Dominik
Wehrli
,
Matthieu
Génévriez
and
Frédéric
Merkt
*
Laboratory of Physical Chemistry, ETH Zurich, CH-8093 Zurich, Switzerland. E-mail: merkt@phys.chem.ethz.ch
First published on 30th April 2021
Although numerous doubly positively charged diatomic molecules (diatomic dications) are known from investigations using mass spectrometry and ab initio quantum chemistry, only three of them, NO2+, N22+ and DCl2+, have been studied using rotationally resolved optical spectroscopy and only about a dozen by vibrationally resolved double-ionization methods. So far, no thermodynamically stable diatomic dication has been characterized spectroscopically, primarily because of experimental difficulties associated with their synthesis in sufficient densities in the gas phase. Indeed, such molecules typically involve, as constituents, rare-gas, halogen, chalcogen, and metal atoms. We report here on a new approach to characterize molecular dications based on high-resolution photoelectron spectroscopy of the singly charged parent molecular cation and present the first spectroscopic characterization of a thermodynamically stable diatomic dication, MgAr2+. From the fully resolved vibrational and partially resolved rotational structures of the photoelectron spectra of 24MgAr+ and 26MgAr+, we determined the potential-energy function of the electronic ground state of MgAr2+, its dissociation (binding) energy (D0 = 10690(3) cm−1), and its harmonic (ωe(24MgAr2+) = 327.02(11) cm−1) and anharmonic (ωexe(24MgAr2+) = 2.477(15) cm−1) vibrational constants. The analysis enables us to explain quantitatively how the strong bond arises in this dication despite the fact that Ar and Mg2+ both have a full-shell rare-gas electronic configuration.
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Fig. 1 Schematic potential-energy functions for molecules of the type BA2+ corresponding to the situations leading to metastable DIDIs (a and b) and thermodynamically stable DIDIs (c and d). (e) Potential-energy function of the singly charged precursor molecule BA+. Right of panels (c–e): arrows indicating the energetic order of the dissociation limits dependent on the ionization energies of A and B+. Inspired by Fig. 2 of ref. 4. |
The large majority of the DIDIs known today are metastable, i.e., their lowest level is located above the dissociation asymptote A+ + B+. Metastability typically arises when the ionization energy of B+ is significantly larger than that of A and results from an avoided crossing between the repulsive potential function dissociating into A+ + B+ and the attractive potential function correlating with A + B2+ (see Fig. 1(b)), or if a potential barrier is formed at short range in the otherwise repulsive Coulomb potential by binding valence interactions13,15–17 (Fig. 1(a)). The best and earliest known case of a DIDI, He22+, belongs to the latter category.15,18,19 Today, the most reliable source of information on the structure and binding of DIDIs is ab initio quantum chemistry, see ref. 20 for a recent example concerning thermodynamically stable DIDIs.
Experimentally, the vast majority of DIDIs has been identified by mass-spectrometric methods, which enable their unambiguous detection but do not provide structural information. Only very few DIDIs have been characterized by spectroscopic methods which provide quantitative information on their structure. High-resolution, rotationally resolved spectra have been obtained for only three DIDIs, N22+,21–25 NO2+,26 and DCl2+,27 and the vibrational structures of about 10 DIDIs have been studied by double-photoionization coincidence methods starting from the ground state of the neutral molecules (see ref. 11 and references therein). All cases for which spectroscopic information is available concern metastable DIDIs and, to our knowledge, no spectroscopic information has ever been obtained on a thermodynamically stable DIDI. One of the reasons for this absence of spectroscopic data is that these dications typically involve rare-gas, halogen, or chalcogen, and metal atoms. It is thus difficult to generate potential precursor neutral or singly-charged molecules BA and BA+ in the gas phase with sufficient densities. Another reason is that the double-ionization thresholds of diatomic molecules lie in the vacuum-ultraviolet (VUV) or soft X-ray ranges and are difficult to reach with table-top laboratory radiation sources.
We present here the first spectroscopic characterization of a thermodynamically stable DIDI, MgAr2+. To obtain high-resolution spectroscopic information on this dication, we have recorded the photoelectron spectrum of MgAr+ using the techniques of pulsed-field-ionization zero-kinetic-energy photoelectron (PFI-ZEKE-PE)28,29 and mass-analyzed threshold ionization (MATI) spectroscopy.30 Until this work, high-resolution photoelectron spectroscopy of molecular cations had been deemed impossible because of (i) the very limited density of ions that can be generated in the gas phase as a result of space-charge effects and (ii) the high ionization energies of cations. We demonstrate here that high-resolution photoelectron spectroscopy can be applied to samples of less than 1000 state-selected cations and that cations can be efficiently ionized despite their high ionization energies by resonant multiphoton excitation.
The photoelectron spectra we obtained were sufficiently resolved (∼2 cm−1) to obtain information on the rotational contours of the successive vibrational bands of the photoelectron spectrum of MgAr+ and to determine isotopic shifts in the spectra of 24MgAr+ and 26MgAr+. From these observations, we could extract an accurate potential-energy function for the electronic ground state of MgAr2+, prove experimentally that it is thermodynamically stable, and analyze the nature of the bond. We found the binding energy to be more than 1.3 eV (125 kJ mol−1), i.e., comparable to a typical covalent bond, despite the fact that both constituents (Mg2+ and Ar) have full-shell rare-gas electron configurations.
MgAr2+ had been observed by mass spectrometry prior to our work.31–35 It appears as an undesirable species in inductively-coupled-plasma mass spectrometry and complicates the chemical analysis of S isotopes.34,35 From the analysis of the density of MgAr2+ at different plasma temperatures, Hattendorf et al. could estimate the ground-state dissociation energy to be in the range between 124 and 130 kJ mol−1.34 In addition, Gardner et al.36 have characterized the electronic and vibrational structure of MgAr2+ in high-level ab initio quantum-chemical calculations. These studies provided very useful and important reference data with which our new results are compared.
Our approach to obtain spectroscopic information on DIDIs relies on the preparation of the precursor singly-charged molecule BA+ by photoionization of the neutral molecule BA. The photoelectron spectra of BA+ are then recorded following resonance-enhanced multiphoton excitation. The scheme used to study MgAr2+ is illustrated in Fig. 2, which depicts the potential-energy functions of all relevant states, as described in more detail in Section 2. It enables us to efficiently ionize MgAr+, despite its high ionization energy of about 13.9 eV, using commercial lasers operating in the UV region of the electromagnetic spectrum. This aspect is of central importance in the present work because of the low densities (typically ∼104 cm−3) and low numbers (typically 200 per experimental cycle at a repetition rate of 25 Hz, i.e., 5000 s−1) of MgAr+ ions generated in our experiments.
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Fig. 2 (1 + 1′ + 1′′) three-photon excitation sequence used to photoionize MgAr+ X+(v+) via the A1/2+(v′) and 3dπ1/2+(v′′) intermediate levels. MgAr+ was produced in its X+ ground electronic state by photoionization of metastable MgAr. The MgAr+ potential-energy functions were taken from ref. 39 and that of the ground state of MgAr2+ was taken from ref. 36. |
The term symbols and quantum numbers used to designate the different states are cumbersome. To define and simplify the notation of states and transitions, we use the nomenclature summarized in Table 1. For example, 3dπ1/2+(v′′, J′′) ← A1/2+(v′,
J′) designates the transition between the rovibrational level with vibrational and rotational quantum numbers v′ and J′ of the Ω = 1/2 spin–orbit component of the A+
2ΠΩ electronic state of MgAr+ and the rovibrational level with quantum numbers v′′ and J′′ of the Ω = 1/2 spin–orbit component of the 3dπΩ+ Rydberg state of MgAr+. More generally, we designate the rotational and vibrational quantum numbers of the a state of MgAr with unprimed letters, those of the X+, AΩ+ and 3dπΩ+ of MgAr+ using letters with a plus (+), a prime (′) and a double-prime (′′) superscript, respectively, and those of the X2+ state of MgAr2+ with letters with a double-plus (2+) superscript. The integer quantum numbers N+ and N2+ used to label the rotational levels of the electronic states of Σ symmetry correspond to the standard notation for states following Hund's angular-momentum coupling case (b) and the quantum numbers J, J′ and J′′ used for the rotational levels of electronic states of Π symmetry correspond to the standard notation for states following Hund's angular-momentum coupling case (a), as described, e.g., in ref. 37 and 38, to which we refer for details.
State label | Molecule | Diss. asymptote | Term symbol | Rovibrational quantum numbers |
---|---|---|---|---|
a | MgAr | Mg(3s3p 3P) + Ar(1S0) | 3Π0 |
v,![]() |
X+ | MgAr+ | Mg+(3s) + Ar(1S0) | 2Σ+ |
v
+,![]() |
AΩ+ | MgAr+ | Mg+(3p) + Ar(1S0) | 2ΠΩ |
v′,![]() |
3dπΩ+ | MgAr+ | Mg+(3d) + Ar(1S0) | 2ΠΩ |
v′′,![]() |
X2+ | MgAr2+ | Mg2+(1S0) + Ar(1S0) | 1Σ+ |
v
2+,![]() |
All results presented below are for 24MgAr and its ions, unless stated otherwise.
The only electronic states of MgAr+ that had been characterized prior to this work are the X+, AΩ+ and B+ states (see Fig. 2).39,41–46 The resonant excitation sequence thus necessitated the identification and characterization of a suitable intermediate state between the AΩ+ and the X2+ states. In a broad search in the region near the Mg+(3d) + Ar(1S0) dissociation asymptote, we identified the lowest vibrational levels of the 3dπ1/2+ state to be ideal intermediate states because of their long lifetimes (>50 ps) and large Franck–Condon factors.47Fig. 3(a) shows the rotationally resolved spectrum of the A1/2+(v′ = 1, J′) ← X+(v+ = 5,N+) transition recorded by monitoring the yield of Mg+ photodissociation product as a function of the wavenumber 2 of laser 2.42,43 The sticks indicate the positions and relative intensities of individual rovibronic transitions, calculated for a rotational temperature of 4 K using standard expressions37,38 for transitions between rovibrational levels of 2Σ+ and 2Π1/2 states. The red arrow corresponds to the position of laser 2 which selects the J′ = 3.5, 4.5, and 6.5 rotational levels from which the spectrum of the 3dπ1/2+(v′′ = 3,
J′′) ← A1/2+(v′ = 1,
J′) transition depicted in Fig. 3(b) was measured. This spectrum was recorded by scanning laser 3 and setting laser 4 to 46
290 cm−1, while monitoring the MgAr2+ signal. It consists of three branches characterized by J′′ − J′ = 0, ±1 and the assignments are grouped and colored according to the selected A1/2+ rotational levels.
![]() | ||
Fig. 3 (a) Rotationally resolved spectrum of the A1/2+(v′ = 1,J′) ← X+(v+ = 5,N+) transition of MgAr+ recorded by monitoring the Mg+ photodissociation yield as a function of the wavenumber ![]() ![]() |
The band origins and the rotational constants
of the 3dπ1/2+ levels were determined from the rotational line positions using the formula for the transition energy,37
![]() | (1) |
The shift ΔEI of the ionization thresholds induced by a single pulsed field of strength F is given in good approximation by49–51
![]() | (2) |
![]() | (3) |
The main difference between PFI-ZEKE-PE and MATI spectroscopy is that with the former method one detects the electrons generated by the pulsed field ionization whereas in the latter one detects the ions, which offers the advantage of mass selectivity. This advantage was crucial in the present work to separately record the spectra of 24MgAr2+ and 26MgAr2+ and determine the absolute assignment of the vibrational levels of MgAr2+ from the isotopic shifts. However, the advantage comes at the cost of a reduced resolution because larger electric fields are typically required to distinguish the much heavier ions generated by the successive pulses through their times of flight.
To record the PFI-ZEKE-PE spectra of MgAr+ (Z = 2) we used a four-pulse sequence (typically F1 = +0.34 V cm−1, F2 = −0.52 V cm−1, F3 = −1.12 V cm−1, and F4 = −1.72 V cm−1) and, for each laser scan, we recorded the three spectra corresponding to F2, F3, and F4 simultaneously. We recorded the MATI spectra with optimized pulse sequences, e.g., F1 = −0.86 V cm−1, F2 = −1.72 V cm−1, and F3 = +172.4 V cm−1, the spectra obtained from F2 being the high-resolution ones. Because of the small numbers of state-selected MgAr+ ions (∼200 per laser shot), the pulsed-field-ionization signal was very weak (less than 1 count per laser shot) and the spectra had to be measured several times and averaged to improve the signal-to-noise ratio.
Fig. 4 depicts the photoionization spectrum of MgAr+ from its 3dπ1/2+(v′′ = 2) state to the region of the first three vibrational levels of the ground state of MgAr2+. The spectrum shows two distinct steps that indicate the ionization thresholds associated with the v2+ = 0, 1 levels of the X2+ state. Several sharp resonances are also present in the spectrum, which we attribute to autoionizing Rydberg states of MgAr+. Just above the ionization threshold associated with the X2+(v2+ = 0) state, we could assign several of these resonances to Rydberg states of MgAr+ with principal quantum numbers n = 37–40 belonging to series converging to the X2+(v2+ = 1) level of MgAr2+, as indicated along the lower assignment bar. The blue bars represent the Franck–Condon factors of the X2+(v2+ = 0–2) ← 3dπ1/2+(v′′ = 2) transitions calculated using the potential-energy functions shown in Fig. 2. The very weak Franck–Condon factor to the X2+(v2+ = 2) state explains why no step could be detected in the photoionization spectrum at the v2+ = 2 ionization threshold.
High-resolution PFI-ZEKE-PE and MATI spectra of the X2+(v2+ = 0) ← 3dπ1/2+(v′′ = 2) transition are presented in Fig. 5(a) and (b). The red dashed lines depict least-squares fits of Gaussian functions to determine the line positions. The slightly asymmetric base line in Fig. 5(b) is caused by an incomplete separation in the TOF spectrum of the MgAr2+ signals that were produced by the different field-ionization pulses. Fig. 5(c) and (d) show the corresponding MATI spectra of 24MgAr+ and 26MgAr+, respectively, recorded using the two-pulse sequence −0.86, +172.4 V cm−1. We determined the isotopic shift (Δ4 = 9.7 cm−1) of the transition by fitting the error function53 to the high-energy edges of the spectra and extracting the difference in the inflection points shown as black vertical lines. From the isotopic shift of the 3dπ1/2+(v′′ = 2) level (Δ3dπ = 15.1 cm−1, see ref. 47) we determined the isotopic shift of the X2+(v2+ = 0) level to be ΔX2+(0) = Δ3dπ − Δ
4 = 5.4(20) cm−1. A similar measurement of the isotopic shift of the X2+(v2+ = 1) vibrational threshold yielded ΔX2+(1) = 10.9(20) cm−1. These results, together with the vibrational constants determined for 24MgAr2+ (see below), were used to unambiguously establish the vibrational assignment in a standard isotopic shift analysis.48 The fall of the MATI signal below the ionization threshold (Fig. 5(c)) is twice as broad for 24MgAr+ as it is for 26MgAr+ (Fig. 5(d)). This difference has its origin in a different initial population of rotational states caused by the slightly different rotational constants and the multiphoton excitation.
Fig. 6(a) and (b) show MATI spectra of the X2+(v2+ = 3) ← 3dπ1/2+(v′′ = 3) transition recorded using the sequence of field-ionization pulses of +0.26, −1.12, −1.72, and +172.4 V cm−1 and collecting the ionization signal from the −1.72 V cm−1 pulse. Although the resolution was not sufficient to resolve the rotational structure in the spectra, we could observe a broadening of the rotational contour when selecting different rotational levels of the 3dπ1/2+(v′′ = 3) state, i.e., J′′ = 1.5 (Fig. 6(a)) and J′′ = 4.5 (Fig. 6(b)). This effect results from the increasing spread of the rotational transitions at increasing J′′ values, as illustrated by the assignment bars, which indicate the expected dominant transitions to rotational levels of the X2+(v2+ = 3) state corresponding to branches with N2+ − J′′ = −1.5,…,+1.5. From simulations (not shown) of the rotational contour using the rotational constants B3′′ = 0.1813 cm−1 (see Table 2) and B32+ = 0.2017 cm−1 (from ref. 36) of the initial and final states, respectively, we estimated the experimental resolution (full width at half maximum of a single line) to be ∼2 cm−1. The linewidth estimated from the field-ionization pulse is ∼1.5 cm−1 (see eqn (3)) and we attribute this slight discrepancy to power broadening induced by the lasers.
The results of our measurements of the vibrational structure of the X2+ ground state of MgAr2+ are summarized in Table 3, where all values are corrected for the field-induced shifts of the ionization thresholds. The specified uncertainties are all ≲3 cm−1 and represent an improvement in measurement accuracy of approximately two orders of magnitude compared to previous studies of the structure of DIDIs using double-photoionization coincidence methods (see ref. 11 and references therein). The uncertainties of the vibrational term values are smaller than the uncertainties of the transitions because of the cancellation of systematic errors in the determination of the field-induced shifts of the ionization thresholds and in the frequency calibration. From these results, we determined the harmonic and first anharmonic vibrational constants of the X2+ state to be ωe = 327.02(11) cm−1 and ωexe = 2.477(15) cm−1, respectively, which are very close to the values of ωe = 328.2 cm−1 and ωexe = 2.55 cm−1 calculated ab initio by Gardner et al.36 Using the wavenumbers of the A1/2+(v′ = 1) ← X+(v+ = 0) (31704.6 cm−1, see ref. 41 and 43) and the 3dπ1/2+(v′′ = 2) ← A1/2+(v′ = 1) (35596.2 cm−1, see Table 2) band origins, we further determined the adiabatic ionization energy of MgAr+ to be EI(X+)/(hc) = 111
824(4) cm−1, which, to our knowledge, is the most accurate value for the ionization threshold of a molecular cation obtained to date.
v 2+ | v′′ |
![]() |
![]() |
![]() |
|
---|---|---|---|---|---|
a Vibrational term values with respect to the X2+(v2+ = 0) level. b Vibrational term values with respect to the X+(v+ = 0) level. c Vibrational term values calculated using the potential function given in eqn (6) and the parameters listed in Table 4. | |||||
0 | 2 | 44![]() |
0.0(10) | 111![]() |
0.8 |
1 | 2 | 44![]() |
322.0(10) | 112![]() |
0.1 |
2 | 3 | 44916.4(19) | 639.0(10) | 112463.0(24) | −0.4 |
3 | 3 | 45228.6(19) | 951.3(10) | 112![]() |
−0.6 |
4 | 4 | 45296.3(20) | 1259.3(10) | 113![]() |
0.1 |
5 | 3 | 45838.0(18) | 1560.7(10) | 113384.7(24) | −0.6 |
6 | 4 | 45894.6(24) | 1857.6(10) | 113![]() |
−0.7 |
7 | 4 | 46![]() |
2151.0(10) | 113![]() |
0.8 |
8 | 4 | 46474.4(19) | 2437.5(10) | 114261.5(24) | 0.6 |
We determined the dissociation threshold D0 of the X2+ state via the thermodynamic cycle
![]() | (4) |
To provide an accurate description of the bond in the MgAr2+ ground state we used a model potential of the form
V(R) = VMorse(R) + Vlr(R) | (5) |
![]() | (6) |
![]() | ||
Fig. 7 Potential-energy function for the lowest two (X2+ and A2+) electronic states of MgAr2+. The potential-energy function corresponding to the atomic Mg2+ + Ar limit was determined by fitting the potential parameters in eqn (6) to match the measured vibrational levels (shown in blue) and the dissociation threshold (D0). The dashed and dotted lines show the long-range and Morse-type contribution to the potential energy, respectively. The repulsive potential-energy function corresponding to the atomic Mg+ + Ar+ limit (horizontal dashed line at position Drep above the ground rovibronic level) is approximated by a pure Coulomb potential. |
![]() | (7) |
25 years have elapsed since Falcinelli et al.14 reported their extensive list of thermodynamically stable DIDIs. In this time, progress in the characterization of their structure and dynamics has been exclusively theoretical (see, e.g., ref. 9, 20 and 36 and references therein). This lack of spectroscopic data may appear surprising at first sight but is explainable by experimental challenges. The spectroscopic methods used to study DIDIs, emission21,26 and photofragment22–25,27 spectroscopy of the doubly charged systems and single-photon or electron-impact double ionization spectroscopy of the neutral parents,11 are all particularly challenging for thermodynamically stable DIDIs. The first electronically excited state in these DIDIs is typically repulsive in the Franck–Condon region of the stable vibrational levels (see Fig. 1(c) and (d)) so that electronic spectra are structureless (continuous). Rotational and vibrational absorption or emission spectra in the electronic ground state are in principle observable, but their detection is severely complicated by the very low densities of BA2+ molecules that can be generated in the gas phase. The parent neutral molecules BA are highly reactive and must be generated in situ, which leads to insufficient concentrations for the detection of single-photon double-ionization coincidence events. In the future, we believe that non-destructive measurements of absorption processes of individual DIDIs in ion traps will offer an attractive route to obtain high-resolution rotational and vibrational spectra of these systems.63
In this article, we have demonstrated the successful use of high-resolution photoelectron spectroscopy of the singly-charged parent ion BA+ as a powerful method to study DIDIs. The advantages are obvious: (i) the measurement of high-resolution photoelectron spectra does not require high-density samples (here 5000 ions per second at 104 cm−3 density) and is ideally suited for the study of charged species, as is well known for anions (see, e.g., ref. 64 and references therein), which can be ionized with commercial VIS and UV lasers. So far its application to cations has been hampered by their high ionization energies. (ii) In the case of thermodynamically stable DIDIs, the ionization energy of BA+ is comparable to that of B+ (EI/(hc) = 121267.64 cm−1 in the case of Mg+54), which is low as explained in Section 1. The metallic nature of B further guarantees that B+ and therefore also BA+ have low-lying electronic states that can be used as intermediate states to efficiently ionize BA+ in resonant multiphoton processes. (iii) The parent cation BA+ can be produced in selected rovibrational levels by photoexcitation from the ground state of BA using threshold ionization techniques (see ref. 30 and 65), which can be exploited to access a broad range of vibrational levels of BA2+.
Photoelectron spectroscopy of singly charged cations can also be used to study metastable DIDIs. The requirements for the efficient photoionization of BA+, however, are more stringent because the energies are higher in this case and adequate multiphoton ionization sequences may be more difficult to find. Nevertheless, the list of metastable DIDIs presented in the review of Sabzyan et al.9 makes one optimistic that several of them can be studied with the method presented here. Studies of He22+, O22+, and CO2+ would be of particular importance for fundamental reasons and also for applications in atmospheric chemistry and astrophysics. In the future, we expect that progress in the development of powerful narrow-band VUV radiation at free-electron laser facilities will offer the possibility of efficiently ionizing molecular cations in single-photon processes and recording their high-resolution single-photon photoelectron spectra.
The experimental method presented here to study molecular dications is not restricted to DIDIs, but can of course be equally well applied to polyatomic systems.
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