the analysis of the calculated as response properties. This is based on the HFS constants. For example, Pernpointner et al.150 fact that for any method satisfying the Hellmann- demonstrated the importance of including relativistic Feynman theorem,126,127 the expectation value of and electron correlation effects in the quantum an operator perturbing the Hamiltonian can be chemical calculations when computing reliable EFG determined by differentiating the total energy of the values for heavy atoms. This was confirmed by perturbed system with respect to the perturbation Arcisauskaite et al.151 in high-level 4-component parameter(s). In case of the NESC EFG at the calculations on a series of mercury compounds. position of nucleus K, one obtains the perturbed

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TABLE 5 Electric Field Gradients Vcc (in Atomic Units) Calculated NESC Quadrupole Coupling Constants for Hydrogen Halides HX (X = F, Cl, Br, I, At) Using the NESC/HF and and the Nuclear Volume NESC/MP2 Method with a Finite Size Nucleus Model1 A nonspherical distribution of the nuclear charge Molecule 4c-DC-HF2 NESC/HF NESC/MP2 leadstoanNQMQ.144 Although the NQM plays HF 2.809754 2.809268 2.554123 an important role in and molecular HCl 3.591314 3.590261 3.402235 spectroscopy, its direct experimental measurement is difficult and, currently, the most reliable way of its HBr 7.540289 7.536556 7.254653 determination is based on measurement of an NQCC HI 11.623332 11.620941 11.047529 νQ in connection with accurately calculated EFGs Vcc HAt 25.979844 26.506524 26.273005 (compare with Eq. 66):

1From Ref 96. 24-component Dirac–Coulomb Hartree–Fock calculations taken from Ref h 1 154. Q = νQ (69) e < Vcc > energy by adding the nuclear quadrupole interaction where in the case of diatomic molecules < Vcc >= operator (63) to the potential energy operator of < Vzz > with z corresponding to the molecular axis. the NESC Hamiltonian and then differentiating the The NQM and NQCC of two of the NESC K resulting total energy E Qαβ with respect to the same element with atomic number Z can differ. The components of NQM QK : molecular NQCC includes a number of contributions αβ which were analyzed in detail by Pyykko.¨ 155 Thus it

was predicted that, in molecules with closed electronic   NESC K ∂E Qαβ K = | shells, the variation of the nuclear volume in isotopes Vαβ K → K Qαβ 0 I1andI2 of a given element Z should lead to the ∂Qαβ emergence of a quadrupole anomaly I1I2,which,by  − 2 Z 3Xα,KLXβ,KL δαβ RKL analogy with the hyperfine anomaly, can be defined + ZL (67) R5 according to Eq. (70). L =K KL

ν (I1) where the second term on the r.h.s. represents the Q = QI1 +I1 I2 1 Z (70) nuclear–nuclear part of the EFG and Xα,KL are the νQ (I2) QI2 Cartesian components of the internuclear distance = − 96 vector RKL RK RL. According to FZC, the first FZC156 investigated the quadrupole anomaly by term on the r.h.s. of Eq. (67) is given by expanding the EFG of linear molecules at the position   of an isotopic nucleus I1 in terms of the rms nuclear NESC   ∂E Qαβ ∂V = = ˜ + + ( )† charge radius < RK > a: K tr P P0V P0V K ∂Qαβ ∂Qαβ   ˜ † † ∂W ν (I1) Vzz (a2) + (∂Vzz/∂a)|a=a (a1 − a2) + ... + + + ( ) Q = QI1 2 tr UPU P0W P0W K (68) ∂Q νQ (I2) QI2 Vzz (a2) αβ    ∂  = QI1 + 1 Vzz  + 2 ˜ 1  a12 O a12 (71) where matrices P, P0V,andP0W are obtained from QI2 Vzz ∂a = a a2 the usual molecular density matrix as described in Refs 92 and 97. Since no approximations are made in Eq. (68) the exact EFG is obtained.96 The derivatives in Eq. (68) are formulated entirely In Eq. (71), the rms nuclear charge radius is given in terms of traces of matrix products and the by a and the expansion is truncated at first order practical application of these formulae requires only in a in view of its small variation between different a fraction of the time needed, e.g., for a single HF isotopes. Thus, one can evaluate the magnitude of I1 I2 iteration. the quadrupole anomaly Z as the second term of FZC96 investigated a series of molecules and the expansion given in parentheses in Eq. (71). By I1 I2 found that with correlation corrected methods defining a relative quadrupole anomaly δZ as the I1 I2 such as NESC/MP2 (second-order Moller-Plesset difference between the Z values of two different perturbation) accurate EFG values were obtained (see molecules, M1andM2, they obtained an expression Table 5). that depended only on the EFG principal component

© 2014 John Wiley & Sons, Ltd. Advanced Review wires.wiley.com/wcms in the z-direction and its derivative with respect to shifts have been measured for samples containing iron a:156 (57Fe), (119Sn), zinc (67Zn), gold (197Au), mercury (199Hg and 201Hg), and many rare earth elements I1 I2 I1 I2 I1 I2 151 145,160–163 δ =  |M1 −  |M2 (e.g., Eu). Z Z Z    Upon absorbing the γ -radiation, the a-nucleus QI2 νQ (I1) νQ (I1) =  −  undergoes a γ -transition, which leads to a change Q ν (I2) ν (I2) I1 Q M1 Q M2 of the radius R of the a-nucleus and, by this, to a     change in the electron–nucleus attraction potential, 1 ∂Vzz ≈  164  which depends on Ra. Filatov suggested the use of Vzz ∂a = a a2 M1 linear response theory to calculate the isomer shift δ      (and ρ) as the electronic energy derivative with respect − 1 ∂Vzz   a12 (72) to the nuclear charge radius Ra of the a-nucleus: Vzz ∂a a=a 2 M2     a  s  c ∂E (R) ∂E (R) where a12 is the variation of the rms nuclear charge δ =  −  Ra (74) E ∂R ∂R radius between the isotopes I1andI2ofelementZ. γ R=Ra R=Ra The NESC/CCSD values of FZC for the 195 197 where Ea and Es denote the electronic energy of the relative quadrupole anomaly δAu for pairs of gold molecules reached values large enough to be reflected absorbing and source systems, respectively. by the measured  by NQCC  values. Thus, the NQCC A fully analytic approach for obtaining effective 195 197 ρ ratio νQ Au /νQ Au for AuCl referenced to contact densities within the linear response 79 79 98 other gold molecules gave the largest magnitude of formalism based on NESC was presented by FZC. the quadrupole anomaly, far above the precision of Assuming a nuclear charge distribution according to microwave spectroscopy, and by this provided a way Eq. (25), the nuclear attraction potential adopts the of measuring changes in the nuclear volume for a form given in Eq. (26), where the exponent ζ is related 195 197 = 111 to the nuclear charge radius Ra of the a-nucleus by Eq. variation from 79 Au to 79 Au (a 5.43439 fm ). (27). Utilizing these equations, the effective contact density is obtained as160,164 NESC Contact Densities and Mossbauer¨   Shifts 1 1 ∂E (ζ) ρ =  (75) a 2π Z ζ ∂ζ The Mossbauer¨ effect involves the recoil-free emission a ζ=ζ0 and absorption of γ -radiation by atomic nuclei 157 which are embedded in a solid environment. The in which ζ 0 is the value of the parameter obtained frequency of the resonant γ -radiation depends on from the experimentally measured rms charge radius the electronic environment of the resonating nucleus of the resonating nucleus a. The effective contact which is reflected by a frequency shift. To compensate density can be directly compared to the NESC for the corresponding frequency shift, the Doppler density calculated as the expectation value of the effect is used, which implies that the source of the γ - density operator and used in connection with Eq. radiation is accelerated through a range of velocities (73).98,160,164 until the resulting small energy shift reestablishes FZC98 calculated the derivatives of molecular the resonance condition for the absorbing nucleus. integrals with respect to the nuclear charge radius The isomer shift δ is a measure for the electronic or with respect to the parameter ζ of the Gaussian environment of the absorbing nucleus.158,159 It can be charge distribution given in Eq. (25), used the NESC expressed as response formalism for first-order properties, and   obtained the effective contact density ρa at a specific δ = α ρ(a) − ρ(s) (73) nucleus a. These authors investigated the contact densities (in e bohr− 3)ofmercuryasafreeatomor where δ (in mm s−1) is given by the electron contact bonded in a molecule, where in the latter case contact − densities ρ at the position of the absorbing (a) density differences ρHg ρmol were determined (see and source (s) nucleus (in bohr− 3)andα is a Table 6).98 Trends in the calculated contact density calibration constant depending on details of the differences were reasonably reproduced already at the nuclear γ -transition. Typically, α is determined by NESC/HF and NESC/MP2 levels of theory, although a linear regression analysis of the quantum chemically NESC/CCSD densities were the most reliable values.98 calculated contact densities against the experimental The values of the contact density difference are values of the isomer shifts.145,160 Mossbauer¨ isomer large when the electronic environment strongly differs

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TABLE 6 Effective Contact Densities (e bohr−3) of the Hg Atom contributions to the enthalpy and entropy at a given Obtained at the NESC Level of Theory temperature. Atom/Molecule NESC/HF NESC/MP2 NESC/CCSD The quantum chemical calculation of second- order response properties with nonrelativistic methods Hg 2,104,944.971 2,105,047.821 2,105,035.382 is a widely used standard procedure.113 However, + Hg 112.876 127.943 121.136 there is less computational data available for Hg2 + 278.394 305.695 293.217 molecules containing relativistic atoms because in HgF 98.086 81.294 76.872 this case reliable methods have to be applied, which include both correlation and relativistic HgF2 121.352 108.368 104.387 corrections.1,13,14 The complexity of the full 4- HgF 96.586 109.453 96.264 4 component relativistic formalism restricts the reliable HgCl 108.118 94.572 91.592 2 calculation of molecular properties to atoms and small Hg(CH3)2 49.001 43.610 42.184 molecules.166–169 This makes the use of Dirac-exact 2+ Hg (H2O)6 240.820 245.550 237.066 methods such as NESC particularly attractive.

1 In the following, we will present the basic theory The absolute contact density is given for Hg( S0), whereas contact density − 97 of calculating second-order response properties, difference values ρHg ρmol are listed for ions and molecules. which requires a derivation of the analytical second derivatives of the electronic energy with respect to a from that of the free Hg atom. The differences stretch parameter λ. With the help of the analytical energy from about 40 e bohr−3 in dimethyl mercury to 293 gradient of Eq. (28), the analytical second derivatives e bohr−3 in the mercury dication. With increasing of E can be calculated according to electronegativity of the Hg-substituents, the difference −3 contact density increases to 104 e bohr ,which ∂2E ∂2S ∂2H − = tr  + tr P 1 e confirms that the isomer shifts δ of Mossbauer¨ ∂μ∂λ ∂μ∂λ ∂μ∂λ spectroscopy reliably describe the environment of the  

Hg nucleus.98 1 ∂2 ∂ ∂S + tr P (J − K) + tr 2 ∂μ∂λ ∂μ ∂λ  

∂P ∂H − 1 ∂P ∂ SECOND-ORDER RESPONSE + tr 1 e + tr (J − K) (76) PROPERTIES ∂μ ∂λ 2 ∂μ ∂λ The analytical calculation of the energy Hessian with respect to external perturbations such as There are six contributions of which two (terms 1 the displacement of the nuclear coordinates, the and 3) can be directly determined utilizing standard 113 components of the electric field, or other quantities, is nonrelativistic methods. Contributions 4, 5, and a prerequisite for obtaining second-order response 6 require either ∂P/∂μ or ∂W/∂μ and can be properties of a molecule (vibrational frequencies, calculated with the help of the coupled perturbed 113,170 electric polarizabilities, infrared intensities, etc.). It equations using the gradient ∂H1 − e/∂μ.The is also one of the criteria when assessing the general solution of the NESC coupled perturbed equations 99 applicability of a new quantum chemical method.113 was published by ZFC. Hence, the major problem The eigenvalues of the Hessian matrix of second is the derivation of the second derivatives of the one- derivatives of the molecular energy with respect electron part given by contribution 2. This in turn leads to second derivatives of the NESC Hamiltonian to the nuclear coordinates are used to characterize ˜ the nature of a stationary point obtained on the matrix L and the renormalization matrix G,which potential energy surface (PES) via optimization of the can be simplified by deleting those terms that are − 4 molecular energy, so that one can distinguish between of the order O(c ). The important terms of the minima, first-order and higher-order saddlepoints of second and the fifth contribution of Eq. (76) are the PES. Furthermore, they determine the curvature given by of a PES at a stationary point and by this the vibrational force constants of a molecule, which, by ∂P ∂H − ∂2H − tr 1 e + tr P 1 e solving the basic equation of vibrational spectroscopy, ∂μ ∂λ ∂μ∂λ lead to the molecular vibrational frequencies in 2 165 ∂ T their harmonic approximation. These in turn are = tr UP˜ + PU˜ † − UPU˜ † needed to calculate zero-point energies and vibrational ∂μ∂λ

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in the gas phase, whereas most measured intensi- 2 2 ties are given relative to the most intensive infrared ˜ † ∂ W ˜ ∂ V + tr UPU + tr P 171 ∂μ∂λ ∂μ∂λ band.    The infrared intensity  is a response property, ˜ ∂P ∂G† ∂G ∂L which can be calculated if the analytical derivatives + tr LG˜ + G†L˜ + G† G ∂μ ∂λ ∂λ ∂λ of the energy with regard to nuclear coordinates  and the components of the electric field F α are ∂2G† ∂2G + tr D + D† available. Alternatively, one can express it in the form ∂μ∂λ ∂μ∂λ of derivatives of the components of the molecular    dipole moment with respect to the normal coordinates ∂G† ∂L˜ ∂G† ∂L˜ + tr P + G according to Eq. (78):171 ∂μ ∂λ ∂λ ∂μ      2 ˜ ˜ 3  ∂μ  ∂L ∂G ∂L ∂G i = 8π NAg/3hc   (78) +G† + (77) ∂Q ∂λ ∂μ ∂μ ∂λ i

Constant NA is the Avogadro number, h the Planck In Eq. (77), the major contributions result from the constant, and Qi a normal coordinate of degeneracy g. first four terms on the r.h.s. Whenever highly accurate Usually, the dipole moment derivatives are calculated values of the Hessian matrix are not needed (for for Cartesian coordinates α, which leads to Eq. (79). example, for the calculation of vibrational frequencies There, the intensity of mode i is given as needed for thermochemical corrections), terms 5 = † = † † and 6 can be neglected and term 4 approximated, i δi δi li li (79) thus significantly saving computer time and core memory.99 As in the case of the analytical NESC δi = li (80) gradient, an accurate calculation of the second derivatives of the one-electron part involves the where atomic units are used and  denotes the accurate calculation of the second derivatives of U and rectangular dipole moment derivative matrix of G, where in the former case the application of response dimension 3 × 3N given in Cartesian coordinates. theory and the consideration of the positronic states The mass-weighted vibrational normal mode vectors of the D-Hamiltonian is mandatory as was discussed li are determined when solving the vibrational secular 99 by ZFC. equation in Cartesian coordinates.165 The NESC infrared intensity is obtained by calculating the derivative of Eq. (57), i.e., the NESC NESC Infrared Spectra: Vibrational dipole moment, with respect to an atomic coordinate 95 Frequencies and Infrared Intensities Xn: Using the formalism described above, NESC vibra-      tional frequencies can be calculated in combination ∂2 ˜ ∂ ∂ ˜ = ˜ L + P † L with any electron correlated nonrelativistic method α,n tr P tr G G ∂Xn∂Fα ∂Xn ∂Fα for which second derivatives are available. This is  the case for most methods.113 Although the calcula- ∂2V ∂P ∂V = tr P˜ + tr G† G (81) tion of vibrational frequencies is important for the ∂Xn∂Fα ∂Xn ∂Fα characterization of stationary points on the PES or the conversion of energies into enthalpies and free where again first and second derivatives of matrices energies (see above), an obvious challenge of quan- U and G are neglected because they make negligible tum chemistry is the prediction of infrared spectra contributions to the infrared intensity.95 in connection with the identification and structural ZFC95,99calculated a number of infrared spectra description of unknown compounds containing rela- using NESC/PBE0. In Table 7, geometries, vibrational tivistic atoms. For this purpose, one has to be able frequencies, and infrared intensities are compared to calculate infrared intensities. Calculated infrared with experimental results, some of which were intensities are nowadays often the only source for obtained in the solid state as indicated. The reliable values of this property because absolute calculated vibrational frequencies are in reasonable (rather than relative) infrared intensities are difficult agreement with the available experimental data to measure.171 Therefore, absolute infrared inten- considering the harmonic approximation and the fact sities are only known for some small molecules that NESC/PBE0 gives the calculated bond lengths

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TABLE 7 Comparison of NESC/PBE0 Geometries (Distances in A),˚ Harmonic Vibrational Frequencies (cm− 1), and Infrared Intensities (km mol−1) with the Corresponding Experimental Values Measured in the Gas or the Solid Phase1 Molecule (Sym.) Method Geometry Frequency (Infrared Intensity, Mode Symmetry) + AuH (C∞v ) NESC/PBE0 Au–H: 1.530 2283.7 (14.7; σ ) Expt.116 Au–H: 1.524 2305.0 (σ +) − + + AuH2 (D∞h ) NESC/PBE0 Au–H: 1.652 773.8 (115.7; π u), 1685.2 (1035.8; σu ), 1994.9 (0; σg ) 172 + Expt. 1636.0 (σu ) − AuH4 (D4h ) NESC/PBE0 Au–H: 1.631 776.4 (0; b2g), 793.9 (66.6; eu), 828.7 (42.3; a2u), 843.1 (0; b2u) 1780.6 (2318.0; eu), 2113.7 (0; b1g), 2118.1 (0; a1g) 172 Expt. 1676.4 (eu) + AuF (C∞v ) NESC/PBE0 Au–F: 1.923 556.7 (52.3; σ ) Expt.129 Au–F: 1.918 563.7 (σ +) − + + AuF2 (D∞h ) NESC/PBE0 Au–F: 1.963 184.4 (25.0; π u), 516.3 (0; σg ), 548.1 (182.7; σu ) − AuF4 (D4h ) NESC/PBE0 Au–F: 1.916 184.0 (0; b2u), 217.7 (0; b2g), 233.1 (25.8; a2u), 253.8 (8.7; eu) 572.0 (0; b1g), 597.1 (0; a1g), 613.4 (383.9; eu) 173 Expt.(solid) 230 (b2g), 561 (b1g), 588 (a1g) + ThO (C∞v ) NESC/PBE0 Th–O: 1.826 926.1 (245.7; σ ) Expt.174 Th–O: 1.840 895.8 (σ +)

Th2O2 (D2h ) NESC/PBE0 Th–O: 2.089 155.7 (4.8; b3u), 192.7 (0; ag), 373.1 (0; b3g), 527.2 (35.2; b2u),

O–Th–O: 74.4 623.8 (297.9; b1u), 633.9 (0; ag) 175 Expt. 619.7 (b1u)

UF6 (Oh ) NESC/PBE0 U–F: 1.994 139.1 (0; t 2u), 184.0 (51.7; t 1u), 199.3 (0; t 2g), 539.1 (0; eg)

629.4 (810.3; t 1u), 681.4 (0; a1g) 176,177 Expt. U–F: 1.996 142 (t 2u), 186.2 (∼38; t 1u), 202 (t 2g), 532.5 (eg), 624 (750; t 1u)

667.1 (a1g)

OsO4 (T d ) NESC/PBE0 Os–O: 1.686 352.6 (22.4; t 2), 356.5 (0; e), 1031.9 (465.8; t 2), 1063.9 (0; a1) 178,179 Expt. Os–O: 1.711 322.7 (t 2), 333.1 (e), 960.1 (t 2), 965.2 (a1) 265 HsO4 (T d ) NESC/PBE0 Hs–O: 1.757 316.1 (32.9; t 2), 335.2 (0; e), 1010.4 (463.2; t 2), 1056.2 (0; a1)

1For details, see Ref 95, 99.

−1 somewhat too long. In general, stretching frequencies 17 to 25 km mol (π u-bending mode). Apart from are somewhat too large (due to the harmonic the fact that infrared intensities are essential for approximation), whereas bending frequencies are identifying unknown compounds via their infrared somewhat too small (due to the somewhat too long spectra, they are also useful for deriving effective bond lengths). atomic charges.180 In the case of UF6, experimental absolute 177 intensities are available. The t1u-symmetrical vibrational modes at 184 (exp.: 186) and 629 (exp.: NESC Static Electric Dipole Polarizabilities 624) cm− 1 with intensities of 52 (exp.: 38) and Another second-order response property important 810 (exp.: 750) km mol−1 are in good agreement for the elucidation of the electronic structure of with the experimental values (see Table 7). ZFC95 atoms and molecules is the static electric dipole showed that according to their calculated infrared polarizability, henceforth called polarizability for intensities the polarity of an AuX (X = Br, Cl, F) bond brevity. When a molecule is exposed to an external strongly influences the intensity of the AuX stretching electric field, the electric dipole moment reflects the vibration. The calculated NESC/PBE0 values of the separation of positive and negative charge in the intensity increased from 5.1 to 12.9 to 52.3 km mol−1 molecule, whereas the polarizability measures the in this series. For the corresponding series of anions deformation of the electron density distribution of XAuX−, there is an increase from 35 to 70 to an atom or molecule.181 Knowledge of atomic and −1 + 183 km mol (σu -stretching mode) and from 6 to molecular polarizabilities is important in many areas

© 2014 John Wiley & Sons, Ltd. Advanced Review wires.wiley.com/wcms of chemistry ranging from electronic and vibrational electron correlation effects necessitates the use of spectroscopy to molecular modeling, drug design, and accurate theoretical methods for explaining trends in nanotechnology. Especially for molecules containing a series of related molecules.182 ZFC95 investigated relativistic atoms, measured values of polarizabilities the change in the isotropic polarizability α for are sparse, and therefore their reliable prediction with Au- and Hg-containing molecules as well as a the help of relativistic quantum chemical methods is number of other molecules by using the NESC desirable. formalism. Some of their results are summarized in The second-order term in the Taylor expansion Table 8.95 given in Eq. (54) defines the polarizability tensor: The relativistic corrections for the isotropic  polarizabilities are between −0.2 and −2.0 A˚ 3,andthe 2  =− =−∂ E (F ) largest effect is found for HgH (α: 5.83–7.86 2.03 α  (82) ˚ 3 ∂F ∂F F =0 A , see Table 8). These trends can be related to the contraction of the 6 s-orbital of Hg, which dominates Rather than using the tensor α, one normally prefers scalar relativistic effects of mercury compounds. An to work with the scalar isotropic polarizability, which exception is found for HgF2 where the 6 s-orbital is given by the average of the trace of the polarizability contraction is balanced by the electron-withdrawing tensor181 ability of two electronegative F atoms so that the   relativistic and nonrelativistic isotropic polarizabilities 1 (4.13 and 4.06 A˚ 3, Table 8) become comparable. α = αxx + αyy + αzz (83) 3 Apart from this, the isotropic polarizability follows some general trends: (1) the α values are larger and which is invariant with respect to coordinate for anions than for neutral molecules or cations; transformations. (2) they are larger for radicals than for closed shell ZFC95 derived the formulas for the NESC systems (see, e.g., HgH and HgH : 5.46 vs 5.01 A˚ 3, polarizability, which takes a relative simple form after 2 Table 8); (3) they increase with increasing atomic deleting small contributions involving the derivatives volume, i.e., with each additional electronic shell; and of W, U,andG; (4) molecules with more electropositive atoms possess      2 ˜ ˜ larger α values than those with more electronegative ˜ ∂ L ∂P † ∂L ααβ =−tr P − tr G G atoms. ∂Fα∂Fβ ∂Fα ∂Fβ ZFC95 compared the isotropic polarizability  2 of osmium tetroxide, OsO4, and tetroxide, ˜ ∂ V ∂P † ∂V =−tr P − tr G G (84) HsO4, obtained at the NESC level with experimental ∂Fα∂Fβ ∂Fα ∂Fβ or previously published values. They found that the NESC/MP2 value of the isotropic polarizability (8.23 Since V is a linear function of the external electric field A˚ 3) is in close agreement with the experimental (see Eq. 54), the second derivative of V in the first value of 8.17 A˚ 3. NESC/MP2 also predicted that the term on the r.h.s vanishes, and Eq. (84) simplifies to isotropic polarizability of HsO4 is somewhat larger 3 Eq. (85) (8.30 A˚ , Table 8) than that of OsO4 in agreement  with the expectation that with increasing number of ∂P † ∂V electrons and a more electropositive central atom the ααβ =−tr G G (85) ∂Fα ∂Fβ polarizability increases. The NESC/PBE0 results for α of the group 8 Hence, the scalar relativistic formula for the polar- tetroxides are more than 1 unit too small (OsO4: 6.89 izability differs from the nonrelativistic calculation A˚ 3). In general, NESC/MP2 polarizabilities are more only by the fact that the derivative ∂V/∂F β has to be reliable than the NESC/PBE0 results for α,which renormalized by matrix G. The derivative of P has to means that DFT can only be used for considering be calculated via a coupled-perturbed approach.99 general trends. NESC polarizabilities were found to In view of the fact that scalar relativistic effects help correct flawed experimental data.95 For example, lead to a contraction of the s- and p-orbitals and to an the measured isotropic polarizability of UF6 was expansion of the d- and f-orbitals and that the latter measured to be 12.5 A˚ 3,184 which is far too large effect is normally weaker than the former, one can in in view of a NESC/MP2 value of 8.03 A˚ 3 (Table 8). 184 general expect a decrease of the electric polarizability The value of α(HgCl2) was given in the literature as long as atoms are considered. However, in as 11.6 A˚ 3, whereas the calculated NESC/MP2 value molecules, the interplay between relativistic and is 8.60 A˚ 3.95

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TABLE 8 Polarizabilities (in A˚ 3) at Optimized Geometries as Obtained with NESC/MP2, NESC/PBE0, or Nonrelativistic (NR) Calculations

Molecule Method αxx αyy αzz α AuH NESC/MP2 5.05 5.05 6.01 5.37 − AuH2 NESC/MP2 7.01 7.01 9.34 7.79 − AuH4 NESC/MP2 9.85 9.85 6.38 8.69 AuF NESC/MP2 4.12 4.12 4.91 4.38 − AuF2 NESC/MP2 5.34 5.34 6.30 5.66 − AuF4 NESC/MP2 7.52 7.52 4.34 6.46 UF6 NESC/MP2 8.03 8.03 8.03 8.03 183 OsO4 NESC/MP2 8.23 8.23 8.23 8.23 (8.17)

HsO4 NESC/MP2 8.30 8.30 8.30 8.30 HgH NESC/PBE0 5.05 5.05 7.38 5.83 NESC/MP2 4.56 4.56 7.27 5.46 NR/PBE0 7.50 7.50 8.57 7.86

HgH2 NESC/PBE0 4.31 4.31 6.77 5.13 NESC/MP2 4.19 4.19 6.66 5.01 NR/PBE0 5.23 5.23 7.29 5.91

HgH4 NESC/PBE0 7.58 7.58 4.32 6.49 NESC/MP2 7.55 7.55 4.28 6.46 NR/PBE0 9.05 9.05 4.95 7.68 HgF NESC/PBE0 4.37 4.37 6.53 5.09 NESC/MP2 3.87 3.87 6.85 4.86 NR/PBE0 6.35 6.35 6.65 6.45

HgF2 NESC/PBE0 3.31 3.31 5.75 4.13 NESC/MP2 3.33 3.33 5.89 4.18 NR/PBE0 3.30 3.30 5.57 4.06

HgF4 NESC/PBE0 7.35 7.35 3.39 6.03 NESC/MP2 8.23 8.23 3.44 6.64 NR/PBE0 8.92 8.92 3.38 7.08

Experimental values are given in parentheses for comparison.95

NESC AS A TWO-COMPONENT FZC103 developed a 2-component NESC method METHOD: SPIN-ORBIT COUPLING closely following Dyall’s work.68 This required the inclusion of the SOC operator, which is split into The SOC effect causes a splitting of the orbital a one- and a two-electron part. For heavy elements, energy levels (especially the p-levels of heavy atoms) SOC is dominated by the one-electron term. The two- 1,12–14,24,185–187 according to the jj-coupling scheme. electron spin-orbit (SO) contributions often reduce the This affects the strength of the chemical bond in former term by about 5% for elements with a filled molecules with heavy atoms, reaction and activation 5d shell and by about 10% in the case of elements 94 energies, ionization potentials and electron affinities, with a filled 6d shell,103 which is an indication of their and many other spectroscopic properties. In addition, overall screening effect. These contributions are not SOC can lead to dynamic phenomena such as negligible, however, in most cases they are parallel to spin symmetry-forbidden transitions in molecular the one-electron SO terms.188 spectra or intersystem crossings between molecular In view of the much smaller two-electron states with different multiplicity. The calculation contributions and the significantly larger costs to of SOC with NESC requires a 2-component calculate them,189 FZC103 estimated the magnitude formulation (2cNESC) as it was originally developed of the two-electron part from the magnitude of the by Dyall.1,68 one-electron SO part, where the latter was accurately

© 2014 John Wiley & Sons, Ltd. Advanced Review wires.wiley.com/wcms determined. They employed the screened-nuclear- atoms with 1 ≤ Z ≤ 120 and l ≤ 6 (i.e., i-type basis spin-orbit (SNSO) approach of Boettger,190 which functions) an agreement of the calculated SO splittings was originally formulated within the DKH quasi- within 0.02 hartree (spinors with j ≥ 7/2) compared relativistic approximation49–51 and which had been to 4-component DHF results. These authors used used by several other authors.191–193 the 2-component NESC(SNSO) or NESC(mSNSO) In the modified Dirac equation1,68 given in approach in connection with the general HF (GHF) Eq. (7), the matrix W = (σ · p)V(r)(σ · p)/4m2c2 can or general Kohn-Sham (GKS) formalism for obtaining be split into a spin-free (sf) and spin-dependent part the total energy and spinor energies of many-electron according to Eq. (86): systems.194–196 The performance of NESC(SNSO) is illustrated W = Wsf + iσ· WSO (86) in Figure 3 for spinor energy splittings of Z = 120 (Ubn: unbinilium) by plotting their deviation (in The separation is achieved by the use of the Dirac percentage) from exact splittings obtained with the identity (σ · A)(σ · B) = A · B + iσ · (A × B)andthesf 4-component DHF method. and the SO parts of the W matrix are defined in The one-electron SO contributions (given in red) Eq. (8). exaggerate calculated np-splittings on the average     by 2%, nd-splittings by 10%, and nf-splittings by    1  33% with the deviations becoming somewhat larger Wsf =− μ  ∇· V (r) ∇ ν (87a) μν 4m2c2 with increasing principal quantum number n.This     exaggeration is largely corrected by the screened    1  nucleus two-electron contributions so that final 2- WSO =− μ  ∇ ×V (r) ∇ ν (87b) μν 4m2c2 component NESC(SNSO) values differ by just 2% from the Dirac values. After the mSNSO correction, In these equations, a spinor basis set χ is used which thedeviationsare1%fornp-splittings and only 103 comprises basis functions for both α and β spin. As increase to 3% for the nf-splittings. pointed out above, the sf-NESC formalism is obtained This observation was confirmed when calculat- 103 by neglecting the SO part of the W matrix.1,44 The ing the SO splitting of spinor energies in molecules. − 1 inclusion of the spin-dependent part of W needed for In Table 9, calculated SO splittings in cm are given SOC is still practical for large molecules as long as only for hydrogen halides HX (valence-shell npπ splittings) = = the one-electron potential (i.e., the electron-nuclear with X F, Cl, Br, I, At, Uus (ununseptium, Z 117) attraction potential) has to be determined.44 and mercury(II) halides HgX2 (mercury 5dπ and 5dδ = By calculating just the one-electron part in splittings) with X F, Cl, Br, I. For HX molecules, − 1 Eq. (87b), SO splittings in many-electron systems the splittings range from 380 to 23,955 cm , with are seriously overestimated. Including however the the NESC values always being somewhat larger (up − 1 SNSO approximation,14,190 the SOC terms of the to 60 cm ) indicating that they slightly exaggerate one-electron NESC Hamiltonian are effectively scaled the splittings because of the approximate two-electron down so that reasonable SO splittings are obtained.103 contributions to SOC. However, the deviations when This is accomplished with the help of basis-function- given in percentage are similar to those found for dependent scaling factors, which simulate the effect of atoms. In the case of HgX2 molecules, the overall the missing two-electron SO terms: magnitude and the relative precision of the calculated SO splittings were of the same order of magnitude as NESC = NESC for the bare Hg atom. FZC observed that with the H1e,SNSO H1e,SO μν μν 2-component NESC(mSNSO)/GHF approach reliable     SO splittings and SOC corrections of relative energies Q l Q l 103 − μ NESC ν can be calculated. H1e,SO (88) Zμ μν Zν CONCLUSIONS In Eq. (88), Zμ is the charge of the nucleus at which  the spinor basis function μ is centered and The last two decades have seen a rapid development Q lμ is a screening factor that depends on the of relativistic 1-component and 2-component methods orbital angular momentum of the function μ;in derived from the exact 4-component Dirac formalism. particular, Q(l) = 0, 2, 10, 28, ··· for l = 0, 1, 2, 3, ···. This was triggered by Dyall’s 1997 article68 on the By further improving the SNSO approach (called NESC method and his development of programmable modified SMSO or mSNSO), FZC103 obtained for NESC equations. Although it needed more than

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Z=120 35

30 2cNESC/SOC(SNSO) 2cNESC/SOC 25

20

15

SO splitting error (%) 10

5

0 1/2 1/2 1/2 1/2 1/2 1/2 3/2 3/2 3/2 3/2 5/2 5/2 - 4f - 5f - 2p - 3p - 4p - 5p - 6p - 7p - 3d - 4d - 5d - 6d 7/2 7/2 3/2 3/2 3/2 3/2 3/2 3/2 5/2 5/2 5/2 5/2 4f 5f 2p 3p 4p 5p 6p 7p 3d 4d 5d 6d

FIGURE 3| Deviations (in percentage) of the 2-component (2c) NESC/SOC/GHF and NESC/SOC(SNSO)/GHF spinor energy splittings from exact 4-component DHF splittings given in the case Z = 120.

− 1 71–74 83,86 TABLE 9 SO Splittings (in cm ) of the Valence npπ Orbitals of HX Wolf, and Hess, Barysz and Kedziera, and and the 5dπ,δ Orbitals of HgX2 as Given by 4-Component Dirac/HF and many others. This was reflected by the development 2-Component NESC(mSNSO)/GHF Calculations, Both Obtained with a of the infinite-order DKH, the IOTC, or the X2C 103 Finite Nucleus Model. methods. Furthermore, Dyall’s work was essential for Dirac NESC(mSNSO) a paradigm shift from an operator-driven to a matrix- Molecule Splitting1 4-Component 2-Component driven development of relativistic quantum chemical methods. HF 2pπ -2pπ 381 371(−2.6) 3/2 1/2 Today the NESC method can be routinely HCl 3pπ 3/2 -3pπ 1/2 758 762(0.5) applied in its spin-free, 1-component form to HBr 4pπ 3/2 -4pπ 1/2 2994 3025(1.0) determine first-order response properties such as HI 5pπ 3/2 -5pπ 1/2 5942 5979(0.6) geometries, electron density distributions, electric

HAt 6pπ 3/2 -6pπ 1/2 15513 15538(0.2) moments, electric field gradients, hyperfine structure constants, contact densities and Mossbauer¨ isomer HUus 7pπ 3/2 -7pπ 1/2 23955 23978(0.1) shifts or nuclear quadrupole coupling constants, etc. HgF 5dπ -5dπ 5362 5357(−0.5) 2 3/2 1/2 Also, there is the possibility of determining in a 5dδ5/2 -5dδ3/2 18769 19076(1.6) standard manner second-order response properties HgCl2 5dπ 3/2 -5dπ 1/2 16266 16579(1.9) such as vibrational frequencies and vibrational force 5dδ5/2 -5dδ3/2 17613 17955(1.9) constants in the harmonic approximation, static

HgBr2 5dπ 3/2 -5dπ 1/2 16095 16415(2.0) electric dipole polarizabilities, infrared intensities, magnetic shieldings, etc. Clearly, the repertoire of 5dδ5/2 -5dδ3/2 17446 17794(2.0) molecular properties which can be calculated with the HgI 5dπ -5dπ 15196 15506(2.0) 2 3/2 1/2 NESC method will be successively extended in the 5dδ5/2 -5dδ3/2 17286 17637(2.0) near future, hopefully including properties such as

1Different ω-spinors with the same symmetry are differentiated by labeling anharmonic corrections to the vibrational frequencies them according to the dominant spin-free orbital. For Uus (Z = 117), a mass or the indirect spin–spin coupling constants of nuclear number of 2.556Z was used. Relative deviations (in %) from the 4-component Dirac/HF values are given in parentheses. magnetic resonance spectroscopy. The usefulness and general applicability of 2- component NESC methods is also steadily growing. 10 years to solve the NESC equations exactly with The calculation of SOC effects with the GHF method an algorithm that could also be applied to large is surprisingly successful, although setbacks in the molecules with thousands of basis functions,44 Dyall’s form of symmetry-breaking or variational problems work represented directly or indirectly an instigator will probably emerge. In this connection, one will of work by Kutzelnigg and Liu,45,76,77 Saue,85 Reiher, need also more experience with both the GHF and

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GKS method. The inclusion of analytical derivatives where it is sufficient to achieve chemical accuracy will be the next step in this development to routinely (±1kcalmol−1) rather than a spectroscopic accuracy calculate SOC-corrected geometries and other first- of a few cm− 1. order response properties. In view of the challenges posted by the chemistry NESC is built on the DC-Hamiltonian. Its of heavy and superheavy elements, we foresee also for extension to the DCB-Hamiltonian will be a challenge this decade an active and rapid development of new and necessity for molecules containing transactinides. relativistic methods, for which Dirac-exact methods Much work has been carried out in this connection, will provide a solid fundament. Apart from this, however easy applicable methods, which can be used NESC will be the basis for numerous investigations on for large basis set calculations and in connection molecules and chemical reactions involving relativistic with correlation corrected nonrelativistic methods, atoms, which will be facilitated once the computer are not available. For highly accurate calculations, programs based on NESC will become generally QED effects have to be considered. However, available. these challenges are outside the realm of chemistry

ACKNOWLEDGMENTS This work was financially supported by the National Science Foundation, Grant CHE 1152357. We thank SMU for providing excellent computational facilities.

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