Damian
Trzybiński
a,
Beata
Zadykowicz
b,
Michał
Wera
b,
Illia E.
Serdiuk
b,
Andrzej
Sieradzan
bc,
Artur
Sikorski
b,
Piotr
Storoniak
b and
Karol
Krzymiński
*b
aFaculty of Chemistry, Biological and Chemical Research Centre, University of Warsaw, Żwirki i Wigury 101, 02-089 Warsaw, Poland
bFaculty of Chemistry, University of Gdańsk, Wita Stwosza 63, 80-308 Gdańsk, Poland. E-mail: karol.krzyminski@ug.edu.pl
cBlirt S.A., Trzy Lipy 3/1.38, 80-172 Gdańsk, Poland
First published on 16th June 2016
9-Carboxy-10-methylacridinium chloride and trifluoromethanesulfonate, the parent compounds for a wide range of chemiluminogenic salts of practical importance, were synthesized and thoroughly investigated to address problems concerning structural and thermodynamical issues of these cognitively interesting molecular systems. Under various conditions of crystallization, the title salts disclosed three types of crystals: one built from the monomeric form of cations and two containing homoconjugated cations. The title compounds made the first described derivatives of acridine, expressing homoconjugated cationic forms, both in crystalline solid and gaseous phases. The monocrystals were characterized, employing X-ray crystallography and spectroscopic methods such as MALDI-TOF MS, ESI-QTOF MS, NMR and UV-Vis. X-ray crystallography studies revealed the occurrence of the three different molecular architectures, in which not only the counter ions and stoichiometry are different, but also the space group and number of molecules in the unit cell. The energetics and intermolecular interactions occurring within the crystals were explored, applying crystal lattice energy calculations and Hirshfeld surface analysis. In order to elucidate the thermodynamics and origin of the experimentally revealed forms, computations based on the density functional theory were performed, assuming vapour and liquid phases.
The compounds under study, containing the N-methylated ACA moiety, are the simplest and oldest acridinium derivatives investigated in the context of the chemiluminescence phenomenon.8 9-Carboxy-10-methylacridinium cations (CMA) form the structural base of a wide range of chemiluminogenic compounds that have been widely employed as labels and indicators, specially designed molecular systems utilized in medical diagnostics and trace analysis.9 However, derivatives of CMA are also interesting from the cognitive point of view. CMA, similar to ACA and related molecular systems, can occur in liquid phases in various forms, depending on the degree of their ionization.10 The structural similarity of CMA to betaines and isonicotinic acids is an intriguing fact in the context that the latter compounds are able to interact effectively with biological molecules through the formation of complexes, or by a wide range of short-range interactions.11 Like other carboxylic acids, molecules of CMA are prone to the formation of H-bonded forms involving the carboxyl group, which opens up opportunities for the molecules to occur in various structural forms.
The molecular architecture and the intermolecular interactions occurring in various phases in the group of quaternary salts containing 9-carboxy-10-methylacridinium or hydrogen bis(9-carboxy-10-methylacridinium) cations and chloride or trifluoromethanesulfonate (triflate) anions, were the main tasks of the presented work. The abovementioned molecular systems adopt various crystalline forms, denoted as 1, 2 and 3, which contain structural moieties that originate from CMA chemiluminogenic salts of practical importance.1,9 We focused primarily on the investigation of various crystalline forms with the participation of CMA, since we were interested in the number of structural variants and under what conditions they appear in solid, gaseous and liquid phases. We assumed that an extensive analysis of the structural problems concerning CMA-based cationic forms would be helpful in disclosing the factors determining the chemical and physicochemical properties of a wide range of related acridinium salts. Since CMA makes one of the products secreted upon chemiluminescence of acridinium esters and sulphonamides, the structural study presented here may also shed some light on the mechanism of this complicated process, which has been studied by us for a long time.2,12,13 In this work we employed a broad set of experimental methods, such as single crystal X-ray crystallography and spectroscopic techniques including UV-Vis, 1H and 13C NMR, MALDI-TOF and ESI-QTOF mass spectrometry. Moreover, we also applied various theoretical tools, such as determination of Hirshfeld surfaces, calculation of crystal lattice energies, as well as computations at the level of density functional theory (DFT). All these approaches provided us with a chance to take a deep look at the intermolecular interactions occurring among neighboring fragments of molecules and cations in various forms, energetics of cohesion forces in crystals and the “molecular shapes”, characteristic of crystalline solid phases. Quantum chemistry calculations disclosed information concerning structural and thermodynamic aspects of the investigated compounds, their stabilities in the gaseous and liquid phases and enabled us to propose a pathway leading to the formation of the CMA-based molecular systems described here.
Diffraction measurements were performed using an Oxford Diffraction Gemini R ULTRA Ruby CCD diffractometer with MoKα (λ = 0.71073 Å) radiation. Data collection and cell refinement were carried out with CrysAlis CCD and data reduction with CrysAlis RED software,14 applying multiscan absorption corrections (empirical absorption correction based on spherical harmonics, implemented in the SCALE3 ABSPACK scaling algorithm). The SHELXS-97 package was used to solve the structures by direct methods, and SHELXL-97 to carry out refinements by full-matrix least-squares on F2.15 The H-atoms bound to carboxylic oxygen atoms in 2 and 3 were located in a Fourier-difference map and refined freely with occupancy factors of 0.5. The H-atom bound to carboxylic oxygen atom in 1 was located in a Fourier difference map and refined as riding with Uiso(H) = 1.5Ueq(O). In all cases, the water H atoms were located in a Fourier-difference map, restrained by DFIX command 0.85 for O–H distances and by DFIX 1.39 for H⋯H distances and refined as riding with Uiso(H) = 1.5Ueq(O). All other H-atoms were positioned geometrically, with C–H = 0.93 Å and 0.96 Å for the aromatic and methyl H-atoms, respectively, and constrained to ride on their parent atoms with Uiso(H) = xUeq(C), where x = 1.2 for the aromatic H-atoms and x = 1.5 for the methyl H-atoms. All interactions demonstrated were found by PLATON program.16 To prepare molecular graphics, ORTEPII,17 PLUTO-7818 and Mercury19 programs were employed.
EL = Eel + Ed + Er | (1) |
−C6/R6 + Aexp(−R/ρ) | (2) |
The mass spectra of 1–3 were recorded employing a Biflex III MALDI-TOF mass spectrometer, working in the positive polarity mode with the 150–600 m/z scan range and the attenuation of the laser beam set at 60%. The samples of 1–3 (3–5 mg) were dissolved in the solution of dihydroxybenzoic acid (DHBA) in water. Additionally, samples of 1–3 were dehydrated (denoted as 1dh, 2dh, 3dh) and dissolved in a non-aqueous matrix (DHBA/anhydrous acetonitrile) and the above mixtures were also subjected to MALDI-TOF MS experiments. Results obtained for 1, 2 and 3 and 1dh, 2dh, 3dh are summarized in Tables S2 and S3 (ESI†), and exemplary mass spectra are presented in Fig. S2 (ESI†).
The ionization constant (pKa), denoting protolytic dissociation of the monocationic (c) to zwitterionic (z) form of 1 (Ka = [1z][H3O+]/[1c]) was obtained by spectrophotometric acid–base titration at 298 K in water–ethanol (9:1, v:v) solutions (Table S4 and Fig. S3, ESI†). To a stirred solution of 1 (2.00 ml, 2.50 × 10−5 M) in DI H2O (UP-grade), concentrated hydrochloric acid was gradually added in 10–100 μl portions until the final volume of 4.00 ml was attained. The actual pH of the mixtures with c(HCl) <0.1 M was determined using a portable pH-meter (GPX-105s, Elmetron, Poland). The acidity constants (H0) were determined instead of pH for the highly acidic mixtures,31,32 using the mass concentration of HCl in the cell, established gravimetrically after each addition. The electronic absorption UV-Vis spectra for each solution were recorded using a Lambda 40 UV-Vis spectrophotometer (Perkin-Elmer, USA) in the range of 300–500 nm (slit = 1 nm). The registered spectra were multiplied by the dilution coefficient d (d = Vi/V0, where Vi is the volume of the actual solution, in ml; V0 is the volume of the starting solution, 2.00 ml). To calculate the values of pKa by monitoring changes in absorbance at selected wavelengths, the Henderson–Hasselbalch equation, implemented in Spectra Data Lab software,33 was applied. This method relates pH and pKa to the equilibrium concentrations of dissociated [A−] and non-dissociated form [HA] of the acid, according to the following equation (eqn (3)):34
pH = pKa + log([A−]/[HA]) | (3) |
The predominant role in the packing of ions in the crystal of 3 is played by C–H⋯O and π–π intermolecular interactions (Fig. 1, 4 and Fig. S6, Tables S11 and S12, ESI,† CCDC 981471). Each homoconjugated cation interacts with neighbouring cations and anions through weak C–H⋯O hydrogen bonds involving the methyl H-atom and carbonyl oxygen atom (length 3.199 Å) or methyl or acridine skeleton H atoms and O atoms of triflate anions (lengths of 3.360(20) and 3.370(30) Å, respectively).
Repetition of the above mentioned C–H⋯O interactions brings about the formation of endless chains of ions running along the [001] direction (Fig. 4A). Parallely oriented chains are linked by the network of C–H⋯O (involving methyl H atoms and O atoms of anions) and π–π intermolecular interactions (between aromatic rings of neighbouring acridinium moieties) forming layers spreading along the (011) plane (Fig. 4B). Parallely oriented layers are stabilized by the network of π–π intermolecular interactions between aromatic rings of adjacent acridinium moieties, which results in the formation of a continuous multi-layered framework of ions in the crystal (Fig. 4C).
The scattergrams correlating lengths of hydrogen bonds (DIST1 and DIST2) and histograms imaging the distribution of the O⋯O distances (DIST3) in homoconjugated cations of 23 aromatic carboxylic systems are demonstrated in Fig. S8 (ESI†). Analysis of the data stored in the Cambridge Structural Database and summarized in the figures discloses that the lengths of the symmetrical O⋯H⋯O hydrogen bonds span from 1.21 to 1.24 Å, and O⋯O distances from 2.422 to 2.480 Å. The hydrogen bond lengths and O⋯O distances in 2 and 3, equal to 1.22, 1.22 and 2.435(3), 2.449(2) Å, respectively, fall within the range of the above determined values.
Predicted high values of EL reflect the substantial ionic character of lattices investigated herein (for comparison, purely molecular crystals of phenyl acridine-9-carboxylate derivatives studied previously were characterized by EL of magnitude around −160 kJ mol−1).7
The strongest cohesion force was found for 3 (EL equals 653 kJ mol−1). The lattice of compound 1 is less stable than the lattice of 3 by ca. 80 kJ mol−1 (EL equals to −575 kJ mol−1), whereas the lattice of 2 is less stable by almost 120 kJ mol−1, when compared to 3 (EL is equal to −535 kJ mol−1).
Various thermodynamic stabilities of the investigated compounds result from different contributions of Eel, Ed and Er to their total lattice energy. For 1, we have predicted the largest Coulombic term, Eel, among investigated crystals, which constitutes the dominant contribution to EL for this compound (−548 kJ mol−1). Values of Eel obtained for crystals containing the homoconjugated forms of cations are smaller by about 240 kJ mol−1 (2) and 150 kJ mol−1 (3).
Compound 2, which appears to be the least stable among the investigated crystals, is distinguished from the others because of the high value of the dispersion term (−472 kJ mol−1), which surpasses its electrostatic term (−312 kJ mol−1). In contrast, dispersive attractions, represented by the Ed term in the case of 1 and 3, are smaller than the coulombic forces. It may also be noted that the Ed term in 3 assumes a similar value to Eel calculated for this compound (−398 vs. −356 kJ mol−1) and both terms significantly overcome repulsive forces within the crystal lattice (Er = 101 kJ mol−1). Regarding repulsion, compounds involving chloride anions and water molecules (1, 2) exhibit almost identical Er terms, ca. 250 kJ mol−1.
To estimate the influence of water molecules on the cohesive forces occurring within the crystalline solid phases of 1 and 2, we performed additional calculations involving crystals, from which we removed the water. Resulting EL values along with the corresponding contributions (labelled with superscript a) are shown in Table 1.
When comparing the EL and EaL values collected in Table 1, it can be observed that neglecting water molecules leads to the destabilization of crystals 1 and 2 by 115 and 103 kJ mol−1, respectively. Despite a similar decrease in the total cohesive forces within 1 and 2 upon the removal of water, the changes in the individual components of EL are not uniform. Thus, reducing Eel in 1 amounts to 190 kJ mol−1, while in 2, it amounts to 72 kJ mol−1 (Table 1). In turn, the larger decrease in Ed takes place in 2 compared to 1 (180 vs. 131 kJ mol−1). Taking into account the sum of the Eel and Ed values, it can be estimated that co-crystallized water molecules introduce attractive interactions into the crystal lattices equal to −321 kJ mol−1 (1) and −253 kJ mol−1 (2). Moreover, water molecules also exert significant repulsive effects, which in the case of 1, amounts to 207 kJ mol−1 and in the case of 2 – to 150 kJ mol−1. Interestingly, removing water from 2 yields the Er value of 98.6 kJ mol−1, which is almost identical to that predicted for 3, and also involves the homoconjugated CMA cation. According to the above findings, it can be inferred that the interplay between attractive and repulsive effects, due to the presence of water molecules, results in the enhancement of the cohesive forces within 1 and 2; however, this effect does not seem to be the main factor determining the stability of CMA-based crystals investigated here.
Fig. 5 The Hirshfeld surfaces (front (left) and reverse (right) views) of the 9-carboxy-10-methylacridinium moieties reflecting the normalized contact distances (dnorm) with selected interactions. |
The analysis of the Hirshfeld surfaces mapped by the dnorm property verified the presence of both hydrogen bonds and π–π interactions listed by the PLATON programme (Fig. 5 and Tables S6–S12, ESI†). For the molecular systems investigated (1–3), the π–π interactions are represented by relatively large, flat areas in the curved surfaces (Fig. S9, ESI†). For 1, the strong O–H⋯O hydrogen bond between O16 and O1W marked on the dnorm surface as the red region, is also present in the de and di surfaces (Fig. 5 and Fig. S9, ESI†). In the case of compounds 2 and 3, weak hydrogen bonds of type C–H⋯O and C–H⋯Cl are marked as pale red areas. The large red regions marked on the maps reflect short distances between O atoms, external and internal to the surface (de and di, respectively), as well as the presence of mutual H atoms. All the abovementioned interactions are presented in the two-dimensional fingerprint plots (de/di) (Fig. S10 and S11, ESI†). The majority of the surfaces arise from the contribution of H⋯H interactions (from ca. 29% for 3 up to ca. 44% for 2) (Fig. 6 and Fig. S10 and S11, ESI†), which is characteristic of molecular crystals.54 For 1, the O16–H16⋯O1W hydrogen bond between the acridinium cation and water molecule is represented by a single long spike (di between 0.6 and 1.2) in the O⋯H and H⋯O fingerprint plots (Fig. S10 and S11, ESI†). For 2 and 3, such spikes do not occur; however, smaller spikes (di values in the range of 1.1–1.6) indicating the presence of C–H⋯O hydrogen bonds among water molecules and CMA moieties, or among CMA moieties themselves, are observed. Calculations for all compounds, performed with the assistance of the PLATON programme, disclose no signs of the existence of C–H⋯π interactions, which is further confirmed by the lack of characteristic wing motifs in the appropriate C⋯H and H⋯C fingerprint plots (Fig. S11, ESI†). The acridinium acid moieties are involved in π–π type contacts, which are illustrated by the presence of green areas of the C⋯C contributions to the Hirshfeld surfaces (Fig. S11, ESI†).
The relatively high amounts of the Cl⋯H and H⋯Cl contacts for 1 (4.5%) suggest the presence of a C–H⋯Cl interaction between the acridinium moiety and the chloride ion; however, such an interaction was not found by the PLATON programme. In the case of compound 2, the presence of the above-mentioned interactions is confirmed by both PLATON and the Hirshfeld surface (Cl⋯H and H⋯Cl fingerprint plot, Fig. S11, ESI†). Relatively high contributions of H⋯F and F⋯H interactions (9.8%) disclosed for 3, presumably result from the occurrence of disordered anionic fragments (CF3OSO2−), in which the oxygen atoms may exchange with the fluorine atoms.
The most deshielded protons, located in the spatial proximity of the nitrogen and oxygen atoms (H1/H8 and H4/H5, respectively (Fig. 1 and Scheme S2, ESI†)), are manifested by the signals appearing in the form of two clear doublets. The remaining aromatic protons of the acridine ring system appear as two distinct triplet systems; these are, in order of increasing shielding, H3/H6 and H2/H7, respectively (Table S1A, ESI†).
In general, the results of the 1H NMR experiments performed in various liquid phases (deuterium oxide, acetonitrile-d3, methanol-d4 and dimethylsulphoxide-d6), do not suggest the existence of more than one form of the cations involved in 1–3, or their mutual interconversion is too fast in comparison to the experiment time scale. Such a statement can be strictly drawn from the spectra, which present only clear and well-shaped signals of all protons involved in the systems investigated, as well as no changes in their intensity or shape upon lowering the temperature (in CD3OD) (Fig. S2B, ESI†). This observation differentiates the behaviour of the compounds investigated in liquid environment from their behaviour in the crystalline solid or in the gas phase (discussed below), where various forms of these molecular systems are observed. Similar conclusions can be drawn from 13C NMR spectra, recorded for 1–3 in deuterium oxide and dimethylsulphoxide-d6 (Table S1B and Fig. S3, ESI†). The latter resemble the spectra obtained for other quaternary derivatives of acridine-9-carboxylic acid investigated by us.55
The MALDI-TOF mass spectra recorded for 1–3 (Table S2 and Fig. S12, ESI†) indicate that in the case of 1 and 2, the monocationic form prevails over the homoconjugated form of CMA in the gas phase; however, for 3 the situation seems to be reversed (Fig. 7 and Table S3, ESI†). Contents of the homoconjugated cations in the gas phase increase in the order of 1, 2 and 3, which reveals that cations involved in 1 (appearing in a crystalline solid phase in the monomeric form) and 3 (appearing in a crystalline solid phase in the homoconjugated form) are characterized by the lowest and the highest amounts of the homoconjugated cation, respectively. This allows us to conclude that the molecular systems under investigation are characterized by the occurrence of equilibrium between the two above-mentioned forms, and their population in the gas phase depends on the chemical environment and experimental conditions. The latter statement is supported by the comparison of the population of monocationic vs. homoconjugated forms, characterizing cations 1–3 when a protic (water) vs. non-protic (acetonitrile) medium is used for preparation of samples (Fig. 7 and Table S3, ESI†). The experiments reveal that the amount of the monocationic form of CMA decrease in anhydrous conditions, compared to aqueous conditions, indicating the occurrence of equilibrium between both forms in the gaseous phase. High-resolution UPLC/ESI-QTOF mass spectra were additionally recorded for 1 and 3 (see Fig. S13 and S14 and text below, ESI†).
To understand the origin of the unique behaviour of CMA in the solid phase, one should take into account the composition of the solutions used for crystal growth. Since CMA contains groups that are able to participate in protolytic transformations, its actual form in aqueous solutions depends on the acidity of the environment (pH/H0). The protolytic forms of CMA are characterized by different spectral properties that allowed us to determine the ranges of pH/H0 in which these species are thermodynamically stable, by performing spectrophotometric UV-Vis acid–base titrations (Table S4 and Fig. S15, ESI†). In solutions of high acidity (H0 < −2.0) CMA exists in the mono-protonated form (monocation, Fig. 8). In solutions of lower acidity (−2.0 < H0/pH < 2.0) the monocationic form coexists with the zwitterionic one (Fig. 8); the pKa value of this protolytic equilibrium is 0.05 ± 0.01 (Table S4, ESI†). The pKa values calculated at various wavelengths from the UV-Vis spectra, change slightly in a systematic manner, which likely arises from the changes in the ionic strength of the titrated solutions.
Fig. 8 Mole fractions of the forms of 1versus pH/H0 estimated based on the experimentally determined first ionization constant (pKa (1) = 0.05) and the theoretically predicted second ionization constant (pKa (2) = 6.0). See also Table S4 and Fig. S13 (ESI†). |
The equilibrium between the monocationic and zwitterionic forms, characterized by a pKa value of 1.72, was assessed in the past in the aqueous solutions containing 3-carboxy-1-methylpyridinium cation, which is structurally related to CMA.56 The zwitterionic form of CMA is thermodynamically stable in solutions of low acidity and it transforms to a pseudo-base form in neutral and basic environments (Fig. 8), in a similar fashion to other 10-methylacridinium derivatives.57 Since the crystals of 1–3 were grown in protic solutions of various acidity, the co-existence of monocationic and zwitterionic forms in such media is of special interest for understanding the origin of formation of CMA-based homoconjugated cations; this is discussed below.
Entity | Methoda | Geometry of the O–H⋯O hydrogen bond | Angle (°) | ΔHrel | ΔGrel | μ | ||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|
O–H | H⋯O | O⋯O | <(OHO) | A | B | C | D | |||||
a DFT – the DFT(B3LYP)/6-31G** level of theory. b A, between the mean plane of the first acridine nucleus (C1–C14, N10) and the second acridine nucleus (C1A–C14A, N10A); B, between the mean planes delineated by C15, O16, O17 and C15A, O16A, O17A; C, between the mean plane of the first acridine nucleus (C1–C14, N10 or C1A–C14A, N10A) and the mean plane of the carbonyl group of the same acridine nucleus (C15, O16, O17 or C15A, O16A, O17A); D, between the mean plane of the first acridine nucleus (C1–C14, N10 or C1A–C14A, N10A) and the mean plane of the carbonyl group of the second acridine nucleus (C15A, O16A, O17A or C15, O16, O17). c μ represents the dipole moment of the compounds (indicated in Fig. S16, ESI), in D. d ΔHrel and ΔGrel represent the enthalpy and the Gibbs' free energy of a given conformers (indicated in Fig. S16, ESI) relative to the enthalpy and the Gibbs' free energy of 1a form; ΔHrel and ΔGrel values, in kJ mol−1. e ΔHrel and ΔGrel represent the enthalpy and the Gibbs' free energy of a given conformer (indicated in Fig. S16, ESI) relative to the enthalpy and the Gibbs' free energy of 2b form; ΔHrel and ΔGrel values, in kJ mol−1. f ΔHrel and ΔGrel represent the enthalpy and the Gibbs' free energy of a given conformer (indicated in Fig. S16, ESI) relative to the enthalpy and the Gibbs' free energy of 2d form; ΔHrel and ΔGrel values, in kJ mol−1. g ΔHrel and ΔGrel represent the enthalpy and the Gibbs' free energy of a given conformer (indicated in Fig. S16, ESI) relative to the enthalpy and the Gibbs' free energy of 3a form; ΔHrel and ΔGrel values, in kJ mol−1. | ||||||||||||
1a | X-ray | 89.6 | ||||||||||
DFT | 51.5 | 17.6 | ||||||||||
1b | DFT | 58.5 | 292.2d | 291.8d | 11.0 | |||||||
1c | DFT | 57.6 | 292.5d | 288.4d | 11.5 | |||||||
2a | X-ray | 1.220 | 1.220 | 2.435 | 180 | 0.0 | 0.0 | 84.8 | 84.8 | |||
DFT | 1.068 | 1.419 | 2.486 | 176 | 3.8 | 61.4 | 64.5/69.2 | 67.3/60.9 | 27.4e | 29.9e | 11.5 | |
2b | DFT | 1.047 | 1.472 | 2.513 | 172 | 49.2 | 74.8 | 66.6/72.7 | 38.8/38.5 | 29.1 | ||
2c | DFT | 1.056 | 1.448 | 2.498 | 172 | 55.6 | 75.2 | 71.0/73.3 | 40.3/38.5 | 2.6f | −0.9f | 28.6 |
2d | DFT | 1.038 | 1.517 | 2.492 | 154 | 60.3 | 72.6 | 68.8/75.3 | 44.4/82.2 | 6.9 | ||
2e | DFT | 1.117 | 1.320 | 2.434 | 174 | 47.3 | 77.6 | 69.2/70.7 | 38.5/34.4 | 14.9 | ||
3a | X-ray | 1.220 | 1.220 | 2.449 | 180 | 0.0 | 0.0 | 88.2 | 88.2 | |||
DFT | 1.042 | 1.509 | 2.485 | 153 | 51.5 | 72.3 | 78.8/79.3 | 50.3/82.5 | 7.2 | |||
3b | DFT | 1.052 | 1.456 | 2.502 | 172 | 52.3 | 73.4 | 74.0/69.7 | 38.0/42.7 | 13.5g | 5.5g | 37.3 |
3c | DFT | 1.158 | 1.261 | 2.416 | 174 | 44.1 | 76.7 | 68.2/68.4 | 39.2/38.1 | 4.0 |
The computational studies carried out on the homoconjugated forms of CMA enabled us to propose the three types of structure: linear (2a, 2c and 3b), bent (2b, 2d and 3a) and flat (2e and 3c) (Fig. S16, ESI†). Linear and bent forms refer to the hydrogen bond (O–H⋯O) geometry; the flat form refers to the anion⋯cation–H–cation⋯anion geometry. Regarding the homoconjugates, type 2 and 3 (the bent structures) are characterized by small values of the dipole moment and are thermodynamically preferred in the gas phase (Table S14, ESI†). In both types of salts, i.e., the ones comprised of Cl− and CF3SO3− counter anions (2d and 3a, respectively, Fig. S16, ESI†), the more stable bent structures are also characterized by lower values of the dipole moment (Table 2). However, in the case of complexes composed of the homoconjugated cation, chloride anion and two molecules of water (structures 2a and 2b, Fig. S16, ESI†), the dipole moment assumes substantially higher values (11.5 and 29.1, respectively), although the energetically favourable arrangement is also bent (2b). The latter feature likely results from the replacement of the Cl− and H2O moieties towards one of the N atoms of the acridine ring system (in the case of 2b), while in the linear complex (2a), the Cl− and H2O remain in a central position, i.e., in the vicinity of the H-bond, binding both CMA moieties. In the case of negatively charged molecular complexes containing two anions (2e and 3c, Fig. S16, ESI†), the more stable structure is flat, with the anions shifted towards the nitrogen atoms (N10 and N10A). In the case of the linear homoconjugated forms (2a, 2c, 3b, Fig. S16, ESI†), the O⋯H–O hydrogen bond is slightly shorter, compared to the length specified for the bent arrangements (2b, 2d, 3a, Fig. S16, ESI†) although the enthalpy and Gibbs free energies of such complexes are higher (Table 2 and Table S14, ESI†). The geometry of hydrogen bonding in the homoconjugated cations resembles that determined in the case of the crystalline solid phases (2 and 3). However, the H-atom involved is insignificantly shifted towards one of the oxygen atoms, resulting in the formation of slightly unsymmetrical hydrogen bonding (Table 2 and Fig. S16, ESI†). As was discussed above, the stability of the optimized complexes is controlled mainly by the electrostatic interactions occurring among the positively charged N atoms and CF3SO3− or Cl− anions. In the bent complexes (2d, 3a, Fig. S16, ESI†), the N+⋯A− distances are relatively short, attaining the values of 4.045/7.808 Å for CF3SO3− and 3.686/7.680 Å for Cl−, respectively, while in the case of the linear complexes (2c, 3b, Fig. S16, ESI†), shorter (comparable to the above ones) and longer N+⋯A− distances were predicted (5.228/15.878 Å for CF3SO3− and 4.319/14.121 Å for Cl−). The situation is different in the case of complexes containing molecules of water; in the flat structure 2a, the distances are comparable (7.539 and 7.360 Å for CF3SO3− and Cl−, respectively), while in the bent complex 2b, these distances are similar to those found for the linear ones, attaining values of 4.265 and 14.403 Å, respectively. The latter effect is presumably a consequence of a distinct shift of the chloride anion, together with water molecules, towards one of the nitrogen atoms (N10 or N10A), followed by the bending of the whole molecular arrangement.
Generally, DFT calculations indicate that the incorporation of water molecules into the investigated molecular complexes is manifested in the thermodynamic stabilization of resultant structures; linear complexes are less stable than the bent ones by about 27.2 and 29.7 kJ mol−1 (respective differences in enthalpy and Gibbs free energy). In the case of the chloride complex, this effect is not distinctly pronounced and the linear architecture is less stable than the bent one by 2.5 kJ mol−1 (enthalpy). In the linear complex 2a the N10⋯O(w) distances are comparable and are distributed quite symmetrically (values of 5.769, 6.657, 6.771 and 10.661 Å), while in the bent complex 2b, a distinct shift of water molecules towards the acridinium N atom is observed (values of 4.149, 14.917, 4.653 and 15.934 Å).
The vapour phase-optimized structure of the monomeric form, associated with two molecules of water and the chloride counter ion (1a), closely resembles the architecture characterizing the crystalline solid phase (1). As was mentioned above, the latter form is also energetically favoured among considered monocationic forms, since the other ones are less stable by about 290 kJ mol−1 (Table S14 and Fig. S16, ESI†).
Stepb | Phase | Method | ΔH | ΔG |
---|---|---|---|---|
a ΔH and ΔG denote enthalpy and Gibbs free energy of the reaction (step), respectively. b For possible pathways of formation of the title cation see Scheme 1. | ||||
I | Gaseous | DFT/6-31G** | −78.0 | −27.7 |
Liquid | DFT (PCM-H2O)/6-31G** | 34.5 | ||
DFT (PCM-CH3CH2OH)/6-31G** | 31.9 | |||
II | Gaseous | DFT/6-31G** | −100.6 | −104.4 |
Liquid | DFT (PCM-H2O)/6-31G** | −72.6 | ||
DFT (PCM-CH3CH2OH)/6-31G** | −73.3 | |||
III | Gaseous | DFT/6-31G** | −358.7 | −353.0 |
Liquid | DFT (PCM-H2O)/6-31G** | −144.0 | ||
DFT (PCM-CH3CH2OH)/6-31G** | −150.7 | |||
IV | Gaseous | DFT/6-31G** | −178.6 | −132.1 |
Liquid | DFT (PCM-H2O)/6-31G** | −38.0 | ||
DFT (PCM-CH3CH2OH)/6-31G** | −41.4 |
Scheme 1 Probable pathways of formation of homoconjugated bis(9-carboxy-10-methylacridinium) cations proposed at the level of the DFT method. |
The theoretically predicted thermodynamic data for possible transformation pathways summarized in Table 3, indicate that the above described steps are probable only in the gaseous phase. In the liquid phase (H2O or CH3CH2OH), step I seems to be thermodynamically unfavourable (positive value of Gibbs free energy). Predicted thermodynamic data suggest that formation of the homoconjugated cations presumably takes place according to the transformation steps denoted as III and IV (Scheme 1). These pathways underline our above-stated findings, indicating that the formation of homoconjugated cations of CMA occurs in solid crystalline and gaseous phases.
Compounds 1–3 presented in Fig. 1 are in general similar in terms of molecular geometry to other acridinium salts investigated by us, being characterized by the planar acridine ring system and a carboxyl group twisted at approximately right angles, relative to the acridine nucleus. Chlorides 1 and 2 crystallize in the monoclinic space group, while the triflate 3 crystalizes in the triclinic space group. As was detected using the PLATON program, the predominant role in the crystal packings of 1–3 is played by hydrogen bonds of various strength (O–H⋯O, C–H⋯O), or halogen (X)-containing specific intermolecular interactions, such as O–H⋯X and C–H⋯X. Parallely oriented aromatic layers in the crystals are stabilized by the network of π–π contacts and non-specific dispersive interactions that occur between aromatic rings of adjacent acridinium moieties, resulting in the formation of characteristic multi-layered frameworks. In the homoconjugated forms 2 and 3, symmetric O–H⋯O hydrogen bonding occurs, in which the H-atom is located directly in the inversion centre. The observed features of the crystalline networks are responsible for major differences in conformation, H-bond patterns and calculated lattice energies, characterizing the crystalline solid phases of the investigated systems. The reason for the observed physicochemical features of the crystalline solids presumably lies in the presence or absence of water molecules and fluorine atoms involved in a complex network of short-range interactions revealed in 1, 2 and 3.
Computational methods implemented in the GULP program, used for evaluation of the crystal lattice energies, provided the thermodynamic characteristics of the systems. Theoretically predicted lattice energies (EL, Table 1) reveal that the lattices characterizing 1–3 significantly differ in terms of their stability, i.e., compound 3 appears as the one forming the most stable crystals and compound 2, the least stable. In 1, the major attractive force occurring within the crystal lattice was found to be electrostatic (Eel). Here, the dispersive term (Ed) is almost entirely suppressed by the repulsion term (Er). In turn, dispersion dominates in EL assessed for crystals of 2, whereas in crystals of 3, Eel and Ed contributions to EL express comparable magnitude. The influence on the thermodynamic stability of crystals, exerted by water molecules within the lattices of 1 and 2, was also elucidated. In general, the presence of H2O within the crystal structures is manifested by the increase in total cohesive forces by more than 100 kJ mol−1; however, this effect, when compared to the large EL values, seems not to be of fundamental importance for the stabilization of the crystal lattices of 1 and 2.
The analysis of the Hirshfeld surfaces designated for 1–3 verified the presence of hydrogen bonds and π–π contacts, commonly occurring within the investigated molecular systems (Fig. 5 and 6). The red or pale red areas on the surfaces correspond to various types of hydrogen bonds and indicate shorter or longer mutual distances of the selected atoms. The O–H⋯O and C–H⋯O interactions are represented by longer or shorter single spikes on the fingerprint plots, according to the relative energy of the above interactions, while π–π contacts are represented by large flat regions characterizing the Hirshfeld surfaces.
Spectroscopic methods, such as MALDI-TOF MS, ESI-QTOF MS, 1H and 13C NMR and UV-Vis, allowed us to get further insight into the structures of 1–3 in gaseous and liquid phases. The mass spectra revealed that in the gas phase, the equilibrium occurs between the monocationic and homoconjugated forms of CMA, where their population depends on the experimental conditions; hydrated cations, involved in crystals of 1 and 2, were not observed in the MS experiments. 1H and 13C NMR spectra obtained for 1–3 in various liquid phases (D2O, DSO-d6, CD3OD, CD3CN) and at different temperatures (298 K and 233 K), disclosed that forms of CMA are not distinguishable by this method, or one form is present under the conditions of experiments. Spectrophotometric acid–base titration of 1 (built of the monocationic form of CMA in crystalline solid phase), performed in an aqueous environment, revealed that CMA may exist in the monocationic or zwitterionic forms under the conditions of crystal growth, which gives rise to the formation of the homoconjugated cations found in crystals of 2 and 3.
According to quantum chemistry calculations (DFT) conducted for 1–3 in the gas phase, the structural data obtained theoretically are comparable to the experimental findings (single crystal X-ray crystallography, Tables 2, 3 and Table S13, ESI†). Thermodynamic stability of the homoconjugated cations relates to the O–H⋯O hydrogen bond length, as well as attractive electrostatic interactions occurring among the oppositely charged groups of atoms (the N atoms experiencing a deficit of electron density, and the Cl− or CF3OSO2− anions). The above-mentioned features of the investigated molecular systems are also reflected in their various dipole moments. Based on the DFT approach, we proposed a possible pathway for the formation of CMA-based forms studied here. Calculated thermodynamic data emphasize the experimental findings, revealing that the formation of the homoconjugated forms of CMA is likely to occur in crystalline solid and liquid phases.
Footnote |
† Electronic supplementary information (ESI) available: Synthesis, chemical data and canonical structures of the investigated crystals (1–3) (Schemes S1 and S2) and their precursors (Fig. S1), crystal data and structure refinement for 1–3 (Table S5), parameters of hydrogen bondings found in 1–3 (Tables S6, S8 and S11), parameters of π–π interactions (Tables S7, S9 and S12), parameters of Cl⋯O contacts (Table S10), crystal packing in 1–3 (Fig. S4–S6), CSD database data (Fig. S7 and S8), chemical shifts of 1–3 in 1H and 13C NMR spectra (Table S1, Fig. S2, S3), MS data (Tables S2, S3 and Fig. S12–S14), the Hirshfeld surfaces representing distances external and internal to the surface for 1–3 (Fig. S9) and fingerprint plots of acridinium moieties in 1–3 (Fig. S10, S11), spectrophotometric titration data for 1 (Fig. S15 and Table S4) structural parameters of 1–3 (Table S13) and thermodynamic data for monomeric and dimeric conformers of 1 and 2 (Table S14) and the DFT structures (Fig. S16). CCDC 981470–981472. For ESI and crystallographic data in CIF or other electronic format see DOI: 10.1039/c6nj00725b |
This journal is © The Royal Society of Chemistry and the Centre National de la Recherche Scientifique 2016 |