2.1. First-Row-Transition-Metal MBs
All previous theoretical and experimental data on the ground states of the first-row-transition-metal borides are summarized in
Table 1 [
21,
22,
23,
24,
25,
26,
27,
28,
29,
30]. The first study of each first-row-transition-metal boride (MB) was carried out by Wu in 2005, who studied the MB molecules via DFT methodology, i.e., B3LYP/6-311++G(3df) [
22]. In 2008, Tzeli and Mavridis, using multireference methods (MRCI), systematically studied the electronic structure and bonding of the ground and some low-lying states, up to twenty-four excited states, of all first-row-transition-metal borides (MBs). They used multireference methods employing correlation-consistent basis sets of quintuple cardinality (cc-pV5Z) [
21]. Full potential-energy curves were constructed at the MRCI/cc-pV5Z level for the lowest up to five states, while about twenty states for every MB species were examined at the MRCI/cc-pVQZ
BANO-4Z
M level of theory. At the MRCI/cc-pV5Z level, total energies, dissociation energies, dipole moments, and common spectroscopic parameters of the nine diatomic borides, MBs, M = Sc–Cu, were reported. Ground states of the MBs along with “recommended” bond distances, dissociation energies, and dipole moments were calculated, and boron atoms’ exceptional ability to participate in a variety of bonding schemes was stressed; the bonding in these MB series varied from three half bonds to full triple bonds. Furthermore, the core correlation using the cc-pwCV5Z basis set was calculated for specific molecules as well as the Scalar relativistic effects through the second-order Douglas–Kroll–Hess approximation, i.e., at C-MRCI+DKH2/cc-pwCV5Z-DK. This study [
21], using very accurate methodology, calculated bond distances, dissociation energies, dipole moments, and spectroscopic parameters in excellent agreement with experimental studies which were subsequently conducted the following decade; see
Table 1 and discussion below.
ScB: In 2008, the electronic structure and bonding of the ground and some low-lying states of ScB were calculated employing MRCI methodology, including the scalar relativistic effects and the correlation of the core electrons [
21]. The ground state,
X5Σ
–, was calculated at the C-MRCISD+DKH+Q/cc-pV5Z level of theory, and a value of 2.094 Å was found for the bond length, 3.309 eV was found for the dissociation energy with respect to the adiabatic atomic products, and 603 cm
−1 was found for the vibrational frequency. In 2021, Merriles et al. performed resonant two-photon ionization spectroscopy (R2PI) experiments to measure the predissociation threshold in ScB and found a value of
D0 (ScB) = 1.72(6) eV with respect to the ground state products [
25], while the theoretical dissociation energy with respect to the atomic ground state was 1.74 eV [
21], in excellent agreement with the experimental value of 1.72(6) eV [
25]. The bonding in the ground state consists of three half bonds [
21].
TiB: The ground state of TiB is the
X6Δ state. Its bond distance was calculated to be 2.080 Å with a dissociation energy of 2.797 eV and a vibrational frequency of 583 cm
−1 using icMRCISD/cc-pV5Z [
21]. Recently, Merriles et al. measured the predissociation threshold in TiB to be
D0 (TiB) = 1.956(16) eV via R2PI spectroscopy [
25]. Finally, in the ground state, three half bonds are formed.
VB: The its ground state of VB,
X7Σ
+, presents similar bonding behavior to the ground state of the ScB and TiB molecules, i.e., three half bonds are formed [
21]. Its bond distance is 2.043 Å, with a dissociation energy,
De, of 2.381 eV with respect to the adiabatic products, and 2.143 eV with respect to the atomic ground state products, while the vibrational frequency,
ωe, is 589.9 cm
−1 [
21]. The R2PI predissociation threshold in VB,
D0, was measured to be 2.150(16) eV [
25], in excellent agreement with the theoretical value.
CrB: The bonding of the CrB ground state,
X6Σ
+, is a
σ2 bond and two half
π bonds, i.e.,
σ2π1π1 [
21]. Using the icMRCISD+Q/cc-pV5Z methodology, the Cr-B distance was calculated to be 2.183 Å with a binding energy of 1.353 eV, a rather small dissociation energy, while the
ωe value was 405 cm
−1. The B3LYP bond distance, 2.187 Å [
22], is in very good agreement with the corresponding value obtained using the icMRCISD+Q/cc-pV5Z methodology [
21].
MnB: The relative ordering of twenty-six states of MnB has been calculated [
21]. The ground state is the
X5Π state, with a value of 2.183 Å for the bond length, 0.854 eV for the dissociation energy, and 391.9 cm
−1 for the vibrational frequency. The bonding is
σ2π1π1; however, the dissociation energy is very small. On the contrary, the first excited state,
A5Σ
−, which lies 0.09 eV above the
X state, has three bonds,
σ2π2π2, a short bond length of 1.832 Å, and a significant larger dissociation energy of 3.131 eV than the
X state obtained using the icMRCISD+Q/cc-pV5Z methodology [
21]. Note that in the
A5Σ
− state, Mn is excited at its
5D atomic state.
FeB: In 2005, the ground state,
4Σ
−, of the FeB molecule was calculated at the DFT(B3LYP)/6-311++G(3df) level [
22]. Then, in 2008, nineteen electronic states were calculated using MRCI, while the electronic structure and chemical bonding of the ground and the first excited states were examined [
21]. At the icMRCISD+Q/cc-pV5Z level of theory, the
X4Σ
− ground state values are
re = 1.743 Å and
De = 2.346 eV. In 2019, Merriles et al. measured the predissociation threshold in FeB via R2PI spectroscopy and found a value of
D0 = 2.43(2) eV [
26]. This work included the first experimental measurement of the BDE of FeB.
CoB: The ground state of CoB,
X3Δ, was calculated in 2005 via the DFT methodology [
26], and in 2008, it was calculated using icMRCISD+Q/cc-pV5Z [
21]. Eighteen states were calculated. In the ground state, a triple bond is formed with a bond distance of 1.700 Å and a binding energy of 2.849 eV. In 2011, Ng et al. observed and analyzed the electronic transition spectrum of CoB in the visible region between 495 and 560 nm using laser-induced fluorescence spectroscopy [
27]. The ground state of CoB was identified to be
X3Δ
3 with
re = 1.705 Å. The ground state’s identity was reconfirmed to be
X3Δ
3 by Dore et al. [
31]. In 2019, Merriles et al. performed resonant two-photon ionization spectroscopy experiments to measure the predissociation threshold of CoB, obtaining a value of
D0 = 2.954(3) eV [
26].
NiB: The
X2Σ
+ state of NiB is the ground state, presenting a triple bond. It was calculated via DFT methodology in 2005 [
22] and the MRCI method in 2008 [
21]. Via MRCI, twenty states were studied. At the icMRCISD+Q/cc-pV5Z level, its bond length was calculated to be 1.681 Å with a binding energy of 3.434 eV and
ωe = 803 cm
−1. Also in 2008, Balfour et al. characterized NiB spectroscopically using laser-induced fluorescence spectroscopy [
28]. The ground state of NiB was identified to be
X2Σ
+ with an electronic configuration of 1
σ22
σ21
π41
δ43
σ1,
re = 1.698 Å,
ωe = 778.0 cm
−1, and
ωexe = 4.90 cm
−1 [
28]. In 2010, Zhen et al. investigated NiB using LIF spectroscopy to resolve the rotational structure of a band belonging to a newly discovered band system with a
2Π
3/2 upper state [
32]. In 2015, Goudreau et al. [
33] investigated the 0-0, 2-0, and 3-0 bands of NiB belonging to the
2Π
3/2 ← X2Σ
+ band system assigned by Zhen et al. [
32] at high resolution. The fine structure splitting in each state was determined for the first time, confirming the assignment of the ground state as
2Σ
+ with an electronic configuration of 1
σ22
σ21
π41
δ43
σ1. Finally, in 2019, Merriles et al., via R2PI spectroscopy, measured the predissociation threshold in NiB to be
D0 = 3.431(4) eV [
26].
CuB: In 1997, Barysz and Urban investigated the spectroscopic constants and dipole moment curves of the ground states,
Χ1Σ
+, of the coinage metal diatomic molecules with boron, i.e., BCu, using high-level-correlated methods combined with quasi-relativistic Douglas–Kroll (no-pair) spin-averaged approximation [
29]. At the CCSD(T)/[9s7p3d2f/
Cu5s3p2d/
B] computational level, the values
re = 1.909 Å,
De = 1.522 eV, and
ωe = 555.0 cm
−1 were found. In 2005, Wu also studied the
X state via DFT [
22], while in 2008, Tzeli and Mavridis investigated nineteen states using the MRCI+Q methodology [
21]. At the icMRCISD+Q/cc-pV5Z level of theory, they found values of
re = 1.922 Å,
De = 2.129 eV, and
ωe = 553 cm
−1. The
De value at the icMRCISD/cc-pV5Z level was significantly larger than the corresponding values at the CCSD(T)/[9s7p3d2f/
Cu5s3p2d/
B] level due to its significantly larger basis set. In 2023, Merriles and Morse studied CuB experimentally for the first time via R2PI spectroscopy and obtained the first BDE measurement for this molecule. They found that CuB remains bound at energies that far surpass its bond dissociation energy (BDE), and bonds break only when excited at or above an excited sharp predissociation threshold (SAL). Nevertheless, a BDE value of
D0 = 2.26(15) eV was derived [
30], which was in very good agreement with the calculated value of 2.129 eV using icMRCISD+Q/cc-pV5Z [
21].
ZnB: Only one theoretical study was found for ZnB. Its ground state,
Χ2Π, was calculated via the DFT methodology, B3LYP/6-311++G(3df) [
22], obtaining a value of
re = 2.274 Å with a very small binding energy of 0.370 eV. Here, we calculated the X state at the B3LYP, TPSSh, and MN15/aug-cc-pVQZ(-PP) levels of theory. Both B3LYP and TPSSh provided the same D
e values, i.e., 0.373 eV, while TPSSh overestimated it. Here, we found that the B3LYP/aug-cc-pVQZ(-PP) methodology is in very good agreement with the available experimental data on MBs compared with the other functionals. Thus, we consider it to be our best DFT methodology. The bond distance was found to be 2.258 Å and the dipole moment was found at 1.65 D.
2.2. Second-Row-Transition-Metal MBs
All previous theoretical and experimental data on the ground states of the diatomic metal borides including the second-row transition metals are summarized in
Table 2. Below, they are discussed in detail. There is no experimental or theoretical study on TcB except a D
0 value for the
5Σ
−, obtained via DFT(B97-1). Note that Tc is a synthetic element, and all its isotopes are radioactive. In this paper, we fill this gap by studying the TcB molecule.
YB: The first report on YB was in 1969 by K. A. Gingerich [
24], who estimated the dissociation energy of the molecule to be 2.99 eV using the Pauling method of electronegativities [
24,
25]. In 2009, Kharat et al. calculated the ground spin states of the second-row (4d) transition metals (except for Tc) and their cationic and anionic counterparts at the DFT(B3LYP)/LANL2DZ level. They calculated the bond distances,
re; binding energies,
De; electron affinities (EA); ionization potentials (IP); vibrational frequencies,
ωe; and dipole moments,
μ [
34]. For the diatomic YB, a quintet (
S = 2) ground spin state was established. The report lacks details about its electronic configuration, and as such, its ground spin state electronic symmetry is not included. The associated bond distance was found to be 2.254 Å, the binding energy was 2.17 eV, the EA was 0.69 eV, the IP was 6.16 eV,
ωe = 582.4 cm
−1, and
μ = 4.65 D. The most recent investigation into the electronic structure of the YB dimer was made in 2021 by Merriles et al. [
25]. They measured the predissociation thresholds of several early-transition-metal boride diatomics using resonant two-photon ionization (R2PI) spectroscopy. For the YB molecule, a
D0 value of 2.057(3) eV was obtained. Additionally, they provided an insight into the chemical bonding and electronic structures of those same species by performing quantum chemical calculations using the DFT (B97-1) methodology. Computational results showed excellent agreement with the measurements for YB, and its ground state was computed to be the wavefunction
X5Σ
− (with a dominating 1
σ22
σ13
σ11
π2 configuration determinant), resulting in a bond distance
re of 2.306 Å, a dissociation energy
D0 of 1.96 eV, and
ωe = 517 cm
−1.
ZrB: This molecule has only been studied together with other similar species, once in 2009 by Kharat et al. [
34] and in 2021 by Merriles et al. [
25]. In the first study, a sextet (
S = 5/2) ground spin state was determined, with r
e = 2.189 Å, D
e =3.92 eV, EA = 0.48 eV, IP = 7.03 eV, ω
e = 582.4 cm
−1, and μ = 3.48 D. In the latter, the predissociation threshold revealed a
D0 value of 2.573(5) eV, and the ground electronic spin state corresponded to the
X6Δ symmetry wavefunction (with a dominating 1
σ22
σ13
σ11
π21
δ1 configuration determinant), resulting in a 2.159 Å bond distance, a 2.61 eV dissociation energy,
D0, and an
ωe value of 610 cm
−1.
NbB: Similarly to the previous molecule, there are two studies on NbB [
25,
34]. In the first study [
34], a triplet (
S = 1) ground spin state was found, with a bond distance of 1.996 Å, a binding energy of 3.40 eV, EA = 1.05 eV, IP = 7.03 eV,
ωe = 662.7 cm
−1, and
μ = 3.84 D. In the latter [
25], the predissociation threshold revealed a
D0 value of 2.989(12) eV, and the computed ground spin state corresponded to the superposition
X5Π/
5Φ (with a 1
σ22
σ13
σ11
π31
δ1 configuration determinant), due to the calculations using real forms of the 1
π and 1
δ orbitals, providing a bond distance of 1.988 Å, a dissociation energy of 3.07 eV, and a vibrational frequency of 698 cm
−1. Here, we carried out MRCISD(+Q)/aug-cc-PVQZ(-PP) calculations, and we clarified that the X state is the
X5Π state, while the
A5Φ is located 0.084(0.093) eV above the X state; see discussion below.
MoB: In the first report of MoB [
34], it was claimed that the ground state is doublet (
S = 1/2), with a 1.817 Å bond distance, a 6.40 eV binding energy, EA = 0.21 eV, IP = 8.68 eV,
ωe = 826 cm
−1, and
μ = 4.05 D. In 2011, Borin and Gobbo [
35] investigated the electronic structure of the Χ state and the low-lying electronic states of MoB and its cationic MoB
+ counterpart by employing quantum computational CASSCF protocols on the CASPT2+DKH/4
ζ-8
s7
p5
d3
f2
g-ANO-RCC
Mo/4
ζ-5
s4
p3
d2
fB level. MoB’s ground spin state was computed to be the wavefunction X
6Π (with a dominant 1
σ22
σ13
σ11
δ21
π3 configuration determinant) with a bond distance,
re, of 1.968 Å, a vibrational frequency,
ωe, of 664 cm
−1, and a dipole moment,
μ, of 2.7 D. The binding energy was also determined to be 2.18 eV.
TcB: TcB is the least studied molecule. Its only study resulted in a
D0 value calculated to be 3.31 eV [
25] via the B97-1/(aug)-cc-pVTZ-(PP) methodology for the
X5Σ
− state. Tc is the lightest element, and all its isotopes are radioactive. In this paper, we fill this research gap, and we study three states of the TcB molecule. The main spectroscopic data are provided; see discussion below and tables of
Section 3 below. Here, we found that the ground state is an
X3Σ
− state which presents a quadruple bond; see discussion below.
RuB: This molecule was studied experimentally via mass spectrometry for the first time by Auwera-Mahieu et al. in 1970 [
36]. Via the Knudsen effusion method, they determined its dissociation energy,
D0, to be 4.59(22) eV. The
ωe value of 915 cm
−1 was estimated from the values of the corresponding carbides using the
D0(A)/
D0(B) =
μAωA2/
μBωB2 equation, where
μ is the reduced mass. The internuclear distance was estimated from the values of the carbides using the formula
rMB =
rMC + ½ (
rB₂ −
rC₂), resulting in a value of 1.75 Å. Finally, they proposed that the X state is a
2Σ state. It took nearly four decades for this molecule to be inspected again, and in the 2009 work of Kharat et al. [
34], a doublet (
S = ½) ground spin state was reported for the diatomic RuB, with a bond distance of 1.761 Å, a binding energy of 6.48 eV, an
EA of 0.35 eV, an
IP of 9.06 eV, an
ωe of 910.8 cm
−1, and a dipole moment of 3.49 D. In 2012, Wang et al. [
37] studied the laser-induced fluorescence spectrum of RuB in the visible region between 500 nm and 575 nm. They determined that the ground state symmetry is
X2Δ, consistent with an electronic configuration obtained using molecular orbital energy level diagrams, while the bond length,
r0, is 1.7099 Å. In 2019, Merriles et al. [
26] used R2PI spectroscopy and accurately assigned the bond dissociation energies of the diatomic late-transition-metal monoborides from the measurement of a predissociation threshold. The measured predissociation threshold resulted in
D0 = 4.815(3) eV. Continuing their work, in 2022, Merriles et al. [
45] investigated the ionization energies and the cationic dissociation energies of the diatomic second- and third-row-late-transition-metal borides they had previously examined. Resonant two-photon ionization spectroscopy was employed, and the ionization threshold of RuB was measured to be 7.879(9) eV. Regarding the ground state, it was characterized as
X2Σ via Knudsen effusion [
36] and
2Δ
5/2 via LIF spectroscopy. Here, we clarify that the
X2Δ state is the ground state, and that it presents a quadruple bonding; see discussion in the next section.
RhB: In 1970, Auwera-Mahieu et al. [
36], via the Knusden effusion method, yielded a value of 4.89(22) eV for the
D0, dissociation energy, of RhB. The vibrational frequency, the bond distance, and the ground state were proposed to be 915 cm
−1, 1.75 Å, and
1Σ, respectively. In 2006, Chowdhury and Balfour [
38] measured the gas phase electronic spectrum of RhB in the visible region; it was elucidated that the ground electronic state is of
X1Σ
+ symmetry, with an internuclear distance of 1.691(2) Å. The following year, in 2007, Gobbo and Borin [
39] studied the low-lying
1Σ
+ states of RhB at the CASSCF/MS-CASPT2/4
ζ-ANO-RCC
Rh/14
s9
p4
d3
fB level to answer some questions raised by the previous experiments. In agreement with the experiment, their results indicated that the ground electronic state corresponded to the X
1Σ
+ wavefunction (with a dominant 1
σ22
σ21
π41
δ4 configuration determinant) with an internuclear distance,
r0, of 1.698 Å. In the same year, another study by Chowdhury and Balfour [
40] resumed their previous spectroscopic studies, with a clear focus on the intrinsic details of the emerging bands. In 2008, A.C. Borin and J.P. Gobbo [
41], in order to gain further insight into the structural and spectroscopic properties of RhB, investigated its first two atomic dissociation channels. The first regarded the adiabatic coupling of the two atoms in their ground atomic states, B(2
s22
p;
2P) and Rh(4
d8(
3F)5
s;
4F), while in the second, the rhodium atom participated in its first excited atomic electronic state, Rh(4
d9;
2D), at the CASSCF/MS-CASPT2/4
ζ-ANO-RCC
Rh/14
s9
p4
d3
fB level of theory. Results showcased that
X1Σ
+ correlates with the second atomic dissociation limit. The researchers predicted a 5.6 eV dissociation energy,
D0; a 924 cm
−1 vibrational frequency,
ωe; and a dipole moment of 4.54 D. The Mulliken population analysis yielded a charge of +0.35
e on Rh. In the 2009 work of Kharat et al. [
34], a singlet (
S = 0) ground state was reported for RhB, with a 1.745 Å bond distance, a 6.48 eV binding energy, EA = 0.85 eV, IP = 8.19 eV, and
μ = 2.84 D. Later, in the 2019 work by Merriles et al. [
26], a predissociation threshold of
D0 = 5.252(3) eV was measured with the use of R2PI spectroscopy. In 2020, two works concerning the bonding structure of RhB were published, where the formation of a quadruple bond was reported. The first study conducted by Cheung et al. [
2] explored the bonding nature of RhB(BO)
− and RhB species. With the use of PES, an electronic fingerprint was obtained, and the electron affinity of the dimer was measured experimentally to be 0.961 eV. In all computational levels, ADF, DFT, CCSD(T), it was found that the electronic ground state corresponds to an
X1Σ
+ wavefunction (with a dominant 1
σ21
π42
σ21
δ4 configuration determinant), resulting in a quadruple bond consisting of two
π bonds formed between the Rh 4
dxz/4
dyz and B 2
px/2
py orbitals and two
σ bonds between the Rh 4
dz² and B 2
s/2
pz orbitals, followed by internuclear distances ranging from 1.685 Å to 1.689 Å. At the ADF/PBE/TZ2P level, it was also possible to obtain a 5.27 eV value for the dissociation energy. The second study, carried out by Tzeli and Karapetsas [
4], investigated the bond occurring inside isoelectronic species between transition metals and the main group elements TcN, RuC, RhB and PdBe. For the RhB molecule, at various levels of theory, i.e., MRCISD, MRCISD+Q, and RCCSD(T)/aug-cc-pV5Z-PP
Rh aug-cc-pV5Z
B, the common spectroscopic constants were computed, presenting great agreement among themselves, as well as with the experimental values. Specifically, values of
re =1.6872 Å,
De = 5.490 eV, and
ωe = 942.1 cm
−1 were found, along with anharmonic corrections of
ωexe =3.78 cm
−1 and
μ = 2.965 D [
4]. It was deduced that the ground electronic state (
X1Σ
+) has a dominant 1
σ22
σ21
π41
δ4 configuration determinant and correlates adiabatically to the atomic electronic spin states B(
X2P;2
s22
p) + Rh(
a2D;4
d9), resulting in a four-fold quadruple bond. Tzeli and Karapetsas [
4] found that, except for the ground state of RhB, its two lowest excited states, i.e.,
a3Δ and A
1Δ, also present quadruple bonds [
4]. Additionally, in the ground and the first excited states of the RhB
− anion,
Χ2Σ
+ and A
2Δ quadruple bonds are also formed [
5]. In 2021, Schoendorff et al. [
42] also studied the bonding in RhB both qualitatively and quantitively at a MCSCF-IOTC/DKH-TZP-2012
Rh/Sapporo-TZP-2012
B level of theory and reached the same results as those in previous works. They concluded that the ground electronic spin state corresponded to the
X1Σ
+ symmetry wavefunction (with a dominant 1
σ22
σ21
π41
δ4 configuration determinant), with an equilibrium bond length of 1.701 Å and a binding energy of 5.165 eV. Finally, in 2022, Merriles and Morse [
45] measured the ionization potential and obtained a value of 8.234(10) eV.
PdB: Via the Knusden effusion method, the dissociation energy,
D0, of PdB was measured to be 4.89(22) eV, with
ω = 650 cm
−1 and a bond distance of 2.00 Å, while the proposed ground state was
2Σ [
36]. In 1992, Knight Jr. et al. [
43], via electron spin resonance (ESR) spectroscopy, revealed that the ground electronic state of the dimer is
X2Σ. Unrestricted Hartree–Fock (UHF) calculations were also carried out and a 1.608 Å internuclear distance was deduced. In 2009, a DFT study [
34] predicted a doublet (
S = ½) ground state with a bond distance of 1.856 Å and a binding energy of 3.33 eV. The most recent study on PdB was published in 2012 by Ng et al. [
44], marking its first electronic spectroscopic investigation using laser-induced fluorescence spectroscopy in the visible region between 465 and 520 nm. An
X2Σ
+ ground state was revealed, with
r0 = 1.7278 Å. Moreover, a molecular-orbital-energy-level diagram was designed to understand the observed ground state, and the proposed configuration was determined to be 1
σ22
σ21
π41
δ43
σ1.
AgB: In 1997, Barysz and Urban [
29] investigated the spectroscopic constants of AgB at many levels of theory and the plotted dipole moment curves of AgB using high-level-correlated methods combined with quasi-relativistic Douglas–Kroll (no-pair) spin-averaged approximation. The obtained ground state was
X1Σ
+ in all of them. At the DK-CCSD(T)-20/NpPolMe level of theory, a bond length of 2.115 Å and a dissociation energy of 0.910 eV were obtained, while the corresponding values at the DK-CASPT2/NpPolMe level were 2.098 Å and 1.684 eV. It was highly advised that both relativistic as well as correlation effects be carefully considered to obtain accurate results. Note that due to the relativistic shrinkage of
s valence shell electrons, stronger bonds are formed which would, otherwise, not be described successfully. Finally, Kharat et al. [
34] predicted via DFT a singlet (
S = 0) ground state with a 2.187 Å bond distance and a 1.60 eV binding energy.
CdB: There is only one DFT study in the literature. Kharat et al. [
34] reported a doublet (
S = ½) ground state with a 2.668 Å bond distance, a 0.22 eV binding energy, an EA of 0.09 eV, an
IP of 7.05 eV,
ωe = 198.3 cm
−1, and
μ = 1.67 D.
2.3. Third-Row-Transition-Metal MBs
Table 3 summarizes the previous experimental and theoretical data obtained for LaB, HfB, TaB, WB, ReB, OsB, IrB, PtB, AuB, and HgB. The calculations are mainly DFT apart from those of HfB [
46], PtB [
47], and AuB [
29,
47], for which CCSD(T), CASPT2, and MRCI calculations were carried out.
LaB: In 1969, K. A. Gingerich [
24] estimated the binding energy at 3.51 eV. In 2010, Kalamse et al. [
48] studied the 5
d-metal mononitrides and monoborides using DFT methodology with the B3LYP functional set and both LANL2DZ and SDD basis sets. The lowest electronic spin states at these two DFT levels of theory, as well as
EA,
IP, binding energies, and electronic configurations of the MBs, were discussed, while the orbitals involved in bond formation were identified. At the B3LYP/LANL2DZ level, it was deduced that the most stable state for LaB is
X5Σ
–, with a bond length of 2.435 Å, a binding energy of 2.49 eV,
μ = 4.29 D, EA = 1.01 eV, and IP = 5.61 eV. On the other hand, for the B3LYP/SDD level, the most stable state was found to be
X3Π, with
re = 2.336 Å and
De = 2.49 eV. In 2018, Elkahwagy et al. [
49] studied LaB and its anionic LaB
− counterpart with the diffusion Monte Carlo method in combination with three different trial functions to calculate the potential energy curves for the lowest electronic states of those species, along with some spectroscopic constants of neutral LaB. Irrespectively of the functional used, it was found that the quintet state of LaB is the ground state, while the triplet state is higher in energy, elucidating the mystery that the previous work arose. The 2021 study by Merriles et al. [
25] also suggested that the ground spin state corresponded to an
X5Σ
− symmetry wavefunction (with a dominant 2
σ13
σ11
π2 configuration determinant) with a dissociation energy,
D0, of 2.54 eV; a bond length,
re, of 2.372 Å; and a vibrational frequency,
ωe, of 521 cm
−1. The experimental part of their study yielded a 2.086(18) eV value for the dissociation energy from the predissociation threshold. Here, both the lowest triplet and quintet states were calculated, and we found that the ground one is the
X5Σ
− state.
Table 3.
Previous theoretical and experimental data on the ground states of the 3rd-row-transition-metal boride molecules, MBs (M = La, Hf, Ta, W, Re, Os, Ir, Pt, Au, and Hg): bond lengths re (Å), dissociation energies De (eV) and/or D0 (eV), electron affinities EA (eV), ionization potentials IP (eV), vibrational frequencies ωe (cm−1), anharmonic corrections ωexe (cm−1), and dipole moments μ (μFF = δE/δε) (Debye).
Table 3.
Previous theoretical and experimental data on the ground states of the 3rd-row-transition-metal boride molecules, MBs (M = La, Hf, Ta, W, Re, Os, Ir, Pt, Au, and Hg): bond lengths re (Å), dissociation energies De (eV) and/or D0 (eV), electron affinities EA (eV), ionization potentials IP (eV), vibrational frequencies ωe (cm−1), anharmonic corrections ωexe (cm−1), and dipole moments μ (μFF = δE/δε) (Debye).
MB | Methodology | Ref. | State | re | De a | D0 | ωe | ωexe | μ (μFF) |
---|
LaB | DFT: B3LYP/LANL2DZ | [48] | X5Σ− | 2.435 | 2.49 | | 511 | | 4.29 |
| DFT/B3LYP/SDD | [48] | X3Π | 2.336 | 2.10 | | 496 | | 5.02 |
| DMC(B3LYP)/CRENBS-ECPLaBurkatzki-PPB | [49] | S = 2 | 2.150 | 3.37 | | | | 4.22 |
| DMC(B3PW91)/CRENBS-ECPLa Burk.-PPB | [49] | S = 2 | 2.145 | 3.81 | | | | 4.19 |
| R2PI spectroscopy | [25] | | | | 2.086(18) | | | |
| DFT: UB97-1/AVTZ-PPLa VTZB | [25] | X5Σ− | 2.372 | 2.57 | 2.54 | 521 | | |
| Pauling method | [24] | | | | 3.51 | | | |
HfB | DFT: B3LYP/LANL2DZ | [48] | X4Σ– | 2.157 | 2.70 | | 613 | | 2.44 |
| DFT/B3LYP/SDD | [48] | X4Σ– | 2.195 | 2.64 | | 580 | | 2.68 |
| R2PI spectroscopy | [25] | | | | 2.593(3) | | | |
| DFT: UB97-1/AVTZ-PPLa VTZB | [25] | X4Σ– | 2.128 | 2.64 | 2.60 | 584 | | |
| c-CCSD(T)/wCV5Z-PPHf AV5ZB | [46] | X4Σ− | 2.144 | 2.841 | 2.840 | 607 | 2.8 | |
| MRCI/c-CCSD(T)/wCVQZ-PPHf AVQZB | [46] | X4Σ− | 2.174 | | | 610 | 3.0 | |
| BP86/def2-QZVP | [46] | | | 3.182 | | | | |
| BLYP/def2-QZVP | [46] | | | 2.803 | | | | |
| BPE/def2-QZVP | [46] | | | 3.311 | | | | |
| MN15-L/def2-QZVP | [46] | | | 3.071 | | | | |
| LRC-ωPBEh/def2-QZVP | [46] | | | 2.174 | | | | |
| DSD-PBEB95-D3BJ/def2-QZVP | [46] | | | 1.923 | | | | |
TaB | DFT: B3LYP/LANL2DZ | [48] | X3Σ+ | 2.001 | 2.49 | | 721 | | 2.68 |
| DFT/B3LYP/SDD | [48] | X5Δ | 2.184 | 2.48 | | 555 | | 1.44 |
| R2PI spectroscopy | [25] | | | | 2.700(3) | | | |
| DFT: UB97-1/AVTZ-PPTa VTZB | [25] | X5Δ | 2.085 | 3.00 | 2.95 | 754 | | |
WB | DFT: B3LYP/LANL2DZ | [48] | X6Σ− | 2.161 | 2.74 | | 526 | | 2.61 |
| DFT/B3LYP/SDD | [48] | X6Σ− | 1.990 | 2.88 | | 725 | | 2.67 |
| R2PI spectroscopy | [25] | | | | 2.730(4) | | | |
| DFT: UB97-1/AVTZ-PPW VTZB | [25] | X6Σ+ | 1.891 | 2.94 | 2.89 | 730 | | |
ReB | DFT: B3LYP/LANL2DZ | [48] | X3Σ− | 1.842 | 2.77 | | 867 | | 2.99 |
| DFT: B3LYP/SDD | [48] | X5Σ− | 1.875 | 4.18 | | 853 | | 2.29 |
OsB | R2PI spectroscopy | [26] | GS | | | 4.378(3) | | | |
| B3LYP/aug-cc-pVQZ-PP | [45] | X4Σ− | 1.770 | | | 938 | | 2.24 |
| B3LYP/LANL2DZ | [48] | Χ4Δ | 1.813 | 3.99 | | 955 | | 2.17 |
IrB | LIF spectroscopy | [50] | Χ3Δ3 | 1.7675 | | | | | |
| B2PLYP/AVQZ(-PP)M | [47] | Χ3Δ | 1.763 | | | | | |
| CCSD(T)/AVQZ(-PP) | [47] | Χ3Δ | | | 5.085 | | | |
| R2PI spectroscopy | [26] | GS | | | 4.928(10) | | | |
| Mass spectrometry | [36] | GS | | | 5.27(18) | | | |
| B3LYP/LANL2DZ | [48] | Χ3Δ | 1.806 | 4.86 | | 936 | | 1.72 |
PtB | R2PI spectroscopy | [26] | GS | | | 5.235(3) | | | |
| Mass spectrometry | [51] | GS | | | 4.91(17) | | | |
| LIF spectroscopy | [52] | Χ2Σ+ | 1.741 | | | 903.6 | | |
| B3LYP/LANL2DZ | [48] | Χ2Σ+ | 1.809 | 5.43 | | 906 | | 1.18 |
| B2PLYP/AVQZ(-PP) | [47] | Χ2Σ+ | 1.755 | | | | | |
| CCSD(T)/AVQZ(-PP) | [47] | Χ2Σ+ | | | 5.668 | | | |
AuB | Mass spectrometry | [36] | GS | | | 3.50(16) | | | |
| Knudsen cell experiment | [53] | GS | | | 3.773 | | | |
| B3LYP/LANL2DZ | [48] | Χ1Σ+ | 1.997 | 2.96 | | 559 | | 0.68 |
| B2PLYP/AVQZ(-PP) | [47] | Χ1Σ+ | 1.906 | | | 710 | | |
| CCSD(T)/AVQZ(-PP) | [47] | Χ1Σ+ | | | 3.734 | | | |
| Nonrelativistic CASPT2/PolMe | [29] | Χ1Σ+ | 2.256 | 1.261 | | 362 | 3.06 | |
| No-pair DK CASPT2/NpPolMe | [29] | Χ1Σ+ | 1.931 | 3.519 | | 676 | 4.76 | |
| No-pair DK CCSD(T)-20/NpPolMe | [29] | Χ1Σ+ | 1.960 | 2.709 | | 663 | 4.01 | |
| R2PI spectroscopy | [30] | Χ1Σ+ | | | 3.724(3) | | | |
HgB | B3LYP/LANL2DZ | [48] | Χ2Σ+ | 4.381 | 0.002 | | 19 | | 0.27 |
HfB: The B3LYP/SDD methodology [
48] was used to predict
X4Σ
– as the ground state of HfB with a bond length of 2.195 Å,
μ = 2.60 D, EA = 1.05 eV, IP = 5.01 eV, and a binding energy of 2.64 eV. The researchers found that, in contrast to the rest of the 5
d-metal monoborides, it is the 5
d orbital of the metal that loses an electron in the case of HfB. In the 2021 study by Merriles et al. [
25], the authors measured the predissociation threshold, i.e.,
D0(HfB) = 2.593(3) eV, and the calculated ground spin state corresponded to the
X4Σ
− symmetry wavefunction (with a dominant 2
σ13
σ21
π2 configuration determinant) with a bond distance of 2.128 Å, a dissociation energy of 2.60 eV, and a vibrational frequency of 584 cm
−1 at UB97-1/AVTZ-PP
LaVTZ
B. In 2022, Ariyarathna et al. [
46] conducted a comparative study on the outcomes of several computational methods on the basis of high-level, multi-reference configuration interaction theory and coupled cluster quantum chemical calculations, with large quadruple-
ζ and quintuple-
ζ quality-correlation-consistent basis sets, as well as DFT, with numerous exchange-correlation functionals that span multiple rungs of “
Jacob’s ladder”, through the inspection of HfO and HfB, to investigate their performance on species containing third-row transition metals. Ab initio studies of HfB showed, unanimously, that
X4Σ
– is the ground electronic state, owing to a 1
σ22
σ13
σ21
π2 configuration dominant determinant with a bond length of 2.144 Å, dissociation energy at 2.841 eV, and
ωe = 607 cm
−1 at the c-CCSD(T)/wCV5Z-PPHf AV5ZB level. DFT calculations were performed on the closed-shell single-reference ground state to evaluate the errors in the predictions from distinct density functionals. The resulting trends were discussed, plotted, and compared.
TaB: DFT calculations predict different states to be the ground state of TaB depending on the methodology. B3LYP/LANL2DZ predicted
X3Σ
+ to be the ground state, with a 2
π45
σ16
σ1 electronic configuration,
re = 2.001 Å, and
De = 2.49 eV. However, at the B3LYP/SDD level, the calculated ground state was
X5Δ state, with
re = 2.184 Å,
μ = 1.44 D,
ΕA = 1.43 eV,
ΙP = 7.35 eV, and
De = 2.48 eV [
48]. In 2021, Merriles et al. [
25] determined the
D0 value to be 2.700(3) eV, and they found that at the UB97-1/AVTZ-PP
TaVTZ
B level, the ground state corresponded to
X5Δ (with a dominant 2
σ13
σ21
π21
δ1 configuration determinant) with
re = 2.085 Å,
De = 2.95 eV, and
ωe = 754 cm
−1.
WB: In WB, as in TaB, DFT calculations predict different states to be the ground state, depending on the methodology. Kalamse et al. [
48], at both the B3LYP/LANL2DZ and SDD levels, found that the ground state is
X6Σ
−, where
re = 1.990 Å,
μ = 2.67 D, and
De = 2.88 eV at the B3LYP/SDD level [
50]. In 2021, Merriles et al. [
25] measured
D0 = 2.730(4) eV and calculated the ground state to be
X6Σ
+, with a dominant 2
σ13
σ21
π21
δ2 configuration determinant,
re = 1.891 Å,
De = 2.89 eV, and
ωe = 730 cm
−1, using the UB97-1/AVTZ-PP
WVTZ
B methodology [
25]. Here, we found that the ground state is the
X6Π state, while the
X6Σ
+ state lies 0.137 eV above the X state; see tables of the
Section 3 and discussion below.
ReB: There is only a single theoretical study on the ReB molecule at a DFT level; however, different basis sets predict different states to be the ground state. B3LYP/LANL2DZ predicted the ground state to be
X3Σ
−, with
re = 1.842 Å and
De = 2.77 eV, while B3LYP/SDD predicted
X5Σ
− to be the ground state, with
re = 1.875 Å and
De = 4.18 eV [
48]. Here, we found that the ground state is
X5Σ
−, while the
a3Σ
− state lies 0.099 eV above the X state; see tables of
Section 3 and discussion below.
OsB: Kalamse et al., via B3LYP/LANL2DZ and B3LYP/SDD, predicted that the ground state of OsB is the
Χ4Δ state. It corresponds with a
π4δ35
σ16
σ1 electronic configuration, with
re = 1.813 Å,
ωe = 955 cm
−1,
μ = 2.17 D, and
De = 3.99 eV at the B3LYP/LANL2DZ level [
48]. In 2019, Merriles et al. performed R2PI spectroscopy experiments to measure the predissociation threshold, and it was found to be
D0 = 4.378(3) eV [
26]. Furthermore, they investigated the electronic ground state at the B3LYP/Def2TZVPP [
26] and B3LYP/aug-cc-pVQZ-PP levels [
45], and they found that it is a triply bonded 1
σ22
σ21
π41
δ23
σ1, at the
X4Σ
− state, which contradicts with the prediction of Kalamse et al. [
48], with a bond distance of 1.770 Å. In 2022, Merriles et al. measured, for the first time, the ionization energy of OsB using resonant two-photon ionization spectroscopy, obtaining a value of
IE (OsB) = 7.955(9) eV [
45].
IrB: In 1969, Auwera-Mahieu et al. determined the dissociation energy of IrB to be 5.27(18) eV via a mass spectrometric study at high temperatures [
36]. In 2005, Ye et al. investigated IrB using LIF spectroscopy [
50]. In this study, the ground state of IrB was found to be
X3Δ
3, with an electronic configuration of 1
σ21
π41
δ32
σ1 and
re = 1.7675 Å. In 2010, using the B3LYP/LANL2DZ methodology, it was also found that the most stable state for IrB is
Χ3Δ raised from a
π4δ35
σ26
σ1 electronic configuration, with
re = 1.806 Å,
μ = 1.72 D,
ΕA = 5.06 eV,
ΙP = 4.66 eV, and
De = 4.86 eV [
48]. In 2011, Pang et al. investigated the electronic transition spectrum of IrB in the spectral region between 400 and 545 nm using LIF spectroscopy [
54]. Its ground state was also identified to be
X3Δ
3 with an electronic configuration of 1
σ22
σ2π4δ33
σ1. In 2019, Merriles et al., using R2PI spectroscopy, measured the predissociation threshold of IrB, obtaining a value of
D0 = 4.928(10) eV [
26]. In 2020, Wang et al. investigated the nature of the chemical bonding in IrB, employing high-resolution photoelectron imaging and theoretical B2PLYP and CCSD(T)/aug-cc-pVQZ(-PP) calculations. They calculated a bond distance of 1.763 Å using B2PLYP and a dissociation energy of 5.085 eV at the CCSD(T) level of theory, in good agreement with the experimental values [
47]. In 2022, Merriles and Morse measured, for the first time, the ionization energy of IrB using R2PI spectroscopy, obtaining
IE = 8.301(15) eV [
45].
PtB: In 1968, via Knudsen effusion mass spectrometry, McIntyre et al. measured the dissociation energy of gaseous PtB to be 4.91(17) eV [
51]. Via the B3LYP/LANL2DZ (B3LYP/SDD) levels of theory, the ground state was assigned to be
Χ2Σ
+, derived from a
π45
σ2δ46
σ1 electronic configuration, with
re = 1.809(1.815) Å and
De = 5.43(4.86) eV [
48]. In 2012, Ng et al. investigated the optical spectrum of PtB in the visible region between 455 and 520 nm using LIF spectroscopy [
52]. The ground state of PtB was identified to be
Χ2Σ
+, determined using an electronic configuration of 1
σ22
σ21
π41
δ43
σ1, with
re = 1.741 Å and
ωe = 903.60 cm
−1. In 2019, Merriles et al. performed R2PI spectroscopy measurements, and they found
D0 = 5.235(3) eV [
26]. In 2020, Wang et al. investigated the nature of the chemical bonding in PtB, employing high-resolution photoelectron imaging and theoretical calculations using the B2PLYP and CCSD(T)/aug-cc-pVQZ(-PP) methodologies [
47]. They calculated a bond distance of 1.755 Å using B2PLYP and a dissociation energy of 5.668 eV at the CCSD(T) level of theory [
47]. In 2022, Merriles and Morse measured, for the first time, the ionization energy of PtB using R2PI spectroscopy, obtaining a value of
IE = 8.524(10) eV [
45].
AuB: In 1969, via mass spectrometry at high temperatures, Auwera-Mahieu et al. measured the dissociation energy of AuB to be 3.50(16) eV [
36]. In 1971, Gingerich investigated AuB using a combination of Knudsen effusion and mass spectroscopic techniques. The reaction enthalpies determined by the second and third law method yielded
D0 = 3.77 eV [
53]. In 1997, Barysz and Urban investigated the spectroscopic constants and dipole moment curves of the AuB ground state,
Χ1Σ
+, using high-level-correlated methods combined with quasi-relativistic Douglas–Kroll (no-pair) spin-averaged approximation [
29]. At the CCSD(T)/[13s11p7d4f/
Au5s3p2d/
B] computational level, they found values of
re = 1.960 Å,
De = 2.709 eV,
ωe = 663.0 cm
−1, and
ωexe = 4.01 cm
−1. In 2010, via B3LYP/LANL2DZ and SSD, values of
De = 2.96 eV and 3.04 eV, respectively, were calculated [
48]. In 2020, Wang et al. investigated the nature of the chemical bonding in AuB, employing high-resolution photoelectron imaging and theoretical calculations [
47]. They calculated r
e = 1.906 Å using B2PLYP)/aug-cc-pVQZ(-PP) and a dissociation energy of 3.734 eV at the CCSD(T) level of theory [
47]. This dissociation energy was in excellent agreement with the experimental value of 3.724(3) eV measured by Merriles and Morse in 2023 [
30], who examined the AuB molecule experimentally using R2PI spectroscopy. They found that it remains bound at energies that far surpass its bond dissociation energy (BDE), and bonds break only when excited at or above an excited sharp predissociation threshold (SAL) [
30].
HgB: There is only one theoretical study on HgB. The ground state was assigned to be the
Χ2Σ
+ via the B3LYP/LANL2DZ and B3LYP/SDD methodologies. Values of
re = 4.381 (2.535) Å,
ωe = 19 (177) cm
−1,
μ = 0.27 (1.20) D, EA = 0.63 (0.90) eV, IP = 7.10 (7.40) eV, and D
e = 0.002(0.17) eV were calculated at the B3LYP/LANL2DZ(B3LYP/SDD) levels of theory [
48]. The differences between the two methods indicate that more accurate calculations should be performed using larger basis sets than the double zeta quality of the LANL2DZ and SDD basis sets.