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L. Thøgersen, J. Olsen / Chemical Physics Letters 393 (2004) 36–43 41<br />

A smaller than the FCI value, but the frequency is 6<br />

cm 1 too large. The deviations of the various CC<br />

methods obtained here for CN are very similar to the<br />

previously obtained deviations for N 2 . Thus, it has<br />

previously been reported that the contribution from<br />

connected quadruple excitations to the harmonic frequency<br />

for this molecule [23,32] is 20 cm 1 .<br />

It is currently not feasible to obtain FCI energies for<br />

CN in the cc-pVTZ basis with an accuracy that is<br />

sufficient to obtain the frequency with an accuracy of<br />

1cm 1 or less. One can instead estimate the convergence<br />

by examining the changes in the constants through the<br />

CC hierarchy. It is seen from Table 4 that the changes<br />

between the CCSDT and CCSDTQ results are very<br />

similar in the cc-pVDZ and cc-pVTZ basis sets. In both<br />

basis sets, the quadruple excitations increase the distance<br />

by 0.0020 A and reduce the harmonic frequency<br />

by about 20 cm 1 . This suggests that it may be feasible<br />

to obtain the quadruple corrections to these constants in<br />

rather small basis sets. It should be noted that although<br />

the quadruple corrections to the properties are rather<br />

constant, the quadruples corrections to the raw energies<br />

are very different in the two basis sets.<br />

The errors of the harmonic frequencies arise from<br />

two sources. First of all, the positive curvatures of the<br />

CC deviation curves around the equilibrium geometries<br />

lead to CC frequencies that are larger than the FCI<br />

frequency. Furthermore, as the third derivative of the<br />

energies with respect to the distance in general is large<br />

and negative, the somewhat shorter internuclear distances<br />

obtained with the CC methods than with FCI<br />

lead also to frequencies that are too large. These two<br />

sources of errors may be analyzed in the cc-pVDZ basis<br />

by evaluating the CC frequencies at the FCI equilibrium<br />

geometry. For the orbital based methods one then obtains<br />

the frequencies 2035, 2027 and 2022 cm 1 for the<br />

CCSD, CCSDT and CCSDTQ methods. Whereas, the<br />

CCSDT frequency evaluated at the optimized CCSDT<br />

distance deviates from the FCI frequency by 23 cm 1 ,<br />

the CCSDT frequency evaluated at the FCI geometry<br />

thus deviates by only 7 cm 1 . Although the errors connected<br />

with the positive curvatures of the deviation<br />

curves are not vanishing, the major errors of the frequencies<br />

seem to arise from the errors of the equilibrium<br />

distances.<br />

The experimental values for the equilibrium distance<br />

and the harmonic frequency are 1.1718 A and 2069<br />

cm 1 , respectively, [30]. Comparing the results obtained<br />

using the cc-pVTZ basis to the experimental values, it is<br />

observed that the CCSDT results are in better agreement<br />

with experiment than the CCSDTQ results. A<br />

better estimate of the importance of the quadruples<br />

corrections may be obtained using CCSDT results for<br />

large basis sets. Feller and Sordo [2] have calculated the<br />

CCSDT spectroscopic constants for CN using the augcc-pVQZ<br />

basis and obtained the equilibrium distance<br />

1.1739 A and the harmonic frequency of 2082 cm 1 .<br />

Adding our quadruples correction to these CCSDT results<br />

gives an equilibrium geometry of 1.1759 A and a<br />

harmonic frequency of 2060 cm 1 . To obtain spectroscopic<br />

constants that are significantly more accurate<br />

than the CCSDT results, other corrections, most important<br />

core-correlation contributions, must be included<br />

together with the quadruple excitations.<br />

3.4. Atomization energy<br />

It has previously been reported that quadruple and<br />

even quintuple excitations may be important to obtain<br />

atomization energies with high accuracy [3,4,12] In<br />

Table 5, we list the atomization energies using the<br />

CCSD, CCSDT, CCSDTQ, and FCI approaches with<br />

the cc-pVDZ basis and the CCSD, CCSDT, and<br />

CCSDTQ approaches with the cc-pVTZ basis set. All<br />

molecular calculations were carried out at the experimental<br />

equilibrium distance.<br />

It is again noticed that there are no significant difference<br />

between the results obtained using the CC(orb)<br />

and CC(spin–orb) approaches. The two approaches<br />

differ by only 0.1 kJ/mol at the CCSDT and CCSDTQ<br />

levels.<br />

The quadruple excitations change the atomization<br />

energy by 4 kJ/mol with both the cc-pVDZ and the ccpVTZ<br />

basis sets. These results are in agreement with<br />

previous calculations of the contributions from connected<br />

quadruple excitations [4]. From the difference<br />

between CCSDTQ and the FCI atomization energy, it is<br />

seen that the quintuple excitations contribute 0.5 kJ/mol<br />

to the atomization energy. The above contribution from<br />

quadruple and quintuple excitations are very similar to<br />

the results previously reported for N 2 [3]. The contribution<br />

from higher excitations to the atomization energy<br />

of CN has previously been studied by Feller and Sordo<br />

[2]. They obtained a significantly smaller contribution<br />

from quadruple excitations, 0.3 kcal/mol or 1.2 kJ/mol.<br />

There are several experimental measurements of the<br />

atomization energies, and Feller and Sordo [2] quotes<br />

Table 5<br />

The electronic contribution to the dissociation energy (kJ/mol) for CN<br />

CCSD(orb) cc-pVDZ 631.6<br />

CCSDT(orb) cc-pVDZ 663.0<br />

CCSDTQ(orb) cc-pVDZ 666.5<br />

CCSD(spin–orb) cc-pVDZ 629.2<br />

CCSDT(spin–orb) cc-pVDZ 662.9<br />

CCSDTQ(spin–orb) cc-pVDZ 666.4<br />

FCI cc-pVDZ 667.0<br />

CCSD(spin–orb) cc-pVTZ 674.2<br />

CCSDT(spin–orb) cc-pVTZ 714.4<br />

CCSDTQ(spin–orb) cc-pVTZ 718.5<br />

D e

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