Deborah A Penchoff1,2, Charles C Peterson3, Mark S Quint4,5, John D Auxier6, George K Schweitzer7, David M Jenkins7, Robert J Harrison8,9, Howard L Hall1,6,10. 1. Institute for Nuclear Security, University of Tennessee, 1640 Cumberland Avenue, Knoxville, Tennessee 37996, United States. 2. Joint Institute for Computational Sciences, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, United States. 3. Research Information Technology Services, University of North Texas, 225 South Avenue B, Denton, Texas 76201, United States. 4. Department of Nuclear Engineering, University of Tennessee, 301 Middle Drive, Pasqua Nuclear Engineering Building, Knoxville, Tennessee 37996, United States. 5. US Army Nuclear and Countering Weapons of Mass Destruction Agency (USANCA), United States Army, Ft. Jackson, South Carolina 29715, United States. 6. Radiochemistry Center of Excellence (RCOE), University of Tennessee, 1508 Middle Drive, Ferris Hall, Knoxville, Tennessee 37996, United States. 7. Department of Chemistry, University of Tennessee, 1420 Circle Drive, Knoxville, Tennessee 37996, United States. 8. Institute for Advanced Computational Science, Stony Brook University, 100 Nicolls Road, Stony Brook, New York 11790, United States. 9. Brookhaven National Laboratory, Computational Science, Building 725, Upton, New York 11973, United States. 10. Y-12 National Security Complex, Oak Ridge, Tennessee 37830, United States.
Abstract
Efficient predictive capabilities are essential for the actinide series since regulatory constraints for radioactive work, associated costs needed for specialized facilities, and the short half-lives of many actinides present great challenges in laboratory settings. Improved predictive accuracy is advantageous for numerous applications including the optimization and design of separation agents for nuclear fuel and waste. One limitation of calculations in support of these applications is that the large variations observed from predictions obtained with currently available methods can make comparisons across studies uncertain. Benchmarking currently available computational methodologies is essential to establish reliable practices across the community to guarantee an accurate physical description of the systems studied. To understand the performance of a variety of common theoretical methods, a systematic analysis of differences observed in the prediction of structural characteristics, electron withdrawing effects, and binding energies of [An(NO3)]2+ (with An = Ac to Lr) in gas and aqueous phases is reported. Population analysis obtained with Mulliken and Löwdin reflect a large dependence on the level of theory of choice, whereas those obtained with natural bond orbital show larger consistency across methodologies. Predicted stability across the actinide series calculated with coupled cluster with perturbative doubles and triples at the triple ζ level is equivalent to the one obtained when extrapolated to the complete basis set limit. The ground state of [Fm(NO3)]2+ and [Md(NO3)]2+ is predicted to have an electronic structure corresponding to An III state in gas and An IV in aqueous phase, whereas the ground state of [An(NO3)]2+ (with An = Ac to Es, Lr) presents an electronic structure corresponding to An IV in the gas and aqueous phase. The compounds studied with No in gas and aqueous phase present a preferred No III state, and the Lr compounds did not follow trends predicted for the rest of the actinide series, as previously observed in studies regarding its unusual electronic structure relative to its position in the periodic table.
Efficient predictive capabilitin class="Chemical">es are essential for the actinide series since regulatory constraints for radioactive work, associated costs needed for specialized facilities, and the short half-lives of many actinides present great challenges in laboratory settings. Improved predictive accuracy is advantageous for numerous applications including the optimization and design of separation agents for nuclear fuel and waste. One limitation of calculations in support of these applications is that the large variations observed from predictions obtained with currently available methods can make comparisons across studies uncertain. Benchmarking currently available computational methodologies is essential to establish reliable practices across the community to guarantee an accurate physical description of the systems studied. To understand the performance of a variety of common theoretical methods, a systematic analysis of differences observed in the prediction of structural characteristics, electron withdrawing effects, and binding energies of [An(NO3)]2+ (with An = Ac to Lr) in gas and aqueous phases is reported. Population analysis obtained with Mulliken and Löwdin reflect a large dependence on the level of theory of choice, whereas those obtained with natural bond orbital show larger consistency across methodologies. Predicted stability across the actinide series calculated with coupled cluster with perturbative doubles and triples at the triple ζ level is equivalent to the one obtained when extrapolated to the complete basis set limit. The ground state of [Fm(NO3)]2+ and [Md(NO3)]2+ is predicted to have an electronic structure corresponding to An III state in gas and An IV in aqueous phase, whereas the ground state of [An(NO3)]2+ (with An = Ac to Es, Lr) presents an electronic structure corresponding to An IV in the gas and aqueous phase. The compounds studied with No in gas and aqueous phase present a preferred No III state, and the Lr compounds did not follow trends predicted for the rest of the actinide series, as previously observed in studies regarding its unusual electronic structure relative to its position in the periodic table.
All
of pan class="Chemical">the pan class="Chemical">actinides are radioactive, with a broad range of half-lives
ranging from seconds to millions of years.[1] Yet despite their radioactivity, these elements are of considerable
importance in a number of disparate areas, including military nuclear
applications,[2] civilian nuclear power,[3−5] neutron radiography,[6−8] and radiothermal generators for space missions.[9] Furthermore, they are also employed in cancer
treatments and neutron therapy,[10−14] in geological analysis in marine sediment modeling,[15] and in astronomy.[16] Due to their
radioactivity and often short half-lives, they present challenges
for experimental science, which intimatesthat effective theory could
aide many applications without the need for specialized radiation
laboratories.[17−23] Unfortunately, electronic structure calculations performed with
traditional approaches become increasingly more difficult as the number
of electrons and relativistic effects increase, which leads to a higher
computational cost to achieve accuracy.[24] Theoretical considerations, including electronic correlation, multireference
character, the interaction of core and valence electrons, and relativistic
effects, intensify challenges and contribute to limitations in investigations
involving the actinide series.[25]
One rpan class="Chemical">esearch area where improved, reliable calculations would have
immediate impan>ct is on selective binding of ligands to pan class="Chemical">actinides,
which is critical for a range of applications, but in particular,
the civilian nuclear fuel cycle.[3−5] Optimization and design of extracting
agents with high binding selectivity depend largely on computational
feedback to reduce the processing cost.[26−28] In 2012, Glatz cataloged
all of the industrial processes for handling spent nuclear fuel[29] and he noted that nitric acid was essential
in the first step of this process. In the initial phases of nuclear
fuel treatment, all of the actinide elements, such as Ac, Th, Pa,
U, Np, Pu, Am, Cm, and Bk, are present in the nuclear fuel depending
on the reactor type. The URanium EXtraction (UREX) and Plutonium URanium
EXtraction (PUREX) methods of removing weapons usable U or Pu from
the fuel cycle both employ nitrates, whereby the spent fuel is divided
into small pieces and dissolved into nitric acid in molarities of
0.5–4 M depending on the process.[30] Therefore, we chose the [An(NO3)]2+ (with
An = Ac to Lr) as a model system for calculations due to the importance
of nitric acid binding in actinide separation processes.
Understanding
structural characteristics, electron win class="Chemical">thdrawing
effects, and binding energies is essential for optimization of separations,
and computational tools can greatly aid in the prediction of these
properties.[31,32] Yet, to our knowledge, in-depth
evaluations of level of theory dependence on structural and population
predictions for actinide-containing compounds withnitrates for the
entire series have not been performed. Three metrics have been advanced
across the actinide series for understanding ligand–actinide
interactions: population analysis, structural characteristics, and
binding energies. Population analysis is a useful aid for the analysis
of electron withdrawing effects and their effect on selective binding
to actinides.[33,34] Mulliken population analysis
has been extensively used withuranium compounds,[35−42] but this type of analysis is largely dependent on the level of theory
of choice, which makes comparisons across different studies uncertain.
Structural characteristics include careful comparisons on bond distances
and angles between the ligand and actinide. Finally, Dolg and co-workers
evaluated the hydration energy across the actinide seriesthrough
electronic structure calculations, showing an accuracy of the methodologies
employed to be within 1% of experimental values; however, there was
only experimental data for two actinides (uranium and plutonium).[23] In some cases, all of these aspects were evaluated
for a ligand (cyclic imide dioximes) but only with a small subset
of the actinides.[33] Last, we note that
the extent of variations in the prediction of these properties for
actinide-containing compounds from utilizing different methodologies
or levels of theory is often problematic as few methods have been
used in systematic studies across the entire actinide series.
One of pan class="Chemical">the most challenging aspects when applying electronic structure
calculations to pan class="Chemical">actinides is assuring the calculation is reaching
the true ground state for the actinide. In many instances, the user
needs to manually alter orbitals to ensure correct orbital occupancies.
However, as the number of atoms increases in compounds, the orbital
mixing is often challenging to fix due to the closely degenerate f
orbitals. Moreover, without a computational protocol that ensuresthe compound is in the true ground state, various results can be obtained,
as illustrated in the Results and Discussion section.
In pan class="Chemical">this manuscript, we showcase an exhaustive compan>rison
of different
methodologies and levels of theory to generate an in-depth understanding
of the performance of electronic structure methods illustrated through
nitrate binding across the entire series of actinides. We address
the dependence of population analysis (part I), structural characteristics
(part II), and binding energies (part III) on the level of theory
of choice through a systematic study of [An(NO3)]2+ structures (with An = Ac to Lr). To this end, gas-phase structures
are optimized with local density approximation (LDA), TPSS, B3LYP,
PBE0, B972, M06, and M11, the Stuttgart RSC 1997 ECP and associated
basis set for the actinide atoms including and excluding the most
diffuse basis functions, withthe 6-31G*, cc-pVDZ, 6-311++G**, cc-pVTZ,
and cc-pVQZ basis sets for the nitrogen and oxygen atoms. Single-point
energy calculations are obtained with coupled cluster with perturbative
doubles and triples (CCSD(T)) and all-electron correlation-consistent
basis sets. Additionally, [An(NO3)]2+ (with
An = Ac to Lr) structures are optimized with an implicit solvation
model and a subset of functionals and basis sets. Evaluation of methodologies
in the prediction of differences amongst contiguous actinides is included
to aid in targeted selective separations across the series.
Results
and Discussion
Unlpan class="Chemical">ess otherwise indicated, the results discussed
in this section
correspond to An IV configuration and gas-phase calculations. The
An IV and An III notation follows the NIST Atomic Spectra Database
spectra name classifications, which correspond to a defined electronic
structure associated with each state, as shown in Table .[43]
Table 1
Electronic Configuration for An IV
and An III[43]
An
An IV
An III
Ac
[Hg]6p6
[Rn]7s
Th
[Rn]5f
[Rn]5f6d
Pa
[Rn]5f2
[Rn]5f26d
U
[Rn]5f3
[Rn]5f4
Np
[Rn]5f4
[Rn]5f5
Pu
[Rn]5f5
[Rn]5f6
Am
[Rn]5f6
[Rn]5f7
Cm
[Rn]5f7
[Rn]5f8
Bk
[Rn]5f8
[Rn]5f9
Cf
[Rn]5f9
[Rn]5f10
Es
[Rn]5f10
[Rn]5f11
Fm
[Rn]5f11
[Rn]5f12
Md
[Rn]5f12
[Rn]5f13
No
[Rn]5f13
[Rn]5f14
Lr
[Rn]5f14
[Rn]5f147s
Proper considerations were given to include pan class="Chemical">the ground
state for
all compounds. Several combinations of methods and basis sets initially
converged to an An III configuration. After altering the orbital occupancies
to reflect an An IV configuration, a lower energy was obtained for
[Bk(NO3)]2+ and [Es(NO3)]2+. Calculations withCCSD(T) indicate a preferred An III state for
[Fm(NO3)]2+, [Md(NO3)]2+, and [No(NO3)]2+ in the gas phase, with Fm
and No having energies at least 100 kcal mol–1 lower
than in the An IV state, and Fm and Md in an An IV state in solution.
It has been previously observed that No is found in a divalent state
(An III) configuration in solution,[44] due
to stabilization of the 5f shell, which corroboratesthe correctness
in the evaluated lowest energy configuration state in this study.
Differences in predicted ΔGrxn calculated
between some compounds withthe actinide in An IV and An III states
are shown in Table .
Table 2
Predicted Difference in ΔGrxn for An-Containing Compounds with an An III
to An IV Configuration Changea
An
method
An basis
set
N and O basis
set
Δ(ΔG)rxn (kcal mol–1)
configuration
change
Bk
M11
ad
cc-pVDZ
–49.08
An III to An IV
6-311++G**
–62.45
An III to An IV
cc-pVQZ
–70.38
An III to An IV
nd
6-311++G**
–44.01
An III to An IV
Es
PBE0
ad
6-311++G**
–19.66
An III to An IV
cc-pVQZ
–18.88
An III to An IV
nd
6-311++G**
–16.14
An III to An IV
B972
ad
cc-pVTZ
–13.04
An III to An IV
M11
ad
6-31G*
–16.36
An III to An IV
cc-pVDZ
–14.70
An III to An IV
6-311++G**
–13.49
An III to An IV
cc-pVTZ
–24.16
An III to An IV
nd
cc-pVTZ
–11.87
An III to An IV
cc-pVQZ
–21.42
An III to An IV
Fm
CCSD(T)
cc-pVTZ-X2C
cc-pVTZ-DK
–106.70
An IV to An III
V∞Z
V∞Z
–111.23
An IV to An III
No
CCSD(T)
cc-pVTZ-X2C
cc-pVTZ-DK
–138.50
An IV to An III
V∞Z
V∞Z
–141.88
An IV to An III
The “method”
column
indicates CCSD(T) or the functional of choice when utilizing DFT.
The “An basis set” column indicates ad or nd for DFT,
and cc-pVTZ-X2C or CBS (V∞Z) for CCSD(T). (An III to An IV
is calculated as ΔGrxn in An IV
state – ΔGrxn in An III state.)
pan class="Chemical">The “method”
column
indicatesCCSD(T) or the functional of choice when utilizing DFT.
The “An basis set” column indicates ad or nd for DFT,
and cc-pVTZ-X2C or CBS (V∞Z) for CCSD(T). (An III to An IV
is calculated as ΔGrxn in An IV
state – ΔGrxn in An III state.)
Spin–orbit corrections
are not included in pan class="Chemical">the thermochemical
data and discussion throughout this study. The calculated spin–orbit
contribution to [Ac(NO3)]2+ and [Lr(NO3)]2+ following the proposed reaction in eq is −0.92 and −3.24
kcal mol–1, respectively (calculated withthe DIRAC16
software, using the eXact-2-Component (X2C)–Dirac–Hartree–Fock
and a triple ζ level basis set[45] developed
by Dyall).
Figure shows pan class="Chemical">the
identifying atom labels in the proposed [An(NO3)]2+ complex.
Figure 1
Identifying labels in [An(NO3)]2+ (An = Ac
to Lr).
Identifying labels in pan class="Chemical">[An(NO3)]2+ (An = Ac
to pan class="Chemical">Lr).
Part I: Population Analysis
Level of
Theory Dependence
Overall, it is observed
pan class="Chemical">that the partial atomic charges calculated with natural bond orbital
(NBO) are largely independent from the level of theory of choice,
whereas partial charges calculated with Mulliken and Löwdin
showed larger ranges of predicted populations and a strong dependence
on the level of theory of choice. Figures and 3 show the predicted
charge of An in [An(NO3)]2+ calculated with
NBO, Mulliken, and Löwdin, where is it apparent that predicted
charges with Mulliken and Löwdin show fluctuations when utilizing
different combinations of functionals and basis sets, whereas partial
charges calculated with NBO seem largely independent of the level
of theory of choice for all functionals tested. Variations in predicted
partial charge of An in the compounds evaluated withthe levels of
theory proposed show a range calculated with NBO, Mulliken, and Löwdin
(indicated order as NBO/Mulliken/Löwdin) for Ac (0.15/0.37/0.65),
Th (0.13/0.47/0.66), Pa (0.24/0.44/0.72), U (0.22/0.45/0.74), Np (0.17/0.39/0.71),
Pu (0.28/0/42/0.80), Am (0.19/0.53/0.75), Cm (0.25/0.52/0.80), Bk
(0.29/0.46/0.75), Cf (0.34/0.46/0.68), Es (0.34/0.48/0.75), Fm (0.42/0.58/0.72),
Md (0.26/0.18/0.35), No (0.14/0.13/0.29), and Lr (0.19/0.44/0.73),
as shown in Figures and 3. Including and excluding the most diffuse
basis functions in the An basis set give negligible differences in
the predicted partial charge of An in the compounds tested with NBO
and the levels of theory previously specified, as shown in Figures and S.1 in the Supporting Information (SI). Significant
differences including and excluding the most diffuse functions with
Mulliken are observed for Ac (up to 0.17), Th (up to 0.32), Fm (up
to 0.28), and Lr (up to 0.11), and with Löwdin for Ac (up to
0.14), Th (up to 0.38), Pu (up to 0.13), Am (up to 0.22), Cm (up to
0.14), Fm and Lr (up to 0.31) (also shown in Figures and S.1 in the
SI). Partial charges calculated with Löwdin show larger overall
differencesthan those with NBO and Mulliken for Th, Pu, Am, Cm, Fm,
and Lr. All calculated differences in partial charges with NBO, Mulliken,
and Löwdin ad and nd are included in Tables S.1–S.3 in the SI.
Figure 2
NBO, Mulliken, and Löwdin charge
calculated for An3+ in [An(NO3)]2+ with LDA, TPSS, B3LYP, PBE0,
B972, M06, and M11 with the Stuttgart RSC 1997 ECP and associated
basis set, including all diffuse basis functions on the An basis set.
The lines are included as a visual aid and do not represent function
continuity.
Figure 3
NBO, Mulliken, and Löwdin
charge calculated for An3+ in [An(NO3)]2+ with LDA, TPSS, B3LYP, PBE0,
B972, M06, and M11 with the Stuttgart RSC 1997 ECP and associated
basis set, excluding the most diffuse basis functions on the An basis
set. The lines are included as a visual aid and do not represent function
continuity.
Figure 4
NBO, Mulliken, and Löwdin
ranges calculated for An3+ in [An(NO3)]2+ with LDA, TPSS, B3LYP, PBE0,
B972, and M06, with the Stuttgart 1997 ECP including all diffuse functions
(ad) and without most diffuse functions (nd). (Range = largest predicted
charge – smallest predicted charge, as indicated in eq .)
NBO, Mulliken, and Löwdin charge
calculated for An3+ in pan class="Chemical">[An(NO3)]2+ wipan class="Chemical">th LDA, TPSS, B3LYP, PBE0,
B972, M06, and M11 withthe Stuttgart RSC 1997 ECP and associated
basis set, including all diffuse basis functions on the An basis set.
The lines are included as a visual aid and do not represent function
continuity.
NBO, Mulliken, and Löwdin
charge calculated for An3+ in pan class="Chemical">[An(NO3)]2+ wipan class="Chemical">th LDA, TPSS, B3LYP, PBE0,
B972, M06, and M11 withthe Stuttgart RSC 1997 ECP and associated
basis set, excluding the most diffuse basis functions on the An basis
set. The lines are included as a visual aid and do not represent function
continuity.
NBO, Mulliken, and Löwdin
rangpan class="Chemical">es calculated for An3+ in pan class="Chemical">[An(NO3)]2+ with LDA, TPSS, B3LYP, PBE0,
B972, and M06, withthe Stuttgart 1997 ECP including all diffuse functions
(ad) and without most diffuse functions (nd). (Range = largest predicted
charge – smallest predicted charge, as indicated in eq .)
Electron Withdrawing Effects and Orbital Occupancies in [An(NO3)]2+
An An IV configuration is predicted
for all pan class="Chemical">[An(NO3)]2+ structurpan class="Chemical">es in the gas phases
for Ac, Th, Pa, U, Np, Pu, Am, Cm, Bk, Cf, Es, and Lr, whereas an
An III is obtained in the gas phase for Fm, Md, and No. The orbital
occupancies of optimized [An(NO3)]2+ structures
(for An = Ac, Th, Pa, U, Np, Cm, Bk, Es, Fm, Md, No, and Lr) in solution
calculated with NBO show the 5f occupancy is less than 0.12 from the
values calculated in the gas phase for Ac, Pa, U, Np, Cm, Bk, Es,
and Lr for all options tested. The calculated 5f occupancy is approximately
0.4, 0.9, and 0.7 lower in aqueous phase than in gas phase in [Th(NO3)]2+, [Fm(NO3)]2+, and [Md(NO3)]2+, respectively, for all functional/basis set
options tested, suggesting an An III in the gas phase and an An IV
in solution for Fm and Md.
Overall, pan class="Chemical">the occupan>ncy of the 5f
orbital for the actinides predicted in the optimized structures in
the gas phase is within 0.1 units of those obtained when applying
a solvation model for an aqueous environment for Ac, Pa, U, Np, Cm,
Bk, and Es, predicting an An IV state with all the options tested.
For [Fm(NO3)]2+, optimized structures in gas
phase predict an Fm III state, whereas optimized structures in an
aqueous environment predict an Fm IV configuration. Similarly, optimized
[Md(NO3)]2+ structures in the gas phase predict
an Md III state and aqueous structures predict an Md IV configuration.
For [No(NO3)]2+, the aqueous environment reducesthe 5f occupancy by approximately 0.4 units but it is not fully changed
to an An IV state, which suggests an No III preference in gas and
solution. The change in 5f occupancy in gas and aqueous phase for
[Th(NO3)]2+, [Fm(NO3)]2+, [Md(NO3)]2+, and [No(NO3)]2+ is included in Table .
Table 3
Predicted Electronic Occupancy of
the 5f Orbital of Th, Fm, Md, and No in [An(NO3)]2+ in Gas (g) and Aqueous (aq) Environments Calculated with NBO
5f
An
functional
N and O basis set
(g)
(aq)
Th
B3LYP
6-31G*
0.7
0.4
6-311++G**
0.7
0.4
PBE0
6-31G*
0.7
0.3
6-311++G**
0.7
Fm
B3LYP
6-31G*
6-311++G**
12.0
11.1
PBE0
6-31G*
12.0
11.1
6-311++G**
12.0
11.1
Md
B3LYP
6-31G*
13.0
6-311++G**
13.0
12.3
PBE0
6-31G*
13.0
6-311++G**
13.0
12.3
No
B3LYP
6-31G*
14.0
13.6
6-311++G**
14.0
13.7
PBE0
6-31G*
14.0
13.7
6-311++G**
14.0
13.7
pan class="Chemical">The partial
charge of the actinides in [An(NO3)]2+ in the
gas phase calculated with NBO reveals a charge approximately
between 2.4 and 2.6 for Ac to Es and Lr and approximately 1.9 for
Fm, Md, and No. The 5f orbitals show an occupancy of approximately
1 for Th, 2 for Pa, 3 for U, 4 for Np, 5 for Pu, 6 for Am, 7 for Cm,
8 for Bk, 9 for Cf, 10 for Es, 12 for Fm, 13 for Md, and 14 for No
and Lr. No significant differences are observed in the predicted 5f
orbital occupancies, including and excluding the most diffuse basis
functions in the An basis set. It is possible that these occupancies
suggest an An IV configuration for Ac to Es and Lr and An III for
Fm, Md, and No when bound to only one nitrate in the gas phase, as
proposed in this study. The partial charge calculated with NBO for
An and NO3 in [An(NO3)]2+ is shown
in Figure . Predicted
orbital occupancies for all actinides are shown in Tables S.4 and S.5 in the SI.
Figure 5
An and NO3 partial charges
calculated with NBO in [An(NO3)]2+ in gas and
aqueous phases with the Stuttgart
RSC 1997 ECP and basis set, including all diffuse basis functions
for the actinides, with the 6-31G* and 6-311++G** basis sets for oxygen
and nitrogen, and the B3LYP and PBE0 functional. (Numerical labels
shown correspond to values obtained with PBE0 and 6-311++G**. Lines
are included as a visual aid, and do not represent function continuity.)
An and pan class="Gene">NO3 partial chargpan class="Chemical">es
calculated with NBO in [An(NO3)]2+ in gas and
aqueous phases withthe Stuttgart
RSC 1997 ECP and basis set, including all diffuse basis functions
for the actinides, withthe 6-31G* and 6-311++G** basis sets for oxygen
and nitrogen, and the B3LYP and PBE0 functional. (Numerical labels
shown correspond to values obtained with PBE0 and 6-311++G**. Lines
are included as a visual aid, and do not represent function continuity.)
Part II: Structural Analysis
Level
of Theory Dependence
Optimized structurpan class="Chemical">es wipan class="Chemical">th
the levels of theory previously indicated predict structures with
an An–O1 distance with variations between 0.05 and 0.53 Å
and between 0.05 and 0.48 Å when including and excluding the
most diffuse basis functions in the An basis set, respectively, as
shown in Figure .
Overall, the largest ranges (as defined in eq ) when including all the basis functions
in the An basis set are predicted when utilizing the M06 and M11 functionals,
with differences in predicted An–O1 distance larger than 0.05
Å for Md with B3LYP, PBE0, B972, and M11, Fm with B972, and Es
withTPSS. When excluding the most diffuse basis functions, predicted
ranges larger than 0.05 Å are found with LDA for Pa, TPSS for
Fm, B3LYP for Md, M06 for Md, Fm, Es, and Cf, and M11 for Pa. All
An–O1 predicted distances are shown in Tables S.6 and S.7 in the SI.
Figure 6
Predicted An–O1 distance range
in [An(NO3)]2+ calculated with LDA, TPSS, B3LYP,
PBE0, B972, M06, and M11,
the 6-31G*, 6-311++G**, cc-pVDZ, cc-pVTZ, and cc-pVQZ basis set for
N and O, and the Stuttgart RSC 1997 ECP for An including (ad) and
excluding (nd) the most diffuse basis functions in the basis set.
Inset shows the overall range per actinide for all predicted values
with all functional and basis set combinations. (Values shown are
in angstrom. Ranges are calculated as indicated in eq .)
Predicted An–O1 distance range
in pan class="Chemical">[An(NO3)]2+ calculated wipan class="Chemical">th LDA, TPSS, B3LYP,
PBE0, B972, M06, and M11,
the 6-31G*, 6-311++G**, cc-pVDZ, cc-pVTZ, and cc-pVQZ basis set for
N and O, and the Stuttgart RSC 1997 ECP for An including (ad) and
excluding (nd) the most diffuse basis functions in the basis set.
Inset shows the overall range per actinide for all predicted values
with all functional and basis set combinations. (Values shown are
in angstrom. Ranges are calculated as indicated in eq .)
pan class="Chemical">The O1–An–O2 angle in predicted structurpan class="Chemical">es
shows
a range between 1.45 and 11.24° when including all basis functions
and between 1.32 and 11.46° when excluding the most diffuse basis
functions in the An basis set, as shown in Figure . Ranges larger than 1° are predicted
for structures optimized with M11 for Pa, B972 for Md, PBE0 for Fm,
B3LYP for Md, TPSS for Es, and LDA for Cf when including all the basis
functions in the An basis set. When excluding the most diffuse basis
functions in the An basis set, a range larger than 1° is predicted
with M11 for Md, M06 for Cf, B972 for Es and Pa, B3LYP for Pa, TPSS
for Fm and Cf, and LDA for Cf and Pa.
Figure 7
Predicted O1–An–O2 angle
range in [An(NO3)]2+ calculated with LDA, TPSS,
B3LYP, PBE0, B972, M06,
and M11, the 6-31G*, 6-311++G**, cc-pVDZ, cc-pVTZ, and cc-pVQZ basis
set for N and O, and the Stuttgart RSC 1997 ECP for An including (ad)
and excluding (nd) the most diffuse basis functions in the basis set.
Inset shows the overall range per actinide for all predicted values
with all functional and basis set combinations. (Values shown are
in degrees. Ranges are calculated for angles, as indicated in eq for interatomic distances.)
Predicted O1–An–O2 angle
range in pan class="Chemical">[An(NO3)]2+ calculated wipan class="Chemical">th LDA, TPSS,
B3LYP, PBE0, B972, M06,
and M11, the 6-31G*, 6-311++G**, cc-pVDZ, cc-pVTZ, and cc-pVQZ basis
set for N and O, and the Stuttgart RSC 1997 ECP for An including (ad)
and excluding (nd) the most diffuse basis functions in the basis set.
Inset shows the overall range per actinide for all predicted values
with all functional and basis set combinations. (Values shown are
in degrees. Ranges are calculated for angles, as indicated in eq for interatomic distances.)
Structural Changes in [An(NO3)]2+
pan class="Chemical">The predicted An–O1 distance
has an overall gradual decrease
from Ac to pan class="Chemical">Lr from 2.3 to 2.1 Å; however, structures with Fm,
Md, and No showed an An–O1 distance of approximately 2.6 Å
(Figure ). It is likely
that this difference of almost 0.5 Å is due to Fm, Md, and No
presenting an An III configuration (instead of the An IV from the
rest of the actinide series). Figure S.2 in the SI shows the An–O1 trend for Ac to Es/Lr calculated
with PBE0 including all basis functions. Moreover, Fm, Md, and No
presented variations in An–O1 distance when calculated withthe proposed methodologies, giving an Fm–O1 distance between
2.1 and 2.6 Å, an Md–O1 distance between 2.2 and 2.6 Å,
and No–O1 between 2.3 and 2.6 Å (shown in Figure S.3 in the SI).
Figure 8
Calculated An–O1
distance in [An(NO3)]2+ in gas and aqueous phase
with the B3LYP and PBE0 functional, the
6-31G* and 6-311++G** basis set for N and O atoms, and the Stuttgart
RSC 1997 ECP and basis set including all diffuse basis functions in
the basis set (in angstrom). Labels shown correspond to results obtained
with PBE0 and 6-311++G**. Th and No are shown in Figures and 11. (Lines are included as a visual aid and do not represent function
continuity.)
Calculated An–O1
distance in pan class="Chemical">[An(NO3)]2+ in gas and aqueous phase
withthe B3LYP and PBE0 functional, the
6-31G* and 6-311++G** basis set for N and O atoms, and the Stuttgart
RSC 1997 ECP and basis set including all diffuse basis functions in
the basis set (in angstrom). Labels shown correspond to results obtained
with PBE0 and 6-311++G**. Th and No are shown in Figures and 11. (Lines are included as a visual aid and do not represent function
continuity.)
Figure 10
Calculated Th–O1 and Th–O2 distance
in [Th(NO3)]2+ in gas and aqueous phase with
the B3LYP and
PBE0 functional, the 6-31G* and 6-311++G** basis set for N and O atoms,
and the Stuttgart RSC 1997 ECP and basis set including all diffuse
basis functions in the basis set (in angstrom). Labels shown correspond
to results obtained with PBE0 and 6-311++G**. (Lines are included
as a visual aid and do not represent function continuity.)
Figure 11
Calculated No–O1 and No–O2 distance in [No(NO3)]2+ in gas and aqueous phase with the B3LYP and
PBE0 functional, the 6-31G* and 6-311++G** basis set for N and O atoms,
and the Stuttgart RSC 1997 ECP and basis set including all diffuse
basis functions in the basis set (in angstrom). Labels shown correspond
to results obtained with PBE0 and 6-311++G**. (Lines are included
as a visual aid and do not represent function continuity.)
pan class="Chemical">The predicted O1–An–O2
angle has an overall gradual
increase from 55.6 to 62.3° from Ac–pan class="Chemical">Es to Lr (Figure ). Similar to the
analysis in the An–O1 distance, the O1–An–O2
angle for Fm, Md, and No shows a large difference in which the O1–An–O2
angle is approximately 10° more narrow than the contiguous actinides
(Es and Lr). Furthermore, a variation in predicted O1–An–O2
angles is observed for Fm, Md, and No structures optimized withthe
levels of theory listed in which the O1–Fm–O2 angle
ranges from 49 to 60°, O1–Md–O2 ranges from 49
to 57°, and O1–No–O2 ranges from 49 to 55°.
All values discussed in this paragraph are included in Figures S.4 and S.5 in the SI (with S.5 showing
‘ad’ in grey, and ‘nd’ in black).
Figure 9
Calculated
O1–An–O2 angle in [An(NO3)]2+ in
gas and aqueous phase with the B3LYP and PBE0 functional,
the 6-31G* and 6-311++G** basis set for N and O atoms, and the Stuttgart
RSC 1997 ECP and basis set, including all diffuse basis functions
in the basis set (in degrees). Labels shown correspond to results
obtained with PBE0 and 6-311++G**. Th is shown in Figure . (Lines are included as a
visual aid and do not represent function continuity.)
Calculated
O1–An–O2 angle in pan class="Chemical">[An(NO3)]2+ in
gas and aqueous phase withthe B3LYP and PBE0 functional,
the 6-31G* and 6-311++G** basis set for N and O atoms, and the Stuttgart
RSC 1997 ECP and basis set, including all diffuse basis functions
in the basis set (in degrees). Labels shown correspond to results
obtained with PBE0 and 6-311++G**. Th is shown in Figure . (Lines are included as a
visual aid and do not represent function continuity.)
pan class="Chemical">The An–O1 distance in solvated pan class="Chemical">[An(NO3)]2+ compounds is longer than in gas-phase structures
for Ac,
Pa, U, Np, Pu, Am, Cm, Bk, Cf, Es, No, and Lr (less than 0.16 Å
for Ac, Pa, U, Np, Pu, Am, Cm, Bk, Cf, and Er). It is shorter for
Md and Fm (between 0.33 and 0.36 Å). Similarly, the O1–An–O2
angle is smaller in solvated compounds than in the gas phase for Ac,
Pa, U, Np, Pu, Am, Cm, Bk, Cf, Es, and Lr and larger for Th, Fm, Md,
and No. (The An–O1 distances are shown in Figure , and the O1–An–O2
angles in Figure .)
The O1 and O2 are predicted to be equidistant to the An in [Th(NO3)]2+ and [No(NO3)]2+ in the
gas phase. However, the solvated [Th(NO3)]2+ structures have a difference of up to 1 Å between the An–O1
and An–O2 distance for structures optimized with B3LYP and
0.5 Å for [No(NO3)]2+ compounds optimized
with B3LYP and PBE0, as shown in Figures , 11 and S.9, S.10 in the SI.
Calculated pan class="Chemical">Th–O1 and pan class="Chemical">Th–O2 distance
in [Th(NO3)]2+ in gas and aqueous phase withthe B3LYP and
PBE0 functional, the 6-31G* and 6-311++G** basis set for N and O atoms,
and the Stuttgart RSC 1997 ECP and basis set including all diffuse
basis functions in the basis set (in angstrom). Labels shown correspond
to results obtained with PBE0 and 6-311++G**. (Lines are included
as a visual aid and do not represent function continuity.)
Calculated No–O1 and No–O2 distance in [pan class="Chemical">No(NO3)]2+ in gas and aqueous phase withthe B3LYP and
PBE0 functional, the 6-31G* and 6-311++G** basis set for N and O atoms,
and the Stuttgart RSC 1997 ECP and basis set including all diffuse
basis functions in the basis set (in angstrom). Labels shown correspond
to results obtained with PBE0 and 6-311++G**. (Lines are included
as a visual aid and do not represent function continuity.)
pan class="Chemical">The structural characteristics of [pan class="Chemical">Lr(NO3)]2+ illustrated in Figures and 9 do not follow
the trend that
would have otherwise been expected from extrapolation of An–O1
distances and O1–An–O2 angles calculated for other actinides
in the series, which is likely due to the electronic rearrangement
occurring due to relativistic effects[46−48] that prevents inference
of chemical characteristics for transactinides. This break in the
trendline along the periodic table was similarly observed by Toyoshima.[49] A decrease in ionic radii from Cf to Md has
been previously discussed within changes of actinide contractions
across the series,[50−53] which is likely affecting the bond length predicted in our study.
The second break to Lr is consistent with recent experimental and
theoretical results that treat it as similar to Lu but distinct from
other later transactinides.[54−57]
pan class="Chemical">The An–O1 distance (for An = Fm, Md,
and No) in pan class="Chemical">[An(NO3)]2+ compounds is approximately
0.3 Å longer
than in [An(NO3)]+. The O1–An–O2
angle is approximately 8° wider in [An(NO3)]+ than in [An(NO3)]2+, and the O1–N–O2
angle is approximately 10° wider in [An(NO3)]2+ than in [An(NO3)]+. All values are
shown in Table S.8 in the SI.
Part III:
Gibbs Free Energies of Reaction
Level of Theory Dependence
Calculated Gibbs free energipan class="Chemical">es
of reaction of the [An(NO3)]2+ compounds (from
Ac to Lr), as shown in eq withCCSD(T), the cc-pVTZ-DK and cc-pVQZ-DK basis set for N and
O atoms, and the cc-pVTZ-X2C and cc-pVQZ-X2C basis set for the actinides
show the same stability trend as when calculated at the CBS limit,
as indicated in eqs and 2. The predicted Gibbs free energies of
reaction calculated with cc-pVQZ-X2C/cc-pVQZ-DK are within 2 kcal
mol–1 from those calculated at the CBS limit. The
predicted Gibbs free energies of reaction with cc-pVTZ-X2C/cc-pVTZ-DK
are within 3 and 8 kcal mol–1 of those calculated
at the CBS limit (with a difference of 8 kcal mol–1 for Ac and Th; 7 for Pa; 6.0 for U, Np, Pu, Am, Cm, Bk, Cf; 5 for
Es and Lr; 4 for Md and No; and 3 for Fm). Predicted Gibbs free energies
of reaction calculated withCCSD(T) are shown in Figures , 13, and Table S.11 in the SI.
Figure 12
Calculated
ΔGrxn for [An(NO3)]2+ (with An = Ac to Lr) with CCSD(T)/cc-pVTZ-X2C:cc-pVTZ-DK
(indicated as TZ), CCSD(T)/cc-pVQZ-X2C:cc-pVQZ-DK (indicated as QZ),
and CCSD(T)/cc-pV∞Z-X2C:cc-pV∞Z-DK (indicated as CBS).
Figure 13
Calculated ΔGrxn for [An(NO3)]2+, with An = Ac to
Lr, with CCSD(T)/cc-pVTZ-X2C:cc-pVTZ-DK,
CCSD(T)/cc-pV∞Z-X2C:cc-pV∞Z-DK, and LDA, TPSS, B3LYP,
PBE0, B972, M06, and M11 with the Stuttgart RSC 1997 ECP and associated
basis set for An, and the 6-311++G** basis set for N and O. Values
are reported in kcal mol–1. LDA is indicated in
blue, the meta-GGA functional (TPSS) in orange, the hybrid GGA (B3LYP,
PBE0, and B972) functionals in gray, and the meta-hybrid GGA functionals
(M06 and M11) in green. (Lines for CCSD(T) are included as a visual
aid and do not represent function continuity.)
Calculated
ΔGrxn for pan class="Chemical">[An(NO3)]2+ (wipan class="Chemical">th An = Ac to Lr) withCCSD(T)/cc-pVTZ-X2C:cc-pVTZ-DK
(indicated as TZ), CCSD(T)/cc-pVQZ-X2C:cc-pVQZ-DK (indicated as QZ),
and CCSD(T)/cc-pV∞Z-X2C:cc-pV∞Z-DK (indicated as CBS).
Calculated ΔGrxn for pan class="Chemical">[An(NO3)]2+, wipan class="Chemical">th An = Ac to
Lr, withCCSD(T)/cc-pVTZ-X2C:cc-pVTZ-DK,
CCSD(T)/cc-pV∞Z-X2C:cc-pV∞Z-DK, and LDA, TPSS, B3LYP,
PBE0, B972, M06, and M11 withthe Stuttgart RSC 1997 ECP and associated
basis set for An, and the 6-311++G** basis set for N and O. Values
are reported in kcal mol–1. LDA is indicated in
blue, the meta-GGA functional (TPSS) in orange, the hybrid GGA (B3LYP,
PBE0, and B972) functionals in gray, and the meta-hybrid GGA functionals
(M06 and M11) in green. (Lines for CCSD(T) are included as a visual
aid and do not represent function continuity.)
Including and excluding pan class="Chemical">the most diffuse basis functions
in the
basis set of the actinide in the calculated Gibbs free energies of
reaction give a difference of less than 6 kcal mol–1 with most levels of theory tested. Exceptions are predicted (listed
in this paragraph specifying the basis set used for the N and O atoms,
in kcal mol–1) when utilizing TPSS for U with cc-pVQZ
(13.20) and Fm with cc-pVTZ (9.98); for B3LYP with Np with 6-31G*
(10.49), cc-pVDZ (13.52), 6-311++g** (10.70), cc-pVTZ (13.64), and
cc-pVQZ (13.35); for Pu with 6-31G* (6.73), cc-pVDZ (10.59), 6-311++G**
(8.02), cc-pVTZ (9.10), and cc-pVQZ (20.31); and for Es with 6-31G*
(11.24), cc-pVDZ (9.46), and cc-pVTZ (9.25); for PBE0 with Np and
cc-pVQZ (6.39), Pu with 6-311++G** (12.90) and cc-pVQZ (10.57), and
Es with 6-31G* (23.40), cc-pVDZ (21,65), 6-311++G** (22.90), cc-pVTZ
(23.50), and cc-pVQZ (20.30); with B972 for Pu, Cf, and Es with 6-311++G**
(10.13, 7.78, 6.28), and for Md with 6-31G* (16.77); with M06 for
Pu with 6-311++G** (12.50), Md with cc-pVTZ (17.27) and cc-pVQZ (17.54),
and No with cc-pVQZ (17.12); and with M11 for U with cc-pVTZ (24.51),
Pu with 6-311++G** (10.99), and cc-pVTZ (8.59), Cf with 6-311++G**
(12.26), Es with cc-pVTZ (19.77), Md with cc-pVDZ (7.69), and No with
6-3G* (12.33) and cc-pVDZ (12.24). All predicted differences between
including and excluding the most diffuse basis functions in the basis
set of the actinide are shown in Figures , S.6, and Tables S.12–S.16 in the SI.
Figure 14
Δ(ΔG)rxn for [An(NO3)]2+ normalized to Ac calculated with LDA, TPSS,
B3LYP, and PBE0 with the Stuttgart RSC 1997 ECP and basis set including
(ad) and excluding (nd) the most diffuse basis functions for An, and
the 6-31G*, cc-pVDZ, 6-311++G**, cc-pVTZ, and cc-pVQZ for N and O.
Δ(ΔG)rxn calculated with CCSD(T),
the cc-pV∞Z-X2C (CBS) basis set for An, and the cc-pV∞Z-DK
(CBS) basis set for N and O is included as reference (indicated as
CCSD(T)/CBS in labels). Values are reported in kcal mol–1. [Δ(ΔG)rxn = ΔGrxn,An – ΔGrxn,Ac, as indicated in eq , with An = Th to Lr.] The lines are included as a
visual aid, and do not represent function continuity.
Δ(ΔG)rxn for pan class="Chemical">[An(NO3)]2+ normalized to Ac calculated wipan class="Chemical">th LDA, TPSS,
B3LYP, and PBE0 withthe Stuttgart RSC 1997 ECP and basis set including
(ad) and excluding (nd) the most diffuse basis functions for An, and
the 6-31G*, cc-pVDZ, 6-311++G**, cc-pVTZ, and cc-pVQZ for N and O.
Δ(ΔG)rxn calculated withCCSD(T),
the cc-pV∞Z-X2C (CBS) basis set for An, and the cc-pV∞Z-DK
(CBS) basis set for N and O is included as reference (indicated as
CCSD(T)/CBS in labels). Values are reported in kcal mol–1. [Δ(ΔG)rxn = ΔGrxn,An – ΔGrxn,Ac, as indicated in eq , with An = Th to Lr.] The lines are included as a
visual aid, and do not represent function continuity.
pan class="Chemical">The difference between the predicted Gibbs free
energies of reaction
with LDA, TPSS, B3LYP, PBE0, B972, M06, and M11 withthe Stuttgart
RSC 1997 ECP and basis set including all basis functions and varying
the basis set of N and O amongst contiguous actinides show that the
Δ(ΔG)rxn for Ac/Th is within
12 from those predicted by CCSD(T)/CBS for all options tested.
Differencpan class="Chemical">es between Pa and pan class="Chemical">Th (Th/Pa) are between 19 and 36 kcal
mol–1 from those predicted withCCSD(T)/CBS. The
Δ(ΔG)rxn difference is between
−19 and 7 kcal mol–1 for Pa/U, between −8
and 17 kcal mol–1 for U/Np, between −15 and
4 kcal mol–1 for Np/Pu, between −47 and −24
kcal mol–1 for Pu/Am, and between 11 and 17 kcal
mol–1 for Am/Cm. The predicted Δ(ΔG)rxn with all options tested is between −4
and 10 kcal mol–1 for Cm/Bk, between −6 and
12 kcal mol–1 for Bk/Cf, between 11 and 46 for Cf/Es,
between −10 and 30 kcal mol–1 for Es/Fm,
between −38 and −6 kcal mol–1 for
Fm/Md, between −10 and 37 kcal mol–1 for
Md/No, and between −36 and −8 kcal mol–1 for No/Lr (as shown in Figures , S.7–S.9, and Tables S.17–S.21 in the SI).
Figure 15
Calculated ΔGrxn (left)
and difference
between contiguous actinides (right) for [An(NO3)]2+ (with An = Ac to Lr) with LDA, TPSS, B3LYP, and PBE0, the
Stuttgart RSC 1997 ECP and associated basis set, including all diffuse
functions for An, and the 6-31G*, cc-pVDZ, 6-311++G**, cc-pVTZ, and
cc-pVQZ for N and O, and CCSD(T)-FC1/cc-pV∞Z-X2C:cc-pV∞Z-DK
(indicated as CCSD(T)/CBS in labels). Values are reported in kcal
mol–1. (Δ(ΔG)rxn An1/An2 = ΔGrxn,An2 – ΔGrxn,An1, as indicated in eq , with An = Ac to Lr. The lines are included
as a visual aid and do not represent function continuity.)
Calculated ΔGrxn (left)
and difference
between contiguous pan class="Chemical">actinides (right) for pan class="Chemical">[An(NO3)]2+ (with An = Ac to Lr) with LDA, TPSS, B3LYP, and PBE0, the
Stuttgart RSC 1997 ECP and associated basis set, including all diffuse
functions for An, and the 6-31G*, cc-pVDZ, 6-311++G**, cc-pVTZ, and
cc-pVQZ for N and O, and CCSD(T)-FC1/cc-pV∞Z-X2C:cc-pV∞Z-DK
(indicated as CCSD(T)/CBS in labels). Values are reported in kcal
mol–1. (Δ(ΔG)rxn An1/An2 = ΔGrxn,An2 – ΔGrxn,An1, as indicated in eq , with An = Ac to Lr. The lines are included
as a visual aid and do not represent function continuity.)
Binding Energies in [An(NO3)]2+
Overall, it is calculated pan class="Chemical">that the [An(NO3)]2+ compounds increase in stability as the atomic number
increases (i.e.,
the Gibbs free energies of reaction, as proposed in eqs and 4a, decrease)
from Ac to Pu and from Cm to No. The stability from Pu to Am is predicted
to decrease withCCSD(T)/CBS and increase with other methods tested
(as shown in Figure ). There is a slight decrease in predicted stability (less than 6
kcal mol–1) from Fm to Md and a decrease from No
to Lr (approx. 80 kcal mol–1). For [An(NO3)]2+ compounds with solvation, the difference in predicted
ΔGrxn amongst contiguous actinides
was within 20 kcal mol–1 from those predicted in
the gas phase in most cases, with larger differences when calculated
with B3LYP/6-31G* and B3LYP/6-311++G** of approximately 40 and 50
kcal mol–1 for Ac/Th and Th/Pa, respectively, with
B3LYP/6-31G* for Cf/Es, and 30 kcal mol–1 for Md/No
with B3LYP and PBE0 with 6-311++G** (shown in Figures S.10–S.11 in the SI).
pan class="Chemical">The contribution
of the enthalpy (ΔHrxn) to the Gibbs
free energy of reaction (ΔGrxn)
of [An(NO3)](g)2+ is approximately
99%, and the contribution from the entropy term (TΔSrxn) is approximately 1% (shown
in Tables S.22–S.27 in the SI).
When applying the implicit solvation model, the enthalpy contribution
to the Gibbs free energy of reaction to [An(NO3)](aq)2+ is between 84 and 96% and the entropy term contribution
is between 4 and 16% (shown in Table S.28 in the SI).
T1/D1 Diagnostics
pan class="Chemical">The T1 and D1 diagnostic valupan class="Chemical">es for [An(NO3)]2+ are between 0.018 and 0.029 for T1 and between 0.065 and 0.136 for D1 for
all actinides except for Pa. The T1 and D1 values for [Pa(NO3)]2+ are 0.075 and 0.358, respectively. T1/D1 diagnostic limits are 0.02/0.10,[58,59] 0.05/0.15,[60] and 0.045/0.12[61] for main group, 3d, and 4d metals, respectively.
To our knowledge, there is no such set limit to determine multireference
characters for actinides. The known guidelines for main group, 3d,
and 4d metals are applied to the T1 and D1 values obtained for the [An(NO3)]2+ compounds in this study (shown in Figure ). The only compound with
both T1 and D1 values higher than limits set for 3d and 4d is [Pa(NO3)]2+. It is possible that a limit set for actinides in
the future could also find [Th(NO3)]2+, [Es(NO3)]2+, [Fm(NO3)]2+, [Md(NO3)]2+, and [No(NO3)]2+ to
have a T1/D1 diagnostic indicative of multireference character. This suggests
that [Pa(NO3)]2+, and likely [Th(NO3)]2+, [Es(NO3)]2+, [Fm(NO3)]2+, [Md(NO3)]2+, and [No(NO3)]2+ should be studied with multireference methods
(which is the focus of future work). All T1 and D1 values are included in Table S.29 in the SI.
Figure 16
T1/D1 diagnostics
for [An(NO3)]2+ (with An = Ac to Lr). Lines
represent limits for main group elements (T1 = 0.02, D1 = 0.1), 3d metals (T1 = 0.05, D1 = 0.15),
and 4d metals (T1 = 0.045, D1 = 0.12).
T1/D1 diagnostics
for pan class="Chemical">[An(NO3)]2+ (wipan class="Chemical">th An = Ac to Lr). Lines
represent limits for main group elements (T1 = 0.02, D1 = 0.1), 3d metals (T1 = 0.05, D1 = 0.15),
and 4d metals (T1 = 0.045, D1 = 0.12).
B1 Diagnostics
pan class="Chemical">The B1 diagnostic for pan class="Chemical">[An(NO3)]2+ (with An = Ac to Es) calculated as indicated in eq is between 6 and 21 for n1, between 3 and 11 for n2, between 2 and 7 for n3, and
between 1 and 5 for n4 (as shown in Figure ). As explained
in the methods, the B1 diagnostics was
designed for dissociation energies and establishesthat the system
for which the B1 is greater than 10 kcal
mol–1 presents multireference character.[62] Although there is no bond dissociation in the
proposed reaction, there are two An–O bonds, which would likely
infer an n2 for the B1 diagnostic. For n2, only
[Es(NO3)]2+ is slightly above 10 kcal mol–1 (10.68 kcal mol–1), whereas all
remaining [An(NO3)]2+ (with An = Ac to Cf) had n2B1 values below
10 kcal mol–1. All compounds tested have B1 diagnostic values below 10 kcal mol–1 for n3 and n4. The B1 diagnostic for n1 was above 10 kcal mol–1 for [An(NO3)]2+ (with An = U to Es), but n1 is an nonphysical representation for bonding in the
binding reaction proposed. Nonetheless, it is provided as reference.
All B1 diagnostic values are included
in Table S.30 in the SI.
Figure 17
B1 diagnostics for [An(NO3)]2+ (with An
= Ac to Lr). (Lines are included as visual
aid, but do not constitute function continuity.)
B1 diagnostics for pan class="Chemical">[An(NO3)]2+ (wipan class="Chemical">th An
= Ac to Lr). (Lines are included as visual
aid, but do not constitute function continuity.)
Conclusions
Computational predictions
are n class="Chemical">essential for understanding binding
selectivity preferences for actinide separations. Establishing differences
in predictive capabilities from available electronic structure methodologies
and their effect on optimization of structures containing actinide
atoms is essential for the design of selective extracting agents.
This study analyzesthe effects various methodologies have in the
prediction of population analysis, structural characteristics, and
Gibbs free energies of reaction in a systematic study of [An(NO3)]2+ structures (with An = Ac to Lr). An An IV
electronic configuration is predicted for [An(NO3)]2+ structures in the gas phase across the series except for
Fm, Md, and No that have an An III configuration; whereas in solution,
all structures except for No present an An IV configuration.
pan class="Chemical">The predicted Gibbs free energipan class="Chemical">es of reaction calculated with coupled
cluster with perturbative doubles and triples (CCSD(T)) withthe eXact-2-Component
(X2C) Hamiltonian, the all-electron, correlation-consistent basis
sets (cc-pVnZ-X2C) for the actinide atoms and the cc-pVnZ-DK basis
sets for N and O shows the same trend as that when calculated at the
CBS limit, withthe triple ζ level providing a ΔGrxn between 2 and 8 kcal mol–1 lower than those predicted at the CBS limit. Predicted Gibbs free
energies of reaction amongst contiguous actinides seem largely independent
from the basis set of the nonactinide atoms with most functionals
and show a larger dependence on the functional of choice.
Understanding
electron win class="Chemical">thdrawing effects is essential to design
selective binding agents for actinide separations, and population
analysis can greatly aid in this analysis. On the basis of the findings
in this study, utilizing NBO would minimize having to choose amongst
functional and basis set combinations, as large dependence on level
of theory of choice is observed when utilizing Mulliken and Löwdin.
Excluding and including the most diffuse basis functions in the basis
set of the actinide shows negligible variations with NBO and larger
differences with Mulliken and Löwdin. Although Mulliken population
analysis has been largely the method of choice for various population
analyses in the field, this research suggests a shift to NBO is advantageous
for improved comparisons between studies.
pan class="Chemical">The An–O1 bond
lengpan class="Chemical">th shows larger variations with respect
to the functional than with respect to the basis set of choice for
the N and O atoms. Moreover, the An–O1-predicted distances
show differences of less than 0.09 Å when including and excluding
the most diffuse basis functions for the actinide atoms. The decrease
in the An–O1 bond length and increase in O1–An–O2
angle in [An(NO3)]2+ across the actinide presents
discontinuities in An–O1 distance for [Fm(NO3)]2+, [Md(NO3)]2+, and [No(NO3)]2+, which showed a longer bond length and smaller angle
in the gas phase due to being in an An III state instead of An IV.
However, for solvated structures, an overall trend is followed from
Ac to Md but not for No, which has an An III configuration in [No(NO3)]2+ both in gas and solution when calculated withthe methods included in this study. Calculations for compounds withLr show an An IV preferred state, but structural characteristics including
interatomic distances and angles do not follow the trend including
Ac to Md, as expected given their electronic configuration.
Finally, T1/D1 and B1 diagnostics are performed
to provide insight into n class="Chemical">the multireference character of the [An(NO3)]2+ complexes studied. Future determination of
limits for the B1, T1, and D1 values for actinide systems
and multireference calculations on the same or similar complexes can
be aided by the B1, T1, and D1 coefficients included
in this study. This study provides in-depth and systematic findings
that can be used as an initial assessment for future work involving
multireference and spin–orbit effects on physicochemical and
thermochemical characteristics across the actinide series (including
other single-reference ab initio methods, as well as basis sets including
all-electron descriptions for the actinides). The results obtained
in this study will provide a strong baseline for future studies evaluating
functionals to provide recommendations for actinide-containing compounds.
Future in-depth studies for NBO predictions will encompass a more
exhaustive set of levels of theory in gas and liquid phases.
Methods
Partial chargpan class="Chemical">es, structural characteristics, and Gibbs free energipan class="Chemical">es
of reaction are calculated with various levels of theory for [An(NO3)]2+ structures (with An = Ac to Lr) in the gas
phase optimized with local density approximation (LDA),[63] the meta-GGA TPSS[64] functional, the hybrid-GGA B3LYP,[65] PBE0,[66] and B972[67] functionals,
the meta-hybrid-GGA M06[68] and M11[69] functionals, the Stuttgart RSC 1997 ECP and
associated basis set for actinide atoms (including and excluding the
most diffuse s, p, d, and f basis functions) for the actinide atoms,
and the 6-31G*,[70] cc-pVDZ,[71] 6-311++G**,[70] cc-pVTZ,[71] and cc-pVQZ[71] basis
sets for nitrogen and oxygen atoms. The ECP on the actinide atom accounts
for scalar relativistic effects by replacing 60 electrons with a relativistic
pseudopotential. Partial charges, electron withdrawing effects, and
orbital occupancies are calculated with Mulliken, Löwdin, and
natural bond orbital (NBO). Aqueous-phase calculations are included
withthe B3LYP and PBE0 functional and the 6-31G* and 6-311++G** basis
set for the nitrogen and oxygen atoms. The COSMO[72] solvation model is utilized for accounting for implicit
solvation effects.
Additionally, Gibbs free energipan class="Chemical">es of reaction
as single-point calculations
are obtained wipan class="Chemical">th coupled cluster with single-double, and perturbative
triple (CCSD(T)) method with all-electron, correlation-consistent
basis sets (cc-pVnZ-X2C)[19] (where n = ζ
level) for the actinide atoms to account for scalar relativistic effects.
The cc-pVnZ-X2C basis sets are used for the actinide atoms, and the
cc-pVnZ-DK basis sets are used for N and O. The CCSD(T) calculations
include the eXact-2-Component (X2C) Hamiltonian[73] to account for scalar relativistic effects. The spin unrestricted
CCSD(T) method [UCCSD(T)] is used for open-shell CCSD(T) calculations.[74,75] Complete Basis Set (CBS) energies are included following a two-point
extrapolation using energies from cc-pVTZ-X2C and cc-pVQZ-X2C calculations.
Values obtained at the CBS limit are referred to as cc-pV∞Z-X2C.
The Hartree–Fock energy is extrapolated using a formula from
Karton and Martin[76] showed in eq .The correlation energy is
extrapolated as
described by eq .[77]The CCSD(T) calculations
correlate the 6s6p5f
electrons of the actinide atom and the 2s2p electrons of the oxygen
and nitrogen atoms in the correlation space. The T1(58)D1(59) diagnostics for multireference
analysis is obtained withCCSD/cc-pVQZ-X2C.
pan class="Chemical">The model reaction
proposed for this study is shown in eq , with eq describing binding in the gas phase
and eq binding in an
aqueous environment.The Gibbs free energy of reaction
for eq and 3bis calculated as shown in eqs and 4b, respectively.Relative Gibbs free energies of reaction,
Δ(ΔG)rxn, between two compounds
with contiguous actinides are calculated as indicated in eqs and 5b.with An.1 and An.2 representing the
An of
the compounds being compared.
pan class="Chemical">The equation representing the
difference between including (denoted
“ad”) and excluding (denoted “nd”) the
most diffuse basis functions in the calculation of Gibbs free energy
of reaction is indicated (eq ).Ranges are defined as the difference
between
the largest and smallest data points in the calculation of partial
charges (C), bond lengths (re), and Gibbs free energies (ΔGrxn), as indicated in eqs , 7b, and 7c, respectively.Effects of including (ad) and excluding
(nd)
the most diffuse basis functions in population analysis to calculate
particle charges (C), bond lengths (re), and Gibbs free energies (ΔGrxn) are calculated as indicated in eqs , 8b, and 8c, respectively.The B1LYP-diagnostic (B1)[62] developed by Schultz and
co-workers
is utilized to provide insight into possible multireference character
of [An(NO3)]2+ structures (with An = Ac to Es).
This diagnostic is defined as indicated in eq where n corresponds to the
number of bonds being broken.[62]
pan class="Chemical">The
proposed binding reaction in this study (shown in eq ) does not provide bond dissociations.
Since the B1 diagnostic was developed
for dissociations,[62] there is no equivalent n for the proposed reaction. Therefore, n is evaluated from 1 to 4 to illustrate the dependence of the B1 diagnostic on n for the proposed
reaction. The n variable evaluated at 1, 2, 3, and
4 is indicated as n1, n2, n3, and n4, respectively.
Additional calculations for [An(pan class="Gene">NO3)]+ structurpan class="Chemical">es
are included when needed for discussion purposes, given findings obtained
for structural characteristics.
Geometry optimization calculations
are obtained wipan class="Chemical">th tight tolerancpan class="Chemical">es
and extra fine grid. The optimizations are performed without symmetry
constraints to avoid enforcing a preconceived symmetry. Harmonic vibrational
frequencies are included for thermochemical corrections and to verify
that no complex frequencies are obtained. Thermochemical corrections
are calculated for each structure at each level of theory at 298.15
K, except for CCSD(T) calculations that include thermochemical corrections
and geometries obtained withthe B3LYP functional, the Stuttgart RSC
1997 ECP including all diffuse basis functions for the actinide atoms,
and the 6-311++G** basis set for nitrogen and oxygen atoms. Harmonic
vibrational frequency calculations reveal that the optimized structures
have all real frequencies (i.e., no complex frequencies are observed).
CCSD(T) single-point calculations utilize MOLPRO2015 defaults.
pan class="Chemical">The NWChem 6.6 package[78] is used to
obtain DFT geometry optimizations, harmonic vibrational frequency
calculations, as well as Mulliken and Löwdin population analysis.
The NBO[79] population analysis is obtained
withthe Natural Bond Orbital 6.0 (NBO6) program.[80] Molpro2015[81] is used for CCSD(T)
calculations. The DIRAC16[82] package is
used for Dirac–Hartree–Fock calculations. Basis sets
and effective core potentials are obtained from EMSL[83,84]
Authors: Thibault Cantat; Christopher R Graves; Kimberly C Jantunen; Carol J Burns; Brian L Scott; Eric J Schelter; David E Morris; P Jeffrey Hay; Jaqueline L Kiplinger Journal: J Am Chem Soc Date: 2008-12-24 Impact factor: 15.419
Authors: Jennifer J Charlton; Nickolay Lavrik; James A Bradshaw; Michael J Sepaniak Journal: ACS Appl Mater Interfaces Date: 2014-10-06 Impact factor: 9.229
Authors: Deborah A Penchoff; Charles C Peterson; Jon P Camden; James A Bradshaw; John D Auxier; George K Schweitzer; David M Jenkins; Robert J Harrison; Howard L Hall Journal: ACS Omega Date: 2018-10-24