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High-resolution spectroscopy of buffer-gas-cooled phthalocyanine

Chemistry

High-resolution spectroscopy of buffer-gas-cooled phthalocyanine

Y. Miyamoto, R. Tobaru, et al.

Discover how high-resolution rovibronic spectroscopy can now be applied to larger molecules! This groundbreaking research on free-base phthalocyanine (FBPc) by Yuki Miyamoto, Reo Tobaru, Yuiki Takahashi, Ayami Hiramoto, Kana Iwakuni, Susumu Kuma, Katsunari Enomoto, and Masaaki Baba offers fascinating insights and guides future quantum chemical calculations.... show more
Introduction

High-resolution molecular spectroscopy encodes the quantum nature of molecules in their spectra, and resolving rotational structure is key for accurate structural determination. However, for large molecules the small rotational energy spacings are obscured by Doppler broadening unless samples are cooled to very low temperatures, and traditional supersonic jets struggle to introduce large molecules in sufficient quantities for high-resolution rovibronic spectroscopy. Buffer-gas cooling—thermalizing molecules via collisions with a cryogenic noble gas—has gained attention for preparing cold, slow molecules for diverse applications and as a precursor to further cooling. While rotationally resolved spectroscopy in buffer-gas cells has focused on smaller species, it remained unclear how well very large molecules can be cooled. Prior work achieved rotational resolution for C60 in the infrared near 150 K, where Doppler widths are much smaller than in the visible, but achieving rotational resolution for visible rovibronic transitions requires lower temperatures. This study targets free-base phthalocyanine (FBPc, M = 514) and asks whether buffer-gas cooling in helium at cryogenic temperatures can produce sufficiently cold, abundant gas-phase samples to resolve rotational structure in the visible S1 ← S0 0-0 band, determine the transition type, and benchmark rotational and translational temperatures, thereby informing both spectroscopy and quantum chemical modeling of large molecules.

Literature Review

Supersonic jets have long enabled low temperatures for spectroscopy, but large molecules are difficult to entrain at adequate densities for high-resolution rovibronic studies. Buffer-gas cooling, established decades ago and recently revitalized due to interest in cold molecules for precision measurements, quantum information, and ultracold chemistry, provides robust thermalization via collisions with cryogenic noble gases and is widely used as a source for further cooling and for high-resolution spectroscopy of small diatomics and small polyatomics (e.g., BaF, BaH, MgF, acetylene). For very large molecules, prior rotationally resolved work includes IR comb spectroscopy of C60 at ~150 K in Ar buffer gas; because Doppler width scales with transition frequency, visible rovibronic resolution demands substantially lower temperatures. For phthalocyanine, earlier studies reported spectra in various environments (clusters, droplets) and theory predicted rotational constants and transition types, but high-resolution visible gas-phase rotational structure at cryogenic temperatures had not been clearly demonstrated. A contemporaneous (2022) supersonic jet study revisited FBPc electronic spectroscopy and suggested predominantly a-type character, differing from the conclusions here, indicating ongoing debate and the need for further experimental and theoretical scrutiny.

Methodology

FBPc gas-phase molecules were produced by laser ablation of an FBPc tablet mounted on the wall of a cryogenic buffer-gas cell and cooled via collisions with helium atoms nearly in equilibrium with the 5 K cell. The apparatus was housed within a 40 K shield inside a room-temperature vacuum chamber. A 532 nm nanosecond-pulsed Nd:YAG laser (∼2 mJ pulse energy, ∼10 ns pulse width; Litron nano) was loosely focused onto the tablet to ablate material. The cell was cooled by a 4 K pulse tube refrigerator (0.5 W at 4 K; Sumitomo Heavy Industries) to 4.7 K and typically heated to ~5 K during ablation. Helium buffer gas, precooled to ~40 K, was introduced into the cell, thermalized with the cell, and cooled the ablated molecules; gases exited through a 5 mm diameter aperture into the vacuum vessel, where He was cryopumped by charcoal cooled to ~5 K. Absorption of a narrow-linewidth continuous-wave ring dye laser at ~660 nm (Coherent 899, dye DCM; linewidth ~1 MHz) probing the S1 ← S0 band was detected by a silicon photodetector after passing through the cell. The probe power was attenuated to ~100 µW to avoid detector saturation; half of the laser power was routed to iodine sub-Doppler spectroscopy for absolute frequency calibration. Time-resolved absorption following ablation (t=0) rose rapidly, peaking at ~1 ms and decaying over several milliseconds; spectra were recorded at t≈1 ms. To mitigate ablation-induced signal fluctuations and decay, the ablation spot was continuously moved. Spectra were simulated using PGOPHER (v10.1.182), modeling FBPc as a near-oblate top with literature/theory rotational constants and including Doppler broadening to estimate translational temperature; simulations explored rotational and translational temperatures and transition type (a- vs b-type) by comparing band shapes, Q-branch behavior, and the observed oscillatory structure. A higher-temperature experiment used neon buffer gas at a 15 K cell temperature (helium cannot be effectively cryopumped at this temperature) to assess temperature effects on band shape; spectra were compared to simulations at 20 K.

Key Findings
  • The observed S1 ← S0 0-0 band of FBPc spans ~15131.0–15132.4 cm⁻¹ and exhibits a clear oscillation-like structure with a period of ~0.003 cm⁻¹ attributable to rotational structure of a near-oblate symmetric top (consistent with theoretical rotational constants A = 0.00298 cm⁻¹, B = 0.00297 cm⁻¹).
  • Simulations reproducing the overall band envelope indicate a rotational temperature ≈5 K; conservatively, T_rot < 10 K.
  • The visibility of the oscillatory rotational structure requires a narrow Doppler width; simulations with linewidth ≈0.0011 cm⁻¹ (corresponding to ~5 K translational temperature) agree well with data, implying T_trans < 10 K.
  • Spectral shape near the Q-branch shows a deep central dip without strong peaks, strongly indicating a b-type transition dipole (parallel to molecular y-axis), contrary to prior prediction of an a-type transition.
  • A neon buffer-gas experiment at 15 K yields broader spectra without resolvable rotational structure, consistent with broader rotational populations and larger Doppler widths; simulations at 20 K reproduce this broadening. No significant transition frequency shift was observed between He and Ne buffer gases, arguing against buffer-gas atom clustering (which would cause GHz-scale shifts).
  • An additional vibrational band centered at 15258.9 cm⁻¹ was observed with intensity ~100× weaker than the 0-0 band, refining the previously reported value (15258.7 cm⁻¹) by 0.2 cm⁻¹ (~6 GHz) with improved uncertainty (≥10× better than prior pulsed-laser measurements).
  • Time dynamics: absorption rises rapidly after ablation, peaks at ~1 ms, and decays over a few ms, consistent with other buffer-gas cell ablation sources.
  • The spectra show slight differences from a recent supersonic-jet study, likely due to differing rotational distributions and absence of hot bands here; that study’s conclusion of predominantly a-type character conflicts with the present b-type assignment.
Discussion

The results demonstrate that buffer-gas cooling with helium at cryogenic temperatures can prepare large, complex molecules like FBPc in the gas phase with both rotational and translational temperatures below 10 K, enabling rotationally structured high-resolution rovibronic spectroscopy in the visible. The oscillation-like band structure and Q-branch behavior confirm a b-type transition, providing critical symmetry information for the excited electronic state and constraining quantum chemical models. The lack of measurable frequency shift when changing buffer-gas species suggests that the observed absorbers are monomers rather than clusters, which is essential for interpreting spectra and benchmarking theory. Comparison with higher-temperature (Ne, 15 K) spectra underscores the necessity of cryogenic cooling to reveal rotational structure in large molecules. These findings directly address the longstanding challenge of obtaining high-resolution rovibronic spectra for large molecules and provide precise electronic, vibrational, and rotational energy data to guide and validate first-principles calculations, where large-molecule excited-state methods and basis sets remain challenging. Discrepancies with supersonic-jet analyses highlight the importance of temperature control and detailed band-shape diagnostics (including Q-branch structure) in assigning transition types, motivating further experimental and theoretical work.

Conclusion

High-resolution rovibronic spectra of buffer-gas-cooled free-base phthalocyanine were recorded, revealing an oscillatory rotational structure in the visible S1 ← S0 0-0 band. Simulations indicate both rotational and translational temperatures below 10 K, establishing buffer-gas cooling as a viable route to cryogenic, gas-phase samples of large molecules for high-resolution spectroscopy. The transition is predominantly b-type, informing the symmetry of the excited electronic state, and an additional vibrational band was measured at 15258.9 cm⁻¹ with improved accuracy. Compared to measurements at 15 K using neon buffer gas, the cryogenic helium-cooled spectra underscore the critical role of very low temperatures in resolving rotational structure. These results provide quantitative benchmarks for quantum chemical calculations of large molecules. Future work should aim to increase sensitivity and resolution—e.g., via laser-induced fluorescence detection and Doppler-free techniques—to further resolve fine spectral features and refine molecular constants, and to combine with high-level ab initio calculations for comprehensive structural determination.

Limitations

The analysis is limited by the signal-to-noise ratio, primarily due to statistical fluctuations inherent to laser ablation; continuous ablation also causes intensity fluctuations and decay, partially mitigated by moving the ablation spot. Rotational constants and structural parameters were not fully refined and will require collaboration with high-level ab initio calculations. At 15 K (neon buffer gas), the SNR was insufficient to analyze detailed spectral structure. The current absorption-based, Doppler-limited measurements may obscure finer features that could be revealed by more sensitive or Doppler-free methods.

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