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. 2019 Dec 11;4(26):21741–21760. doi: 10.1021/acsomega.9b02486

Electronic Structure with Rovibrational Calculations of the Magnesium Monohalides MgX and Their Cations MgX+ (X = Cl, Br, and I)

Nariman Abu el kher , Nayla El-Kork ‡,*, Mahmoud Korek
PMCID: PMC6933579  PMID: 31891053

Abstract

graphic file with name ao9b02486_0002.jpg

Alkaline-earth monohalides are popular compounds that are used in various applications. Little is known, however, in terms of electronic structure, about their cations and their low-lying electronic states. We present in this work electronic structure ab-initio calculations based on multireference configuration interaction plus Davidson correction of three magnesium monohalides and their cations (MgCl, MgBr, MgI, MgCl+, MgBr+, and MgI+). We determine the spectroscopic constants Te, Re, ωe, Be, and αe and the dissociation energies De for their bound states. Additionally, we investigate their vibrational properties by calculating the vibrational eigenvalue Ev, the rotational constant Bv, and the centrifugal distortion constant Dv. We additionally study the electric charge distribution of several states by determining their permanent dipole moment and transition dipole moment curves. Finally, we calculate the Franck–Condon factors and the radiative lifetimes as precursors for laser cooling experiments.

1. Introduction

Metal-containing molecules such as alkaline-earth monohalides are of high interest for scientists working in different types of disciplines such as astrophysics, high- and low-temperature physics, etc. They have been detected in the interstellar medium,1 in the upper atmosphere,2 and in high-temperature reactions that occur in flames, catalysis, and corrosion processes.3 Moreover, alkaline-earth halides can be used as scintillators4 and utilized in laser window materials.5 In recent years, different laser cooling schemes have been proposed for the production of cold and ultracold diatomic molecules. Ultracold molecules, compared with ultracold atoms, have a more complex structure due to their rotational and vibrational motions. One can take advantage of this manifold configuration to propose new cooling techniques. The alkaline-earth materials have potential for laser cooling and are promising candidates for the controlled preparation of many-body entangled states.6 These molecules are consequently attractive for the fabrication of fundamentally new condensed-matter phases, which may be later used for state of the art applications such as qubit encoding and quantum memory engineering.7 The alkaline-earth halides SrF8 and CaF9 have been successfully cooled experimentally. In addition, RaF10 and BeF11 molecules are suggested as good candidates for direct laser cooling. Ultracold molecules are largely used, for example, in quantum information processing,12 chemical dynamics,13 and controlling chemistry.14 In addition, they can be used in Bose−Einstein condensate materials.15 Moreover, trapped cold ions16 can be exploited in a wide range of applications such as quantum computing,17 atom-ion sympathetic cooling1820 ultracold quantum and superchemistry,14,2125 precision measurements,26,27 and local probing of quantum degenerate gases.28

The first few low-lying excited electronics states of the molecules MgCl, MgBr, and MgI have already been examined.2946 A study on the MgCl+ molecule has already been published;47 however, it only considered the two low-lying singlet states of the molecule. MgBr+ and MgI+ remain uninvestigated until now. Given the lack of information on the electronic structure of MgX and MgX+ molecules in the literature (X = Cl, Br, and I), we were strongly motivated to perform an accurate analysis of the electronic states of these molecules and their corresponding cations.

Therefore, we investigate in this work 127 electronic states for MgCl, MgBr, MgI, MgCl+, MgBr+, and MgI+ molecules and molecular ions by using an ab initio method (CASSCF/MRCI+Q). A full spectroscopic analysis was carried out for these electronic states in order to calculate the spectroscopic constants Te, Re, ωe, Be, αe, and De, the permanent and transition dipole moments, the rovibrational parameters Ev, Bv, and Dv, the abscissas of turning points Rmin and Rmax, and their Franck–Condon factors (FCFs).

2. Results and Discussion

2.1. Potential Energy Curves (PECs)

We investigated in this work 127 electronic states for MgCl, MgBr, MgI, MgCl+, MgBr+, and MgI+ molecules. The potential energy curves of these states are plotted as a function of the internuclear distance in Figures 112. All the studied electronic states correlate with the molecular dissociation asymptotes as reported in Table 1. Notably, the (2)2Σ+ state in the MgCl molecule, (4)2Σ+ state in the MgBr molecule, and (4)2Σ+ state in the MgI molecule are not given in Table 1 since they are polarized states. At the dissociation limit, the three molecules dissociate into the ionic fragments Mg+(2S) + Cl(1S), Mg+(2S) + Br(1S), and Mg+(2S) + I(1S), respectively. To check the precision of our calculations, a comparison between our calculated asymptotic energies and those available in the NIST experimental atomic spectra database48 is carried out in the same table. This comparison shows an overall good agreement in which the percentage relative difference ranges between 0.0 and 5.44% for MgCl and MgCl+, 0.0 and 3.09% for MgBr and MgBr+, and 0 and 4.30% for MgI and MgI+. The dissociation limits of higher excited states are missing due to the breakdown of the Born–Oppenheimer approximation, which lead to the undulations in the potential energy curves for these electronic states.

Figure 1.

Figure 1

Potential energy curves of the lowest 2Σ(+/−), 2Π, and 2Δ electronic states of the MgCl molecule.

Figure 12.

Figure 12

Potential energy curves of the lowest 3Σ(+/−), 3Π, and 3Δ electronic states of the MgI+ molecule.

Table 1. Lowest Dissociation Limits of MgCl, MgCl+, MgBr, MgBr+, MgI, and MgI+ Molecules.

dissociation of atomic levels Mg + Cl dissociation energy limit of MgCl levels (cm–1) molecular states of MgCl total dissociation energy limit of Mg + Cl atoms (cm–1) relative error (%)
Mg (2p63s21S) + Cl (3s23p52P0) 0.00a X2Σ+, (1)2Π 0.00b 0.00
Mg (3s3p, 3P0) + Cl (3s22p5, 2P0) 21,501.40a (3)2Σ+, (4)2Σ+, (2)2Π, (3)2Π, (1)2Δ, (1)2Σ, (1)4Σ+, (2)4Σ+, (1)4Π, (2)4Π, (1)4Δ, (1)4Σ 21,850.41b 1.62
Mg (3s3p, 1P0) + Cl (3s22p5, 2P0) 34,750.80a (5)2Σ+, (4)2Π 35,051.26b 0.86
Mg (3s4s, 3S) + Cl (3s22p5, 2P0) 43,565.69a (3)4Σ+, (3)4Π 41,197.40b 5.44
dissociation limit of atomic levels Mg + Cl dissociation energy limit of MgCl+ levels (cm–1) molecular states of MgCl+ total dissociation energy limit of Mg + Cl atoms (cm–1) relative error (%)
Mg+ (2p63s, 2S) + Cl (3s23p52P0) 0.00a X1Σ+, (1)1Π, (1)3Σ+, (1)3Π 0.00b 0.00
Mg+ (2p63p, 2P0) + Cl (3s23p5, 2P0) 34,635.36a (2)1Σ+, (1)1Δ, (3)1Σ+, (2)1Π, (3)1Π, (1)1Σ, (2)3Σ+, (1)3Δ, (3)3Σ+, (2)3Π, (3)3Π, (1)3Σ 35,669.31b 2.90
dissociation limit of atomic levels Mg + Br dissociation energy limit of MgBr levels (cm–1) molecular states of MgBr total dissociation energy limit of Mg + Br atoms (cm–1) relative error (%)
Mg (2p63s21S) + Br (4s24p52P0) 0.00a X2Σ+, (1)2Π 0.00b 0.00
Mg (3s3p, 3P0) + Br (4s24p5, 2P0) 21,174.32a (2)2Σ+, (3)2Σ+, (2)2Π, (3)2Π, (1)2Δ, (1)2Σ, (1)4Σ+, (2)4Σ+, (1)4Π, (2)4Π, (1)4Δ, (1)4Σ 21,850.41b 3.09
Mg (3s3p, 1P0) + Br (4s24p5, 2P0) 35,161.26a (2)2Δ, (2)2Σ 35,051.264b 0.31
dissociation of atomic levels (Mg+ + Br) dissociation energy limit of MgBr+ levels (cm–1) molecular states of MgBr+ total dissociation energy limit of Mg + Br atoms (cm–1) relative error (%)
Mg+(2p63s, 2S) + Br (4s24p52P0) 0.00a X1Σ+, (1)1Π, (1)3Σ+, (1)3Π 0.00b 0.00
Mg+ (2p63p, 2P0) + Br (4s24p5, 2P0) 34,918.37a (2)1Σ+, (1)1Δ, (3)1Σ+, (2)1Π, (3)1Π, (1)1Σ, (2)3Σ+, (1)3Δ, (3)3Σ+, (3)3Π 35,669.31b 2.11
dissociation of atomic levels Mg + I dissociation energy limit of MgI levels (cm–1) molecular states of MgI total dissociation energy limit of Mg + I atoms (cm–1) relative error (%)
Mg (2p63s21S) + I (5s25p52P0) 0.00a X2Σ+, (1)2Π 0.00b 0.00
Mg (3s3p, 3P0) + I (5s25p5, 2P0) 20,909.765a (2)2Σ+, (3)2Σ+, (2)2Π, (3)2Π, (1)2Δ, (1)2Σ, (1)4Σ+, (2)4Σ+, (1)4Π, (2)4Π, (1)4Δ, (1)4Σ 21,850.41b 4.30
Mg (3 s,3p, 1P0) + I (5s25p5, 2P0) 34,538.218a (2)2Δ, (2)2Σ 35,051.26b 1.46
Mg (3s4s, 3S) + I (5s25p5, 2P0) 40,392.704a (3)4Σ+, (3)4Π 41,197.40b 1.95
Mg (3s3d, 3D) + I (5s25p5, 2P0) 47,010.609 (2)4Δ, (4)4Σ+, (4)4Π, (2)4Σ 47,841.12b 1.74
dissociation of atomic levels Mg + I dissociation energy limit of MgI+ levels (cm–1) molecular states of MgI+ total dissociation energy limit of Mg + I atoms (cm–1) relative error (%)
Mg+ (2p63s, 2S) + I (5s25p52P0) 0.00a X1Σ+, (1)1Π, (1)3Σ+, (1)3Π 0.00b 0.00
Mg+ (2p63p, 2P0) + I (5s25p5, 2P0) 35,135.58a (3)1Σ+, (2)1Δ, (4)1Σ+, (3)1Π, (1)1Σ, (2)3Σ+, (1)3Δ, (3)3Σ+, (3)3Π, (2)3Σ 35,669.31b 1.50
a

Present work.

b

Experimental values from the NIST atomic spectra database.

Figure 2.

Figure 2

Potential energy curves of the lowest 4Σ(+/−), 4Π, and 4Δ electronic states of the MgCl molecule.

Figure 3.

Figure 3

Potential energy curves of the lowest 1Σ(+/−), 1Π, and 1Δ electronic states of the MgCl+ molecule.

Figure 4.

Figure 4

Potential energy curves of the lowest 3Σ(+/−), 3Π, and 3Δ electronic states of the MgCl+ molecule.

Figure 6.

Figure 6

Potential energy curves of the lowest 4Σ(+/−), 4Π, and4Δ electronic states of the MgBr molecule.

Figure 7.

Figure 7

Potential energy curves of the lowest 1Σ(+/−), 1Π and1Δ electronic states of the MgBr+ molecule.

Figure 8.

Figure 8

Potential energy curves of the lowest 3Σ(+/−), 3Π, and 3Δ electronic states of the MgBr+ molecule.

Figure 10.

Figure 10

Potential energy curves of the lowest 4Σ(+/−), 4Π, and 4Δ electronic states of the MgI molecule.

Figure 11.

Figure 11

Potential energy curves of the lowest 1Σ(+/−), 1Π, and 1Δ electronic states of the MgI+ molecule.

Depth of potential wells can be an indicator of the strength of the binding forces linking two atoms of a diatomic molecule. A shallow potential usually suggests the dominancy of the forces of repulsion over the forces of attraction. Obviously, as shown in Figures 112, the low doublet and singlet states have deep potential wells, which indicates that the molecules are more stable on lower levels, while the higher excited states have shallower wells. In contrast, the low quartet and triplet states are shallow around the equilibrium positions.

A detailed analysis of the potential energy curves reveals some crossings and avoided crossings between them. Their positions are given in Table S1 in the Supporting Information, where Rc is the position of crossing between two electronic states, RAC is the position of avoided crossing, and ΔE is the energy gap separation. In Figures 1, 5, and 9, the PECs of the lowest two 2Π states show avoided crossing at about 2.60, 2.54, and 2.64 Å for MgCl, MgBr, and MgI molecules, respectively. However, it is clear that the avoided crossings are more abundant in the magnesium monohalide molecules MgCl, MgBr, and MgI compared with their molecular cations MgCl+, MgBr+, and MgI+.

Figure 5.

Figure 5

Potential energy curves of the lowest 2Σ(+/−), 2Π and2Δ electronic states of the MgBr molecule.

Figure 9.

Figure 9

Potential energy curves of the lowest 2Σ(+/−), 2Π, and 2Δ electronic states of the MgI molecule.

2.2. The Spectroscopic Constants

The spectroscopic constants Te, Re, ωe, Be, and αe of the bound electronic states have been calculated for the three magnesium monohalide molecules (MgCl, MgBr, and MgI) and their molecular cations (MgCl+, MgBr+, and MgI+) by fitting the energy data for these states around their equilibrium position Re into a polynomial in terms of the internuclear distance. The calculated spectroscopic constants are reported in Tables 27 in addition to the dissociation energies De and the dipole moments of the considered electronic states at their equilibrium position Re. An acceptable agreement is achieved upon comparison of these values with the available experimental and theoretical data in the literature, which confirms the reliability of our calculations. The absence of the spectroscopic constants of some electronic states is due to the presence of crossing and avoided crossing near their minima.

Table 2. Spectroscopic Parameters for the X2Σ+ and 14 Excited States of the MgCl Molecule (Experimental Values Are Indicated in Bold).

states (2S+1Λ) Te (cm–1) Re (Å) ωe (cm–1) Be (cm–1) De (eV) αe (cm–1) e| (a.u.)
X2Σ+ 0.0a 2.202a 466.44a 0.241a 3.523a 0.0018a 1.37a
0.0b 2.216b 461.90b 0.241b 3.293b 0.0015b  
0.0c 2.199c 462.12c 0.245c 3.291c 0.0016c  
0.0d 2.196d 466.00d 0.246d 3.370d    
0.0e 2.229e 450.30e        
0.0f 2.203f 467.53f 0.241f 3.302f    
0.0g   462.10g 0.246g      
0.0h 2.190h 483.20h 0.250h 3.420h    
(1)2Π 26,427.43a 2.181a 540.00a 0.246a 0.221a 0.0015a 1.76a
26,442.30b 2.190b 443.95b 0.191b 0.549b 0.0019b  
26,469.40c 2.181c 491.60c 0.249c   0.0018c  
26,496.40d 2.169d 490.80d        
26,143.90e 2.220e 482.00e        
26,062.04f 2.178f 492.33f 0.247f 0.536f    
26,739.91g     0.251g      
26,958.71h 2.17h 515.92h 0.250h 0.55h    
(2)2Σ + (ext) 30,673.14a 4.013a 136.16a 0.073a 1.813a 0.0009a 2.64a
30,867.66h 3.660h 179.32h 0.090h 2.260h    
(2)2Π 32,869.02a 2.611a 772.24a 0.172a 2.040a   1.26a
31,945.56f 2.554f 622.72f 0.179f 2.013f    
32,363.35h 2.520h 681.20h 0.190h 2.07h    
(2)2Σ + (int) 37,562.76a 2.161a 498.74a 0.250a 0.958a 0.0011a 1.98a
38,613.09h 2.150h 540.39h 0.260h 0.10h    
(3)2Σ+ (ext) 41,859.09a 2.477a 680.02a 0.191a 0.906a 0.0013a 0.60a
42,918.81h 2.370h 705.16h 0.210h 0.77h    
(3)2Σ+ (int) 43,102.32a 2.124a 550.02a 0.259a 0.751a 0.0013a 0.99a
(1)4Σ + 48,152.87a 2.871a 124.60a 0.138a 0.174a 0.039a 0.72a
(1)4Δ 48,833.67a 3.043a 120.67a 0.124a 0.09a 0.043a 0.60a
(1)4Σ 49,240.68a 3.299a 78.61a 0.106a 0.041a 0.018a 0.45a
(3)4Π 68,785.22a 2.756a 235.50a 0.154a 0.373a 0.0053a 0.31a
(3)4Σ + 71,834.18a 6.887a 18.30a 0.025a 0.001a 0.0014a 0.12a
(4)4Π 75,248.12a 2.884a 124.65a 0.130a 0.267a 0.1667a 1.67a
(4)4Σ+ 77,409.02a 4.943a 21.65a 0.048a 0.016a 0.0014a 0.09a
(5)4Π 79,591.18a 2.529a 257.36a 0.183a 0.240a 0.0024a 0.79a
a

Present work.

b

Ref (42).

c

Ref (33).

d

Ref (34).

e

Ref (40).

f

Ref (43).

g

Ref (36).

h

Ref (45).

Table 7. Spectroscopic Parameters for the X1Σ+ and 14 Excited States of the MgI+ Molecule.

states (2S+1Λ) Te (cm–1) Re (Å) ωe (cm–1) Be (cm–1) De (eV) αe (cm–1) e| (a.u.)
X1Σ+ 0.0a 2.478a 369.68a 0.135a 2.133a 0.00065a 4.68a
(1)3Π 11,673.57a 3.009a 161.88a 0.091a 0.606a 0.00104a 2.79a
(1)1Π 12,653.15a 3.022a 168.23a 0.090a 0.461a 0.00089a 2.86a
(2)1Σ+ 31,740.14a 2.848a 224.17a 0.102a 1.814a 0.00023a 3.23a
(1)3Σ 34,711.03a 4.709a 50.80a 0.037a 0.074a 0.01494a 0.62a
(2)3Π 34,737.44a 5.018a 40.74a 0.033a 0.065a 0.00151a 0.61a
(2)3Σ+ 37,635.82a 2.755a 259.27a 0.109a 1.658a 0.00068a 2.58a
(1)3Δ 38,553.28a 2.780a 238.56a 0.107a 1.547a 0.00058a 2.56a
(1)1Δ 38,802.35a 2.816a 256.08a 0.104a 0.957a 0.00053a 2.55a
(1)1Σ 39,201.07a 2.819a 239.79a 0.103a 1.432a 0.00079a 2.53a
(3)1Σ+ 43,104.35a 2.952a 201.68a 0.095a 0.936a 0.00082a 2.97a
(2)1Π 46,096.60a 4.841a 44.33a 0.035a 0.039a 0.06990a 0.53a
(2)1Δ 46,856.47a 4.069a 251.49a 0.049a 0.479a –0.05451a 0.80a
(3)1Π 48,725.56a 3.938a 142.28a 0.053a 0.255a 0.00081a 4.27a
(3)3Σ 54,455.42a 5.278a 54.42a 0.029a 0.085a 0.00005a 0.63a
a

Present work.

Table 3. Spectroscopic Parameters for the X1Σ+ and 13 Excited States of the MgCl+ Molecule.

states (2S+1Λ) Te (cm–1) Re (Å) ωe (cm–1) Be (cm–1) De (eV) αe (cm–1) e| (a.u.)
X1Σ+ 0.0a 2.111a 562.45a 0.263a 3.363a 0.00161a 1.77a
  2.101b 583.0b   3.20b    
(1)3Π 24,042.15a 2.699a 168.05a 0.161a 0.397a 0.00344a 1.30a
(1)1Π 24,474.31a 2.754a 164.16a 0.152a 0.322a 0.00183a 1.30a
22,514.0b 2.746b 167.0b   0.41b    
(2)1Σ+ 38,157.51a 2.642a 226.06a 0.167a 2.886a 0.00041a 0.68a
(2)3Σ+ 51,888.97a 2.426a 335.34a 0.199a 1.220a 0.00162a 0.96a
(1)3Δ 52,790.17a 2.446a 327.63a 0.195a 1.094a 0.001819a 0.99a
(1)1Δ 53,183.47a 2.484a 288.65a 0.189a 1.013a 0.00177a 1.09a
(1)1Σ 53,516.58a 2.489a 277.33a 0.188a 0.980a 0.00199a 1.10a
(1)3Σ 53,676.89a 2.464a 350.90a 0.193a 0.990a 0.00193a 1.04a
(3)1Σ+ 56,127.71a 2.614a 217.21a 0.172a 0.681a 0.08764a 1.01a
(2)3Π 60,291.31a 2.778a 66.97a 0.146a 0.155a –0.52311a 0.84a
(3)3Π 61,503.71a 3.184a 140.45a 0.115a 0.021a 0.00168a 0.70a
(4)1Π 82,152.33a 2.445a 338.97a 0.196a 0.206a 0.00144a 1.21a
(5)1Π 91,788.59a 2.353a 346.58a 0.211a 0.088a 0.00125a 0.75a
a

Present work.

b

Ref (47).

Table 4. Spectroscopic Parameters for the X2Σ+ and 16 Excited States of the MgBr Molecule (Experimental Values Are Indicated in Bold).

states (2S+1Λ) Te (cm–1) Re (Å) ωe (cm–1) Be (cm–1) De (eV) αe (cm–1) e| (a.u.)
X2Σ+ 0.0a 2.378a 367.44a 0.160a 2.241a 0.00098a 1.29a
0.0b 2.371b 370.52b 0.163b 3.221b 0.00087b  
  2.360c 373.80c 0.165c 3.351c    
0.0f 2.356f 369.18f 0.163f 2.781f    
0.0j 2.396j 365.90j        
0.0k   374.23k 0.166k      
0.0l 2.371l 369.21l 0.163l 3.157l 0.00086l  
0.0m 2.347m   0.166m   0.00092m  
(1)2Π 25,564.30a 2.381a 323.63a 0.159a –0.906a 0.00350a 1.39a
25,726.22b 2.340b 407.93b 0.167b 0.353b 1.22345b  
25,766.90c 2.332c 393.90c 0.169c      
25,414.31f 2.328f 391.89f 0.167f 0.235f    
25,362.80j 2.354j 397.40j        
25,824.31k   392.76k 0.169k      
25,890.69l 2.337l 407.69l 0.167l 0.346l 0.01271l  
(2)2Σ + 24,043.15a 3.654a 163.78a 0.068a 1.868a –0.02812 1.61a
26,539.35l 3.895l 146.06l 0.060l   –0.02823  
(2)2Π 27,211.88a 2.564a 580.33a 0.138a 1.481a 0.00041a 0.69a
28,720.01f 2.607f 561.13f 0.133f 1.928f    
29,096.07l 2.628l 605.46l 0.132l 1.864l 0.00032l  
(1)4Σ+ 38,089.29a 3.179a 136.96a 0.089a 0.109a –0.05099a 0.67a
(1)4Δ 38,748.25a 3.423a 88.89a 0.079a 0.042a 0.01133a 0.50a
(1)2Δ 38,959.95a 3.942a 24.23a 0.058a 0.021a 0.00347a 0.23a
(3)2Σ+ 39,061.39a 2.474a 387.59a 0.148a 0.009a 0.00414a 0.85a
39,820.55l 2.505l 575.91l 0.146l 0.538l 0.00564l  
(1)4Σ 39,066.40a 3.949a 29.29a 0.058 0.006a 0.00749a 0.24a
(1)2Σ 39,113.69a 4.567a 411.41a 0.086a 0.003a 0.00351a 0.09a
(2)2Δ 52,388.82a 3.138a 126.99a 0.093a 0.109a 0.00480a 0.93a
(2)2Σ 52,790.59a 3.366a 86.63a 0.079a 0.055a 0.00215a 0.74a
(3)4Σ+ 66,882.09a 2.695a 206.59a 0.125a –0.130a 0.00109a 3.69a
(2)4Δ 68,821.61a 2.684a 208.18a 0.126a 0.790a 0.00124a 3.41a
(3)4Π 63,469.59a 2.910a 186.42a 0.107a 0.298a 0.00078a 0.90a
(4)4Π 69,076.35a 2.716a 202.15a 0.123a 0.668a 0.00159a 3.89a
(2)4Σ 70,290.34a 2.685a 227.13a 0.125a 0.538a 0.00202a 3.25a
a

Present work.

b

Ref (42).

c

Ref (33).

f

Ref (46).

j

Ref (41).

k

Ref (37).

l

Ref (44).

m

Ref (35).

Table 5. Spectroscopic Parameters for the X1Σ+ and 10 Excited States of the MgBr+ Molecule (Experimental Values Are Indicated in Bold).

states (2S+1Λ) Te (cm–1) Re (Å) ωe (cm–1) Be (cm–1) De (eV) αe (cm–1) e| (a.u.)
X1Σ+ 0.0a 2.276a 467.79a 0.175a 2.267a 0.00028a 4.65a
(1)3Π 15,199.53a 2.898a 149.66a 0.109a 0.385a 0.00411a 2.79a
(1)1Π 15,989.60a 2.958a 115.81a 0.103a 0.290a 0.00668a 2.95a
(2)1Σ+ 33,729.84a 2.701a 260.07a 0.124a 2.369a 0.00038a 3.16a
(2)3Σ+ 42,913.11a 2.592a 299.90a 0.134a 1.222a 0.00105a 2.43a
(1)3Δ 43,798.28a 2.622a 264.77a 0.132a 1.115a 0.00122a 2.45a
(1)1Δ 44,043.71a 2.651a 255.38a 0.129a 1.089a 0.001860a 2.43a
(1)1Σ 44,432.83a 2.656a 240.27a 0.129a 1.042a 0.00300a 2.44a
(1)3Σ 44,595.67a 2.652a 244.09a 0.129a 0.242a 0.00269a 2.45a
(2)1Δ 58,638.68a 4.501a 55.55a 0.044a 0.099a 0.00679a 1.17a
(3)1Σ+ 47,776.13a 2.826a 259.33a 0.113a 0.673a 0.00872a 2.83a
a

Present work.

Table 6. Spectroscopic Parameters for the X1Σ+ and 10 Excited States of the MgI Molecule (Experimental Values Are Indicated in Bold).

states (2S+1Λ) Te (cm–1) Re (Å) ωe (cm–1) Be (cm–1) De (eV) αe (cm–1) e| (a.u.)
X2Σ+ 0.0a 2.5887a 317.38a 0.123a 1.88a 0.00057a 1.11a
0.0b 2.6005b 315.92b 0.124a 2.82b 0.00057b  
    316.00c   2.90c    
0.0d 2.5975d 314.27d 0.123d 2.27d    
(1)2Π 23,654.78a 2.5489a 301.27a 0.128a 1.04a 0.00932a 0.86a
24,354.58b 2.5540b 329.33b 0.127b 0.08b 0.00704b  
24,319.00c   323.00c        
23,919.88d 2.5640d 319.40d 0.125d 0.06d    
(2)2Π 24,615.45a 2.7046a 515.28a 0.112a 1.41a 0.00046a 0.76a
25,554.47d 2.7554d 523.32d 0.109d 1.71d    
(1)4Σ+ 34,183.96a 3.1986a 105.09a 0.081a 0.213a 0.00169a 0.95a
(1)2Σ 35,758.61a 3.907a 44.16a 0.053a 0.027a 0.01877a 0.44a
(1)4Σ 35,553.21a 3.5630a 89.02a 0.06370a 0.050a 0.00128a 0.69a
(1)4Δ 35,034.45a 3.3455a 69.36a 0.074a 0.114a 0.00622a 0.86a
(3)2Π 44,426.37a 2.4723a 363.55a 0.135a 1.049a 0.00030a 0.83a
(2)2Σ 47,475.30a 3.137a 123.43a 0.084a 0.214a 0.00172a 1.22a
(3)4Π 51,163.41a 3.0594a 189.57a 0.088a 0.530a 0.00048a 0.68a
(2)4Σ 57,514.93a 2.981a 200.28a 0.093a 0.556a 0.00011a 1.23a
a

Present work.

b

Ref (42).

c

Ref (33).

d

Ref (46).

Our calculated values of the equilibrium bond length Re of the ground state X2Σ+ are relatively consistent with the theoretical data in the literature where the relative differences are as follows: 0.1%43 ≤ ΔRe/Re ≤ 1.2%,40 0.3%42,44 ≤ ΔRe/Re ≤ 0.9%,46 and 0.5%42 ≤ ΔRe/Re ≤ 1.5%46 for MgCl, MgBr, and MgI, respectively. Also, they are in accordance with the experimental data with average relative differences ΔRe/Re = 0.2% for MgCl and ΔRe/Re = 1.0% for MgBr. The harmonic frequencies ωe calculated in the present work are also in a very good agreement with those given in the literature where the average relative differences are 1.4% for MgCl, 1.0% for MgBr, and 0.6% for MgI. There is additionally good conformity in the values of the rotational constant Be between our data and those in the literature, where the average relative errors are ΔBe/Be = 1.5%, ΔBe/Be = 2.8%, and ΔBe/Be = 0.4% for MgCl, MgBr, and MgI respectively. For the higher excited electronic states, one can find that the calculated values of spectroscopic constants are generally compatible with those available in the literature.

Concerning the investigated cations, the spectroscopic constants of MgCl+ are compatible with available theoretical data. However, those of the ions MgBr+ and MgI+ are reported here for the first time to our knowledge.

In terms of the trend among the different neutral molecules and anions, it is noted that, as the halogens and their cations vary from Cl to I, the equilibrium internuclear distances Re of X2Σ+ and A2Π states increase. This tendency can be explained by the decreasing value of the electronegativity of the halide elements as we go down through the periodic table. Also, the vibrational force constant ωe is much smaller for the ground state of the neutral molecules compared to their corresponding ions. For example, for MgCl, ωe = 466.44 cm–1 for the X2Σ+ state, while for the ground state of MgCl+, ωe = 562.45 cm–1. This is most probably attributed to a higher bond in the ions consistent with the removal of an extra electron. A similar behavior applies to MgBr/MgBr+ and for MgI/MgI+.

2.3. Electric Dipole Moments

2.3.1. The Permanent Dipole Moment Curves (PDMCs)

The permanent dipole moment curves play an essential role in the representation of the charge distribution and the types of bonds (ionic or covalent) of diatomic molecules. The dipole moment curves (DMCs) of the investigated doublet and singlet electronic states for the six molecules as a function of internuclear separation R have been plotted in Figures 1315, while those of the quartet and triplet states are given in Figures S1–S6 in the Supporting Information, where Mg is taken at the origin in the molecules. One can notice the agreement between the position of the avoided crossing of the PECs and the positions of the crossing of the DMCs of these states, which confirm the accuracy of the present work.

Figure 13.

Figure 13

(a) Dipole moment curves of the lowest 2Σ(+/−), 2Π, and 2Δ electronic states of the MgCl molecule. (b) Dipole moment curves of the lowest 1Σ(+/−), 1Π, and 1Δ electronic states of the MgCl+ molecule.

Figure 15.

Figure 15

(a) Dipole moment curves of the lowest 2Σ(+/−), 2Π, and 2Δ electronic states of the MgI molecule. (b) Dipole moment curves of the lowest 1Σ(+/−), 1Π, and 1Δ electronic states of the MgI+ molecule.

Figure 14.

Figure 14

(a) Dipole moment curves of the lowest 2Σ(+/−), 2Π, and 2Δ electronic states of the MgBr molecule. (b) Dipole moment curves of the lowest 1Σ(+/−), 1Π, and 1Δ electronic states of the MgBr+ molecule.

The majority of electronic states for MgCl, MgBr, and MgI molecules dissociate into neutral atoms at the asymptotic limit of dissociation over the range R > 8 Å (the permanent dipole moment curve tends to zero). However, for the states, (2)2Σ+ state in the MgCl molecule, (4)2Σ+ state in the MgBr molecule, and (4)2Σ+ state in the MgI molecule, the bond character is of covalent character at small internuclear distances, and the dipole moments increase to a constant value at the asymptotic limit of dissociation, where these states become ionic. The dipole moment of the ground states X2Σ+ of MgCl, MgBr, and MgI molecules presents negative values with maximum magnitudes |μ| = 3.77 a.u. at R = 3.66 Å, |μ| = 2.70 a.u. at R = 3.38 Å, and |μ| = 2.29 a.u. at R = 3.48 Å, respectively. This indicates partially ionic bonds for Mgδ+Clδ−, Mgδ+Brδ−, and Mgδ+Iδ− at small internuclear distances. The dipole moment values then decrease to zero at large internuclear distances, which is an indicator of covalent character near dissociation. The PDMCs of the molecular cations present many crossings between their different electronic states, which correlate to the corresponding potential energy curves avoided crossing.

Concerning the ionic molecules, the 1Π curves for MgCl+, MgBr+, and MgI+ molecules show a significant number of crossings, especially between the two states (2)1Π and (3)1Π at small distances (about 3.18, 2.74, and 3.72 Å, respectively). The PDMCs of singlet ion MgCl+ are plotted in Figure 13, and the triplet states are given in Figure S2 in the Supporting Information, where the interatomic distance R is extended between 1.4 and 6.4 Å. As shown, several maxima with high amplitude for most of the states are observed at small distances, where the ionic character dominates. At large distances, all the states tend to zero, except states (4)1Π and (5)1Π, which are correlated to (Mgδ− + Clδ+) as they tend toward ( + μ). The PDMCs of ions MgBr+ and MgI+ have two different directions at large distances. States that dissociate to Mgδ+ tend to ( – μ), while those dissociating to Brδ+ (MgBr+) and Iδ+ (MgI+) progressively go toward ( + μ).

2.3.2. The Transition Dipole Moments Curves (TDMCs)

The TDMCs of the allowed transitions from the lowest-lying excited states to the ground state (X)Σ+ have been investigated for the molecules MgCl, MgBr, and MgI and their ionic systems MgCl+, MgBr+, and MgI+ and are plotted in Figures 16 and 17. All the TDMCs of the (X)Σ+–(1)Π transition tend to zero at the asymptotic limit of dissociation (R ≈ 5.2 Å) in the six magnesium monohalide molecules.

Figure 16.

Figure 16

Transition dipole moment curves of X2Σ+2Σ+ and X2Σ+2Π transitions for MgCl, MgBr, and MgI.

Figure 17.

Figure 17

Transition dipole moment curves of X1Σ+1Σ+ and X1Σ+1Π transitions for MgCl+, MgBr+, and MgI+.

On the basis of the calculated TDMs values, the radiative lifetimes have been computed using the following formula49

2.3.2.
2.3.2.

where σν′ν is the wavenumber of the transition between the upper vibrational level ν′ and lower vibrational level ν (in cm–1), Λ′ and Λ are the projections of electronic orbital angular momentum on the internuclear axis for the upper and lower electronic levels, Reν′ν is the electronic-vibrational transition moment expectation value, which can be obtained from the vibrational wave functions (ν and ν′) and electronic transition dipole moment (in atomic units), and τν′ν is the radiative lifetimes, which are evaluated as the inverse of the Einstein coefficients Aν′ν.

The radiative lifetimes τν′ν for the bound states are calculated between 0 ≤ ν′ ≤ 6 of the upper state and 0 ≤ ν ≤ 6 of the lower state for the investigated transitions corresponding to MgCl+, MgBr+, and MgI+. These values are given in Tables S2–S4 in the Supporting Information.

It can be seen from Tables S2–S4 that the range of the radiative lifetime of the vibrational transitions between the electronic states (X1Σ+–21Σ+) is 30.7 ns ≤ τ ≤ 21.6 μs, 24.9 ns ≤ τ ≤ 596 ns, and 289 ns ≤ τ ≤ 1250 μs for MgCl+, MgBr+, and MgI+, respectively. We attribute the large difference between the radiative lifetimes of the vibrational levels for the same electronic state transition of a given molecule to two factors: (i) the large variation of the transition dipole moment function with internuclear distance for the (X1Σ+–21Σ+) transition in MgCl+, MgBr+, and MgI+ (as shown in Figure 17) and (ii) the remarkable difference between FCF values of the vibrational levels of one given electronic transition, as shown in Tables S11–S13 in the Supporting Information. Such a difference probably emanates from the large shift between the ground state and the excited state for the investigated molecules.

2.4. The Rovibrational Calculations

We calculated, using the canonical function approach50,51 and cubic spline interpolation method between each two consecutive points of the potential energy curves, the vibrational energy Ev, the rotational constant Bv, the centrifugal distortion constant Dv, and the abscissas of the turning points Rmin and Rmax for the vibrational levels of the ground state of the investigated monohalides and their cations. These constants are given in Tables 8 and 9, and those of some excited electronic states are provided in Tables S5–S10 in the Supporting Information. The rovibrational values are missing for some electronic states due to their shallow potential wells and/or the presence of avoided crossing within their potential energy curves. The comparison of our results with the experimental data reported by Rostas et al.34 for the ground state of the three vibrational levels for the MgCl molecule shows a good agreement with an average relative difference ΔBv/Bv = 1.8% and ΔDv/Dv = 5.9%. No comparison for the values of other vibrational levels is available since they are given here for the first time.

Table 8. Rovibrational Constants for the Different Vibrational Levels of X2Σ+ of MgCl, MgBr, and MgI Molecules.

MgCl
state ν Ev (cm–1) Bv (cm–1) Dv × 107 (cm–1) Rmin (Å) Rmax (Å)
X2Σ+ 0 233.82a 0.2403a 2.56a 2.1347 2.2763
  0.2448d 2.72d    
1 698.00a 0.2388a 2.56a 2.0896 2.3357
  0.2432d 2.72d    
2 1157.75a 0.2372a 2.56a 2.0603 2.3794
  0.2416d 2.72d    
3 1613.05 0.2356 2.57 2.0376 2.4167
4 2063.92 0.2340 2.57 2.0187 2.4503
5 2510.36 0.2324 2.58 2.0024 2.4815
6 2952.38 0.2308 2.59 1.9879 2.5109
7 3389.95 0.2292 2.59 1.9749 2.5391
8 3823.13 0.2276 2.59 1.9631 2.5662
9 4251.92 0.2260 2.59 1.952 2.5925
10 4676.35 0.2244 2.60 1.9421 2.6181
11 5096.42 0.2228 2.60 1.9327 2.6432
12 5512.20 0.2212 2.60 1.9239 2.6678
13 5923.79 0.2196 2.59 1.9156 2.6919
14 6331.30 0.2181 2.58 1.9077 2.7157
15 6734.90 0.2166 2.56 1.9003 2.7391
16 7134.73 0.2151 2.57 1.8932 2.7621
17 7530.74 0.2135 2.62 1.8865 2.7848
18 7922.53 0.2119 2.79 1.8801 2.8066
19 8308.88 0.2100 3.03 1.8740 2.8341
20 8688.44 0.2079 2.96 1.8681 2.8573
21 9435.28 0.2059 1.45 1.8572 2.8988
22 9811.26 0.2054 2.21 1.8519 2.9198
23 10185.48 0.2036 3.31 1.8468 2.9409
24 10552.26 0.2016 2.37 1.8419 2.9617
25 10916.43 0.2010 1.57 1.8371 2.9824
26 11281.48 0.1998 3.11 1.8325 3.0032
27 11640.56 0.1977 2.53 1.8280 3.0239
28 11996.21 0.1970 1.65 1.8237 3.0445
29 12351.79 0.1956 3.26 1.8195 3.0652
30 12701.25 0.1938 1.86 1.8155 3.0858
31 13049.52 0.1932 2.42 1.8116 3.1064
32 13394.70 0.1912 2.75 1.8079 3.1270
33 13735.69 0.1903 1.73 1.8042 3.1476
34 14075.62 0.1888 3.10 1.8006 3.1682
MgBr
state ν Ev (cm–1) Bv (cm–1) Dv × 107 (cm–1) Rmin (Å) Rmax (Å)
X2Σ+ 0 181.27 0.1595 1.26 2.3104 2.4517
1 538.79 0.1584 1.31 2.2649 2.5124
2 889.76 0.1575 1.25 2.2355 2.5561
3 1239.45 0.1565 1.31 2.2125 2.5933
4 1585.00 0.1556 1.25 2.1933 2.6266
5 1928.49 0.1546 1.30 2.1767 2.6575
6 2268.59 0.1537 1.26 2.1619 2.6864
7 2606.09 0.1528 1.27 2.1486 2.7140
8 2940.90 0.1519 1.30 2.1365 2.7404
9 3272.60 0.1509 1.23 2.1253 2.7660
10 3602.04 0.1500 1.31 2.1149 2.7908
11 3928.39 0.1492 1.26 2.1051 2.8149
12 4252.22 0.1482 1.26 2.0960 2.8386
13 4573.52 0.1474 1.30 2.0874 2.8618
14 4891.91 0.1465 1.24 2.0793 2.8846
15 5207.93 0.1455 1.27 2.0716 2.9070
16 5521.30 0.1447 1.29 2.0642 2.9291
17 5831.98 0.1438 1.24 2.0572 2.9510
18 6140.27 0.1429 1.28 2.0504 2.9726
19 6445.94 0.1421 1.28 2.0440 2.9940
20 6749.01 0.1412 1.24 2.0379 3.0153
21 7049.68 0.1403 1.27 2.0319 3.0364
22 7347.79 0.1395 1.27 2.0262 3.0573
23 7643.36 0.1386 1.25 2.0207 3.0782
24 7936.51 0.1377 1.26 2.0153 3.0989
25 8227.21 0.1369 1.27 2.0102 3.1195
26 8515.48 0.1360 1.24 2.0053 3.1399
27 8801.39 0.2390 7.08 2.0005 3.1602
28 9084.91 0.2386 10.7 1.9958 3.1808
29 9365.82 0.2381 16.1 1.9913 3.2013
30 9643.98 0.2373 23.8 1.9869 3.2219
31 10192.34 0.2342 47.7 1.9785 3.2629
32 10462.81 0.2440 3.71 1.9745 3.2835
33 10730.63 0.2437 5.74 1.9706 3.3041
34 10995.77 0.2433 8.66 1.9668 3.3248
35 11258.38 0.2426 12.7 1.9631 3.3456
36 11518.33 0.2496 0.69 1.9595 3.3664
37 11775.53 0.2399 24.8 1.9560 3.3873
38 12030.12 0.2494 1.60 1.9526 3.4084
39 12281.91 0.2491 2.35 1.9492 3.4296
40 12530.90 0.2551 0.089 1.9460 3.451
41 12777.10 0.2483 4.52 1.9429 3.4726
42 13020.35 0.2476 5.85 1.9398 3.4943
43 13260.72 0.2466 7.06 1.9368 3.5164
44 13498.01 0.2450 7.62 1.9339 3.5387
45 13732.24 0.2548 0.33 1.9310 3.5613
46 13963.28 0.2546 0.26 1.9283 3.5842
MgI
state ν Ev (cm–1) Bv (cm–1) Dv × 108 (cm–1) Rmin (Å) Rmax (Å)
X2Σ+ 0 156.30 0.1230 7.68 2.5197 2.6657
1 466.51 0.1224 7.68 2.4722 2.7252
2 774.64 0.1217 7.80 2.4413 2.7692
3 1079.77 0.1211 7.66 2.4171 2.8063
4 1383.13 0.1205 7.52 2.3969 2.8396
5 1685.37 0.1200 7.12 2.3793 2.8712
6 1987.94 0.1197 6.52 2.3636 2.8933
7 2292.48 0.1194 7.08 2.3492 2.9193
8 2596.16 0.1187 9.09 2.3359 2.9469
9 2892.64 0.1175 9.83 2.3240 2.9732
10 3181.36 0.1168 6.10 2.3130 2.9980
11 3471.64 0.1166 7.51 2.3027 3.0225
12 3760.11 0.1156 9.92 2.2930 3.0465
13 4042.29 0.1150 5.75 2.2839 3.0697
14 4325.71 0.1146 9.11 2.2752 3.0928
15 4604.86 0.1136 7.87 2.2670 3.1153
16 4881.67 0.1133 6.96 2.2592 3.1376
17 5157.44 0.1124 9.55 2.2517 3.1597
a

Present work.

d

Ref (34).

Table 9. Rovibrational Constants for the Different Vibrational Levels of X1Σ+ of MgCl+, MgBr+, and MgI+ Cations.

MgCl+
state ν Ev (cm–1) Bv (cm–1) Dv × 107 (cm–1) Rmin (Å) Rmax (Å)
X1Σ+ 0 281.06 0.2619 2.28 2.0483 2.1773
1 840.70 0.2605 2.28 2.0066 2.2307
2 1396.23 0.2590 2.28 1.9794 2.2697
3 1947.58 0.2576 2.28 1.9582 2.3027
4 2494.84 0.2562 2.28 1.9405 2.3323
5 3037.96 0.2548 2.28 1.9251 2.3597
6 3576.96 0.2533 2.27 1.9114 2.3853
7 4111.88 0.2519 2.28 1.8991 2.4098
8 4642.67 0.2505 2.27 1.8878 2.4332
9 5169.37 0.2491 2.28 1.8774 2.4559
10 5691.98 0.2477 2.28 1.8678 2.4779
11 6210.48 0.2463 2.28 1.8587 2.4993
12 6724.89 0.2448 2.28 1.8503 2.5203
13 7235.18 0.2434 2.28 1.8423 2.5409
14 7741.34 0.2420 2.28 1.8347 2.5612
15 8243.40 0.2406 2.29 1.8275 2.5812
16 8741.31 0.2392 2.29 1.8207 2.6009
17 9235.06 0.2377 2.29 1.8141 2.6204
18 9724.65 0.2363 2.30 1.8079 2.6398
19 10210.05 0.2349 2.31 1.8019 2.6590
20 10691.18 0.2334 2.33 1.7962 2.6781
21 11167.98 0.2319 2.37 1.7906 2.6970
22 11640.10 0.2304 2.48 1.7853 2.7161
MgBr+
state ν Ev (cm–1) Bv (cm–1) Dv × 107 (cm–1) Rmin (Å) Rmax (Å)
X1Σ+ 0 230.12 0.1744 1.02 2.2149 2.3387
1 684.74 0.1739 1.15 2.1715 2.3920
2 1122.59 0.1727 1.12 2.1440 2.4312
3 1554.82 0.1719 1.17 2.1225 2.4647
4 1980.15 0.1708 1.13 2.1047 2.4949
5 2401.60 0.1699 1.19 2.0892 2.5228
6 2817.63 0.1690 1.12 2.0754 2.5489
7 3230.74 0.1681 1.16 2.0629 2.5739
8 3640.22 0.1673 1.07 2.0516 2.5974
9 4048.59 0.1665 1.07 2.0410 2.6180
10 4455.67 0.1659 1.14 2.0311 2.6389
11 4859.52 0.1647 1.33 2.0219 2.6621
12 5255.90 0.1633 1.47 2.0133 2.6846
13 5643.15 0.1621 1.17 2.0053 2.7065
14 6027.12 0.1613 1.12 1.9977 2.7280
15 6408.78 0.1603 1.37 1.9905 2.7492
16 6784.64 0.1591 1.21 1.9837 2.7699
17 7156.83 0.1582 1.22 1.9772 2.7908
18 7525.46 0.1571 1.36 1.9709 2.8115
19 7888.94 0.1560 1.21 1.9650 2.8320
20 8248.98 0.1551 1.29 1.9593 2.8524
21 8605.09 0.1541 1.25 1.9538 2.8726
22 8957.70 0.1531 1.28 1.9485 2.8922
23 9306.48 0.1520 1.35 1.9435 2.9125
24 9650.74 0.1509 1.43 1.9385 2.9334
25 9989.84 0.1496 1.50 1.9338 2.9543
26 10323.33 0.1484 1.38 1.9292 2.9752
27 10652.47 0.1473 1.38 1.9248 2.9962
28 10977.55 0.1462 1.48 1.9205 3.0174
29 11297.72 0.1449 1.52 1.9164 3.0387
30 11612.85 0.1437 1.40 1.9125 3.0602
31 11923.84 0.1426 1.58 1.9087 3.0819
32 12229.69 0.1412 1.52 1.9051 3.1039
33 12530.73 0.1400 1.51 1.9015 3.1261
34 12827.13 0.1387 1.63 1.8981 3.1487
35 13118.26 0.1374 1.56 1.8948 3.1716
36 13404.62 0.1361 1.71 1.8916 3.1949
37 13685.58 0.1347 1.62 1.8885 3.2186
38 13961.52 0.1333 1.78 1.8855 3.2427
39 14231.93 0.1318 1.75 1.8825 3.2674
40 14496.98 0.1304 1.88 1.8797 3.2926
41 14756.31 0.2651 2.52 1.8770 3.3184
42 15010.00 0.2643 2.44 1.8744 3.3449
43 15257.71 0.2630 1.39 1.8719 3.3721
MgI+
state ν Ev (cm–1) Bv (cm–1) Dv × 108 (cm–1) Rmin (Å) Rmax (Å)
X1Σ+ 0 184.32 0.1344 7.20 2.4128 2.5469
1 550.40 0.1338 7.20 2.3691 2.6020
2 914.18 0.1331 7.18 2.3405 2.6421
3 1275.84 0.1325 7.10 2.3181 2.6758
4 1635.92 0.1320 7.08 2.2993 2.7051
5 1994.28 0.1314 7.28 2.2829 2.7330
6 2349.62 0.1307 7.63 2.2684 2.7597
7 2700.60 0.1299 7.45 2.2553 2.7850
8 3048.41 0.1293 7.15 2.2433 2.8091
9 3394.22 0.1287 7.57 2.2323 2.8326
10 3736.74 0.1280 7.52 2.2220 2.8554
11 4076.20 0.1273 7.41 2.2124 2.8776
12 4413.02 0.1266 7.64 2.2034 2.8994
13 4746.73 0.1259 7.49 2.1949 2.9208
14 5077.71 0.1253 7.70 2.1869 2.9418

Besides, we calculated the Franck–Condon factors (FCFs) for transitions between the ground and excited states of the cations MgCl+, MgBr+, and MgI+ by using the LEVEL8.2 program.52 The FCF study does not include the neutral molecules MgCl, MgBr, and MgI due to the failure of this approach in the presence of avoided crossings. The Franck–Condon factors, fν′ν, are tabulated in Tables S11–S13 in the Supporting Information, where the level ν′ of the upper state and ν for the lower state ranges between 0 ≤ ν′ ≤ 9 and 0 ≤ ν ≤ 9, respectively. Additionally, for the three cations (MgCl+, MgBr+, and MgI+), the Franck–Condon factors of the 1Σ+1Σ+ and 1Σ+1Π transitions are given in Figure 18. The obtained FCFs have a very small value for ν ≥ 0 in the considered transitions for these cations; thus, for these transitions, the FCF array is off-diagonal. Consequently, for the magnesium monohalide cations, the condition for the feasibility of laser cooling is not attained.

Figure 18.

Figure 18

Plotting of the calculated FCFs of the MgCl+, MgBr+, and MgI+ molecules for the lowest nine vibrational levels of the transitions of 1Σ+1Σ+ and 1Σ+1Π.

3. Conclusions

In the present work, the PECs and PDMCs for the ground and excited doublet and quartet electronic states of the magnesium monohalide molecules MgCl, MgBr, and MgI, in addition to the excited singlet and triplet states of their molecular cations MgCl+, MgBr+, and MgI+, were investigated via ab initio CASSCF/(MRCI+Q) calculations. The spectroscopic constants Te, Re, ωe, Be, αe, the dipole moment μe, and the dissociation energies De have been calculated for the bound states. A comparison between our calculated spectroscopic constants and previous data in the literature shows good agreement. A similar type of agreement has been achieved in our previously published works.53,54 Also, the TDMCs of the (X)Σ+–Σ+ and (X)Σ+–Π transitions have been investigated for the six molecules. These calculations were followed by a study in which the rovibrational constants for different vibrational levels of low-lying electronic states are calculated. Finally, the Franck–Condon factors of the magnesium monohalide cations were found to be off-diagonal and therefore cannot be used in laser cooling applications.

4. Computational Approach

The electronic structure calculations of the three magnesium monohalides MgCl, MgBr, and MgI, in addition to their molecular cations MgCl+, MgBr+, and MgI+, were performed by using the quantum computational program package MOLPRO55 taking the advantage of the graphical user interface GABEDIT.56 High-level potential energy curves (PECs) have been investigated by employing the state-averaged complete active space self-consistent field (CASSCF) followed by the multireference single and double configuration interaction (MRCI) method with Davidson correction (+Q). The symmetry point group of MgX and MgX+ is Cv, but all the calculations are done in the C2v subgroup of the Cv point group due to the restriction of the Molpro program. The basis set used for the six entire molecules including their corresponding orbitals are given in Table 10 with the active space of C2v symmetry. The orbitals are distributed into the irreducible representation as follows: 5a1, 2b1, 2b2, and 0a2 for MgCl and MgCl+, 7a1, 3b1, 3b2, and 1a2 for MgBr and MgBr+, and 6a1, 3b1, 3b2, and 1a2 for MgI and MgI+ symbolized by [5,2,2,0], [7,3,3,1], and [6,3,3,1], respectively. The basis sets cc-pwCV5Z, cc-pVTZ, and aug-cc-PVQZ-DK were given by Prascher et al.,57 while aug-cc-pwCV5Z was given by Peterson et al.58 The basis sets ECP28MWB and ECP46MWB known as the quasi-relativistic energy consistent pseudo-potential were given by Dolg et al.59

Table 10. Employed Basis Set and the Active Space Orbitals for the Magnesium Monohalides and Their Cations.

molecule atom basis orbital orbitals of active space
MgCl, MgCl+ Mg cc-pwCV5Z s, p, d, f 5σ (Mg: 3s, 3p0, 4s; Cl: 3p0, 4s), 2π (Mg: 3p ± 1; Cl: 3p ± 1)
Cl aug-cc-pwCV5Z s, p, d, f
MgBr, MgBr+ Mg cc-pVTZ s, p, d 7σ (Mg: 3s, 3p0, 3d0, 3d+2, 4s; Br: 4p0, 5s), 3π (Mg: 3p±1, 3d±1; Br: 4p±1),1δ (Mg: 3d–2)
Br ECP28MWB s, p
MgI, MgI+ Mg aug-cc-pVQZ-DK s, p, d 6σ (Mg: 3s, 3p0, 3d0, 3d+2, 4s; I: 5p0), 3π (Mg: 3p±1, 3d±1; I: 5p±1),1δ (Mg: 3d–2)
I ECP46MWB s, p

Acknowledgments

This publication is based on the work supported by the Khalifa University of Science and Technology under award no. CIRA-2019-054. The authors would like to acknowledge the use of MASDAR high power computer, Khalifa University Nuclear Engineering Department high power computer, and Ankabut high power computer for the completion of their work.

Supporting Information Available

The Supporting Information is available free of charge at https://pubs.acs.org/doi/10.1021/acsomega.9b02486.

  • The static dipole moment curves of the quartet electronic states of MgCl, MgBr, and MgI in addition to the triplet states for MgCl+, MgBr+, and MgI+ molecules (Figures S1–S6), the positions of crossing and avoided crossing among the electronic states (Table S1), the values of the vibrational energy Ev, the rotational constant Bv, the centrifugal distortion constant Dv, and the turning points Rmin and Rmax for some excited electronic states of the considered molecules ( Tables S2–S7), and the FCF values for the considered cations (Tables S8–S10) (PDF)

The authors declare no competing financial interest.

Supplementary Material

ao9b02486_si_001.pdf (777.8KB, pdf)

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