Accounts of Chemical Research, volume 54, issue 2, pages 271-279

Rovibrational Quantum Chemical Treatment of Inorganic and Organometallic Astrochemicals

Publication typeJournal Article
Publication date2020-12-24
scimago Q1
SJR5.948
CiteScore31.4
Impact factor16.4
ISSN00014842, 15204898
General Chemistry
General Medicine
Abstract
ConspectusOur two groups have both independently and collaboratively been pushing quantum-chemical techniques to produce highly accurate predictions of anharmonic vibrational frequencies and spectroscopic constants for molecules containing atoms outside of the typical upper p block. Methodologies employ composite approaches, relying on various levels of coupled cluster theory-most often at the singles, doubles, and perturbative triples level-and quartic force field constructions of the potential portion of the intramolecular Watson Hamiltonian. Such methods are known to perform well for organic species, and we have extended this to molecules containing atoms outside of this realm.One notable atom that has received much attention in this application is magnesium. Mg is the second-most-abundant element in the Earth's mantle, and while molecules containing this element are among the confirmed astrochemicals, its further atomic abundance in the galaxy implies that many more molecules (both purely inorganic and organometallic) containing element 12 exist in astrophysical regions in chemical sizes between those of atoms and dust-sized nanocrystals. Our approach discussed herein is producing quality benchmarks and predicting novel data for magnesium-bearing molecules.The story is similar for Al and Si, which are also notably abundant in both rocky bodies and the universe at large. While Na, Sc, and Cu may not be as abundant as Mg, Al, and Si, molecules containing Na and transition metals have also previously been reported to be detected beyond the Earth. Consequently, the need to produce spectral reference data for molecules containing such atoms is growing. While several experimental groups (including, notably, the groups in Arizona, Boston, and France/Spain) have clearly led the way in detection of inorganic/organometallic molecules in space, computational support and even rational design can provide novel avenues for the detection of molecules containing atoms not typically studied in most laboratories. The application of quantum chemistry to other elements beyond carbon and its cronies at the top right of the periodic table promises a better understanding of the observable universe. It will also provide novel and fundamental chemical insights pushing the central science into new molecular territory.
Gardner M.B., Westbrook B.R., Fortenberry R.C., Lee T.J.
2021-03-01 citations by CoLab: 60 Abstract  
• Quartic force fields of the highest level provide rotational constants to within, on average, 34 MHz of experiment. • Tetraatomic species with low anharmonicities can be within 20 MHz. • These same methods provide vibrational frequencies to within, on average, 5.8 cm −1 . The CcCR quartic force field (QFF) methodology is capable of computing B 0 and C 0 rotational constants to within 35 MHz (0.14%) of experiment for triatomic and larger molecules with at least two heavy atoms. Additionally, the same constants for molecules with four or more atoms agree to within 20 MHz (0.12%) of experiment for the current test set. This work also supports previous claims that the same QFF methodology can produce fundamental vibrational frequencies with a deviation less than 5.7 cm −1 from experiment. Consequently, this approach of augmenting complete basis set extrapolated energies with treatments of core electron correlation and scalar relativity produces some of the most accurate rovibrational spectroscopic data available.
Gardner M.B., Westbrook B.R., Fortenberry R.C.
Planetary and Space Science scimago Q2 wos Q3
2020-11-01 citations by CoLab: 10 Abstract  
Rocky bodies are made of minerals comprised largely of silicon and oxygen. How these minerals are formed from their constituent atoms is not fully known. The rovibrational IR spectral data produced in this work may help to observe small molecules containing silicon and oxygen so that these potential molecular intermediates can be observed. These molecules have strong absorption features between 7.0 ​μm and 8.0 ​μm, most notably, and are fully characterized in the IR from the present quantum chemical data. The antisymmetric Si−O stretches of small silicon oxide clusters also fall in this range and have large intensities. Hence, this quantum chemical analysis provides spectral data for such molecules that may be of significance for astrochemical classification and could play a role in the formation or degradation of mineral nanocrystals from or into their constituent atoms. Both explicitly computed anharmonic fundamental vibrational frequencies and those determined from scaled harmonic frequencies agree well with known experimental data, and spectroscopic constants are provided herein such that astronomical rotational spectral characterization may also be possible for the C2v SiO3 and Si2O3 molecules.
Fortenberry R.C., Trabelsi T., Francisco J.S.
Journal of Physical Chemistry A scimago Q2 wos Q2
2020-10-12 citations by CoLab: 19 Abstract  
The astrophysical buildup of premineral nanocrystals from atoms to the smallest network-covalent solids will require observations of various small molecules containing the most common elements in minerals including aluminum and oxygen. The present work utilizes high-level quantum chemical quartic force field (QFF) approaches to produce anharmonic vibrational frequencies and spectroscopic constants for such species. The computed Beff for the astrochemically known AlOH molecule at 15780.5 MHz is a mere 40 MHz above the experimental value implying that the Beff for OAlOH at 5580.9 MHz is similarly accurate. The additional 7.31 D dipole moment in OAlOH implies that this molecule is a viable target for interstellar observation. Unlike the other anharmonic vibrational frequencies reported in this work, the Al-O-H bending frequencies in both AlOH and OAlOH are poorly described in the present QFF results. However, this failing actually highlights the fact that these bends are exceptionally floppy yet with counterintuitive exceedingly strong bonding. The Al-O bond energies are 128.2 and 107.2 kcal/mol, respective of AlOH and OAlOH, while the barriers to linearity are meager 16.6 and 380.7 cm-1 (0.1 and 1.1 kcal/mol).
Cheng Q., Washington M.C., Burns J.E., Fortenberry R.C., DeYonker N.J.
2020-09-03 citations by CoLab: 4 PDF Abstract  
ABSTRACT Despite its likely importance in astrochemistry, pure rotational spectra are not observable for gas-phase N2 since this molecule has no permanent dipole moment. Complexation of monomeric N2 with a cationic metal (MN2+) may be kinetically and thermodynamically favourable, and the detection of such MN2+ molecules could be useful tracers of N2 in order to probe its abundance and kinetics. Highly accurate quartic force field methods have been applied here to compute rotational and vibrational spectroscopic properties of the NaN2+ and MgN2+ molecules via a coupled cluster-based composite approach with additional corrections for post-CCSD(T) electron correlation and relativistic effects. The relative energies of various isomers have also been computed and show that both NaN2+ and MgN2+ have linear ground electronic states. At the highest level of theory, rotational constants (B0) of 4086.9 and 4106.0 MHz are predicted for NaN2+ and MgN2+, respectively, with dipole moments of 6.92 and 4.34 D, respectively, making them rotationally observable even at low concentrations. Post-CCSD(T) electron correlation corrections lower the N–N stretching frequency while relativistic corrections have a much smaller effect putting the fundamental frequencies at 2333.7 and 2313.6 cm−1, respective of NaN2+ and MgN2+ slightly above that in N2H+. Additive corrections do not significantly change the other two vibrational modes. An anharmonic, zero-point corrected N2 dissociation energy of 7.3 and 7.0 kcal mol−1 is, respectively, reported for NaN2+ and MgN2+ suggesting possible formation of these molecules in protoplanetary discs or planetary nebulae that are metal- and nitrogen-rich.
Burton M.A., Cheng Q., Halfen D.T., Lane J.H., DeYonker N.J., Ziurys L.M.
Journal of Chemical Physics scimago Q1 wos Q1
2020-07-16 citations by CoLab: 5 PDF Abstract  
Pure rotational spectra of Sc13C2 (X̃2A1) and Sc12C13C (X̃2A′) have been measured using Fourier transform microwave/millimeter-wave methods. These molecules were synthesized in a DC discharge from the reaction of scandium vapor, produced via laser ablation, with 13CH4 or 13CH4/12CH4, diluted in argon. The NKa,Kc = 10,1 → 00,0, 20,2 → 10,1, 30,3 → 20,2, and 40,4 → 30,3 transitions in the frequency range of 14 GHz–61 GHz were observed for both species, each exhibiting hyperfine splittings due to the nuclear spins of 13C (I = 1/2) and/or Sc (I = 7/2). These data have been analyzed with an asymmetric top Hamiltonian, and rotational, spin-rotation, and hyperfine parameters have been determined for Sc13C2 and Sc12C13C. In addition, a quartic force field was calculated for ScC2 and its isotopologues using a highly accurate coupled cluster-based composite method, incorporating complete basis set extrapolation, scalar relativistic corrections, outer core and inner core electron correlation, and higher-order valence correlation effects. The agreement between experimental and computed rotational constants, including the effective constant (B + C), is ∼0.5% for all three isotopologues. This remarkable agreement suggests promise in predicting rotational spectra of new transition metal-carbon bearing molecules. In combination with previous work on Sc12C2, an accurate structure for ScC2 has been established using combined experimental (B, C) and theoretical (A) rotational constants. The radical is cyclic (or T-shaped) with r(Sc–C) = 2.048(2) Å, r(C–C) = 1.272(2) Å, and ∠(C–Sc–C) = 36.2(1)°. The experimental and theoretical results also suggest that ScC2 contains a C2− moiety and is largely ionic.
Westbrook B.R., Del Rio W.A., Lee T.J., Fortenberry R.C.
2020-05-26 citations by CoLab: 12 Abstract  
Two vibrational frequencies for this molecule correlate with observed but unknown interstellar infrared emission features.
Doerksen E.S., Fortenberry R.C.
ACS Earth and Space Chemistry scimago Q2 wos Q2
2020-05-12 citations by CoLab: 24 Abstract  
After removal the geologically and astrophysically underabundant Be, B, and F atoms from consideration, the strongest X–Y bonds in HnX–YHm hydrides are for O bonding with Al, Si, and Mg. These are ...
Westbrook B.R., Fortenberry R.C.
Journal of Physical Chemistry A scimago Q2 wos Q2
2020-03-26 citations by CoLab: 31 Abstract  
The low-frequency vibrational fundamentals of D2h inorganic oxides are readily modeled by heuristic scaling factors at fractions of the computational cost compared to explicit anharmonic frequency computations. Oxygen and the other elements in the present study are abundant in geochemical environments and have the potential to aggregate into minerals in planet-forming regions or in the remnants of supernovae. Explicit quartic force field computations at the CCSD(T)-F12b/cc-pVTZ-F12 level of theory generate scaling factors that accurately predict the anharmonic frequencies with an average error of less than 1.0 cm-1 for both the metal-oxygen stretching frequencies and the torsion and antisymmetric stretching frequencies. Inclusion of hydrogen motions is less absolutely accurate but is similarly relatively predictive. The fundamental vibrational frequencies for the seven tetra-atomic inorganic oxides examined presently fall below 876 cm-1 and most of the hydrogenated species do as well. Additionally, ν6 for the SiO dimer is shown to have an intensity of 562 km mol-1, with each of the other molecules having one or more frequencies with intensities greater than 80 km mol-1, again with most in the low-frequency infrared range. These intensities and the frequencies computed in the present study should assist in laboratory characterization and potential interstellar or circumstellar observation.
Puzzarini C., Barone V.
2020-03-05 citations by CoLab: 41 Abstract  
Astrochemistry: toward the molecular complexity in the interstellar medium.
Fortenberry R.C.
2020-03-01 citations by CoLab: 19 Abstract  
Most carbon in the Universe is tied up in carbon monoxide or in polycyclic aromatic hydrocarbons. Even so, a vast majority of the molecules detected in various astrophysical media contain at least one carbon atom in them. These could nearly all be classified as hydrocarbons. However, only a fraction of the atoms in the Universe heavier than helium are actually carbon. This review will explore the past astronomical detections of molecules that do not contain carbon and will discuss the present workings and future outlooks of pure, inorganic astrochemistry. Such molecules have bonding structures that are often “atypical,” have notable spectroscopic intensities, and open the door for new chemical insights. Asking novel questions can lead to novel insights, and inorganic astrochemistry provides a strong motivation for asking the most creative chemical questions.
Kállay M., Nagy P.R., Mester D., Rolik Z., Samu G., Csontos J., Csóka J., Szabó P.B., Gyevi-Nagy L., Hégely B., Ladjánszki I., Szegedy L., Ladóczki B., Petrov K., Farkas M., et. al.
Journal of Chemical Physics scimago Q1 wos Q1
2020-02-20 citations by CoLab: 365 PDF Abstract  
MRCC is a package of ab initio and density functional quantum chemistry programs for accurate electronic structure calculations. The suite has efficient implementations of both low- and high-level correlation methods, such as second-order Møller–Plesset (MP2), random-phase approximation (RPA), second-order algebraic-diagrammatic construction [ADC(2)], coupled-cluster (CC), configuration interaction (CI), and related techniques. It has a state-of-the-art CC singles and doubles with perturbative triples [CCSD(T)] code, and its specialties, the arbitrary-order iterative and perturbative CC methods developed by automated programming tools, enable achieving convergence with regard to the level of correlation. The package also offers a collection of multi-reference CC and CI approaches. Efficient implementations of density functional theory (DFT) and more advanced combined DFT-wave function approaches are also available. Its other special features, the highly competitive linear-scaling local correlation schemes, allow for MP2, RPA, ADC(2), CCSD(T), and higher-order CC calculations for extended systems. Local correlation calculations can be considerably accelerated by multi-level approximations and DFT-embedding techniques, and an interface to molecular dynamics software is provided for quantum mechanics/molecular mechanics calculations. All components of MRCC support shared-memory parallelism, and multi-node parallelization is also available for various methods. For academic purposes, the package is available free of charge.
Trabelsi T., Davis M.C., Fortenberry R.C., Francisco J.S.
Journal of Chemical Physics scimago Q1 wos Q1
2019-12-24 citations by CoLab: 27 PDF Abstract  
As of yet, unexamined aluminum bearing molecules may help elucidate aluminum chemistry and associated refractory atom reactions in the interstellar medium. The flexibility of modern quantum chemistry in the construction and analysis of novel molecules makes it perfectly suited to analyze molecules of astrochemical significance. In this paper, high level ab initio electronic structure calculations using the coupled cluster CCSD(T) and explicitly correlated coupled cluster CCSD(T)-F12 methods with large basis sets extrapolated to the complete basis set limit have been performed on the various [Al,N,C,O] isomers. The anharmonic rotational and vibrational spectroscopic parameters for all isomers are produced with these same levels of theory via quartic force fields and vibrational perturbation theory in order to aid in their potential laboratory or even astrophysical identification. The most stable isomer is determined here to be the aluminum isocyanate radical with linear equilibrium geometry AlNCO (X1Σ+). The NCO antisymmetric stretch of AlNCO has an intensity of 1500 km/mol, which should greatly aid in its infrared detection in the region around 2305 cm−1. Additionally, the AlOCN isomer is relatively low lying, possesses a 5.12 D dipole moment, and has a notable kinetic stability, making it a viable candidate for astronomical observation. All isomers are characterized by small frequencies, which indicates that these are floppy molecules. Isomers with a terminal aluminum atom are especially floppy, with bending modes less than 100 cm−1.
Valencia E.M., Worth C.J., Fortenberry R.C.
2019-11-28 citations by CoLab: 21 PDF Abstract  
ABSTRACT Isolated MgSiO3 and Mg2SiO4 molecules are shown here to exhibit bright infrared (IR) features that fall close to unattributed astronomical lines observed toward objects known to possess crystalline enstatite and forsterite, minerals of the same respective empirical formulae. These molecules are therefore tantalizing candidates for explaining the origin of such features. Furthermore, the C2v monomer minima of each formula set have dipole moments on the order of 10.0 D or larger making them desirable candidates for radioastronomical observation as enabled through rotational spectroscopic data further provided in this high-level CCSD(T)-F12/cc-pVTZ-F12 quantum chemical study. Astrophysical detection of these molecules could inform the build-up pathways for creating nanocrystals from small molecules in protoplanetary discs or could show the opposite in explaining the destruction of enstatite and forsterite minerals in supernovae events or other high-energy stellar processes. This work also shows that the lowest energy isomers for molecules containing the geologically necessary elements Mg and Si have oxygen bonded between any of the other heavier elements making oxygen the glue for pre-mineralogic chemistry.
Burton M.A., Russ B.T., Bucchino M.P., Sheridan P.M., Ziurys L.M.
2019-11-01 citations by CoLab: 7 Abstract  
• First experimental determination of the quadrupole coupling in metal amide species. • First FTMmmW measurements (22–58 GHz) of LiNH 2 and NaNH 2 . • Further evidence for strong ionic bonding in alkali amide molecules. • First computed structure for KNH 2 ( X ~ 1 A 1 ) with a modern basis set for future work. Rotational spectra of LiNH 2 and NaNH 2 have been recorded using Fourier transform microwave/millimeter-wave (FTMmmW) techniques in the range 22 – 59 GHz. The species were created from the reaction of metal vapor and ammonia, diluted in argon, using a Discharge-Assisted Laser Ablation Source (DALAS). The J Ka,Kc = 1 01 → 0 00 transition was measured for both molecules, as well as the J Ka,Kc = 2 02 → 1 01 transition for NaNH 2, all of which exhibited quadrupole coupling splittings. The two data sets were each analyzed with an S -reduced asymmetric top Hamiltonian, establishing the lithium and sodium electric quadrupole coupling parameter, χ aa for the first time, and refining previous rotational constants. Quadrupole and nuclear-spin rotation interactions were also computationally investigated at the MP2/6-311G++(3df,2pd) level for LiNH 2 , NaNH 2 and KNH 2 . These calculations suggest that the major contributor to the quadrupole interactions is the alkali metal nucleus, not that of nitrogen, as confirmed experimentally. Comparison of quadrupole coupling constants suggest that LiNH 2 and NaNH 2 are principally ionic molecules with a charge distribution similar to LiF and NaF.
Agbaglo D., Fortenberry R.C.
Chemical Physics Letters scimago Q2 wos Q1
2019-11-01 citations by CoLab: 50 Abstract  
CCSD(T)-F12b/cc-pVTZ-F12 anharmonic vibrational frequencies match experiment or higher-level theory to within an average of 10.3 cm−1 for a sample set of 11 molecules. This is further reduced below 7.0 cm−1 when extreme differences are removed from the data set. CCSD(T)-F12b/cc-pVTZ-F12 and CCSD(T)-F12b/cc-pVDZ-F12 frequencies differ on average by 4.8 cm−1. The CCSD(T)-F12b frequencies require orders of magnitude less computer time than higher-order theory and cc-pVDZ-F12 less than cc-pVTZ-F12, especially as the number of atoms increases. Hence, utilization of these levels of theory may provide accurate vibrational frequencies for larger molecules provided that the core-electron correlation is not significant.
Dotson J.R., Palmer C.Z., Fortenberry R.C.
2024-11-15 citations by CoLab: 0
Thripati S., Gautam R., Ramabhadran R.O.
ACS Earth and Space Chemistry scimago Q2 wos Q2
2023-01-09 citations by CoLab: 2
Harwick O.A., Fortenberry R.C.
2023-01-01 citations by CoLab: 4 Abstract  
Aluminum forms strong bonds to oxygen, nitrogen, and hydrogen, but these motifs are relatively rare in the interstellar medium (ISM). However, no chemical rationale accounts for this observation. The cyclic molecules AlO2, HAlO2, and (HN)OAlH are quintessential examples of the aforementioned phenomenon, and the latter two are isoelectronic with each other. Matrix-isolation spectroscopic data and prior theoretical computations exist for cyclic AlO2, although it has yet to be observed astronomically. However, high-level theoretical data provided herein generate useful predictions for and insights into spectral data for these three molecules. Anharmonic vibrational frequencies and rotational constants are determined in this work for these molecules via quartic force fields at the CCSD(T)-F12b/cc-pVTZ-F12 level of theory and with canonical CCSD(T) for consideration of basis set convergence, core electron correlation, and relativity (CcCR). The present work finds that these aluminum oxides are weak-to-moderate infrared emitters but are much stronger microwave emitters with dipole moments of 4.95 D, 4.55 D, and 3.76 D respective of cyclic AlO2 (c-AlO2), cyclic HAlO2 (c-HAlO2), and cyclic (HN)OAlH (c-(HN)OAlH). Correlation to argon-matrix experiments for c-AlO2 is within the expected matrix shift for the ν3 bend computed here to be 527.8 cm−1. Astrophysical detection of these molecules could imply their role in the creation or degradation of aluminum-containing nanocrystals and interstellar dust of importance for the formation of rocky bodies, and the spectral data computed in this work should be able to assist in such classification.
Watrous A.G., Fortenberry R.C.
2022-11-22 citations by CoLab: 0 Abstract  
Abstract The recent radioastronomical detection of magnesium dicarbide (MgC2) towards the carbon-rich star IRC+10216 leads to questions about whether this molecule can be observed in other wavelengths, especially with the wealth of IR data being produced by JWST. This present, theoretical spectral characterization, unfortunately, implies that mid-IR observations of MgC2 are unlikely due to small IR transition intensities, overlap with polycyclic aromatic hydrocarbon IR features, low frequencies/long wavelengths, or the relatively small column densities. In spite of this, the full set of fundamental anharmonic vibrational frequencies are provided for each of the 24Mg, 25Mg, and 26Mg isotopologues as are the complete rotational constants for the same set for additional laboratory characterization. Most notably and with regards to 24MgC2, the B0 and C0 (11452.7 MHz and 9362.7 MHz) rotational constants are uniquely provided for the first time. The experimentally-derived A0, (B + C)/2, and (B − C)/4 values are within 0.7% of the presently computed anharmonic results implying similar accuracy for the remaining spectroscopic constants.
Agbaglo D.A., Cheng Q., Fortenberry R.C., Stanton J.F., DeYonker N.J.
Journal of Physical Chemistry A scimago Q2 wos Q2
2022-06-27 citations by CoLab: 7 Abstract  
Magnesium tricarbide isomers are studied herein with coupled cluster theory and multireference configuration interaction to support their possible detection in astrochemical environments such as the circumstellar envelope surrounding the star IRC +10216 or in terrestrial laboratories. Magnesium-bearing species may abound in the interstellar medium (ISM), but only eight (MgNC, MgCN, HMgNC, MgC2H, MgC3N, MgC4H, MgC5N, and MgC6H) have been directly identified thus far. Several possible isomers for the related MgC3 system are explored in their singlet and triplet spin multiplicities. Overall, this work offers quantum chemical insight of rovibrational spectroscopic data for MgC3 using quartic force fields (QFFs) based on the CCSD(T) and CCSD(T)-F12 levels of theory at the complete basis set (CBS) limit. Additional corrections with small basis set CCSDT(Q) and scalar relativistic effects are also included in the analysis. Salient multireference character is found in the singlet diamond electronic state, which makes a definitive assignment of the ground state challenging. Nevertheless, coupled cluster-based composite energies and multireference configuration interaction both predict that the 1A1 diamond isomer is 1.6-2.2 kcal mol-1 lower in energy than the 3A1 diamond isomer. Furthermore, highly accurate binding energies of various isomers MgC3 are provided for comparison to photodetachment experiments. Dipole moments along with harmonic infrared intensities will guide efforts for astronomical and spectroscopic characterization.
Grosselin D., Fortenberry R.C.
ACS Earth and Space Chemistry scimago Q2 wos Q2
2021-12-28 citations by CoLab: 12
Zapata Trujillo J.C., McKemmish L.K.
2021-10-23 citations by CoLab: 18 Abstract  
Vibrational frequency calculations performed under the harmonic approximation are widespread across chemistry. However, it is well-known that the calculated harmonic frequencies tend to systematically overestimate experimental fundamental frequencies; a limitation commonly overcome with multiplicative scaling factors. In practice, multiplicative scaling factors are derived for each individual model chemistry choice (i.e., a level of theory and basis set pair), where performance is judged by, for example, the root-mean square error (RMSE) between the predicted scaled and experimental frequencies. However, despite the overwhelming number of scaling factors reported in the literature and model chemistry approximations available, there is little guidance for users on appropriate model chemistry choices for harmonic frequency calculations. Here, we compile and analyse the data for 1495 scaling factors calculated using 141 levels of theory and 109 basis sets. Our meta-analysis of this data shows that scaling factors and RMSE approach convergence with only hybrid functionals and double-zeta basis sets, with anharmonicity error already dominating model chemistry errors. Noting inconsistent data and the lack of independent testing, we can nevertheless conclude that a minimum error of 25cm-1 -- arising from insufficiently accurate treatment of anharmonicity -- is persistent regardless of the model chemistry choice. Based on the data we compiled and cautioning the need for a future systematic benchmarking study, we recommend wB97X-D/def2-TZVP for most applications and B2PLYP/def2-TZVPD for superior intensity predictions. With a smaller benchmark set, direct comparison strongly prefers wB97X-D/6-31G* to B3LYP/6-31G*.
Doerksen E.S., Fortenberry R.C.
2021-08-13 citations by CoLab: 2 PDF Abstract  
The atoms contributing to the strongest “single bonds” on the periodic table do not continue to produce the strongest “double bonds” or “triple bonds.” In fact, the opposite appears to be the case. This quantum chemical examination of nominal X = Y and X ≡ Y bonds in model molecules of atoms from the first three rows of the periodic table shows that the strongest “double bond” is in formaldehyde once the astrophysically-depleted Be and B atoms are removed from consideration. The strongest “triple bond” is a close match between acetylene and N2. However, these results indicate that astrophysical regions containing a high abundance of hydride species will likely be areas where inorganic oxide formation is favored. Those where H2 molecules have already been dissociated will favor organic/volatile astrochemistry.
Thripati S., Ramabhadran R.O.
Journal of Physical Chemistry A scimago Q2 wos Q2
2021-04-16 citations by CoLab: 9 Abstract  
The chemistry occurring in the interstellar medium (ISM) is an active area of contemporary research. New aspects of interstellar chemistry are getting unraveled regularly. In this context, the role of metal-ions in the chemistry occurring in the ISM is not well-studied so far. Herein, we highlight the role of metal-ions in interstellar chemistry. For this purpose, we choose the problem of gas-phase formamide formation in interstellar molecular clouds. Formamide is a key biomonomer and contains the simplest peptide [-(C═O)-NH-] linkage. With its two electronegative atoms (O and N), it provides an excellent platform to probe the role of the metal-ions. The metal-ions chosen are Na+, K+, Al+, Mg+, and Mg2+-all of them present in the ISM. The metal-ions are studied in three different forms as bare positively charged ions, as hydrated metal-ions co-ordinated with a molecule of water, and when the metal-ions are part of a neutral covalent molecule. With the aid of electronic structure calculations [CCSD(T) and DFT methods], we study different gas-phase pathways which result in the generation of interstellar formamide. Throughout our study, we find that metal-ions lower the barriers (with Mg+, Mg++, and Al+ offering maximal stabilization of the transition states) and facilitate the reactions. The chemical factors influencing the reactions, how we consider the putative conditions in the ISM, the astrochemical implications of this study, and its connection with terrestrial prebiotic chemistry and refractory astrochemistry are subsequently presented. Based on our results, we also recommend the detection of two new closed-shell molecules, NH2CH2OH (aminomethanol) and CH2NH2+ (iminium ion), and two open-shell molecules, CONH2 (carbamyl radical) and HCONH (an isomer of carbamyl radical), in the ISM.

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