Issue 
A&A
Volume 559, November 2013



Article Number  A44  
Number of page(s)  5  
Section  Atomic, molecular, and nuclear data  
DOI  https://doi.org/10.1051/00046361/201322371  
Published online  06 November 2013 
Millimeter and submillimeterwave spectrum of methyleneaminoacetonitrile ^{⋆}
^{1} Laboratoire de Physique des Lasers, Atomes, et Molécules, UMR CNRS 8523, Université de Lille 1, 59655 Villeneuve d’Ascq Cédex, France
email: roman.motienko@univlille1.fr
^{2} École Nationale Supérieure de Chimie de Rennes, CNRS, UMR 6226, 11 allée de Beaulieu, CS 50837, 35708 Rennes Cedex 7, France
Received: 26 July 2013
Accepted: 11 September 2013
Context. Aminoacetonitrile has been detected in the interstellar medium, and the Streckertype synthesis is considered as one of its possible formation mechanisms in this medium. Methyleneaminoacetonitrile (CH_{2}NCH_{2}CN, MAAN) is one of the byproducts of the Strecker reaction and a good candidate for astrophysical detection.
Aims. The rotational spectrum of MAAN has never been studied before. To provide the basis for MAAN detection in the interstellar medium we studied its millimeter and submillimeterwave spectrum.
Methods. The rotational spectrum of MAAN was measured in the frequency range of 120–600 GHz. The spectroscopic study was supported by theoretical calculations of the molecular structure and harmonic force field.
Results. The ground and the two lowest excited vibrational states of the most stable synperiplanar conformation of MAAN were assigned and analyzed. The obtained sets of rotational constants allow us to accurately predict the transition frequencies of MAAN in the frequency range up to 900 GHz.
Key words: ISM: molecules / methods: laboratory: molecular / submillimeter: ISM / molecular data / line: identification
Full Table 2 is available at the CDS via anonymous ftp to cdsarc.ustrasbg.fr (130.79.128.5) or via http://cdsarc.ustrasbg.fr/vizbin/qcat?J/A+A/559/A44
© ESO, 2013
1. Introduction
Alphaaminonitriles are commonly prepared by a Strecker reaction starting from an aldehyde, ammonia, and hydrogen cyanide (see Fig. 1). Their acidic hydrolysis leads to the corresponding αamino acids (Kendall & McKenzie 1941). This twostep sequence has often been proposed as one of the most important reactions that occurred on primitive Earth for the synthesis of many amino acids, the building blocks of life. The quite recent observation in the interstellar medium of the simplest αaminonitrile, the aminoacetonitrile NCCH_{2}NH_{2} (Belloche et al. 2008), generated several investigations on the possibility of its formation in this medium via a Strecker reaction starting from the simplest aldehyde, the formaldehyde (Danger et al. 2011). In laboratory conditions, the aminoacetonitrile easily gives the methylene aminoacetonitrile (MAAN) in the presence of an excess of formaldehyde (Adam & Langley 1956). In a natural medium such as the interstellar medium, it is unrealistic to expect stoechiometric amounts of reagents and this compound as well as other byproducts such as hydroxyacetonitrile (in the absence of ammonia; Danger et al. 2013) or methanimine and then hexamethylenetetramine (in the absence of hydrogen cyanide; Vinogradoff et al. 2012) might be formed. Therefore, the possible role of MAAN in prebiotic chemistry on primitive Earth has been proposed as well several decades ago (Choughuley et al. 1972), but has received a mediocre response even though if it has been described as an efficient substrate in the preparation of peptides (Subbaraman et al. 1975). However, while the aminoacetonitrile decomposes in a few hours at room temperature, MAAN forms a stable trimer that can restore the monomer on heating (Dammel & Bock 1987). As for the aminoacetonitrile, the hydrolysis of MAAN gives glycine, and the trimer can be considered as a stable precursor of this compound. On the other hand, with only one atom more than aminoacetonitrile, the MAAN appears to be a serious candidate for the interstellar medium. To promote its astrophysical detection we report here our study of the rotational spectrum of MAAN in the frequency range of 120–600 GHz.
Fig. 1
Synthesis of MAAN and various other compounds formed starting from formaldehyde, ammonia, and hydrogen cyanide as a function of their abundance. 
Fig. 2
Structure and atom numbering for sp a) and ac b) conformations of MAAN. 
Rotational constants of MAAN.
2. Experiments
The commercially available trimer (1 g) was introduced in a flask connected to a vacuum line. The flask was degassed and then heated with a heat gun to 300 °C to obtain the expected vapor pressure of the monomer (yield > 90%). The microwave analysis was directly performed by analysis of the gaseous flow. Condensation of the product on a cold finger cooled at 77 K led to the oligomerization on heating before the revaporization of the MAAN. In the literature, the trimer was often used considered as the monomer. The same error is still observed for some commercially available samples. MAAN is a kinetically very unstable compound at room temperature. τ_{1/2} (5% in CDCl_{3}, 25 °C): 20 min. τ_{1/2} (5% in CD_{2}Cl_{2}, 25 °C): 2 h.The results of the nuclear magnetic resonance (NMR) spectroscopy of MAAN are given in Appendix A.
The measurements of the rotational spectrum of MAAN were performed in the frequency range of 120–180 GHz using the Lille backward wave oscillator based fastscan spectrometer (Alekseev et al. 2012), and in the frequency range of 180–600 GHz using a spectrometer based on solidstate sources (Motiyenko et al. 2010). The experiment was performed in a static mode, when the stainlesssteel absorption cell was filled with the MAAN sample at an optimum pressure of about 20 μbar. Owing to the kinetic instability of the sample, the absorption cell was refilled after 4–5 h to minimize the spectral features of various decomposition products.
3. Quantum chemical calculations
The spectroscopic work was supported by quantum chemical calculations to provide an initial basis for spectral assignments. The ab initio and density functional theory (DFT) calculations were performed by employing the Gaussian 09 suite of programs (Frisch et al. 2009). Calculations were performed using MøllerPlesset secondorder perturbation calculations (MP2; Møller & Plesset 1934), and density functional theory (DFT) calculations employing Becke’s threeparameter hybrid functional (Becke 1988) and the Lee, Yang and Parr correlation functional (B3LYP; Lee et al. 1988). The Peterson and Dunning’s (Peterson & Dunning 2002) correlationconsistent tripleζ wave function augmented with diffuse function augccpVTZ was employed in the MP2 calculations. The 6311++G(3df, 2pd) wave function augmented with diffuse functions was employed in the B3LYP calculations.
The results of the calculations have shown two stable conformations of MAAN that differ by the value of the τ(C_{4}–C_{1}–N_{5}–C_{7}) dihedral angle. The most stable synperiplanar (sp, τ = 0°) conformation is characterized by the plane of symmetry created by all heavy atoms. The anticlinal (ac, τ = 120°) conformation possesses no symmetry and is less energetically favorable. The energy difference between two conformations is 770 cm^{1} (MP2/augccpVTZ calculations). The ac conformation has two structurally equivalent minima on the potential curve that characterizes the τ dihedral angle (τ = ± 120°). According to the results of the scan of the potential energy surface determined by τ, the interconversion barrier between the sp and ac conformations is about 1100 cm^{1} (MP2/6311++G(3df, 2pd) calculations).
In addition to structural optimizations, we calculated harmonic force field parameters to provide the information on quartic centrifugal distortion constants as well as on lowfrequency vibrational modes. This information is very useful especially at the initial stage of spectral assignment in our case, which usually starts with relatively high values of the J quantum number and where centrifugal distortion corrections provide much more realistic theoretical spectra. The results of the quantum chemical calculations are given in Tables B.1–B.4.
4. Analysis and fit
Owing to the low Boltzmann factor 0.025 for the ac conformer, we did not expect to observe any of its spectral features even at room temperature. Therefore we concentrated our effort on assigning of the most stable sp conformer. It is a prolate asymmetric top (Ray’s asymmetry parameter κ = −0.81) with two nonzero dipole moment components determined from ab initio calculations, μ_{a} = 1.8 D and μ_{b} = 0.8 D.
A part of the table available at the CDS, with assigned rotational transitions of MAAN.
The assignment started from the search for, as expected, the strongest transitions with K_{a} = 0 and 1 and K_{c} = J, accompanied by much less intense transitions with the same K_{a} and K_{c}. For the sp conformer of MAAN for J = 17... 23 these transitions form easily distinguishable quartets with splittings that reduce with J increasing. Starting from J = 24 and for higher values of J, such a quartet is represented by a single line in our spectra. Six transition quartets were easily located and assigned and produced the first experimental set of rotational parameters containing B and C constants as well as the Δ_{J} centrifugal correction term. The frequency predictions calculated on the basis of the experimental rotational parameters allowed the assignment of the next series of quartets with the same selection rules and K_{a} = 1 and 2, and K_{c} = J − 1. In this way, the A rotational constants and δ_{J} and δ_{K} centrifugal distortion terms were determined. The following assignment was carried out in bootstrap manner, for which newly assigned transitions were used to improve the values of rotational parameters and to provide new more precise frequency predictions that were used for new assignments. In total, about 1500 distinct frequency lines were assigned to the ground vibrational state of MAAN. The highest values of the J and K_{a} quantum numbers for the assigned transitions of the ground state are 97 and 41. Most of the lines are atype transitions and only about 20% are btype transitions which were found to be generally much weaker than atype lines. All the assigned ground state rotational transitions of MAAN were fitted within experimental accuracy to a standard Watson Areduction Hamiltonian (Watson 1977) in I^{r} coordinate representation. The set of rotational and centrifugal distortion constants is presented in Table 1. The rms deviation of the fit has a reasonable value of 0.029 MHz, but a somewhat better result of 0.021 MHz can be obtained when the l_{K} octic centrifugal distortion constant is included in the model. However, it also leads to a high correlation between the L_{JK}, L_{KKJ}, and l_{K} parameters and to a poor conditioning of the problem. Therefore, in the final fit the l_{K} parameter was not taken into account.
Rotational and vibrational partition functions at various temperatures for the sp conformation of MAAN.
In addition to ground state lines we assigned in the observed spectra the features belonging to the lowest excited vibrational states. According to the quantum chemical calculations for the sp conformer of MAAN, there are two lowfrequency vibrational modes: ν_{21}, which corresponds to torsional motion and is characterized by the variation of the dihedral angle τ defined previously, and inplane bending vibration ν_{20}, which is characterized by variation of the angle α(C_{4}–C_{1}–N_{5}). The corresponding vibrational frequencies of the modes are 152 cm^{1} and 154 cm^{1}, and therefore one might expect a Coriolistype interaction between them. Indeed, at first we were able to assign the lines belonging only to the ν_{21} state. They were distinguishable by quartet patterns for low K_{a} values similar to the ground state lines. While the intensities of the rotational lines of the ν_{20} were expected to be the same as for ν_{21} state, we were unable to assign any similar pattern at least for low K_{a} transitions of ν_{20} state at first. The only transitions of the ν_{20} state we were able to assign were found in the highfrequency part of the spectra and corresponded to high J quantum number values. Another indicator of the interaction between two states were the anomalous values of the centrifugal distortion constants obtained for the ν_{21} state in a singlestate fit. Typically, vibrational excitation leads to relatively small variations of rotational and centrifugal distortion constants that do not exceed 100%, whereas for the ν_{21} state the Δ_{K} and δ_{K} centrifugal distortion constants differed from the ground state ones by a factor of 10 or more. All the assigned transitions of the coupled states were fitted using the following standard model: (1)where \begin{lxirformule}$H_{\mathrm{rot}}^{(20)}$\end{lxirformule} and are the standard rotational Watson Areduction Hamiltonians, ΔE is the energy difference between two coupled states, and H_{cor} is the offdiagonal Coriolis interaction term.
The equilibrium configuration of the sp conformer of MAAN is described by the C_{s} point group. Inplane bending and outofplane torsion belong to the A′ and A′′ irreducible representations of the group. In this case, Coriolis interaction is allowed along the a and b axes, and the Hamiltonian H_{cor} used in the present study is expressed as (2)where \begin{lxirformule}$G_a$\end{lxirformule} and G_{b} are the Coriolis coupling constants, and all other parameters are their respective centrifugal distortion corrections.
For the initial fit using the Hamiltonian (1), we fixed all centrifugal distortion constants in H_{rot} at values of the ground state ones. We also kept fixed the energy difference between two interacting states and let only vary the G_{a} constant. Starting from the value of the energy difference between two vibrational modes obtained from ab initio calculations (1.8 cm^{1}), we searched for the bestfitting solution by manually changing ΔE with a step of 0.003 cm^{1} and keeping it fixed in the fit. The bestfit solution was found for the value of ΔE ≃ 15 cm^{1}. The consistency of the parameters produced by the first best fit was checked by predicting and assigning new series of highly perturbed transitions of both interacting states. The following assignment did not represent any major difficulty. In total about 1000 rotational transitions of ν_{21} and ν_{20} states were assigned and fitted within the experimental accuracy. The energy difference determined ΔE = 15.1718987(40) cm^{1} is much higher than the theoretical value, but still within the error of the quantum chemical calculations.
The results of the global fit using the Hamiltonian (1) are presented in Table 1. The complete list of measured rotational transitions of the ground, ν_{20}, and ν_{21} states is presented in Table 2. Here only a part of Table 2 is shown as an example.
We also provide the partition function for MAAN given in Table 3 with Q(T)_{tot} = Q(T)_{rot}Q(T)_{vib} for different temperatures. Simple formulas for calculating Q(T)_{rot} and Q(T)_{vib} can be found elsewhere (see for example Haykal et al. 2013). The experimental rotational constants and the calculated harmonic frequencies were used.
5. Conclusions
The spectroscopic information we obtained is expected to be enough to provide the basis for astrophysical detection of MAAN. The present analysis of the ground and the two lowest excited vibrational states covers the frequency range of 150–600 GHz where the most intense transitions are expected at low temperatures. It allows obtaining accurate frequency predictions at least for transitions involving levels with J ≤ 90 and K_{a} ≤ 30 and in the frequency range up to 900 GHz. We resolved no nuclear quadrupole hyperfine structure in the present study, mostly owing to the Dopplerlimited resolution of the spectrometers. However, in the cmwave range for transitions involving low J and K_{a} values the hyperfine structure can be resolved even at Doppler resolution. For this purpose we also provide in the Table B.4 the values of elements of nuclear quadrupole coupling tensors for both nitrogen nuclei. These theoretical values in combination with accurate rotational parameters are expected to result in reliable predictions on the hyperfine splittings.
Acknowledgments
This work was supported by the Programme National “Physique et Chimie du Milieu Interstellaire” (INSUCNRS) and the Centre National d’Études Spatiales (CNES). Gregoire Danger (Université de Provence, Marseille, France) is acknowledged for helpful discussions.
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Appendix A: NMR of MAAN
Nuclear magnetic resonance (NMR) spectroscopy allows one to quickly characterize the expected compound. This technique confirms the monomeric structure of the vaporized product, mainly by the chemical shifts in ^{1}H and ^{13}C NMR of the –H_{2}C=N group, which is substantially different from those of the cyclic (–H_{2}C–N–)_{3} ring of the commercially available trimer precursor (see the section “Experiments” at the end of the first paragraph).
^{1}H NMR (CDCl_{3}, 400 MHz, 25 °C) δ 4.53 (t, 2H, Hz, CH_{2}CN); 7.42 (1H, part A of AB system, Hz, Hz, N=CHH); 7.64 (1H, B part of an AB system, Hz, Hz, N=CHH). ^{13}C NMR (CDCl_{3}, 100 MHz, 25 °C) δ 46.7 ( Hz (t), CH_{2}CN); 114.4 (s, CN), 157.0 ( Hz (d), 9 Hz (d) N=CH_{2}).
Appendix B: Results of the ab initio calculations on MAAN
The calculated MP2/augccpVTZ molecular structure (Zmatrix) of the sp conformation of MAAN.
The calculated MP2/augccpVTZ molecular structure (Zmatrix) of the ac conformation of MAAN.
MP2/augccpVTZ spectroscopic parameters of the ac conformation of MAAN.
Elements of nuclear quadrupole coupling tensors (in MHz) for the sp and ac conformations of MAAN.
All Tables
A part of the table available at the CDS, with assigned rotational transitions of MAAN.
Rotational and vibrational partition functions at various temperatures for the sp conformation of MAAN.
The calculated MP2/augccpVTZ molecular structure (Zmatrix) of the sp conformation of MAAN.
The calculated MP2/augccpVTZ molecular structure (Zmatrix) of the ac conformation of MAAN.
Elements of nuclear quadrupole coupling tensors (in MHz) for the sp and ac conformations of MAAN.
All Figures
Fig. 1
Synthesis of MAAN and various other compounds formed starting from formaldehyde, ammonia, and hydrogen cyanide as a function of their abundance. 

In the text 
Fig. 2
Structure and atom numbering for sp a) and ac b) conformations of MAAN. 

In the text 
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