8 research outputs found
Orbital-Optimized Second-Order Perturbation Theory with Density-Fitting and Cholesky Decomposition Approximations: An Efficient Implementation
An efficient implementation
of the orbital-optimized second-order
perturbation theory with the density-fitting (DF-OMP2) and Cholesky
decomposition (CD-OMP2) approaches is presented. The DF-OMP2 method
is applied to a set of alkanes, conjugated dienes, and noncovalent
interaction complexes to compare the computational cost with the conventional
orbital-optimized MP2 (OMP2) [Bozkaya, U.; Turney, J. M.; Yamaguchi,
Y.; Schaefer, H. F.; Sherrill, C. D. <i>J. Chem. Phys.</i> <b>2011</b>, <i>135</i>, 104103] and the orbital-optimized
MP2 with the resolution of the identity approach (OO-RI-MP2) [Neese,
F.; Schwabe, T.; Kossmann, S.; Schirmer, B.; Grimme, S. <i>J.
Chem. Theory Comput.</i> <b>2009</b>, <i>5</i>, 3060â3073]. Our results demonstrate that the DF-OMP2 method
provides substantially lower computational costs than OMP2 and OO-RI-MP2.
Further application results show that the orbital-optimized methods
are very beneficial for the computation of open-shell noncovalent
interactions. Considering both computational efficiency and the accuracy
of the DF-OMP2 method, we conclude that DF-OMP2 is very promising
for the study of weak interactions in open-shell molecular systems
Orbital-Optimized MP3 and MP2.5 with Density-Fitting and Cholesky Decomposition Approximations
Efficient implementations of the
orbital-optimized MP3 and MP2.5
methods with the density-fitting (DF-OMP3 and DF-OMP2.5) and Cholesky
decomposition (CD-OMP3 and CD-OMP2.5) approaches are presented. The
DF/CD-OMP3 and DF/CD-OMP2.5 methods are applied to a set of alkanes
to compare the computational cost with the conventional orbital-optimized
MP3 (OMP3) [Bozkaya <i>J. Chem. Phys.</i> <b>2011</b>, <i>135</i>, 224103] and the orbital-optimized MP2.5 (OMP2.5)
[Bozkaya and Sherrill <i>J. Chem. Phys.</i> <b>2014</b>, <i>141</i>, 204105]. Our results demonstrate that the
DF-OMP3 and DF-OMP2.5 methods provide considerably lower computational
costs than OMP3 and OMP2.5. Further application results show that
the orbital-optimized methods are very helpful for the study of open-shell
noncovalent interactions, aromatic bond dissociation energies, and
hydrogen transfer reactions. We conclude that the DF-OMP3 and DF-OMP2.5
methods are very promising for molecular systems with challenging
electronic structures
Analytic Energy Gradients and Spin Multiplicities for Orbital-Optimized Second-Order Perturbation Theory with Density-Fitting Approximation: An Efficient Implementation
An
efficient implementation of analytic energy gradients and spin
multiplicities for the density-fitted orbital-optimized second-order
perturbation theory (DF-OMP2) [Bozkaya, U. <i>J. Chem. Theory
Comput.</i> <b>2014</b>, <i>10</i>, 2371â2378]
is presented. The DF-OMP2 method is applied to a set of alkanes, conjugated
dienes, and noncovalent interaction complexes to compare the cost
of single point analytic gradient computations with the orbital-optimized
MP2 with the resolution of the identity approach (OO-RI-MP2) [Neese,
F.; Schwabe, T.; Kossmann, S.; Schirmer, B.; Grimme, S. <i>J.
Chem. Theory Comput.</i> <b>2009</b>, <i>5</i>, 3060â3073]. Our results demonstrate that the DF-OMP2 method
provides substantially lower computational costs for analytic gradients
than OO-RI-MP2. On average, the cost of DF-OMP2 analytic gradients
is 9â11 times lower than that of OO-RI-MP2 for systems considered.
We also consider aromatic bond dissociation energies, for which MP2
provides poor reaction energies. The DF-OMP2 method exhibits a substantially
better performance than MP2, providing a mean absolute error of 2.5
kcal mol<sup>â1</sup>, which is more than 9 times lower than
that of MP2 (22.6 kcal mol<sup>â1</sup>). Overall, the DF-OMP2
method appears very helpful for electronically challenging chemical
systems such as free radicals or other cases where standard MP2 proves
unreliable. For such problematic systems, we recommend using DF-OMP2
instead of the canonical MP2 as a more robust method with the same
computational scaling
Assessment of Orbital-Optimized MP2.5 for Thermochemistry and Kinetics: Dramatic Failures of Standard Perturbation Theory Approaches for Aromatic Bond Dissociation Energies and Barrier Heights of Radical Reactions
An assessment of orbital-optimized
MP2.5 (OMP2.5) [Bozkaya, U.; Sherrill, C. D. J. Chem.
Phys. 2014, 141, 204105] for thermochemistry and kinetics is presented. The OMP2.5
method is applied to closed- and open-shell reaction energies, barrier
heights, and aromatic bond dissociation energies. The performance
of OMP2.5 is compared with that of the MP2, OMP2, MP2.5, MP3, OMP3,
CCSD, and CCSDÂ(T) methods. For most of the test sets, the OMP2.5 method
performs better than MP2.5 and CCSD, and provides accurate results.
For barrier heights of radical reactions and aromatic bond dissociation
energies OMP2.5âMP2.5, OMP2âMP2, and OMP3âMP3
differences become obvious. Especially, for aromatic bond dissociation
energies, standard perturbation theory (MP) approaches dramatically
fail, providing mean absolute errors (MAEs) of 22.5 (MP2), 17.7 (MP2.5),
and 12.8 (MP3) kcal mol<sup>â1</sup>, while the MAE values
of the orbital-optimized counterparts are 2.7, 2.4, and 2.4 kcal mol<sup>â1</sup>, respectively. Hence, there are 5â8-folds
reductions in errors when optimized orbitals are employed. Our results
demonstrate that standard MP approaches dramatically fail when the
reference wave function suffers from the spin-contamination problem.
On the other hand, the OMP2.5 method can reduce spin-contamination
in the unrestricted HartreeâFock (UHF) initial guess orbitals.
For overall evaluation, we conclude that the OMP2.5 method is very
helpful not only for challenging open-shell systems and transition-states
but also for closed-shell molecules. Hence, one may prefer OMP2.5
over MP2.5 and CCSD as an <i>O</i>(<i>N</i><sup>6</sup>) method, where <i>N</i> is the number of basis
functions, for thermochemistry and kinetics. The cost of the OMP2.5
method is comparable with that of CCSD for energy computations. However,
for analytic gradient computations, the OMP2.5 method is only half
as expensive as CCSD
Theoretical Study of Thermal Rearrangements of 1-Hexen-5-yne, 1,2,5-Hexatriene, and 2-Methylenebicyclo[2.1.0]pentane
In this research, a comprehensive theoretical investigation
of
the thermal rearrangements of 1-hexen-5-yne, 1,2,5-hexatriene, and
2-methylenebicyclo[2.1.0]Âpentane is carried out employing density
functional theory (DFT) and high level <i>ab initio</i> methods,
such as the complete active space self-consistent field (CASSCF),
multireference second-order MøllerâPlesset perturbation
theory (MRMP2), and coupled-cluster singles and doubles with perturbative
triples [CCSDÂ(T)]. The potential energy surface (PES) for the relevant
system is explored to provide a theoretical account of pyrolysis experiments
by Huntsman, Baldwin, and Roth on the target system. The rate constants
and product distributions are calculated using theoretical kinetic
modelings. The rate constant for each isomerization reaction is computed
using the transition state theory (TST). The simultaneous first-order
ordinary-differential equations are solved numerically for the relevant
system to obtain time-dependent concentrations, hence the product
distributions at a given temperature. Our computed energy values (reaction
energies and activation parameters) are in agreement with Rothâs
experiments and the product distributions of Huntsmanâs experiments
at 340 and 385 °C with various reaction times, while simulated product fractions are in qualitative accordance with Baldwinâs experiment
Assessment of Orbital-Optimized MP2.5 for Thermochemistry and Kinetics: Dramatic Failures of Standard Perturbation Theory Approaches for Aromatic Bond Dissociation Energies and Barrier Heights of Radical Reactions
An assessment of orbital-optimized
MP2.5 (OMP2.5) [Bozkaya, U.; Sherrill, C. D. J. Chem.
Phys. 2014, 141, 204105] for thermochemistry and kinetics is presented. The OMP2.5
method is applied to closed- and open-shell reaction energies, barrier
heights, and aromatic bond dissociation energies. The performance
of OMP2.5 is compared with that of the MP2, OMP2, MP2.5, MP3, OMP3,
CCSD, and CCSDÂ(T) methods. For most of the test sets, the OMP2.5 method
performs better than MP2.5 and CCSD, and provides accurate results.
For barrier heights of radical reactions and aromatic bond dissociation
energies OMP2.5âMP2.5, OMP2âMP2, and OMP3âMP3
differences become obvious. Especially, for aromatic bond dissociation
energies, standard perturbation theory (MP) approaches dramatically
fail, providing mean absolute errors (MAEs) of 22.5 (MP2), 17.7 (MP2.5),
and 12.8 (MP3) kcal mol<sup>â1</sup>, while the MAE values
of the orbital-optimized counterparts are 2.7, 2.4, and 2.4 kcal mol<sup>â1</sup>, respectively. Hence, there are 5â8-folds
reductions in errors when optimized orbitals are employed. Our results
demonstrate that standard MP approaches dramatically fail when the
reference wave function suffers from the spin-contamination problem.
On the other hand, the OMP2.5 method can reduce spin-contamination
in the unrestricted HartreeâFock (UHF) initial guess orbitals.
For overall evaluation, we conclude that the OMP2.5 method is very
helpful not only for challenging open-shell systems and transition-states
but also for closed-shell molecules. Hence, one may prefer OMP2.5
over MP2.5 and CCSD as an <i>O</i>(<i>N</i><sup>6</sup>) method, where <i>N</i> is the number of basis
functions, for thermochemistry and kinetics. The cost of the OMP2.5
method is comparable with that of CCSD for energy computations. However,
for analytic gradient computations, the OMP2.5 method is only half
as expensive as CCSD
Transition Metal CationâĎ Interactions: Complexes Formed by Fe<sup>2+</sup>, Co<sup>2+</sup>, Ni<sup>2+</sup>, Cu<sup>2+</sup>, and Zn<sup>2+</sup> Binding with Benzene Molecules
A computational investigation
of the structures and interaction
energies of complexes formed by Fe<sup>2+</sup>, Co<sup>2+</sup>,
Ni<sup>2+</sup>, Cu<sup>2+</sup>, and Zn<sup>2+</sup> binding with
benzene (Bz) molecules is performed employing high level <i>ab
initio</i> quantum chemical methods, such as the second-order
perturbation theory (MP2), coupled-cluster singles and doubles (CCSD),
and coupled-cluster singles and doubles with perturbative triples
[CCSDÂ(T)] methods, along with the 6-311++GÂ(2d,2p) and 6-311++GÂ(d,p)
basis sets. As far as we know, the present work is the first to study
the structures and energetics of BzâM<sup>2+</sup> and BzâM<sup>2+</sup>âBz type complexes (M = Co, Ni, Cu, and Zn). Relativistic
effects are also investigated via DouglasâKrollâHess
second-order scalar relativistic computations for the complexes considered.
Our results demonstrate that there are strong bindings between transition
metal cations and benzene molecules. The computed interaction energies,
including relativistic energy corrections, for the BzâM<sup>2+</sup> type complexes at the CCSDÂ(T)/6-311++GÂ(2d,2p) level are
â131.9 (BzâFe<sup>2+</sup>), â172.6 (BzâCo<sup>2+</sup>), â189.8 (BzâNi<sup>2+</sup>), â181.1
(BzâCu<sup>2+</sup>), and â158.2 (BzâZn<sup>2+</sup>) kcal mol<sup>â1</sup>. Similarly, interaction energies for
the BzâM<sup>2+</sup>âBz type complexes at the CCSDÂ(T)/6-311++GÂ(d,p)
level are â206.4 (BzâFe<sup>2+</sup>âBz), â213.4
(BzâCo<sup>2+</sup>âBz), â249.7 (BzâNi<sup>2+</sup>âBz), â258.6 (BzâCu<sup>2+</sup>âBz),
and â235.2 (BzâZn<sup>2+</sup>âBz) kcal mol<sup>â1</sup>. Further, our results also demonstrate that the relativistic
effects are very important in accurate computations of interaction
energies. The predicted relativistic energy corrections to interaction
energies, using the ĎB97X-D functional, are between â1.9
and â7.7 kcal mol<sup>â1</sup>. The transition metal
cationâĎ interactions investigated in this study prove
significantly larger binding energies compared to arbitrary ĎâĎ
interactions and main group cationâĎ interactions. We
believe that the present study may open new avenues in cationâĎ
interactions
Thermal Aromatizations of 2-Vinylmethylenecyclopropane and 3-Vinylcyclobutene
A comprehensive theoretical investigation of thermal
rearrangements
of 2-vinylmethylenecyclopropane and 3-vinylcyclobutene is carried
out employing density functional theory and high level ab initio methods,
such as the complete active space self-consistent field, multi-reference
second-order MøllerâPlesset perturbation theory, and coupled-cluster
singles and doubles with perturbative triples. In all computations,
Popleâs polarized triple-Îś split valence basis set, 6-311GÂ(d,p),
is utilized. The potential energy surface for the relevant system
is explored to provide theoretical insights for the thermal aromatizations
of 2-vinylmethylenecyclopropane and 3-vinylcyclobutene. The rate constant
for each isomerization reaction is computed using the transition state
theory. The simultaneous first-order ordinary-differential equations
are solved numerically for the considered system to obtain time-dependent
concentrations, hence the product distributions at a given temperature.
Our results demonstrate that at high temperatures thermal aromatizations
of 2-vinylmethylenecyclopropane (at 700 °C and higher) and 3-vinylcyclobutene
(at 500 °C and higher) are feasible under appropriate experimental
conditions. However, at low temperatures (at 500 °C and lower),
2-vinylmethylenecyclopropane yields 3-methylenecyclopentene as a unique
product, kinetically, and the formation of benzene is not favorable.
Similarly, at 300 °C and lower temperatures, 3-vinylcyclobutene
can only yield <i>trans</i>-1,3,5-hexatriene (major) and <i>cis</i>-1,3,5-hexatriene (minor). At 300 < <i>T</i> < 500 °C, 3-vinylcyclobutene almost completely yields 1,3-cyclohexadiene.
Hence, our computations provide a useful insight for the synthesis
of substituted aromatic compounds. Further, calculated energy values
(reaction energies and activation parameters) are in satisfactory
agreement with the available experimental results