Yu-Fang
Tseng
a,
Pin-Chia
Liao
a,
Po-Hsiung
Chen
*bc,
Tsai-Sheng
Gau
*bc,
Burn-Jeng
Lin
bc,
Po-Wen
Chiu
bc and
Jui-Hsiung
Liu
*a
aDepartment of Chemistry, National Tsing Hua University, Hsinchu 30013, Taiwan. E-mail: rsliu@mx.nthu.edu.tw
bTSMC-NTHU Joint Research Center, National Tsing Hua University, Hsinchu 30013, Taiwan
cCollege of Semiconductor Research, National Tsing Hua University, Hsinchu 30013, Taiwan
First published on 10th November 2023
This work reports the success in accessing high-resolution negative-tone EUV photoresists without radical chain growth in the aggregation mechanism. The synthesis of a highly hydroxylated Hf6O4(OH)8(RCO2)8 cluster 3 (R = s-butyl or s-Bu) is described; its EUV performance enables high resolution patterns HP = 18 nm under only 30 mJ cm−2. This photoresist also achieves high resolution patterns for e-beam lithography. Our new photoresist design to increase hydroxide substitutions of carboxylate ligands in the Hf6O4(OH)4(RCO2)12 clusters improves the EUV resolution and also greatly reduces EUV doses. Mechanistic analysis indicates that EUV light not only enables photolytic decomposition of carboxylate ligands, but also enhances the Hf-OH dehydration. One additional advantage of cluster 3 is a very small loss of film thickness (ca. 13%) after the EUV pattern development.
Hafnium oxide photoresists are the best-studied clusters for the development of negative-tone EUV photoresists. Hf6O4(OH)4(RCO2)12 clusters6,13,23 were selected as the platform (see Scheme 2). Our desired EUV photoresists are to avoid a radical chain aggregation; a MAA ligand is now replaced with 2-methylbutyrate. The synthesis involves multiple hydroxide (OH−) substitutions of the carboxylated ligands as in Hf6O4(OH)4(RCO2)12 clusters. The molecular sizes of new hafnium clusters become smaller, thus facilitating molecular aggregation. As mentioned before, the potent nucleophilicity of the Hf-OH ligand is also favorable to form dimeric Hf-O-Hf species (see Scheme 1). In our recent work,23 the EUV pattern of Hf6O4(OH)4(s-BuCO2)12 cluster 1 was resolved to HP = 25 nm, with a dose J = 139 mJ cm−2 (see Scheme 2). As a comparison, its doubly hydroxylated cluster Hf6O4(OH)6(s-BuCO2)102 has an EUV pattern resolving to HP = 17 nm, but the dose is still very high (J = 163 mJ cm−2).23 The resolution improvement is attributed to a non-radical chain process, but a high EUV dose for cluster 2 is beyond our photoresist design. We believe that the size of cluster 2 is not sufficiently small. This work reports the synthesis of highly hydroxylated Hf6O4(OH)8(s-BuCO2)8 cluster 3; importantly, the cluster is accessible to a resolution pattern with HP = 18 nm with a small EUV dose (J = 30 mJ cm−2). The energy-saving mechanism has been elucidated to involve two EUV-activated aggregations, including (i) a Hf-OH dehydration and (ii) a photolytic decarboxylation. Apart from EUV performance, this new material can be resolved into HP = 20 nm using an e-beam as the energy source. Unlike common negative-tone EUV photoresists, cluster 3 has a small loss (ca. 13%) of film thickness for EUV lithography after pattern development.24
To ensure that cluster 3 has the same frameworks as clusters 1 and 2, their IR absorption bands in a KBr pellet are depicted in Fig. 2. Notably, clusters 2 and 3 have nearly the same IR absorption characters throughout the whole absorption region. Notably, the strong ν(CO) band at 1709 cm−1 is due to three carboxylic acids embedded in cluster 1 whereas this band is weak for clusters 2 and 3, probably due to a small hydrolysis of an s-BuCO2Hf ligand in the KBr pellet. The sharp band at 3682 cm−1 of clusters 1–3 is assignable to the ν(OH) stretching mode of Hf3(OH).25,26 But a new ν(OH) band at 3532 cm−1 appears only for clusters 2 and 3, which can be assignable to Hf2(OH); this assignment is acceptable because its associated ν(Hf–O) stretching peak appears at 796 cm−1. The resemblance in their IR absorption characters suggests that all three clusters may have the same frameworks. We also made a comparison of the 1H NMR spectra of three clusters 1–3, and again the close resemblance in the NMR patterns and chemical shifts (see Fig. S7†) indicates the same structural frameworks for all clusters.
Thin films of cluster 3 have been characterized with an optical microscope (OM) and atomic force microscope (AFM); the images are provided in Fig. 3. The films were prepared at 2.0 wt% in 4-methyl-2-pentanol before spin coating at a speed of 1500 rpm for 10 s and 2000 rpm for 25 s. PAB (post apply bake) was performed at 80 °C and 90 °C for 60 s before cooling to RT for 24 h. Cluster 3 shows no visible defects over a 500 μm × 600 μm domain, as shown by OM images. With a 24 nm thickness, cluster 3 is very smooth in the film surface with roughness ca. 0.64 nm and 0.68 nm at PAB at 80 °C and 90 °C respectively.
E-beam studies were used as tools to estimate the photosensitivity of cluster 3; cluster 2 was used as a reference. Fig. 4 (left) shows the e-beam contrast curves, which show the remaining fraction of the exposed resist, after treatment with a developer after exposure. The curves were obtained as a function of e-beam doses. These contrast curves indicate typical patterns for negative-tone photoresists. For cluster 2, the curve reaches a maximum at 720 μC cm−2, but small e-beam doses of ca. 400 μC cm−2 are observed for the new cluster 3. The superior sensitivity of species 3, as reflected by the slope, is due to its increasing hydroxide content. One advantage of cluster 3 is a shrinkage in film thickness, notably at a 40% level, relative to its initial height (30.2 nm). The loss of thin film thickness for its reference cluster 2 is up to 67%. With these inspiring low energy doses, the e-beam lithographic patterns are expected to be satisfactory for cluster 3 (vide infra).
Fig. 4 E-beam contrast curves: left figure: 2.5 wt%, initial height 30.2 and 32 nm for clusters 3 and 2 respectively. Right figure: 2.5 wt% initial thickness 30.2 nm, PAB 80 °C, 60–180 s. |
The effects of PAB on e-beam contrast curves are studied; the results are shown in Fig. 4 (right). A thick film (32 nm) was prepared using a 2.5% solution in 4-methyl-2-pentanol. This film was baked at 80 °C for 60 s, 120 s and 180 s before being stored under nitrogen. The respective maxima at three conditions are found at 450 μC cm−2, 450 μC cm−2 and 400 μC cm−2 for the intervals at 60 s, 120 s and 180 s. The photosensitivity, as reflected by the three slopes, is in the order: 60 s > 120 s = 180 s. We postulate that a prolonged PAB (t = 180 s) induces a Hf-OH dehydration in addition to a partial removal of carboxylic acid (s-BuCO2H) from an s-BuCO2Hf ligand; the latter is indicated by IR spectra (see Fig. 2). These actions likely save E-beam energy at a long PAB interval because some molecular aggregations can occur before e-beam exposure. We initially conducted a trial of e-beam lithography using an extended PAB treatment. However, the results showed poor contrast in the lithography. After the standard pattern development, we measured the thickness of the unexposed film, which was approximately 4 nm in thickness. It is believed that the extended PAB treatment reduced the film's solubility to the developer, and this hypothesis also accounts for the reduced thickness of films baked for 120 and 180 seconds (as illustrated in Fig. 4, left).
The e-beam lithographic patterns of cluster 3 were developed with a 24.5 nm thickness using the developer (hexane/2-heptanone = 1/1, 60 s). PAB at 80 °C (60 s) was selected because the film baked for 180 s remains 3–4 nm in thickness after the pattern development. Fig. 5 shows the SEM images of the e-beam patterns of cluster 3 with small HP = 19–20 nm under small e-beam doses (800 μC cm−2); no PEB (post exposure baking) occurs here. A drastic improvement is noted for cluster 3, as compared to the reference cluster 2, which only reaches an HP = 30 nm pattern with a high dose of 1760 μC cm−2. We believe that a small loss of film thickness might be critical to achieve a high resolution pattern. Cluster 2 is only accessible to an HP = 31 nm pattern due to a 67% loss of film thickness. In Fig. 5, the L/S values (L = line; S = space) are estimated to be within 0.72–0.75 for the HP = 50–30 nm e-beam patterns, but increase to L/S = 1.08, due to photoresist blurring in small domains.
Fig. 5 SEM images of e-beam lithographic patterns for cluster 3 at different doses and half-pitches; the design is L/S = 1:1, developer: hexane/2-heptanone 1:1, 60 s. Initial film thickness 24.5 nm. |
Additional e-beam patterns are presented in Fig. 6, along with a PEB (post-exposure baking) treatment (80 °C, 60 s). It is worth noting that the additional PEB procedure does not result in energy savings, as comparable doses of approximately 800 μC cm−2 are still required for pattern development. Within the various e-beam patterns, with HP ranging from 28 to 50 nm, the corresponding L/S values were calculated to be in the range of 0.77 to 0.86 nm. However, the value is quickly increased to L/S = 1.1 for the smaller HP = 21 pattern. These L/S values are slightly larger than those observed without PEB, possibly due to a lower degree of Hf-OH dehydration. The patterns depicted in Fig. 5 and 6 exhibit characteristics of photolytic decarboxylation, where the smaller HP (HP = 21 nm) results in photoresist blurring with a larger L/S value of 1.1. In our forthcoming EUV study, this PEB treatment significantly impacts the EUV energy doses. Additional SEM images of e-beam patterns at different half-pitches under various e-beam doses can be found in the ESI (refer to Fig. S1 and S2).†
Our ultimate goal is to create high-resolution EUV patterns using small energy doses. The EUV exposure experiments were conducted at the Swiss Paul Scherrer Institute EUV Center (PSI) using EUV light at 13.5 nm. When working with a film thickness of 24.5 nm, the exposure contrast curve demonstrates an increase with the rise in EUV doses, starting at 18.5 mJ cm−2 and rapidly reaching its peak at 20.8 nm at a dose of 44.5 mJ cm−2, as illustrated in Fig. 7. We are pleased to state that this critical energy requirement is significantly lower than that of the reference sample 2, which stands at 75 mJ cm−2. In comparison to the initial height of 24.5 nm, we observed only a 13% reduction in film thickness. Consequently, it can be inferred that cluster 3 is more photosensitive than its reference cluster 2 in both EUV and e-beam energy doses.
We conducted the development of high-resolution patterns using PEB at different time intervals (30 and 60 s at 80 °C). The developer was a mixture of hexane and 2-heptanone in a 1:1 ratio, with a 60 second cleaning step. SEM images of EUV patterns under two different PEB durations (60 and 30 s) are presented in Fig. 8 and 9. PEB plays a crucial role in reducing EUV doses as it facilitates molecular aggregation in negative-tone photoresists due to thermal activation. A notable example is the tin cluster (BuSn)12O15(OH)6X2 (ref. 19–22) (X = Cl, OH, and carboxylate), where PEB aids in the dehydration of their six Sn-OH groups, resulting in the formation of three Sn–O–Sn units. Cluster 3 possesses eight Hf-OH groups, making us opt for an extended PEB interval (80 °C, 60 s) to achieve a reduction in EUV energy doses.
Fig. 8 SEM images of EUV lithographic patterns: THK = 24.5 nm, PAB (80 °C, 60 s, THK = 24.5 nm); developer: hexane/heptanone 1:1, 60 s. |
EUV exposure was carried out using an interference mask featuring dense line/space patterns with half pitches ranging from 17 to 50 nm. In the case of our new cluster 3 with a 60 second PEB interval, a pattern begins to form at a low energy level of J = 10 mJ cm−2. However, a well-defined pattern is achieved more effectively with doses in the range of J = 27–30 mJ cm−2. Fig. 7 illustrates a series of SEM images, showcasing resolutions for HP values of 35, 25, 22, and 18 nm. Additional SEM images at different EUV doses can be found in the ESI (Fig. S3).† The EUV patterns in Fig. 7 exhibit significant top loss due to the relatively high threshold energy in the EUV contrast curve, approximately 44.5 mJ cm−2. This top loss is because the exposed photoresist is not fully mature and remains partially soluble in the developer. An interesting observation is the line/space parameters (L/S), which measure 4.2, 3.1, 2.8, and 2.5 for the HP values of 35, 25, 22, and 18 nm patterns, respectively. This trend is typical for most EUV photoresists which tend to exhibit increasing L/S values with smaller HP patterns, primarily due to the occurrence of photoresist blurring at smaller domains.
EUV exposure was also conducted using a brief PEB interval (80 °C, 30 s), which necessitated high EUV doses of 90–110 mJ cm−2. The practice of employing an extended PEB interval to lower EUV doses is well established, and is primarily attributed to the dehydration of two M–OH groups. Scumming of the photoresist was observed in the case of smaller HP values, such as 22 and 18 nm, and this phenomenon was partially influenced by the solvent developer. To mitigate this scumming issue, additional EUV exposure, a change in the solvent developer, or a reduction in film thickness can be considered. Further analysis of L/S values yielded the following results: L/S = 1.0, 1.3, 1.4, and 1.9, respectively, for HP values of 35, 25, 22, and 18 nm. This L/S trend aligns with the typical behavior of EUV photoresists. The use of a short PEB interval increases energy doses due to the relatively limited degree of molecular aggregation within this brief PEB period. Additional SEM images taken under this PEB interval (80 °C, 30 s) can be found in the ESI (Fig. S4).†
Cross-section analysis with TEM images was performed on an HP = 25 nm pattern as shown previously in Fig. 9 (top right). The initial height of this photoresist is estimated at 24.5 nm, which is nearly the same as the thickness (24–25 nm) in this TEM image after lithographic development (see Fig. 10). Negative tone photoresists typically suffer significant shrinkage in the PEB process,24 but we observed nearly no loss of film thickness in this brief PEB interval (80 °C, 30 s) during the development.
High resolution X-ray photoelectron spectroscopy (HRXPS) of the thin film of cluster 3 (THK = 32 nm) was performed at different EUV doses (J = 0, 37, 61 and 123 mJ cm−2). The PAB was conducted at 80 °C (60 s) before EUV exposure. These HRXPS experiments were performed without PEB so that only photo-aggregation is mainly involved. This HRXPS study is to examine the composition change of elements involving hafnium, carbon and oxygen under different EUV doses. As shown in Fig. 11, a decrease in oxygen and carbon contents is observed with increasing EUV doses; a loss of carbon content indicates a photolytic decarboxylation. Nevertheless, the loss of oxygen content is relatively small as compared to carbon content throughout all different EUV doses. In the case of J = 37 mJ cm−2, a loss of 8.3 carbon atoms corresponds to a decomposition of 1.7 molecules of s-BuCO2Hf. The oxygen loss should be around 3.4 atoms for a typical RCO2 → R˙ + CO2, which is actually larger than our observed 2.4 oxygen atoms. This outcome is indicative of a prior photolytic decarboxylation, followed by H2O/O2 exposure before forming species A or B (eqn (1) and (2), Scheme 3). Species A or B are expected to lose only one oxygen for the photolytic decomposition of one s-BuCO2Hf group. Upon EUV-induced decarboxylation, the resulting intermediates Int-1 have two empty sites to further react with μ3-oxide atoms to yield species Int-2, ultimately yielding species A after exposure to air. Alternatively, intermediate Int-1 can undergo a redox reaction with Hf2OH, forming an aggregation intermediate Int-3, finally affording species B after air exposure. Loss of extra oxygen atoms at EUV light J = 37 is probably attributed to a Hf-OH dehydration as depicted in eqn (3). A combined action of a Hf-OH dehydration with two decarboxylations in eqn (1) and (2) well rationalizes our HRXPS studies.
HRXPS is also used to estimate the mass loss at J = 37 mJ cm2; a loss of 8.2 carbon atoms and 2.4 oxygen atoms is observed in Fig. 11. Such a mass loss corresponds to a total loss of 138 g mol−1 for cluster 3 that has a molecular weight of 1381.6 g mol−1. A 10% weight loss is obtained at J = 37 mJ cm−2. In the EUV contrast curve, we observed a loss of height of ca. 13% for the exposed thin film at the threshold energy J = 44.5 mJ cm−2.
Detailed XPS simulations were conducted on the C(1s) and O(1s) absorption peaks to characterize the mechanism. Simulation spectra are shown in Fig. 12 together with their quantitative analysis. Two components were found for the observed C(1s) peaks, including the sp3 C–C carbons and CO2 components centered at 284 and 289 eV respectively. Their relative ratios show little change at different EUV doses J = 37 → 123 mJ cm−2, showing a clean decarboxylation process, as in eqn (1) and (2). In the O(1s) peak analysis, the component centered at 530 eV is assignable to inorganic Hf–O species including Hf2OH, Hf2O and Hf3O; the second component centered at 532 eV is assignable to the s-BuCO2Hf oxygen. At J = 37 mJ cm−2, the inorganic (Hf–O) band gains intensity to 73% while the s-BuCO2Hf oxygen intensity is decreased to 27%. These data well fit our model in eqn (1) and (2) that s-BuCO2Hf was photo-decomposed to inorganic Hf–O species A or B. Notably, with increased J = 37 → 123 mJ cm−2, the inorganic Hf–O component starts to lose intensity while the Hf2(O2C–sBu) band gains intensity. We postulate that a Hf-OH dehydration, as depicted in eqn (3), is still occurring at high EUV doses. Our photolytic decarboxylation model together with a Hf-OH dehydration, as depicted in eqn (1)–(3), well fit these HRXPS simulation spectra.
FTIR in ATR (attenuated total reflectance) mode was used as a tool to study surface composition under EUV light. A film was prepared with 2.5 μm thickness before a PAB process (80 °C, 60 s). After EUV exposures at 0, 37, 61 and 86 mJ cm−2, we were unable to locate the EUV exposure area with our vision. Accordingly, the films were developed with the same developer (2-heptanone/hexane) for 10 s to show the EUV exposure area. The films were dried at 80 °C for 60 s to remove solvent residues. In the unexposed film, there is a small peak of free RCO2H with ν(CO) 1709 cm−1, but this band is not observed with EUV exposure. Before the PAB baking, water residue is embedded with cluster 3, and hydrolysis of Hf2(s-BuCO2) might occur at the baking temperature (80 °C). The IR absorption bands at J = 37–86 mJ cm−2 were scaled up by 6 fold to show the clarity; some bands at 1000–1100 cm−1 are partly due to SiO2 absorption as the film surface is partly cracked. In Fig. 13, the spectra of unexposed film 3 have large ν(OH) absorptions in the 3333–3600 cm−1 range. With a 37 mJ cm−2 dose, this ν(OH) band greatly decreases in intensity whereas ν(C–H) and ν(CO2) bands at 2800–3000 cm−1 and 1600–1450 cm−1 are still strong. A Hf-OH dehydration is evident here. With increasing EUV doses, the ν(C–H) and ν(s-BuCO2Hf) bands decrease in intensity at the same pace. Notably, the inorganic ν(Hf–O) band at 798 cm−1 is relatively strong in IR absorption as compared to ν(C–H) and ν(s-BuCO2Hf) bands. Accordingly, the model in eqn (1) and (2) well rationalizes these data that a photolytic decomposition of one s-BuCO2Hf unit forms one inorganic Hf–O unit. The involvement of photolytic decarboxylation (eqn (1) and (2)) as well as a Hf-OH dehydration (eqn (3)) is again manifested by these FTIR spectra.
Fig. 13 FTIR spectra at different EUV doses; the intensities at J = 37–86 mJ cm−2 were enlarged by 6 fold to show clarity. |
The Hf-OH dehydration in cluster 3 was also examined by FTIR spectra over various PAB intervals. Samples were baked at 80 °C for 60, 120 and 180 s before being moved into nitrogen-filled glassware for cooling. Their KBr pellets were prepared under air as dehydration is shown to be irreversible (vide infra); FTIR spectra were recorded in air without special precaution. Fig. 14 shows three spectra at different intervals. None of the absorption bands including ν(C–H) and ν(OC–O) show any noticeable change in the 3100–500 nm region. An inorganic ν(Hf–O) band at 796 nm−1 remains unchanged in IR intensity at t = 60, 120 and 180 s. But a loss of ν(O–H) intensities at ca. 16% and 24% is evident for t = 60 s and 180 s respectively. Also in Fig. 14 is a very small peak of free s-BuCO2H for all spectra; its formation arises from a slight hydrolysis of the s-BuCO2Hf ligand to form its acid form at the PAB stage. Notably, the ν(O–H) band at 180 s shows little change after exposure to air for 24 h. The film of cluster 3 baked at 80 °C (60 s) can be cleaned completely with 2-heptanone/hexane (60 s, 1:1) but the film baked for 180 s remains 3–4 nm in thickness. This fact is indicative of the irreversible nature of this Hf-OH dehydration.
Mechanistic studies with FTIR and HRXPS studies support two main aggregations as depicted in Scheme 3. First, the Hf-OH dehydration in cluster 3 can be carried out either by thermal or by EUV irradiation. A second process is a photolytic decarboxylation that only occurs with EUV light. In the HRXPS study, we observed a relatively small loss of oxygen that can be rationalized by a combined action of photolytic decarboxylation with a Hf-OH dehydration. Simulation of the C(1s) spectra indicates a clean decomposition of the s-BuCO2Hf ligand. A further analysis of the O(1s) region at J = 37 mJ cm−2 shows the formation of a new inorganic Hf–O unit at the cost of a Hf–O2C(s-Bu) unit. Further EUV irradiation (J = 37–123 mJ cm−2) is compatible with a Hf-OH dehydration. All these results well rationalize our reaction mechanism in Scheme 2. In this work, carbon radicals are generated, but such radicals are not involved in molecular aggregations as for radical acceptor ligands. Photolytic decarboxylation reactions just create two coordination vacant sites around two hafnium centers Int-1 to facilitate aggregation processes.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d3na00508a |
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