Eleanor K.
Ashworth
a,
Cate S.
Anstöter
b,
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, Durham, DH1 3LE, UK. E-mail: j.r.r.verlet@durham.ac.uk
First published on 3rd March 2021
Astrochemical modelling has proposed that 10% or more of interstellar carbon could be tied up as polycyclic aromatic hydrocarbon (PAH) molecules. Developing reliable models of the interstellar carbon lifecycle requires calibration data obtained through laboratory studies on relevant chemical and physical processes, including on the photo-induced and electron-induced dynamics of potential interstellar PAHs. Here, the excited state dynamics of the S1(ππ*) state of 2-naphthoxide are investigated using frequency-, angle-, and time-resolved photoelectron imaging. Frequency-resolved photoelectron spectra taken over the S1(ππ*) band reveal low electron kinetic energy structure consistent with an indirect, vibrational mode-specific electron detachment mechanism. Time-resolved photoelectron imaging using a pump photon energy tuned to the 0–0 transition of the S1(ππ*) band (hν = 2.70 eV) and a non-resonant probe photon provides the excited state autodetachment lifetime at τ = 130 ± 10 fs. There is no evidence for internal conversion to the ground electronic state or a dipole-bound state. These results imply that 2-naphthoxide has no resilience to photodestruction through the absorption of visible radiation resonant with the S1(ππ*) band, and that electron capture by the S1(ππ*) state, which is formally a shape resonance, is not a doorway state to a stable interstellar anion.
Interestingly, of the molecules known to exist in space through assignment of astronomical spectra, only six are anions: C2nH− (n = 2–4) and C2n−1N− (n = 1–3). Theoretical modelling has indicated that larger carbonaceous anions, such as longer-chain polyynes and PAHs, including those with oxygenation, should be present in space.12–15 However, there is a dearth of knowledge on the ultrafast photon- and electron-induced photophysics of isolated PAHs, particularly anionic PAHs; these processes ultimately define the formation, destruction, and photoresilience mechanisms of PAH molecules in space. Determination of these properties is important for defining whether certain molecules or classes of molecules can exist in space and thus inform on the interstellar carbon balance.16,17
The 2-naphthoxide species, 2-Np− shown in Fig. 1, is one of the simplest polycyclic aromatic hydrocarbon (PAH) anions possessing heteroatom functionalisation. This class of PAH molecules are often invoked as probable interstellar carbonaceous species.2 For example, laboratory studies on pristine PAHs encapsulated in icy matrices irradiated with ultraviolet light or impacted with high-energy particles show formation of alcohol, ketone, and carboxylic acid functional groups,14,15,18,19 indicating that oxygenated PAHs, most likely as closed-shell molecules, should contribute to the interstellar carbon balance. Other experiments which subjected PAHs to interstellar conditions found extensive hydrogenation, oxygenation, and hydroxylation, ultimately leading to more complex organics.20 In a recent contribution, one of the present authors reported a photodetachment study on 2-Np− thermalised to T ≈ 300 K,21 providing an action spectrum of the S1(ππ*) band as well as identifying several other weak spectral features spanning the electron detachment threshold, which were attributed to a progression of dipole-bound states. Two recent investigations using cryogenic photoelectron and photodetachment techniques have reported near-threshold spectra of 2-Np−, and also identified dipole-bound states.22,23
In this paper, we report a frequency-, angle-, and time-resolved photoelectron imaging study of 2-Np− thermalised to T ≈ 300 K. The key questions that this study addresses are: (1) What is the lifetime of the S1(ππ*) state when exciting at the 0–0 transition? (2) What are the decay dynamics of the excited state, and is there any internal conversion to recover the ground electronic state? (3) What do the above-threshold dynamics tell us about the photoresiliance and propensity for stable anion formation in space?
For the time-resolved measurements, femtosecond laser pulses were derived from a Spectra-Physics Ti:sapphire oscillator and regenerative amplifier. The hν = 2.70 eV (459 ± 5 nm, ≈20 μJ) pump pulses were produced through fourth-harmonic generation (two successive BBO crystals) of the idler output from an optical parametric amplifier (Light Conversion TOPAS-C). The hν = 1.55 eV (800 nm, ≈100 μJ) probe pulse corresponds to the fundamental output of the femtosecond laser. Pump and probe pulses were delayed relative to each other (Δt) using a motorised delay line. Both pulses were combined colinearly using a dichroic mirror and were loosely focused into the interaction region using a curved metal mirror. The pump–probe cross correlation was ≈60 fs.
Fig. 2 Photoelectron spectroscopy of 2-Np−: (a) example photoelectron spectra; the spectrum in the inset is associated with exciting the dipole-bound state at hν = 2.38 eV, (b) photodetachment spectrum at T ≈ 300 K taken from ref. 21. The ADE is 2.4037 ± 0.0005 eV (taken from ref. 23). The feature denoted by * in the black trace in (a) is attributed to detachment to the ground vibrational state of the 2-naphthoxy neutral (2A′′). |
The photoelectron spectra shown in Fig. 2a show a prompt detachment feature – an eKE distribution that tracks the increase in photon energy – which contains contributions from direct photodetachment and prompt autodetachment without significant nuclear relaxation. Because photoexcitation cross-sections for the S1(ππ*) and S2(ππ*) state will be much larger than cross-sections for direct photodetachment, the prompt detachment feature will be dominated by the prompt autodetachment contribution. The prompt detachment feature is most obvious when comparing all of the photoelectron spectra given in the ESI.† The higher photon energy spectra, e.g. hν = 2.93 eV in Fig. 2a and other spectra in the ESI,† exhibit three spectral features: (i) the low-eKE vibrational structure as described above, (ii) the prompt detachment feature, and (iii) a delayed autodetachment band (e.g. the fixed 0.1 ≤ eKE ≤ 0.4 eV window in the hν = 2.93 eV spectrum and other spectra in the ESI†). The delayed autodetachment band has several possible origins, including changing Franck–Condon factors with photon energy, fast nuclear relaxation followed by autodetachment, and at higher photon energies could have a contribution from excitation of the S2(ππ*) state followed by internal conversion and autodetachment from the S1(ππ*) state. β2 values over the prompt detachment and delayed autodetachment features are approximately zero, consistent with isotropic electron ejection.
The hν = 2.70 eV photoelectron spectrum and others given in the ESI† show vibrational structure on the prompt detachment feature with spacing of 60 ± 10 meV (480 ± 80 cm−1). This vibrational structure is consistent with that observed in the photodetachment action spectrum (Fig. 2b), which was assigned to the principal Franck–Condon active mode for excitation of the S1(ππ*) state (calculated ν32(a′) = 437 cm−1) through Franck–Condon-Herzberg–Teller simulations.21 It is also worth noting that this vibrational structure is consistent with the principal Franck–Condon modes for direct photodetachment characterised by an earlier cryogenic photoelectron spectroscopy experiment,22 involving ν32(a′) = 422 cm−1 (neutral), which is an in-plane CCC bending mode and has most displacement localised on the oxygen-containing benzyl ring. In the present photoelectron spectra, the vibrational structure over the prompt detachment band in the photoelectron spectra is presumably associated with prompt autodetachment through electron shake-off by the ν32 mode of the anion excited state.
The time-resolved photoelectron spectra and velocity-map images do not show any evidence for internal conversion to a dipole-bound state, which would be evident as a sharp feature in the time-resolved spectra at an eKE close to the probe photon energy and present as an anisotropic ring in the velocity-map images.31,33 It is worth noting that although the relative photodetachment cross-section (i.e. probe cross-section) from the dipole-bound state and the S1(ππ*) state are not known, time-resolved imaging experiments on other systems in which a photoexcited valence-localized state internally converts to a dipole-bound state show that population of the dipole-bound state should be evident in the time-resolved spectra, even if only a small fraction (e.g. <10%) of photoelectron signal in the pump-only photoelectron spectrum is attributed to internal conversion to the dipole-bound state.31 We conclude that there is no substantial amount of internal conversion from the S1(ππ*) state to the dipole-bound state. Regardless of the detailed mechanism, the time-resolved experiments show that the excited state population almost exclusively decays by autodetachment, and, therefore, no ground state of the anion is recovered by internal conversion as has been observed for several other anions.25,32,34 Based on the action spectrum, the vibrational period of the dominant nuclear motion (if exciting above the 0–0 transition) involves the 437 cm−1 mode, which has a vibrational period of 76 fs. Hence, with an autodetachment lifetime of 130 fs, only a few vibrations can take place on the excited state before the electron is ejected.
(a) Some fraction of the photoexcited population undergoes an ultrafast intersystem crossing to a triplet state (T), which is situated below the detachment threshold. The triplet state then undergoes a mode-specific autodetachment. The triplet state may have a very low photodetachment cross-section and thus not be observed in the time-resolved experiments using a 800 nm probe. A recent study on a related oxygenated PAH anion has implied an ultrafast intersystem crossing,35 although the study hypothesised that an intermediate dipole-bound state facilitated triplet formation; there was no evidence for internal conversion to a dipole-bound state in the present study. We also note that our earlier study using ion mobility spectrometry coupled with laser spectroscopy on carboxylate substituted versions of 2-Np− infer triplet formation through the observation of fluorine-substitution photoreactions following excitation of the S1(ππ*) band but not the S2(ππ*) band.21 Those experiments indicate that the excited state in the carboxylate substituted versions of 2-Np− must survive for nanoseconds based on the buffer gas pressure and the rate for ion–molecule collisions leading to products. No such photoreactions were observed for 2-Np−. Ultimately, we conclude that assignment of the low-eKE vibrational structure to mode-specific autodetachment from a triplet state is unlikely.
(b) Some fraction of the photoexcited population on the S1(ππ*) state undergoes a mode-specific autodetachment induced by a low-frequency mode, which is presumably thermally populated at T ≈ 300 K in the hν = 2.70 eV experiment since we are exciting at the 0–0 transition. The nuclear motion induced by population of the low-frequency mode leads to a modulation of the vertical detachment threshold and consequently a ‘shake off’ of the electron. The low-eKE vibrational structure with spacing of ≈35 meV (282 cm−1) could potentially correspond to the ν33(a′) = 313 cm−1 mode calculated for the S1(ππ*) state.21 This mode is the lowest frequency a′-symmetry mode involving an in-plane bend. However, it is difficult to reconcile the observation of similar low-eKE structure in the photoelectron spectra for photon energies hν < 2.7 eV (e.g. 2.38 eV, Fig. 2a), where the S1(ππ*) state is not excited and only the dipole-bound state(s) is accessible.
(c) A small fraction of the anions are excited directly to the dipole-bound state, i.e. there is a progression of dipole-bound states. The dipole-bound state autodetaches through mode-specific vibrational autodetachment invoked by modes that strongly couple the dipole-moment to the continuum.31,33,36,37 These modes would be similar to the modes of the final neutral ground state. The lowest frequency mode of a′ symmetry for the D0 electronic state was calculated at ν33 = 310 cm−1 and is moderately infra-red active. This vibrational mode satisfies the criterion for efficient electron ejection or ‘shake off’ when directly exciting the dipole-bound state – modulation of the dipole-bound state orbital by the vibrational motion – and would generate a similar (s-wave) low-eKE spectrum to mode-specific autodetachment proposed in mechanism (b).33,36–41 This detachment mechanism usually involves Δv = −1, where v is a vibrational level, although anharmonicity associated with low-frequency bending modes has shown that Δv = −2 also occurs in this system.23 The proposed low frequency mode, ν33, is likely to be populated at T ≈ 300 K according to Boltzmann statistics. It is worth noting that the recent cryogenic study of 2-Np− by Qian et al.23 performed photoelectron spectroscopy following resonant excitation of 38 levels of the dipole-bound state. They found that seven Franck–Condon-forbidden out-of-plane bending modes were involved in mode-specific autodetachment, including the lowest two frequency a′′ modes at ν48 = 102 cm−1 and ν47 = 171 cm−1. Furthermore, both ν33 and ν32 modes are major features in the resonant photoelectron spectra for various excited dipole-bound levels. Whatever the active modes leading to mode-specific vibrational autodetachment, mechanism (c) readily explains the low-eKE vibrational structure in the hν = 2.38 eV spectrum, although mechanism (c) is unlikely at hν = 2.70 eV (0–0 transition of the S1(ππ*) band) since there was no evidence for a dipole-bound state in the time-resolved measurements. Unfortunately, time-resolved experiments with a pump photon energy tuned to directly excite the dipole-bound state and monitor the autodetachment dynamics were unsuccessful due to the low photoexcitation cross-section. However, such an experiment has been recently performed on cryogenically cooled phenoxide,41 determining lifetimes ranging between 33.5 and 1.4 ps depending on the dipole-bound state vibrational level (the lifetime of the dipole ground vibrational state will be substantially longer). Lifetimes for dipole-bound state levels of 2-Np− are presumably shorter due to the increased density of states and, in the present study, initial ion temperature.
Ultimately, the consistent interpretation for photon energies over the S1(ππ*) band of 2-Np− at T ≈ 300 K is provided by mechanism (b), which involves partial nuclear relaxation of the S1(ππ*) state followed by vibrational electron shake-off by the low-frequency ν33(a′) mode. A similar electron shake off occurs by the corresponding mode of the neutral molecular core when directly exciting the dipole-bound state, consistent with mechanism (c).
It is worth mentioning that in the present experiment we optically prepared the same excited states that could be occupied through an electron capture mechanism.24,37 From an experimental point of view, our approach has two key advantages over an electron capture experiment: (i) the ability to directly probe the dynamics using femtosecond laser strategies, and (ii) mass-selectivity through separation of anions using time-of-flight mass spectrometry.
As we outlined in the introduction, while small oxygenated PAH molecules are likely interstellar species, the present experiments on 2-Np− have shown that population of either the lowest energy dipole-bound state or the S1(ππ*) state does not result in formation of a stable anion, rather that the anion excited states decay through autodetachment. The radiative electron capture mechanism is therefore not important for this species. We acknowledge that the present study considered ions initially thermalised to T ≈ 300 K, which is substantially warmer than typical interstellar molecule conditions of T = 10–20 K.46 However, we expect similar results for cold anions since the S1(ππ*) state is situated in the detachment continuum and is unbound to the electron detachment threshold, and because there was no evidence for internal conversion from the dipole-bound state. The situation is different for other PAH-based anions known to undergo ultrafast internal conversion to the ground electronic state anion after excitation to a resonance,25,32 attributed to the presence of lower-lying bound excited states; 2-Np− has no such states. Known interstellar polyyne anions, e.g. C6H− and C8H−, have similar bound electronic states.47 That being said, we have shown that other molecules such as the radical anion of para-benzoquinone,24 which has no valence-bound excited electronic states, may exhibit a small fraction thermionic emission when excited to the lowest lying above-threshold resonances. Ultimately, we conclude that 2-Np− is unlikely to be formed in the interstellar medium through radiative electron attachment and has no resilience to photodestruction through the absorption of visible radiation resonant with the S1(ππ*) band.
Footnote |
† Electronic supplementary information (ESI) available: Photoelectron spectra recorded at other photon energies. See DOI: 10.1039/d1cp00261a |
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