Joe
Gregory
*a,
Jan R. R.
Verlet
b and
James N.
Bull
a
aSchool of Chemistry, Norwich Research Park, University of East Anglia, Norwich NR4 7TJ, UK. E-mail: james.bull@uea.ac.uk
bDepartment of Chemistry, Durham University, South Road, Durham DH1 3LE, UK
First published on 3rd April 2020
Spectroscopic characterisations of the radical polyinterhalogen molecules IF2 and I2F are reported using anion photoelectron spectroscopy. The corresponding parent anions, IF2− and I2F−, are common products formed in hard Ar–CF3I plasmas and are relevant in the semiconductor manufacture industry. The I2F− species, which is present as the [I–I–F]− isomer, is a “non-classical” polyinterhalogen.
This paper reports a combined photoelectron spectroscopy and electronic structure theory study on the IF2−, I2F−, IF2 and I2F species. There have been several reports of synthesis, crystallography and spectroscopic characterisation of IF2− embedded in a solid state matrix,9,10 and computational studies on IF2− and I2F− and related species,7,10–14 however, a recent review by Riedel and co-workers2 noted “Thus far,… [I2F]− have not been detected experimentally.” While this statement might be true for condensed phases, I2F− appears to be a common product formed in hard Ar–CF3I plasmas.
There are only a handful of examples of gas-phase spectroscopic studies on polyhalogen species, mostly targeting I3−. A series of pioneering investigations by Neumark and co-workers15–18 applied anion photoelectron spectroscopy with different laser sources to characterise vibronic properties of the radical neutral I3, and photodissociation dynamics of the parent anion. Several other studies have focussed on photodissociation dynamics.19–22 There have been two investigations on I2Br− probing the dissociation dynamics, with one of these studies providing a single-colour photoelectron spectrum at 267 nm.23,24 In the present work, we have coupled a jet-cooled plasma discharge source with time-of-flight mass spectrometry and anion photoelectron spectroscopy. This strategy allows for generation and mass selection of IF2− and I2F−, and determination of spectroscopic properties of the radical neutral IF2 and I2F species.
Intriguingly, radical polyinterhalogen molecules may have a significant bearing in industrial plasma processes. In particular, in the present study we produced the IF2− and I2F− species through plasmisation of an Ar–CF3I mixture; this mixture and process is relevant in the semiconductor manufacture industry. In this industry, dry-etching plasma processes utilise the reaction between silicon wafers, which are the substrate for semiconductor and microprocessors, and fluorine atoms and CF3 radicals to etch the substrate at specific locations on the wafer.25 Conventionally, these radical species are produced in a plasma consisting of an inert carrier gas seeded with CF4 or C3F8. In recent years, there has been growing interest in the use of CF3I as an alternative to CF4 because the use of CF4 is restricted in many countries by the Montreal Protocol due to the molecule's high global warming potential (GWP).26,27 For example, even though CF3I is infrared active, CF3I has an atmospheric residence life of ≈1 day and corresponding GWP ≈ 1.28,29 In contrast, CF4 has a residence life of ≈50000 years and corresponding GWP ≈ 6000.29,30 Furthermore, although iodine atoms formed through UV photodissociation of CF3I are exceptionally destructive towards stratospheric ozone,31 the short residence time of CF3I released at terrestrial altitudes means that these molecules do not reach the stratosphere and contribute to ozone destruction. Ultimately, modelling and tuning of the etching process allows maximisation of process efficiency and minimisation of unwanted by-products. Theoretical plasma models require a detailed qualitative and quantitative understanding of the rich ion–molecule and electron–molecule chemistry that occurs in dry-etching plasmas (particularly the chemistry associated with fluorine-containing radicals).32–36
[F–I–F]− | [F–F–I]− | [I–I–F]− | [I–F–I]− | |
---|---|---|---|---|
ADEe | 4.03 ± 0.02 | — | 4.04 ± 0.06 | — |
VDEe | 4.23 ± 0.04 | — | 4.23 ± 0.04 | — |
ADEc | 4.14 (4.15) | 3.17 | 4.22 (4.28) | 3.19 (3.38) |
VDEc | 4.40 (4.50) | 3.88 | 4.40 (4.55) | 3.96 (4.08) |
A Franck–Condon simulation of the photoelectron spectrum for the [F–I–F]− configuration is shown in Fig. 1 and has good agreement with the experimental spectrum. The simulation suggests that the vibrational progression is dominated by detaching transitions to the ν2 (asymmetric stretch) and ν3 (symmetric stretch) vibrations of the [F–I–F] radical neutral species; calculated frequencies suggest that these two vibrations are nearly degenerate – see Table 2. We can therefore assign the experimental value of ν2/ν3 at 600 ± 50 cm−1 for the [F–I–F] species. The small feature denoted by * in the inset in Fig. 1 is probably a hot band from vibrationally-excited ions produced in the plasma (see ESI†). The ADE assignment to the 0–0 transition should be robust based on alignment of the VDE with the Franck–Condon simulation. It is worth noting that a Franck–Condon simulation of the photoelectron spectrum for the [F–F–I]− isomer (see vibrational frequencies for [F–F–I] in Table 2) is inconsistent with the experimental spectra, lending support to the above isomer assignment.
Calculated vertical excitation energies for the [F–I–F]− isomer are given in Table S1 in the ESI.† These data show that although an excited state resonance is energetically accessible with a hν = 4.66 eV photon, oscillator strengths are zero and therefore the photoelectron spectra in Fig. 1 should be described by direct photodetachment to the ground electronic state of the neutral. Calculated vertical excitation energies for neutral [F–I–F], i.e. electronic excited states of [F–I–F] at the [F–I–F]− equilibrium geometry, suggested that only the ground electronic state is accessible using the photon energies in Fig. 1, consistent with a single vibrational progression.
Fig. 3 (a) Photoelectron spectra for I2F− at hν = 4.43, 4.66 and 5.17 eV. Electron binding energy (eBE) and electron kinetic energy (eKE) are related by eBE = hν − eKE, where hν is the photon energy. (b) Franck–Condon simulation of direct photodetachment to the D0 and A1-symmetry neutral electronic states. The simulations suggest that the D0 ← S0 detaching transition is dominated by low frequency modes and combination bands. See ESI† for Franck–Condon simulations at higher temperatures which assign the feature denoted by * to a hot band. |
The ADE and VDE parameters for the lower energy band are consistent with the calculated values for the [I–I–F]− isomer (Table 1), again with a small overestimation by theory. The two bands in Fig. 3a are thus assigned to detaching transitions to the ground and excited electronic states of the [I–I–F] radical neutral. Equilibrium geometries for the I2F− and I2F isomers are shown in Fig. 4; the [I–I–F]− isomer is more stable by 1.35 eV (130 kJ mol−1), consistent with it being the predominant isomer formed in the plasma. There was no evidence for the [I–F–I]− isomer when photoelectron spectra were recorded at photon energies below the ADE for the [I–I–F]− isomer. A Franck–Condon simulation of the photoelectron spectrum to give the ground electronic state of the neutral (red in Fig. 3b) shows no clear vibrational structure, consistent with experimental spectrum. Calculated vibrational frequencies are given in Table 3.
The second, higher binding energy photodetachment band in Fig. 3a was assigned to direct photodetachment to the A1 state of the [I–I–F] species. Geometry optimisation of this state at the EOM-CCSD//def2-TZVPD level of theory produced a linear (C∞h symmetry) structure with rII = 3.02 Å and rIF = 1.96 Å. Using this structure, ADE2 was calculated at 4.79 eV (term energy, Te, of 0.57 eV which is close to the experimental value of Te = 0.56 ± 0.08 eV), which is again ≈4% larger than experiment. Calculated vibrational frequencies for the A1 state are ν1 = 109 cm−1 (bend), ν2 = 157 cm−1 (symmetric stretch) and ν3 = 530 cm−1 (asymmetric stretch). A Franck–Condon simulation of the photoelectron spectrum associated with formation of the A1 state of the neutral is shown in green in Fig. 3b, and predicts that the vibrational structure is predominantly from the ν3 = 530 cm−1 mode. The feature denoted by * in Fig. 3a at eBE = 4.56 eV is assigned to hot band signal (see ESI†).
Calculated vertical excitation energies for the I2F− isomers are given in Table S1 in the ESI.† For the [I–I–F]− isomer, the first few electronic states have very low oscillator strengths and the photoelectron spectra for photon energies <5 eV should be dominated by direct photodetachment. There is, however, a bright A1-symmetry resonance with a calculated vertical excitation energy in the 5.1–5.2 eV range (see ESI†). Fortunately, the photoelectron spectra for both of these species are at lower binding energies and should not interfere with the spectra shown in Fig. 3. It is worth noting that the issue of bright excited state resonances in the detachment continuum is more serious for I3− (ref. 15–18) and larger polyinterhalogen anions due to an increased density of electronic states.
Polyinterhalogen molecules can be divided into two categories, classical and non-classical.3 The former is defined as containing an electropositive central atom surrounded by electronegative halogen atoms, e.g. [F–I–F]−. In contrast, for a non-classical polyinterhalogen molecule, the central halide is more electronegative than the coordinating dihalogen or interhalogen molecules, e.g. Cl(I2)4− in which four I2 molecules coordinate a Cl−.3,37 Interestingly, the [I–I–F]− species satisfies the non-classical criterion, possessing covalent-like bond lengths and a terminal F− coordinated to an I2 molecule (see NBO charges in Fig. 4). Similar arguments have been made about the [I–I–Cl]− species in the solid state.3,38 Finally, it is worth noting that Mabbs et al.23 reported a 267 nm photoelectron spectrum of I2Br−, which presumably exists as the [I–I–Br]− isomer and also is an example of a non-classical polyinterhalogen, however, their photoelectron spectrum showed no vibrational structure.
Our experiments suggest that IF2−, I2F− and most likely the corresponding neutrals are amongst the major products formed in a hard Ar–CF3I plasma. In the semiconductor manufacture industry, radical neutrals including IF2 and I2F formed in the etching plasma may collide and react with etchant substrates. In this context, the bond dissociation energy (BDE) to produce a fluorine atom is related to etching efficiency – a lower BDE gives enhanced etching capacity. For the [F–I–F] and [I–I–F] isomers, BDEs for fluorine atoms were calculated at 1.74 eV and 1.35 eV, respectively, using the CCSD(T)//def2-TZVPD level of theory. For comparison, the calculated BDE for a fluorine atom from the CF3 radical is 3.51 eV, which is substantially larger than that for the [F–I–F] and [I–I–F] isomers and suggests that polyinterhalogen radicals formed in hard Ar–CF3I plasmas are important etching species.
In summary, this paper has reported a combined photoelectron spectroscopy and electronic structure theory study on the IF2−, IF2, IF2− and I2F species, determining the gas-phase structures and electron detachment parameters for the anions and vibrational structure of the neutrals. This determination provides the first vibrationally-resolved spectroscopic characterisation of isolated polyinterhalogen radicals. Whereas IF2− as the [F–I–F]− isomer is a classical polyinterhalogen molecule, IF2− as the [I–I–F]− isomer is a non-classical polyinterhalogen molecule. Theoretical modelling of these species has shown that the CCSD(T)//def2-TZVPD level of theory, on average, predicts ADE and VDE parameters to within ≈4% of experiment, however, this level of theory suffers from some degree of Pauling-point agreement. The IF2 and I2F radicals may play an important role in plasma etching processes due to having low bond dissociation energies to give fluorine atoms.
Footnote |
† Electronic supplementary information (ESI) available: Experimental methods, theoretical methods, calculated vertical excitation energies, further Franck–Condon simulations. See DOI: 10.1039/d0cp01311k |
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