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Quantum Dynamic Approach of B2N(∓,0) and N2B(∓,0) Clusters Study: A Symmetry Breaking due to the JAHN-TELLER Effect

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18 April 2023

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18 April 2023

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Abstract
Boron nitride clusters play an important role as precursors in the formation of ultra-hard thin solid boron nitride films, which have received considerable attention in material science. In this contribution, we investigated the ground and low-lying electronic states of B2N(∓,0) and N2B(∓,0). Triatomic NBN and BNB have been previously investigated using a variety of spectroscopic and calculational methods, and it is generally agreed that both of them are linear in their ground electronic states. The six ions including B2N (-), B2N (+), B2N (0) , BN2 (-), BN2 (+) and BN2 (0) have been studied and been also compared with one another in terms of various basis sets and predication of the symmetry breaking (SB) phenomenon. Artifactual symmetry breaking along the v3 coordinate is observed in the ab initio wave functions for the neutral ground state up to the coupled-cluster level of theory, even when Brueckner orbitals are used. In the D∞h point group of B2N(∓,0) and N2B(∓,0) variants, the unpaired electrons are delocalized, while in the asymmetric C∞v point group, they are localized on either one of the B atoms or N atoms of B2N(∓,0) and N2B(∓,0) , respectively. Structures with broken symmetry,C∞v, can be stable by interaction to the D∞h point group. In viewpoint of quantum chemistry, the second-order Jahn-Teller effect permits the unpaired electron to localize on boron atom, rather than being delocalized. Finally, from a statistical thermodynamical analysis, we calculated the thermochemical stabilities of those six ions.
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1. Introduction

1.1. The structure of boron nitride clusters

It is generally agreed that BNB and NBN are linear in their electronic states, but the controversy as to whether their geometries are symmetric or asymmetric have not yet been definitively settled [1-10]. Six ions including B2N (-), B2N (+), B2N (0) , BN2 (-), BN2 (+) and BN2 (0) compounds have been studied as the most complex items of (SB), both real and artifactual, due to pseudo second-order Jahn–Teller effect. Although various experimental or theoretical investigations were done for these issues [7-10], there are no quantum reports of this phenomenon through various basis sets calculation [11-19]. Paldus [9] investigated the molecular system of B2N (0) through multi-reference coupled cluster optimization with RMR Hamiltonian & CCSD (T) using cc-pVNZ, (N=2-5). In other approaches of CCSD (T), method, it has been also exhibited an asymmetric configuration of unequal BN bound length [1, 3]. B2N(0) structure has been approved by Raman technique [4] which can be also synthesized according to the B ( 2 P ) +   N ( 4 S) B N ( 1 Σ + ) and B ( 2 P ) +   B N ( 1 Σ + ) B N B ( 2 Σ ( u ) + ) reactions [12]. The mathematical extrapolation suggested by Schlegel for the PMP4 calculation can be arranged as: E P M P 4 E U M P 4 + E P M P 3 E U M P 3 and E E 2 + E 3 1 E 4 E 2 . The related optimized parameters are also confirmed based on Figure1. The UHF/6-31G* calculation for spin expectation for <S2> are collected in Table 1 and Figure 1.
An accurate work on the electronic structure of Bx N3-x (x = 1, 2) was exhibited by Martin et al [1, 3, 5, 7 and 10] using both theoretical spectroscopic measurements.
Asmis [2] confirmed the ground state structure of   B 2   N both by photoelectron analysis and theory and indicated its electronic configuration as ( X ~ 1 g +   ). He also demonstrated the situation of B2N (0) ( X ~ 2 u +   ) and ( A ~ 2 g +   ) in excited state by a linear symmetry combination as reaction as follows; X ~ 1 g +   X ~ 2 u + +   e and   X ~ 1 g +   A ~   2 g + +   e . In other side, the IR data exhibited a spectrum at 6000 cm−1 in A   ~ 2 g + X   ~ 2 u + [7, 8]. The Walsh’s idea [17] confirmed all B N ( , 0 , + ) variants of ( X ~ 2 u + ) to ( X ~ 1 g +   ) for B2N (0) and   B 2   N , respectively.
Löwdin [18] exhibited; such broken-symmetry (BS) usually has a lower energy compared with the symmetry-adapted (SA). It is notable the SB phenomenon, is due to the restricted hartree fock or in opposite the ROHF potential energy surfaces (PESs) for the linear ABA type (Such as NB2 or BN2). Wigner [19] confirmed that the Pauli principle and being simultaneously an Eigen function of <S2> and <SZ> can be written as:   ψ S , M x 1 ,   x 2 , . . x N   = ( f N S ) 1 i = 1 f N S Ф i ( r 1   ,   r 2 ,   . . r N ) Θ i ( σ 1 ,   σ 1 , . . σ N ) .
Where, Ф i is the spinless Schrödinger equation and Θ i is spin eigenfunctions, and f N S is the number of spin Eigen-functions [19]. In this article, we focus on the <Sz> and <S2> quantum numbers of various BN compounds (Table 1).
1.2 Thermochemical Considerations
Seifert et al.[20] Calculated the physical and chemical properties of boron-nitrogen clusters based on thermochemical studies. For B2N, basically 3 different structures can be written as: BBN → B2 + N; (b) BBN→B + (BN); (c) BNB→(BN) + B. For BN2, the following three fragmentation reactions were considered: (a) BNN→B + N2; (b) BNN→(BN) + N; (c) NBN →(BN) + N. It is confirmed generally, BNN should be stronger than NBN, and in the other side, BNB will be more stable than NBB. This is in agreement with the data, that B2N is appeared in mass spectra, while BN2 is not. We also calculated the thermochemical properties of our model based on Seifert work.

1.2. Potential energies surfaces (PESs)

PESs of linear triatomic XYX has been done for the cutting along the symmetrical and asymmetrical stretching modes. We mentioned the linear of X-Y and Y-X as R1 and R2, respectively. Cutting of the symmetrical stretching is oriented by the parameters same as R =R1=R2, and the energy minimum on the PEC E(R) describes the symmetrical optimized for R=Re. We also define these stretching coordinates as: ∆(R)=R1-R=R-R2. As well as the two PECs, defined by E(R) and E [∆(R)] , along the R and ∆ orientation, respectively. Consequently, the PEC has been labeled as E( R) or V (R) for the symmetrical stretching form and as well as the E [∆(R)] or V [∆(R)] has been defined for the asymmetric al form. (Figure 2).

2. Computational details and Methods

CASSCF wave functions have been accomplished as a basic calculation for estimating the energies along the BN–B coordinating changes. Since the definition of active space is needed for the CASSCF wave function, all the valence orbitals of the constituent atoms, i.e., 2s 12p have been considered clearly. EPR-III (and II) basis sets of Barone’s model [21] shown the most compatible data for electrostatic potential fitting (ESP).
The EPR(II) is a double-ζ basis set with polarization for B to F [21, 22] that is needed for N2 B ( , 0 ) B2 N ( , 0 ) calculation. EPR(III) is also a triple-ζ including diffuse parameter, of d-orbital, and compared with EPR(II), s-part improved for better energy minimization [20-24].
The correlation of valence basis sets have been investigated by Dunning and coworkers, named by cc-pVxZ, where x =2, 3, 4, 5 & 6 where used in this work. Additionally, these are includes of basically contracted sets of [3s2p1d] (cc-pVDZ), [4s3p2d1f] (cc-pVTZ), [5s4p3d2f 1g] (cc-pVQZ), and [6s5p4d3f 2g1h] (ccpV5Z) that are constructed through adding shell layers orbitals of s,p,d,... to the atomic Hartree–Fock wavefunction. Moreover, the polarization factors, which increase from 1d-cc-pVDZ to 4d-cc-pV5Z are added.
In other sides, the active space for the CASSCF (active electrons / active orbitals) should be defined for all valence orbitals in the post HF methods, such as 11/ 12 for B2N(0) and 10/ 12 for B2N(+) and so on.
The various basis sets in their effect to symmetry breaking of artifactual or trial wave function, the B2 N ( , 0 ) have been optimized through several level of theories such as CASSCF(11/12)/ccPVQZ for B2 N ( ) , CASSCF(11/12)/AUG-ccPVTZ for B2 N ( 0 ) and CASSCF (10/12)/ccPVTZ for B2 N ( + ) [25, 26]. For this purpose, the self correlation consistent orbitals are well increased both in size and accuracy to converge systematically. The augmented functional sets are used from cc-pVNZ (N=2-6) by the addition of a single diffuse orbitals for the anions and in other hand for each item, only the polarization orbitals were used. The configuration interaction (CI) including single and double items [27] have been also used for estimating several physical parameters such as natural bounding orbital (NBO), Atoms in molecules by Bader (AIM) [28], NPA or natural population analysis, electrostatic potentials, and electrostatic potential-derived charge using the Merz-Kollman-Singh[29], chelp[30], or chelpG[31]. The Hyperpolarizability has been calculated via CISD, QCISD, MP2 and CASSCF levels of calculations. The AIM of Bader’s theory was used for measuring the critical point maps to predict the atomic behaviors in B2 N ( , 0 ) species [28].
The atomic charges can be computed over several species of N2 B ( , 0 ) and B 2 N ( , 0 ) using abinitio quantum chemical packages such as Gaussian or GAMESS-US [32]. The potential surfaces(PS) of B2N and BN2 have been studied using the post Hartree Fock methods, such as CASSCF, MP4, PMP4, and QCISD. Spin contamination is shown to present severe problems with the MP4SDQ procedure.

3. Results and Discussion

3.1. Molecular orbital description

3.1.1. B2 N ( , 0 )

Definition of the PS was exhibited to be not entirely enough at the UHF, more not qualitatively. In our calculation B2N variants mostly are found to have a symmetric linear coordination in its ground state ( X   ~ 2 u + ) . Sometimes the asymmetric linear structure possibly being appeared a small amounts at higher temperatures. The B2 N ( 0 ) configuration term of ground state ( X   ~ 2 u + ) with electrons occupancy with the lowest excited state is: 1 σ g 2 , 1 σ u 2 , 2 σ g 2 , 3 σ g 2 , 2 σ u 2 , 1 π u 4 , 4 σ g 2 , 3 σ u 1 that predicted to be A ~ 2 Σ ( g ) + , with an orbital occupancy of 1 σ g 2 , 1 σ u 2 , 2 σ g 2 , 3 σ g 2 , 2 σ u 2 , 1 π u 4 , 4 σ g 1 , 3 σ u 2 . In addition,   B ~ 2 П g exited state can be written 1 σ g 2 , 1 σ u 2 , 2 σ g 2 , 3 σ g 2 , 2 σ u 2 , π u 4 , 4 σ g 2 , 1 π g 1 (above the A   ~ 2 Σ g + ) is subject to the Renner-Teller effect and further exited state depends on the ( 4 П g )   of triplet form. The electron Configuration energies of B 2 N ( , 0 ) both in ground and exited states, with HOMO/LUMO amounts are listed in Table 2.
Seifert confirmed that BNB molecule (Figure 1e.) is much more stable compared with BBN (Figure 1c), and that BNB will not dissociate automatically in BN + B or N. +B2. Bent quartet B2N (2B4) : (a1)2(a1)2 (b2)2(a1)2(a1)2(b2)2(a1)(b1)2(b2)(a1) is also found much more stable compared to other species due to the effect of polarization orbitals. Inspection of (<S>2) denotes an excessive amount of spin contamination, actually increases, rather than decreases, spin contamination. Since B2 is known to have a very low-lying ( X   ~ 5 u ) state besides the ground ( X   ~ 3 g ) state, this fact can be interpreted from connecting the ( X   ~ 5 u ) B2 to the 4S nitrogen atom. Indeed, a ( X   ~ 6 g + ) state B2N(C∞v) ;{(σ)2 (σ)2 (σ)2 (σ)2 (σ)2 (σ)2 (π)2 (σ) (π)2} was found to lie only 23.0 kcal mol- 1 above the doublet state with high value of <S>2. For the sextuplets contaminating B2N(C∞v) ( X   ~ 6 g + ) , the dynamic correlation would be even smaller. Indeed, B2N (C∞v) ( X   ~ 2 g + ) lies 44.9 kcal mol-1 above B2N(C∞v) ( X   ~ 6 g + ) at the UMP4 level, and 69.1 kcal mol- 1 at the PMP4 level. At this situation, B2N has a symmetric linear (D∞h) structure with ( a   ~ 2 u + ) ; ground state with bond distance 1.31 angstrom and frequency around 20201 cm-1 . It is notable that the B2N (   a   ~ 2 u + ) ; ) can be stabilized by resonance configuration as follows:
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For the quartet state, the C2v structure B2N (2B4) will be most stable. It is isoelectronic with B3 except for two unpaired ,while B2N- is isoelectronic with C3 ).

3.1.2. N2 B ( , 0 )

Although our calculations confirm the more stability of BNN than NBN at the global minimum, at the casscf/ccpvxz (x=3, 4) levels, the linear quartet structures of BN2 (D∞h) (4 Π g ) (Tables 1&2) exhibited an symmetrical structure, while (C∞v) (4 Σ g ) shown asymmetrical situation and are predicted to be most stable. At the casscf/cc-pvxz (x=4,5) levels on the other hand, the BN2 (D∞h)(4 Π g ) and (C∞v)(4 Σ g ) is reversed and the bent doublet structure 2B2(C2v) is stabilized. During spin rotation, the symmetric linear doublet form of BN2 (D∞h)(2 Π g ) approaches towards (C∞v)(4 Σ g ) . In addition, an asymmetric linear doublet (C∞v)(2 Π g ) can only be found after considerable amount, even with a lower energy by having a nonzero gradient on the bond angle. At the correlated optimization, BN2 (C∞v)(2 Π g ) convert to be the most stable structure at this point and through spin rotation, BN2 (D∞h)(2 Π g ) has only a little different with above items. Both of them are due to RennerTeller effect that theire frequencies are imaginary. As it can be seen in Table 2, a lower energy exists for BN2 (D∞h)(2 Π g ) at the Hartree-Fock level and also the Hartree fock frequencies may give imaginary variables due to the problem with (C∞v)(2 Π u ) too. At the MP4SDQ/EPR-II//QCISD/EPR-II levels (Table 2), the bent structure is less stable that the linear one. At the MP4SDQ/EPR-III//QCISD/EPR-III levels, the Hartree-Fock result is confirmed at the PMP4 level. At both the CASSCF (11, 12)/UHF levels, the linear structure becomes distinctly more stable, by 6.5 and 6.1 kcalmol-I, respectively. It is remarkable that the BN2 (D∞h)(2 Π g ) can be stabilized by resonance configuration as follows:
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The lowest-lying states Renner-Teller distortions, harmonic frequencies, IR, and Raman are listed in Table 3.

3.2. Thermochemical studies of B2N and BN2

The concerned formulas are exhibited in many textbooks of statistical quantum thermodynamics; expressions may also be found Herzberg book [33, 34] that was used in the present work. Table 4 data exhibit the calculated energies of related reaction at the MP4/6-31G*, PMP4/6-31G*, CCD/6-31G*, and CCD + ST(CCD)/6-31G* levels, along with the LCAO-LDA.
Comparing the quantities optimization of Seifert et al. with our data in this work, it is confirmed that BNB {(D∞h) (2 Σ g ) } is much more stable than BBN ((C∞v) (2 Σ g + ) ), and therefore BNB will not dissociate automatically in either BN + B or B2 + N.

3.3. Quantum symmetry breaking of N2 B ( , 0 ) and B 2 N ( , 0 ) and partial charges

One of the targets of this work is to illustrate the difference among the electromagnetic situation of the B 2 N ( , 0 ) species due to changing basis sets and methods and also the quantum SB report due to trial wave function. In D h position of B 2 N ( , 0 ) , the unpaired electron is delocalized, while in the asymmetric C v , it is localized on either one of the B atoms. C V by SB structure becomes stronger through changing to D h . Based on quantum chemistry theories, the second-order Jahn-Teller effect allows the unpaired electron to localize on boron atom, rather than being delocalized (Table 2 and Figure 3a,b).
The unpaired electron of nitrogen in B 2 N (   0 ) ( D h ) is delocalized and it is localized in the asymmetric ( C v ) for both of B 2 N ( , 0 ) and B 2 N ( ) species. Moreover, there is a restriction for the unpaired electron of nitrogen of BNB for delocalization between D h and C v symmetries states. These limitations between localized and non-localized situations increase the SB effect of the B 2 N ( , 0 ) species. Meanwhile, ESP, forces, γ = ( V B V N ) / r B N , attraction and repulsion energies (eV) of B 2 N ( , 0 ) in ground and exited states are listed in table 2. The MESP fitting for B 2 N ( , 0 ) and the summation of partial charges for two boron and one nitrogen ( B δ q 1 N δ q 2 B δ q 3 ) in all models from = 0.0   t o   0.07   are zero (Table 2). Obviously, the summation of partial charges in B δ q 1 N δ q 2 B δ q 3 for B 2 N (   0 ) radical is not 0.0 and it has changed according to: (0.23+0.23+0.52=0.98) for u = 0.0 , (0.24+0.23+0.52=0.99) for u = 0.02 . The changes among u , k and x is due to various methods and basis sets that are used in our work. Certainly, it is related to the the summation of partial charges in B 2 N (   0 ) radical that is far from 0.0 and varies between 0.00 and 0.16. It could be due to the fact that the unpaired electron of nitrogen is localized while B 2 N (   ) is under the influence of the unpaired electron.
Interestingly, for the exited state of B 2 N (   0 ) , changing of MESP for both exited and ground states of (   B ~ 4 П g ), ( X   ~ 2 u + ) , respectively are small. The sum of partial charges (in B δ q 1 N δ q 2 B δ q 3 ) for all items from = 0.0   to = 0.2   are -1, however, the total partial charges of B δ q 1 N δ q 2 B δ q 3 for B 2 N (   ) are not -1. The nitrogen of B 2 N (   , + , 0 ) is always positive for radical and anion and negative for cation, while in exited states, the sum of partial atomic charges are positive for all three forms. As it can be seen in Figure 4, radical or anion B2 N ( , 0 ) has not been appeared from these kind calculation, though, for cation, there is a critical point at 90 ° for MP4DQ and MP4DSQ methods.
From the SCF calculation, the minimum energy related to a bent structure with an angle around 90 ° , however, for the QCISD(T), MP4DQ, MP4DSQ and HF/aug-cc-pVTZ calculations (Figure 2), the linear situation has the lowest energies for radical and anion . By consideration wave function, when the BNB has D h , the real wave-function might be converting as an irreducible representation of the D h . Table 5 presents data for the association enthalpy, entropy, and free energy from the statistical thermodynamic and partition functions, as well as values for the absolute entropy [35-44].

5. Conclusions

The potential surfaces of B 2 N ( , 0 ) and N 2 B ( , 0 ) , have been studied using several post HF and basis sets methods. CASSCF optimization exhibited SB phenomenon for linear BNB containing an unequal bond length. We found for yielding accurate data doing perturbation theory (CASSCF+PT2) calculation and multi-reference (CI) with (CASSCF+1+2) wave functions are needed. In summary, we have clearly shown , where the SB problem is hidden , usual way to circumvent of peculiarities are the most important feature of this work. In particular, we find the low value for the anti-symmetric stretching fundamental frequency very encouraging, providing an additional support to the idea of actual symmetry breaking in the BNB ground state.

Author Contributions

Majid Monajjemi: Conceptualization and idea, Methodology, , Supervision. Fatemeh Mollaamin: Methodology, Software, Formal analysis, Investigation, Data Curation, Writing-review and editing, Visualization, Resources.

Funding

This research received no external funding.

Conflicts of Interest

The authors declare no conflict of interest.

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Figure 1. Stationary points for BN2, NB2, and B3; Bond distances in Angstrom units.
Figure 1. Stationary points for BN2, NB2, and B3; Bond distances in Angstrom units.
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Figure 2. The cuts of the PES along the symmetric ® and asymmetric ( ) stretching by E( R) and E( ) , respectively.
Figure 2. The cuts of the PES along the symmetric ® and asymmetric ( ) stretching by E( R) and E( ) , respectively.
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Figure 3. The B2 N ( , 0 , + ) relative energies versus B-N-B bond distance in (a) for cation, (b), for radical.
Figure 3. The B2 N ( , 0 , + ) relative energies versus B-N-B bond distance in (a) for cation, (b), for radical.
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Figure 4. Relative energies of B2 N ( ,   + ) versus B-N-B bond angle in various levels of theory.
Figure 4. Relative energies of B2 N ( ,   + ) versus B-N-B bond angle in various levels of theory.
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Table 1. Electronic configurations and expectation values for <S2> by casscf/cc-pvxz (x=3) level of theory
Table 1. Electronic configurations and expectation values for <S2> by casscf/cc-pvxz (x=3) level of theory
Item molecule Point group Term < S 2 > a < S 1 2 > b < S A 2 > c Electronic configuration
(a) B3 D∞h 2 Π g 1.80 1.80 0.84 g)2u)2g)2g)2u)2g)(σu)(πu)3
(b) B3 D∞h 4 Π u 3.80 3.75 3.70 g)2u)2g)2g)2u)2g)(σu)(πu)3
(c) BN2 C∞v 2 Π g 0.85 0.80 0.75 (σ)2 (σ)2 (σ)2 (σ)2 (σ)2 (σ)2 (π)4 (σ)2 (π)
(d) BN2 Cs 4 A 2 1.35 1.30 0.90 (aʹ)2 (aʹ)2 (aʹ)2 (aʹ)2 (aʹ)2 (aʹ)2 (aʹ)2 (aʺ)2 (aʹ)2 (aʹ)2 (aʺ)2
(e) BN2 D∞h 2 Π g 0.90 0.90 0.81 g)2u)2g)2g)2u)2g)2u)4u)2g)
(f) B3 D∞h 2 Π g 1.80 1.80 0.85 g)2u)2g)2g)2u)2g) (σu) (πu)3
(g) B3 D∞h 4 Π g 3.80 3.80 3.70 g)2u)2g)2g)2u)2g) (σu) (πu)3
(h) BN2 C2v 2 A g 1.40 1.30 1.10 (a1)2 (b1)2(a1)2(a1)2(b2)2(a1)2(b1)2
(b2)2(a1)2(a2)
(i) B2N C∞v 2 Σ g + 2.30 2.25 2.60 (σ)2 (σ)2 (σ)2 (σ)2 (σ)2 (σ)2 (σ) (π)4 (b1)2(b2)2(a1)2
(j) B2N C∞v 4 Σ g + , Σ g , 4.00 4.00 3.74 (σ)2 (σ)2 (σ)2 (σ)2 (σ)2 (σ)2 (π)3 (σ) (π)
(k) BN2 C2v 4 B 1 3.80 3.80 3.70 (a1)2 (b2)2(a1)2(a1)2(b2)2(a1)2(b1)2
(a1)2(a1) (b2) (a2)
Table 2. Geometries and electrical properties of B2 N ( 0   ) = 17 e , B2 N (   ) = 18 e and B2 N ( +   ) = 16 e   in ground and exited states.
Table 2. Geometries and electrical properties of B2 N ( 0   ) = 17 e , B2 N (   ) = 18 e and B2 N ( +   ) = 16 e   in ground and exited states.
State
(*Ne)
E e ( H a r t r e e ) Total Configuration
(Energy of α * ( H o m o L u m o ) **
β Configuration
Energy of β *
Beta virtual**
r e B 1 N r e N B 2 A 1 ( 2,1 , 3 , 2 , 1 ) A 2   ( 2,1 , 3 , 1 , 2 )
X   ~ 2Σ+
( C v )
(*17e)
104.078196 a 104.082033 a ' 104.075492 a ' ' A , π 4 , σ 2 , σ 1 α = 0.4464 1 a * E α ( 34.87083 ) a * * ( 0.48614 ) a B σ 1 β = 0.2618 0   a * ( 34.15046 ) a * * ( 0.17697 ) a
X   ~ 2 Σ u +
( D h )
(*17e)
103.639678
A ' π u 4 , 4 σ g 2 , 3 σ u 1 α = 0.4247 7 d * ( 34.74888 ) d * * ( 0.49245 ) d B ' , 4 σ g 1 β =-0.24844d
* ( 34.06924 ) d
** ( 0.18742 ) d
1.317 6d
1.317 6 d
A 1 = 180 . 0 d A 2 = 180.0 d
A   ~ 2 Σ g +
(*17e)
104.10475 9 k 104.07817 3 K ' A ' π u 4 , 4 σ g 1 , 3 σ u 2 α = 0.4463 8 u * ( 34.8744 ) u * * ( 0.48626 ) u A ' π u 4 , 4 σ u 1 , = 0.26134 * ( 34.15408 ) * * ( 0.17666 ) 1.315 4 k 1.315 4 k A 1 = 180 . 0 k A 2 = 180.0 k
  B ~ 4 П g
(*17e)
104.02970 2 h 104.01411 7 a A ' π u 4 , π g , 2 σ g 1 α = 0.2689 9 h * ( 35.04484 ) h * ( 0.30125 ) h A ' , π u 2 β = 0.496 5 h * ( 33.74801 ) * * ( 0.50595 ) * 1.307 9 x * 1.307 9 x * A 1 = 180 . 0 x * A 2 = 180 x
X   ~ 1 Σ g +
(*18e)
104.196567 a 104.20191 4 a ' 104.19501 7 a ' ' A ' 1 π u 4 , 4 σ g 2 , 3 σ u 2 = 0.1390 4 a * E α = 32.486 47 a * * 0.36286 * 1.33 5 y * 1.33 5 y A 1 = * 180 . 0 y A 2 = * 180.0 y
X   ~ 1 Σ g +
(*18e)
104.196566 b * E α = 32.4864 4 b 1.329 1 b 1.3291 A 1 = 180 . 0 b A 2 = 180.0
B   ~ 3Σg
(*16e)
103.76092 2 a 103.77671 1 h 103.76285 5 a ' 103.75905 8 a ' ' { A ' 4 σ g 1 , 3 σ u 1 , π u 4 , } a π u 2 α = 0.7432 3 a * E α ( 37.33372 ) a * * ( 0.53385 ) a { A '   , π u 2 β = 0.75222 } a * E β ( 35.72475 ) a * * ( 0.5213 1 a * 1.297 6 w * 1.297 6 w A 1 = * 180 . 0 w A 2 = * 180 . 0 w
(a)QCISD/EPR-III;(d)CASSCF(11,12)/UHF;(z)b3p86/6-31g*;(a')MP4D/EPR-III//QCISD/EPR-III; (m)CASSCF(10,12)/EPR-III(x)b3lyp/6-31g*;(a'')MP4SDQ/EPR-III//QCISD/EPR-III; (g)CASSCF(10,12)rohfAUG-cc-pvqz;(y)m062x/epr-ii;(b)QCISD/EPR-III( A : 1 σ 2 , 2 σ 2 , 3 σ 2 , 4 σ 2 , 5 σ 2 ; :(w)b3lyp/6-31g*;(c) QCISD/EPR-II A ' : 1 σ g 2 , 1 σ u 2 , 2 σ g 2 , 3 σ g 2 , 2 σ u 2 ; (v)CASSCF(11,12)/AUG-cc-pvqz;(c')MP4D/EPR-II//QCISD/EPR-II: B :   σ 1 , σ 1 , σ 1 , σ 1 , σ 1 , π 2 ; (c'')MP4SDQ/EPR-II//QCISD/EPR-II; [ B ' ]: 1 σ g 1 , 2 σ g 1 , 1 σ u 1 , 3 σ g 1 , 2 σ u 1 , 1 π u 2 ; (f) CBS-lq; (h)QCISD(T)/EPR-III; [C]: 1 σ g 2 , 1 σ u 2 , 2 σ g 2 , 3 σ g 2 , 2 σ u 2 , 4 σ g 2   ; (n)CBS4O; (u) TD/EPR-II ; (k) TD/EPR-III//QCISD (T)/EPR-III; ( K ' ) TD/EPR-III//QCISD /EPR-III; C ' : 1 σ g , 1 σ u , 2 σ g , 3 σ g , 2 σ u ; [D]: 1 σ g 2 , 2 σ g , 2 1 σ u 2 , 3 σ g 2 , 2 σ u 2 .
Table 3. Harmonic frequencies, IR intensities and Raman activities of the most important clusters.
Table 3. Harmonic frequencies, IR intensities and Raman activities of the most important clusters.
ν3 ν3 ν2
Item Point
group
Term cm-1 IR Ram an cm-1 IR Raman cm-1 IR Ra man Esp(kcal.mol
-1)
B2N C∞ν 2 Σ g + 229 9 23 229 9 23 1355 12 10 4.08
B2N D∞h 2 Σ u + 78 4 0 229 9 23 1122 0 4 4.87
BN2 C∞ν 2 Π u 111 12 15 244 10 7 907 12 10 4.45
BN2 Cs 2 A 1 " 109 - - 287 15 6 944 35 23 4.76
BN2 Cν 4 Σ u 85 2 3 400 1 3 1132 15 16 4.23
BN2 D∞h 2 Π g - - - 176 19 0 1565 17 9 4.79
BN2 C 2 A 1 ' - - - 102 - - 1653 78 14 3.54
BN2 C 2 A 2 ' - - - 1088 1 5 1432 14 54 5.01
BN2 C 2 B 1 ' - - - - - - 1343 18 52 3.99
Table 4. Energies (kcal mol- 1 )of boron nitried reactions at various levels.
Table 4. Energies (kcal mol- 1 )of boron nitried reactions at various levels.
Reaction MP4D/EPR-III//
QCISD/EPR-III
QCISD/
EPR-III
CASSCF(10,12)
/EPR-III
TD/EPR-III//
QCISD
QCISD/
EPR-II
CBS-lq
B2N  →  BN + B 6.44 5.34 5.74 5.03 4.99 4.87
B2N → B2 + N 7.35 7.12 7.24 6.99 6.04 5.99
BN2 → BN + N 4.91 4.21 4.33 4.38 4.33 4.21
BN2 → N2 + B 0.15 0.18 0.16 0.19 0.21 0.09
Table 5. Calculated thermodynamic properties at some selected temperatures.
Table 5. Calculated thermodynamic properties at some selected temperatures.
Temperature (K) B2N(-) BN2(-) B2N(+) BN2(+) B2N(0) BN2(0)
Association enthalpy (kcal/mol)
0
300
1000
20000
-266.5
-266.1
-269.1
-269.8
-225.1
-227.1
-228.9
-230.1
-208.5
-211.4
-210.08
-203.05
-199.09
-205.03
-205.96
-202.08
193.07
-201.05
-204.55
-205.01
194.08
-207.02
-203.63
-208.07
Free energy of association (kcal/mol)
0
300
1000
20000
-264.92
-247.97
-203.97
-139.95
-225.04
-206.95
-160.08
-89.92
-206.99
-192.05
-135.95
-65.04
-199.04
-185.09
-131.40
-75.83
200.05
-203.05
-207.95
-204.09
200.49
-200.06
-202.91
-205.06
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