Open Access Article
E. M. Hayden
,
T. J. Hager
,
R. Mata
,
Q. B. Borengasser and
B. M. Broderick
*
Department of Chemistry, University of Missouri, Columbia, Missouri 65203, USA. E-mail: broderickbm@missouri.edu
First published on 6th March 2026
Complex molecules formed in astrophysical ices may exist as different conformers, yet conformer-specific desorption under interstellar medium-relevant conditions remains poorly constrained. This in turn may give rise to uncertainties that impact inferred column densities for these species. Nitrogen-bearing species are particularly advantageous targets to study these issues owing to their large dipole moments, and n-propyl cyanide (n-PrCN), the smallest cyanide exhibiting rotational isomerism, serves as a benchmark system for investigating conformer-dependent ice-gas phase evolution. Here, we report the first measurement of the conformer interconversion barrier of n-propyl cyanide in the condensed phase (2044.9 ± 289 K) obtained using in situ reflection–absorption infrared spectroscopy (RAIRS). Mixed n-PrCN:H2O ices were also examined, yielding a significantly higher interconversion barrier for an 80
:
20 composition. In addition to in situ characterization of the ice, gas-phase detection of products is achieved with chirped-pulse mm-wave detection of molecules during temperature-programmed desorption, where neat n-PrCN ice produces a gauche fraction of 0.80 ± 0.03 in the gas phase. Conformer populations are tracked throughout ice warm-up and phase transitions. Finally, we find that crystallization of n-PrCN in mixed ices is suppressed until the onset of water ice crystallization, demonstrating that ice composition and morphology regulate desorption with conformer-specificity.
N functional group, are widely employed as spectroscopic probes of molecular structure, dynamics, and kinetics owing to their large permanent dipole moments and strong coupling to electromagnetic radiation. Perturbations to the electron density of the nitrile bond are readily interrogated using vibrational spectroscopic techniques, such as Fourier-transform infrared (FTIR) spectroscopy in the mid-infrared region. In particular, the fundamental CN-stretching mode is highly sensitive to its local environment in the condensed phase, where frequency shifts arise from vibrational Stark effects and specific intermolecular interactions.1,2 The magnitude and direction of these shifts provide direct insight into the electrostatic fields and noncovalent forces experienced by the molecule.
An astrochemically relevant environment in which such effects are pronounced is the entrapment of nitriles within hydrogen-bonded water ice networks. Previous experimental and theoretical studies have examined the influence of water on the CN stretching vibration for HCN and CH3CN ices.3,4 However, these investigations have largely been restricted to short chain cyanides. Although longer chain nitriles are less abundant than HCN and CH3CN in the interstellar medium (ISM), several have been detected in the gas phase and are expected to be present within interstellar ices through accretion and subsequent thermal processing.
One such molecule is n-propyl cyanide (n-PrCN, C3H7CN), which has been detected toward the Sagittarius B2 (Sgr B2) molecular cloud alongside its structural isomer i-propyl cyanide (i-PrCN).5,6 n-PrCN exists as two low-energy rotational conformers, gauche and anti, differing in orientation of the –CN group relative to the CCC backbone. Each conformer possesses distinct vibrational signatures within the 650–4000 cm−1 spectral window, enabling simultaneous monitoring of conformer-specific vibrational modes, as well as the CN-stretch. This allows for in situ tracking of conformer populations as a function of ice temperature and composition during temperature programmed desorption (TPD).
In the solid state, n-PrCN exhibits several properties that are not observed in shorter-chain cyanides, arising from the combined effects of molecular flexibility and electronic interactions involving the nitrile group.7,8 Most notably, condensed n-PrCN can form a molecular glass prior to crystallization. This kinetically trapped amorphous phase is characterized by enhanced molecular mobility and viscosity changes, leading to a metastable disordered structure that may be accessed from cooling from the liquid or by warming a vapor-deposited sample. Glass formation and subsequent crystallization have been extensively studied in materials and medicinal chemistry, particularly for aromatic and flexible molecular systems.9–11 Upon further annealing, n-PrCN undergoes a final transition to a thermodynamically stable crystalline phase, which consists exclusively of the gauche conformer when formed from vapor-deposited ice.12 The way in which water modifies these phase transitions and the resulting conformer distributions remains incompletely explored, despite its relevance to interstellar ice evolution.
At higher temperatures, crystalline n-PrCN ultimately desorbs into the gas phase, a process central to astrochemical models of ice sublimation in protostellar environments. Recent observations with the James Webb Space Telescope (JWST) have enabled the first tentative identification of CH3CN and CH3CH2CN in interstellar ices via their strong mid-IR CN stretch vibration.13 These observations allow for a direct comparison of ice-phase and gas-phase abundances of nitriles. However, a key question is whether sublimation preserves or modifies the conformer populations established in the condensed phase.
In SgrB2(N), an [i-PrCN]/[n-PrCN] ratio of 0.4 ± 0.06 has been derived from gas-phase observations.6 While a conformer-specific detection of gauche n-PrCN has not yet been unambiguously established, Belloche et al. (2009) reported a tentative feature, albeit with baseline uncertainty and spectral blending. Assuming this feature represents a gauche detection, and accounting for uncertainty of the energy differences between gauche and anti conformers, the inferred anti to gauche ratio ranges from 0.51
:
0.49 (ΔE = 92 cm−1) to 0.57
:
0.43 (ΔE = 117 cm−1) at 150 K in Sgr B2(N).5 These values highlight the sensitivity of the observed conformer ratios to both energetic parameters and thermal history.
In the condensed phase, water has been shown to alter isomerization barriers for a variety of molecular systems by modifying local potential energy landscapes.14,15 However, experimental constraints on conformational isomerization involving the rotation of heavy (larger than hydrogen) molecular groups under astrochemical ice conditions remain scarce. To our knowledge, only a single study has directly examined this process. Hudson and Coleman investigated the temperature-dependent solid-state isomerization of cyclopropanecarboxaldehyde (C4H6O) in pure and water-rich amorphous ices.16 They observed conformer relaxation toward the thermodynamically favored trans form upon warming from 14 K to 85 K, with complete conversion following crystallization. In mixed water ices, conformer ratios remained temperature dependent, though quantitative analysis was hindered by spectral overlap. Related behavior has been observed for 1,2-dichloroethane, where warming the solid led to an increase in the less stable gauche conformer, indicating that conformer populations in ices are governed by a complex interplay of kinetic, structural, and intermolecular effects rather than simple thermodynamic equilibration.17
In this work, we employ chirped-pulse mm-wave rotational spectroscopy (CP-mmW) in combination with reflection–absorption infrared spectroscopy (RAIRS) to investigate the influence of water on the gauche
:
anti conformer ratio of n-PrCN in both the condensed phase and the gas phase following thermal desorption. We apply our instrument CPICE (Chirped-Pulse Ice), which couples CP-mmW spectroscopy with buffer gas cooling, to obtain conformer-specific sublimation profiles during temperature programmed desorption. This is an extension of our previous study of pure n-PrCN ice to include water-rich ices enabling direct assessment of matrix effects on conformer-resolved binding energies.18 The RAIRS spectra are used to track the n-PrCN conformer distribution during ice warmup. The changes in the frequency and intensity of the vibrational bands measured provides insight to the intermolecular forces the molecules experience during the various phase transitions. The temperature at which the anti conformer is depleted and the gauche conformer grows is used to quantify the condensed-phase isomerization barrier, the first measurement of this value for n-PrCN. Finally, the influence of water on the observed conformer ratio and its temperature dependence is investigated.
For the mixed ice experiments, 18 MΩ resistivity water was deposited through a second deposition arm following three FPT cycles. Laser interferometry was used to monitor the thickness, while the ratio of the molecular components was monitored with a mass spectrometer throughout deposition to ensure the desired ratio remained constant. The column density of n-PrCN was held constant at approximately 3.97 × 1018 molecule cm−2. The water was adjusted to match the column density of n-PrCN to achieve the different ratios used through the experiment. This leads to different ice thicknesses for each ice ratio: 5.7, 6, 7, 9, and 17 microns for pure, 80
:
20, 50
:
50, 25
:
75, and 10
:
90 respectively.
Quantitative determination of infrared band strengths in RAIRS is complicated by the combined effects of ice composition and temperature, both of which can substantially alter intrinsic (neat-ice) band strengths reported in the literature.21,22 In water-rich ices, these effects are further complicated by optical interference inherent to the reflection–absorption geometry. Specifically, interference between photons reflected from the substrate and from the ice-reflected photons causes RAIRS peak areas to deviate from the linear column-density dependence expected under Beer–Lambert behavior.23 These deviations are instrument-specific and depend sensitively on experimental parameters such as the grazing angle of the incident infrared beam.
RAIRS calibration experiments performed in CPICE demonstrate that departures from linearity of peak areas follow a cyclic pattern of constructive and destructive interference as a function of ice thickness. When a sufficiently broad range of ice thicknesses are sampled, a line-of-best-fit can be extracted that yields band strengths comparable to those obtained from transmission FTIR measurements, thereby avoiding bias toward any single phase of the interference cycle. We further observe that RAIRS interference effects are strongly frequency dependent, such that spectral features at widely separated frequencies exhibit distinct interference patterns. As a result, accurate comparison of bands separated by large frequency intervals would require frequency-specific corrections to the measured peak areas as a function of ice thickness.
In the present study, the vibrational bands selected for analysis are closely spaced in frequency and free from spectral overlap, minimizing RAIRS interference effects. Under these conditions, relative band areas can be compared reliably without the application of additional frequency-dependent corrections. Peak areas were measured using the Thermo Scientific OMNIC 9 program.
The transitions associated with each conformer were averaged to determine the overall gauche and anti relative abundances, N. Several corrections were applied in calculating these abundances as shown in eqn (1), including chirp corrected intensity I, conformer-specific partition functions Qi, lower and upper state rotational energy contributions
and
, transition-specific signal line strength factors, Sµ2, as governed by the experimentally measured rotational temperature of the desorbed molecules, as well as the lower state degeneracy g1.
![]() | (1) |
A complete listing of all rotational transitions, their intensities at 18 K as reported in CDMS, and the corresponding line strength factors are provided in Table S2.24 Further experimental details are described in greater depth in Borengasser et al.25
An important advantage of n-PrCN is the presence of clearly resolved infrared bands associated with individual conformers in the condensed phase. While a complete list of the condensed-phase spectrum is given in the Supplementary Information, Table S1, the bands of interest selected to understand the role of water in conformer composition within the ice are the 1260 cm−1 gauche band and the 1277 cm−1 anti band, both of which correspond to the –CH2 twist in each species and which are spectrally distinct throughout the thermal evolution of the ice.12 The integrated areas between 1270–1247 cm−1 and 1287–1270 cm−1, respectively, were used to obtain the gauche
:
anti (g
:
a) ratio in all experiments.
Absolute conformer populations cannot be extracted without reliable conformer-specific band strengths, which are not available for n-PrCN under varying water concentrations and ice morphologies. Moreover, both ice temperature and matrix composition are known to modify intrinsic band strengths, while the reflection–absorption geometry introduces additional optical interference effects. As a result, all conformer ratios reported here are expressed relative to the 10 K n-PrCN reference spectrum, for which the g
:
a ratio is assumed to reflect the gas-phase equilibrium value (3
:
1) frozen in upon deposition at low substrate temperature, consistent with previous studies.16,17 This approach enables accurate determination of the relative changes in conformer populations in the absence of absolute column densities.
Upon warming from 5 K to ∼100 K, both conformer bands sharpen and increase in integrated intensity without a measurable change in their relative ratio (Fig. 2). This behavior indicates structural reorganization within the ice without conformer relaxation. Similar spectral sharpening has been previously associated with the formation of a metastable glassy state in flexible molecular solids, where increased mobility allows local rearrangements while long-range order remains absent.26 Under our experimental conditions, this glass transition (Tg) occurs at 103–104 K (Fig. 3), slightly higher than the 97 K reported previously for n-PrCN under different deposition conditions,7,27 consistent with the known sensitivity of glass formation to thermal history.7
Despite changes in band shapes and absolute intensities upon entering the glassy state, the g
:
a ratio remains consistent across all heating rates examined. This indicates that conformational interconversion is inhibited within both the amorphous and glassy states.
Although the onset temperature of the glassy state is independent of heating rate, the temperature window within which this state persists prior to crystallization does depend on the ramping rate. At the slowest heating rate (0.2 K min−1), the glassy state spans 15 K, whereas at the fastest heating rate (5 K min−1), it extends over ∼26 K. This rate dependence suggests that crystallization and conformer interconversion are kinetically coupled processes that require sufficient time for large-scale molecular rearrangement.
The absence of conformer relaxation prior to crystallization for n-PrCN ices is in contrast to the previously observed behavior by Ishii et al. for 1,2-dicholoroethane (DCE), where the higher-energy gauche conformer increases in abundance upon warming before crystallization.17 In DCE, electrostatic interactions stabilize the polar gauche conformer in the condensed phase, lowering the effective rotational barrier relative to n-PrCN. The lack of analogous behavior here indicates that the barrier to C–C bond rotation in n-PrCN is higher than the barrier associated with chloromethyl group rotation in DCE, precluding conformer equilibration prior to crystallization.
![]() | (2) |
We note that the crystallization and isomerization processes are intertwined kinetically, as both processes are measured using the changes in the peak areas of the conformers. As a result, the experimentally derived activation energy is that of a multi-step process and the value obtained from this simplified kinetic analysis serves as an upper bound on the true energy barrier for conformer isomerization. Nevertheless, this measurement provides the first experimental constraint on conformational dynamics of n-PrCN in the condensed phase.
For comparison, gas-phase calculations yield an anti → gauche barrier height of 1736.4 K at the CCSD(T)-F12 level of theory.30 The modest increase observed in the condensed phase is consistent with previous studies demonstrating higher rotational barriers to interconversion in condensed environments due to intermolecular interactions and restricted molecular mobility. Analogous behavior has been reported for amide bond rotation, where barriers increase from gas phase to neat liquids and further in hydrogen-bonded solutions.31,32
:
20 mixture, where the amorphous-to-glassy transition occurs without any measurable change in conformer ratio, as was observed in the neat ice. However, the crystallization behavior is notably different in the presence of water.
Plots showing integration of these RAIRS peaks for neat and 80
:
20 ices are shown in Fig. 6. For the 80
:
20 mixture, only the slowest heating rate (0.2 K min−1) results in complete conversion to the gauche conformer, i.e. crystallization. At faster rates (1 and 1.5 K min−1), crystallization remains incomplete and the anti conformer is present up to the point of desorption. This suggests that water significantly increases the timescale required for both structural ordering and conformer interconversion. Application of the Kissinger analysis to the slow-rate data yields an effective barrier height of ∼7800 K for the mixed ice. Although this value may not directly reflect the barrier in this case, its magnitude suggests that hydrogen-bonding interactions with water strongly hinder intramolecular relaxation. The delayed onset of n-PrCN crystallization relative to the neat ice further indicates that n-PrCN ordering is coupled to water crystallization, consistent with previous observations of molecular segregation in mixed astrophysical ices.21
![]() | ||
| Fig. 6 Peak area of the gauche and anti conformer CH2 twist mode measured over temperature for the 0.2 K min−1 ramping rate of the pure (green) and mixed ices (blue). | ||
![]() | ||
Fig. 7 RAIRS FTIR of the water-perturbed CN st. frequency (2260 cm−1) and pure CN st. frequency (2247 cm−1) region during ice warmup. (A: pure, B: 80 : 20, C: 50 : 50, D: 25 : 75, E: 10 : 90). | ||
To understand the frequency shifts observed in this work, Gaussian calculations were performed at the B3LYP/aug-cc-pVDZ level of theory. Harmonic vibrational frequencies were computed for an isolated n-PrCN molecule and for a n-PrCN-H2O complex, in which the water –OH group is oriented toward the nitrile nitrogen. This configuration serves as a minimal model for hydrogen bonding in mixed n-PrCN-H2O ices. Comparison of the calculated CN stretching frequencies reveals a blue shift of 13 cm−1 upon complexation with water relative to the isolated molecule. This calculated shift is in agreement with the experimentally observed blue shift of 13 cm−1 (Fig. S8).
In the present study, the intensity of the water-perturbed CN stretch decreases upon warming, while the unperturbed CN stretch peak grows (Fig. 7). This is in contrast to the behavior of the CN stretch peak height within the pure ices, which decreases as the ice is warmed, likely due to temperature effects on band strength. The significant shift in our CN stretch shows a temperature dependence on the interaction between the nitrile group and the surrounding hydrogen-bond network discussed previously. The CN group appears to return to a local environment resembling that of a pure ice at elevated temperatures, where it no longer interacts strongly with the local water molecules. This behavior suggests that n-PrCN forms aggregates within the ice before subliming.
To further investigate this interpretation, quantum chemical calculations were performed at the ωB97X-D/6-311+G(d,p) level of theory to evaluate the binding energies of the H2O–n-PrCN and n-PrCN–n-PrCN dimers. Including zero-point energy corrections, the binding energy of the H2O–n-PrCN complex is 4.06 kcal mol−1, whereas the n-PrCN–n-PrCN dimer is more strongly bound, with a binding energy of 6.15 kcal mol−1. These results are consistent with our experimental observations and indicate that n-PrCN preferentially forms molecular aggregates within the ice prior to sublimation. Because the n-PrCN–n-PrCN interaction is stronger than the H2O–n-PrCN interaction, the latter is thermodynamically less stable and is disrupted first upon warming. This disruption enables n-PrCN molecules to reorganize into more strongly bound aggregates, consistent with the observed temperature-dependent evolution of the CN stretching band, which shifts from a water-perturbed position immediately after deposition toward the characteristic CN stretch of neat n-PrCN upon heating.
:
anti ratio is reflected. In all these experiments, both anti and gauche conformers are detected in the primary desorption feature. However, the RAIRS data shown for neat PrCN in Fig. 2 indicate that crystallization and complete conversion to the gauche form has already occurred. This suggests that conformational isomerization to the anti form must occur either at desorption or just prior to it. Indeed, a close look at the high temperature region of the plots in Fig. 2 and 6 shows the reappearance of the anti species just in the temperature region corresponding to sublimation. In some of the mixed ices, full crystallization may not have occurred, but it seems in any case isomerization accompanies desorption for the main TPD peak.
We note additional details in conformer-specific desorption behavior as a function of ice composition. Increasing water content systematically shifts the primary desorption peak to lower temperatures, consistent with disruption of PrCN-PrCN interactions and substitution with weaker PrCN-H2O interactions in mixed ices. In neat PrCN ice, intermolecular cohesion is dominated by dipole–dipole alignment and van der Waals packing, whereas co-deposition with water inhibits formation of compact PrCN domains through hydrogen bonding and reduced packing efficiency, thereby lowering the effective desorption energy.34–36
In addition to the slight systematic decrease in the primary desorption temperature with increasing water content, gas-phase detection during TPD reveals the emergence of a second desorption feature at the highest water contents (25
:
75 and 10
:
90 PrCN:H2O) that is absent in more PrCN-rich mixtures. This secondary feature coincides with the onset of water desorption and is attributed to co-desorption of PrCN molecules that become trapped within the bulk water matrix during deposition. Similar behavior has been reported previously for volatile species embedded in amorphous water ice where desorption is delayed until the amorphous-to-crystalline transition or bulk water sublimation occurs.37,38 In the present experiments, any potential volcano desorption of PrCN alone would be obscured by the dominant desorption of neat PrCN, suggesting that the observed high-temperature feature is most consistent with water-mediated co-desorption. Independent mass spectrometric measurements of the 10
:
90 mixture confirm that the secondary PrCN sublimation event coincides with the desorption of the bulk crystalline water ice.
Interestingly, only the gauche conformer is detected in this secondary desorption feature. This conformer selectivity indicates that n-PrCN molecules trapped within the water matrix undergo conformational relaxation prior to sublimation, resulting in enrichment of the lower-energy gauche conformer, just as in the PrCN crystallization. Similar behavior has been observed for polycyclic aromatic hydrocarbons (PAHs) embedded in bulk water ice, where molecular reorientation toward minimum-energy configurations occurs during ice crystallization and is subsequently preserved by the rigid crystalline lattice.39 In the case of PrCN, confinement within the water matrix likely facilitates partial conversion of the anti to the gauche form during the amorphous to crystalline transition. However, in contrast to the desorption from the PrCN-dominated peak, in this case there is no conformational isomerism accompanying any sublimation and only the gauche form is detected in the gas phase from the water-dominated peak.
Although these water-driven structural effects are evident in the second desorption feature, the relative conformer abundances in the first desorption feature remain largely insensitive to water content. Again, this suggests characteristic isomerization of the gauche form as the sublimation temperature is reached for the n-PrCN desorption peak. For both neat and mixed ices, only the gauche fraction is reported, as the anti conformer abundance in the second desorption feature falls below the limit of detection and precludes reliable determination of a gauche
:
anti ratio. As we reported previously for the neat n-PrCN, the gauche fraction measured in the first desorption event is greater than a 300 K Boltzmann distribution, although the effect is smaller in the present data. We attribute this difference to greatly improved S/N following incorporation of a cryogenic amplifier in our signal acquisition path. The gauche fraction in the first feature is consistent across all ice compositions investigated.
Fig. 9 and the corresponding Table 1 summarize the gauche fraction for each desorption feature along with the associated peak desorption temperatures for all mixtures studied. For neat n-PrCN, the gauche fraction in the first desorption peak is 0.79 ± 0.03, and comparable values are obtained for all mixed ices. In contrast, the second desorption features observed in the 25
:
75 and 10
:
90 n-PrCN:H2O mixtures exhibit substantially higher gauche fractions of 0.95 ± 0.07 and 0.93 ± 0.01, respectively. These elevated values indicate strong conformer selectivity in water-rich ices, with the lower-energy gauche conformer preferentially retained and released during water-mediated co-desorption. As the water fraction increases, a larger proportion of n-PrCN molecules becomes trapped within the bulk ice, where conformational relaxation prior to desorption is facilitated. In the 25
:
75 mixture, the reduced abundance of n-PrCN molecules trapped within the water matrix then leads to the absence of detectable anti conformer signal in the second desorption feature.
| Neat | 80 : 20 PrCN:Water |
50 : 50 PrCN:Water |
25 : 75 PrCN:Water |
10 : 90 PrCN:Water |
|
|---|---|---|---|---|---|
| a The second desorption temperature. | |||||
| Gauche fraction 1st peak | 0.796 ± 0.029 | 0.813 ± 0.052 | 0.779 ± 0.034 | 0.780 ± 0.002 | 0.838 ± 0.032 |
| Gauche fraction 2nd peak | — | — | — | 0.952 ± 0.067 | 0.932 ± 0.007 |
| Anti Tsub (K) | 177 | 175 | 173 | 171 | 172/193a |
| Gauche Tsub (K) | 175 | 174 | 174 | 171/188a | 173/193a |
These results demonstrate that water ice plays a dual role in mixed molecular ices. While the first desorption feature reflects conformer populations largely inherited from the neat system prior to crystallization, crystallization of the water-rich environments promote bulk trapping and conformational relaxation that selectively enrich the lower-energy conformer prior to co-desorption. Conformer-specific gas-phase detection enabled by CPICE provides direct insight into how ice composition and morphology govern the molecular populations which sublime.
Detection by mm-wave rotational spectroscopy of molecules in the gas phase reveals that the addition of water systematically lowers the primary desorption temperature of n-PrCN, consistent with disruption of PrCN-PrCN cohesive interactions by the surrounding H-bonded matrix. For neat and moderately water-dilute ices, the gauche fraction in the first desorption event remains consistent regardless of ice composition, suggesting limited conformational equilibration during sublimation, However, in water-rich mixtures (25
:
75 and 10
:
90 n-PrCN:H2O), a second desorption feature is observed coincident with crystalline bulk, in which n-PrCN sublimes with an increased abundance of the lower-energy gauche conformer. This behavior is consistent with conformational relaxation of n-PrCN molecules trapped within the water matrix prior to co-desorption.
These findings highlight the role of water and importance of condensed-phase structure and thermal history in shaping the conformational distributions ultimately accessible to gas-phase astronomical observations in cold astrophysical environments. Future work will systematically investigate the influence of deposition conditions, ice morphology, and isomeric composition to further constrain the condensed-phase mechanisms responsible for conformer-selective desorption.
Supplementary information (SI) is available. See DOI: https://doi.org/10.1039/d5cp05060j.
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