Lianjia
Wu
a,
Martijn
Tiekink
a,
Alexandre
Giuliani
b,
Laurent
Nahon
b and
Sonia
Castellanos
*a
aAdvanced Research Center for Nanolithography, Science Park 110, 1098 XG Amsterdam, The Netherlands. E-mail: s.castellanos@arcnl.nl
bSOLEIL, l’Orme des Merisiers, St Aubin, BP48, 91192 Gif sur Yvette Cedex, France
First published on 4th December 2018
The investigation of the photoionization processes of a series of titanium oxo clusters evidenced that doping their organic shell with extended aromatic structures decreases their ionization energy and stabilises the resulting radical cations. Such tunability of their photochemistry arising from ligand exchange gives these hybrid compounds great potential as EUV photoresists.
Metal oxo clusters (MOCs), as molecular hybrid materials with a core/shell-like configuration,7–9 are promising EUV photoresists.10,11 The inorganic metal oxo core gives MOCs enhanced EUV absorption,12 and, as shown by other inorganic photoresists, can potentially yield better mechanical and chemical stability as well as etch resistance in the final patterns, as compared to conventional organic photoresist.13,14 The molecular identity of MOCs, in turn, provides them with small and homogeneous size, which is expected to decrease the roughness of the patterns generated by EUV lithography. Recently, we proved that these types of materials can effectively work as EUV photoresists and that their EUV absorption and sensitivity can be modified by playing with the composition of the inorganic core.10 In addition, because of their exchangeable organic shell,15–17 MOCs have a remarkable synthetic versatility.
In this work, we took advantage of this last feature to tune the photon-induced reactivity of Ti-MOCs. The organic shells of Ti-based MOCs were “doped” with extended aromatic ligands to modify their highest occupied molecular orbital (HOMO) levels. By raising the energy of the HOMO, the ionization energy is lowered. It has been reported that EUV chemically amplified resists (CARs) with lower band gaps lead to the generation of more acids.18 This is attributed to the formation of more electron–hole pairs during the scattering of photoelectrons emitted upon EUV absorption. Meanwhile, the resulting holes can be stabilized in the conjugated structure, which can be used as a channel to modulate hole-induced reactivity. Thus, by tuning the band gap of the materials and of the localization of their frontier orbitals, it is anticipated that their reactivity upon EUV exposure can be also tuned.
The photodissociation and photoionization of this series of Ti-based MOCs towards vacuum ultraviolet (VUV) radiation in the 7–12 eV energy range were investigated in the gas phase by mass spectrometry (MS). Although VUV-MS has been previously used to study metallic nanoparticles,19–21 and very recently to study molecular tin-based oxo-cages,22 to the best of our knowledge, this is the first time that this technique is used to investigate the photochemistry of well-defined metal oxo clusters. These experiments confirm the effect of the doping with aromatic ligands onto the ionization potential and stabilization of the ionized products. Furthermore, the study of the fragmentation processes induced by different photon energies can help to understand the chemistry triggered upon irradiation with higher energy photons, i.e. EUV photons. Specifically, it can give insights on the chemistry induced upon exposure to EUV light during the lithographic application, which mainly leads to the ionization of the material.
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1 mol ratio) in chloroform was added to a solution of Ti8L16 in chloroform. The resulting yellow-green solution was stirred magnetically at room temperature for 1 hour. The solvent was evaporated under vacuum. Acetonitrile was added to the yellow solid. The suspension was filtered and washed with acetonitrile. The product was dried under vacuum and characterized with 1H NMR and IR.
Fig. 1 shows the calculated highest-occupied molecular orbital (HOMO) and lowest unoccupied molecular orbital (LUMO) energy and contour plot of the newly designed titanium oxo clusters when a doping ratio of 1
:
15 is used. To simplify the calculation, Ti oxo acetate clusters, rather than Ti oxo pivalate cluster were used. The two isomers resulting from the substitution of a pivalate ligand in the axial or the equatorial position have been considered. According to the DFT calculations, the HOMOs of the doped Ti oxo clusters are located on the corresponding aromatic ligand and their eigenvalues are hence raised in comparison to the pristine cluster featuring only pivalate ligands, while their LUMOs remain on the ring structure of octameric Ti oxo core regardless of the presence of doping ligands. The calculated HOMO energy of Ti8L16 is 7.37 eV, while this value increases by 1.5–2.2 eV for Ti8L15BTC, Ti8L15CB, and Ti8L15AC (for calculations L = acetate), no matter which position (axial/equatorial) the new ligand exchanged (Table S1 in ESI†).
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| Fig. 1 HOMO/LUMO energies and contour plots of the different Ti oxo clusters calculated with DFT using the hybrid B3LYP functional and the 6-31G(d) basis set. | ||
APPI was used to generate the parent charged species from the initial neutral Ti oxo cluster molecules. In this technique, photons of 10.0 and 10.6 eV emitted by a krypton lamp are shone on the gas phase formed from the neutral molecules and the solvent (toluene). The latter gets ionized and reacts by charge exchange and/or proton transfer reactions with the neutral molecule. In the case of this series of Ti oxo clusters, APPI yielded the product corresponding to the loss of one pivalic acid, [M–L]+. The resulting positively charged [M–L]+ ion was selectively trapped as parent ion [P]+ for VUV-MS experiments. The trapped parent ions were clearly identified as [Ti8L15]+ with m/z 2027.5 (Fig. 2), [TiL14BTC]+ with m/z 2135.4, [Ti8L14CB]+ with m/z 2212.5, and [TiL14AC]+ with m/z 2147.5, respectively. In all cases the isotopic distribution perfectly matches the expected ratios for an octameric Ti oxo cluster (Fig. S9–S11 in ESI†).
Fig. 3 displays the mass spectra of four trapped parent ions after VUV irradiation at 11 eV. For all four parent ions, the main photoproduct is identified as the product of pivalate photodissociation [P–L]+: [Ti8L14]+˙ (m/z 1926), [Ti8L13BTC]+˙ (m/z 2035), [Ti8L13CB]+˙ (m/z 2111), and [Ti8L13AC]+˙ (m/z 2046), respectively. Note that the dissociation of the aromatic ligand from the doped parent to yield [Ti8L14]+ was barely detected. Dicationic species [Ti8L14BTC]2+˙ (m/z 1068), [Ti8L14CB]2+˙ (m/z 1107), and [TiL14AC]2+˙ (m/z 1074) also appear in the spectra, although in much lower concentration. Interestingly, in the case of the non-doped Ti oxo cluster the ionized parent ion [Ti8L15]2+˙ was not detected and only the dication [Ti8L14]2+ (m/z 913) appears in the low mass region of the spectrum. Finally, dicationic species assigned to [P–L]2+, [Ti8L13BTC]2+ (m/z 966), [Ti8L13CB]2+ (m/z 1005), and [TiL13AC]2+ (m/z 972) were present in much lower concentration.
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| Fig. 3 Mass spectra after photon activation at 11 eV (a–d) and fragment yields resulting from ionization of the parent ion [P]+ as a function of photon energy (e–h). | ||
In order to determine the photoionization energy threshold for this set of materials, the relative yield of dication formation upon irradiation in the 7–12 eV energy range for the non-doped [Ti8L15]+ and doped [Ti8L14BTC]+, [Ti8L14CB]+, and [Ti8L14AC]+ was monitored (Fig. 3). In the plots it can be observed that the dicationic species [P–L]2+ is detected above 11 eV in all compounds. However, in the case of the doped clusters an extra curve can be plotted for the “clean” photoionization product [P]2+, which is not accompanied by ligand dissociation. The ionization energy onsets for the doped compounds are 8.98 ± 0.07 eV for [Ti8L14BTC]+, 8.42 ± 0.06 eV for [Ti8L14CB]+ and 8.57 ± 0.03 eV for [Ti8L14AC]+ (Fig. S12–S15 in ESI†).
These results indicate that in the case of the doped MOCs, which feature one aromatic ligand, the hole generated upon photoionization can be stabilized by the conjugated system. The non-doped parent compound, on the other hand, undergoes a dissociative ionization where a pivalate ligand is lost so that no [TiL15]2+˙ species is detected. The lower energy onsets for the photoionization of the doped clusters nicely follow the trends in their calculated HOMO values, where the presence of the aromatic ligands raise the HOMO levels by 1.5 to 2.2 eV. Yet, above 11 eV all compounds undergo a dissociative ionization. The photoreactions in the 7–12 eV energy range for the studied oxo clusters are thus summarized in Scheme 2.
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| Scheme 2 Proposed photoexcitation reactions of the parent ions for the pristine Ti-MOC and the derived doped series. | ||
The plot of the total fragmentation yield normalized by the photon flux as a function of photon energy gives the action spectra (equivalent to an absorption spectrum) of the four Ti oxo clusters (Fig. 4). Photon absorption below 8.4 eV only yields the photodissociation of the pivalate ligands (Fig. S16 in ESI†). Above, multiple decay paths contribute to the spectra: pivalate dissociation, net ionization, and dissociative ionization. A broad band can be observed at 8.5 eV for all compounds except for [Ti8L14CB]+, where it appears as a smooth shoulder. At 10.5 eV, on the other hand, a sharp peak can be observed in all oxo clusters. This spectral feature could be related to a shape resonance in the dissociative ionization channel previously discussed.
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| Fig. 4 Action spectra of parent ions [Ti8L15]+, [Ti8L14BTC]+, [Ti8L14CB]+, and [Ti8L14AC]+. The estimated error is 16% (error bars are omitted for better visualization). | ||
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15 ratio opens an extra ionization channel located at ∼2.0–2.5 eV lower energies. This different reactivity is attributed to the introduction of a new HOMO level that is mainly located in the aromatic doping ligand. This work highlights the great potential of MOCs as photoresists, since the synthetic versatility offered by ligand exchange reactions can be exploited to modify at will the reactivity of their ionized states. This feature makes them ideal molecular materials for the study of EUV induced photochemistry and will assist in the development of new EUV photoresist materials.
Footnote |
| † Electronic supplementary information (ESI) available. See DOI: 10.1039/c8tc05273e |
| This journal is © The Royal Society of Chemistry 2019 |