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Liquid–liquid equilibrium and modelling insight: molecular interaction analysis of water + methanol + dimethyl carbonate + 1-ethyl-3-methylimidazolium methanesulfonate ternary systems

Juho-Pekka Laakso*, Behnaz Asadzadeh, Petri Uusi-Kyyny and Ville Alopaeus
Department of Chemical and Metallurgical Engineering, Aalto University, School of Chemical Engineering, P.O. Box 11000, FI-00076 Aalto, Finland. E-mail: juho-pekka.laakso@aalto.fi

Received 12th June 2025 , Accepted 2nd September 2025

First published on 5th September 2025


Abstract

In this work, ternary liquid–liquid equilibrium (LLE) was measured for water (H2O) + dimethyl carbonate (DMC) + 1-ethyl-3-methylimidazolium ([Emim][MeSO3]) and methanol (MeOH) + DMC + [Emim][MeSO3] mixtures at 293.15 K at atmospheric pressure. LLEs were modelled utilizing COnductor-like Screening MOdel for Real Solvents (COSMO-RS) and non-random two-liquid (NRTL) models. COSMO-RS was utilized to provide insight into interactions at molecular level through chemical potentials corresponding to the sigma profile and predicted excess enthalpies. The nature of COSMO-RS accuracy was qualitative, while NRTL had an accuracy of 0.013 and 0.030 root mean square deviation for LLE of H2O + DMC + [Emim][MeSO3] and MeOH + DMC + [Emim][MeSO3] mixtures, respectively. Hydrogen bonding behavior explained favorable [Emim][MeSO3]–H2O and –MeOH interactions. These interactions might be mainly due to strong hydrogen bond donor interaction between [MeSO3] anion–H2O and –MeOH. The unfavorable [Emim][MeSO3]–DMC interaction was explained by electrostatic repulsion, possibly arising from repulsion between [MeSO3] anion and DMC oxygens.


1. Introduction

Utilizing carbon dioxide (CO2) to synthesize valuable chemicals offers a promising strategy for cost-effective atmospheric CO2 emissions removal, which mitigates the impact of CO2 on the climate while obtaining essential chemicals.1 Dimethyl carbonate (DMC) is a promising environmentally friendly chemical used e.g. as a solvent, battery electrolyte, and fuel additive.2 Traditionally, DMC has been synthesized via methanol (MeOH) phosgenation, transesterification, and oxidative carbonylation. These synthesis routes present drawbacks, such as using toxic phosgene or a high risk of explosion.3 Besides these routes, CO2 and MeOH can be used to synthesize DMC, which is an environmentally sustainable and safe method. However, this synthesis is limited by thermodynamics,3 while equilibrium conversion can be as low as 1%.4 This highlights the significance of strategies for improving equilibrium conversion. One promising approach is to use H2O absorbents for in situ H2O trapping.5

Ionic liquids (ILs) are a class of salts that melt at temperature under 100 °C. These are generally claimed to be non-volatile, non-flammable, and air and H2O-stable.6 One significant advantage of ILs is the ability to tailor their properties by modifying the ion combinations from which they are formed. With at least one million possible ion combinations,7 ILs offer vast potential for customizing their properties. The tunable nature of ILs have been employed in the extraction and separation of bioactive compound,8 where the hydrophilicity or hydrophobicity can be adjusted by varying the cation–anion combination. ILs have also been employed in integrated CO2 capture and conversion,9 where ILs can not only dissolve CO2 but, also act as a catalyst simultaneously.

1-Ethyl-3-methylimidazolium methanesulfonate ([Emim][MeSO3]) has interesting interaction with H2O, MeOH and DMC. Excess enthalpy10 and infinite dilution activity coefficient11,12 measurements indicate strong [Emim][MeSO3]–H2O and slightly weaker [Emim][MeSO3]–MeOH attractive interaction while [Emim][MeSO3]–DMC interaction is repulsive. Gas drying is a possible practical application of [Emim][MeSO3] due to experimentally determined low activity coefficient, low viscosity, and high thermal stability.13

We investigated liquid–liquid equilibrium (LLE) behavior of the H2O/MeOH + DMC + [Emim][MeSO3] ternary system, since LLE data can be helpful in designing solvents for reactive systems.14 It allows one to estimate whether the mixture has more than one liquid phase and how reactants and products will distribute in the liquid phases. Thus, it allows one to design these systems to improve the desired yield of the product. This approach has been used in esterification reactions, where IL was used as a solvent to improve conversion of reaction.15 Phase split into two liquid phases also imply conditions where interactions between the components are strong, allowing for more definite conclusions regarding molecular level phenomena.

Experimental phase equilibrium regarding components relevant to this study has been studied in the literature. Experimental LLE study has been conducted for MeOH + DMC + H2O mixture at different temperatures.16 LLE data have been measured for MeOH + DMC + IL systems using a few ILs. Measured ILs include imidazolium-based cation with hydrogen sulfate,17 dimethyl, and diethyl phosphonium anion.18 The LLE of MeOH and DMC involving hydroxyethyl ammonium cation with different carboxylate anions has been measured.19 Also, binary and quaternary vapor–liquid equilibrium, including MeOH + DMC + H2O + [Emim][MeSO3] has been measured previously.20

Non-random two liquids model (NRTL)21 is a popular for phase equilibrium modeling. The NRTL model is an activity coefficient-based model with a correlative nature. It uses experimental data for regression binary interaction parameters and can accurately estimate phase equilibrium. NRTL has been successfully used to model the LLE of MeOH + DMC + IL systems.17,18 COnductor like screening MOdel for real solvents (COSMO-RS)22 is an activity coefficient-based model, which uses only structural information calculated via quantum chemistry. A key advantage of COSMO-RS is the ability to give phase equilibrium predictions without experimental data.23 This makes COSMO-RS suitable for solvent screening.24 However, COSMO-RS is capable of predicting LLE in general, while a comprehensive analysis of these predictions has been made for binary and ternary mixtures, including ILs.25–28

COSMO-RS can give insight into molecular interactions by predicting the chemical potential corresponding to the sigma profile (μ(σ)). This chemical potential quantifies favorable and unfavorable interactions that compounds have with different polarities. Thus, one can estimate the component's affinity towards hydrogen bond donor (HBA), non-polar, and hydrogen bond acceptor (HBA) characteristics.23 Interaction within mixtures can be evaluated by excess enthalpy (HE). COSMO-RS is able not only to predict HE but also to quantify the contribution of electrostatic (HE(MF)), hydrogen bonding (HE(HB)), and van der Waals (HE(vdW)) interactions to HE, thus giving insight into the interaction present in mixtures. A study on the COSMO-RS ability to predict HE for a wide range of components with ILs indicate that the accuracy of these predictions is generally in good agreement with experiments.29

In this work, we measured the LLE of ternary mixtures including DMC, [Emim][MeSO3], and either H2O/MeOH. As far as we know, this is the first time these LLEs have been experimentally measured. NRTL and COSMO-RS were used to model the LLE behavior in those mixtures. Insight into interactions at the molecular level was studied using COSMO-RS, which was used to explain the LLE behavior. The novelty of this work is not only new LLE experimental data for DMC + H2O + [Emim][MeSO3] and DMC + MeOH + [Emim][MeSO3] mixtures but also the insight into interactions at the molecular level that can be used to explain the behavior of these LLE. The experimental procedure is provided in Section 2 while modeling approaches are in Section 3. The experimental and modeling results are in Section 4, and the conclusions are presented in Section 5.

2. Experimental

2.1 Materials

The compounds utilized in this study are shown in Table 1. Compounds were acquired from Sigma-Aldrich. The H2O content in [Emim][MeSO3] was determined using the Karl–Fischer titrator. Milli-Q ultrapure H2O was produced using the H2O purification system (Direct-Q 5 UV) and applied to prepare the mixtures.
Table 1 Chemicals used in this work
Chemicals CAS number Supplier Purity H2O content mass fraction Purification method
1-Ethyl-3-methylimidazolium methanesulfonate 145022-45-3 Merck ≥98.8 0.0090 Vacuum drying
Dimethyl carbonate 616-38-6 Merck ≥99.0 Undetectable Molecular sieves
2-Propanol 67-63-0 Honeywell ≥99.9 Undetectable Molecular sieves
Methanol 67-56-1 Merck ≥99.9 0.0001 Molecular sieves
H2O 7732-18-5   Type I, k: 0.05 μS cm−1 at 298 K    


2.2 Apparatus and procedure

2.2.1 Determination of binodal curves. We used the cloud-point method30 to determine the binodal curves. We used a 50 cm3 glass cell to determinate the values of binodal curves. Around this cell, H2O at 293.15 K was circulated in a surrounding jacket made of glass a Lauda E200 thermostat (Germany) was utilized for regulating temperature with a u(T) = 0.2 K uncertainty. The formation of two liquid phases was detected by the mixture becoming turbid after titrated with DMC and MeOH to a predefined concentration of (H2O + [Emim][MeSO3]) and (DMC + [Emim][MeSO3]) solution. We measured the mass composition for each binodal measurement, where titration caused turbidity, utilizing analytical balance which has uncertainty of u(m) = 0.002 g.
2.2.2 Determination of tie lines. We performed the LLE measurements at atmospheric pressure by using the glass apparatus detailed by Männistö et al.31 as detailed in our previous work.32 To determine tie lines, we prepared feed samples by mixing needed amount of (MeOH + DMC + [Emim][MeSO3]) and (DMC + [Emim][MeSO3] + H2O) in the apparatus at fixed temperature utilizing the thermostat (Model: Lauda E200, Germany). The inlet and outlet H2O temperatures were measured utilizing calibrated Pt-100 probes connected to an ASL CTR-2000-24 thermometer with u(T) = 0.2 K uncertainty. The samples underwent thorough mixing and were given at least 72 hours to split into two distinct liquid phases. We assumed that equilibrium was achieved once the difference in mass fraction was below 0.0001 for two repeated measurements. After two clear phases separated, samples from each liquid phases were obtained utilizing a Hamilton sample-lock syringe. The collected samples were transformed into vials preloaded with the 2-propanol. After separating the two phases, the DMC, MeOH, and H2O concentrations were determined using Agilent 7890B gas chromatography (GC). In addition, the concentration of [Emim][MeSO3] can be estimated using mass balance. Sampling and analysis for each solution were performed at least three times after equilibrium had been achieved. The configuration for Agilent 7890B GC is shown in Table S1. We calibrated the GC utilizing mixtures with measured masses of 2-propanol with MeOH, DMC, and H2O. We computed the response factor (Fi) according eqn (1).
 
image file: d5cp02239h-t1.tif(1)
where Ai is the peak area for component i, Astd is the peak area for 2-propanol, which is used as a solvent, mi, and mstd are the masses for component i and the solvent, respectively. The response factor of 2-propanol (Fstd) was set to 1. While analyzing the samples, the relative response factor between the component and the solvent peak area described eqn (1) was not considered. Mass fractions of [Emim][MeSO3] for each sample were determined by subtracting the mass of other components from the total mass. In few measurements, this subtraction resulted in small negative mass fractions. Thus, in these measurements the composition was calculated by setting mass fraction of [Emim][MeSO3] to zero.

2.3 Uncertainty of measurement

An essential aspect of experimental work is determining the measurement uncertainty since this reflects the exact knowledge of the measurement value. Guidelines for the determination of measurement uncertainties are explained in the literature.33,34 This can be calculated in different ways, such as standard uncertainty (u), combined standard uncertainty (uc) eqn (2), and expanded standard uncertainty (U) eqn (3). In this work, expanded standard uncertainties with 95% level of confidence (coverage factor of k = 2) were computed for experimental data. The equations used for expanded uncertainty calculations are shown in eqn (S1)–(S4).
 
image file: d5cp02239h-t2.tif(2)
 
U = kuc (3)
where uc = combined uncertainty, f = function, xi = input variable, k = coverage factor and U = expanded uncertainty.

3. Phase equilibria modelling

3.1 Criteria of phase equilibrium

The thermodynamic criteria for phase equilibrium are fulfilled when fugacity (f) of each component in any two co-existing phases is equal, as shown in eqn (4). Under assumption of ideal behavior in the vapor phase, the criteria for the vapor–liquid equilibrium can be described as in eqn (5). The liquid–liquid equilibrium is typically expressed by using activity coefficients (γ). Thus, eqn (4) can be written as eqn (6) when the definition of activity coefficient is used instead of fugacities.35
 
fIi = fIIi (4)
 
yiPtotal = xiγiPi (5)
 
xIiγIi = xIIiγIIi (6)
Where fi = fugacity of component i, yi = vapor phase mole fraction of component i, xi = liquid phase mole fraction of component i, γi = activity coefficient of component i, Ptotal = total pressure of the system, and Pi = vapor pressure of pure component i. In this work, the vapor pressure of pure components was obtained from extended Antoine correlations eqn (S5). Parameters for extended Antoine correlation for MeOH, DMC, and H2O were obtained from ASPEN software, while these parameters were regressed for [Emim][MeSO3]. The resulting regression is shown in Fig. S1, while the parameters are in Table S2.

3.2 Non-random two liquids (NRTL)

The non-random two liquids (NRTL)21 is a popular model base on activity coefficients that has been successfully used to model phase equilibria of mixtures involving ILs.17,18 The NRTL uses two parameters per binary system, which describe the interaction between these two molecules. These parameters are regressed from phase equilibrium data. In addition, NRTL has so-called “non-randomness” parameter (α), which is set to a constant value for each component pair or regressed from data. The general form of the NRTL model is shown in eqn (7). In this work, NRTL modeling was performed in ASPEN V14, which uses NRTL correlation as defined in eqn (7)–(12).36
 
image file: d5cp02239h-t3.tif(7)
 
Gij = exp(−αijτij) (8)
 
image file: d5cp02239h-t4.tif(9)
 
αij = cij + dij(T − 273.15 K) (10)
 
τii = 0 (11)
 
Gii = 1 (12)

The parameters for the NRTL model are typically regressed from binary phase equilibria data, and in the absence of such data, parameters can be obtained from ternary phase equilibrium data. In this work, we regressed NRTL parameters using binary and ternary phase equilibrium data while NRTL parameters fitted to binary data were used as a initial guesses. This way, parameters can describe binary and ternary systems. We used an objective function called “maximum likelihood”, which is described in detail in the ASPEN V14 help.36 During the regression, we fixed the α parameters according to the literature.21 Specifically, α was fixed to 0.2 for binary mixtures which showed LLE behavior, and to 0.3 otherwise. We also evaluated the consistency of NRTL parameters to describe LLE according to the literature.37,38

3.3 COnductor-like Screening Model for Real Solvent (COSMO-RS)

The COnductor-like Screening Model for Real Solvent (COSMO-RS) is a quantum chemistry approach for predicting phase equilibria.22,24,39 The main advantage of COSMO-RS is its predictive ability. The details of COSMO-RS theory are presented in the literature.23 In COSMO-RS, the polarity of molecules in the fluid-like phase is calculated around the molecule's surface, and this polarity is represented as charged surface segments that interact pairwise. The phase equilibria are calculated from statistical thermodynamics using these segments. These segments are represented as charge density, which is represented in a histogram called “σ-profile” Fig. 1. The COSMO-RS model is shown in eqn (13)–(19).40
image file: d5cp02239h-f1.tif
Fig. 1 The unnormalized σ-profiles for H2O, MeOH, [Emim]–cation, DMC, and [MeSO3]–anion. The c0 and c1 are lowest and second lowest energy conformation of molecule.

The σ-profile can be calculated for mixtures, as shown in eqn (13).

 
image file: d5cp02239h-t5.tif(13)

Electrostatics (Emisfit) and hydrogen bonding (EHB) molecular interactions are described by using interaction surface segments σ and σ′ or σacceptor and σdonor. The van der Waals interaction is described in more approximate way. The energetic contribution of these interactions are calculated as showed in eqn (14)–(16).

 
image file: d5cp02239h-t6.tif(14)
 
image file: d5cp02239h-t7.tif(15)
 
EHB = aeffcHBmin(0;min(0;σdonor + σHB)max(0;σacceptor + σHB)) (16)
where aeff = effective contact area, α′ = an interaction parameter, cHB = the hydrogen bond strength, τvdW = an elements specific vdW interaction parameter, σHB = the cut of hydrogen bonding. The chemical potential is a key thermodynamic quantity regarding phase equilibrium which can be calculated for the solvent from ps(σ) according to eqn (17).
 
image file: d5cp02239h-t8.tif(17)

The μs(σ), referred to as “σ-potential”, describes the affinity of the solvent S towards a given surface polarity σ. Interactions are modelled pairwise, thus the term (Ps(σ′)) describes the distribution of surface charge polarities that come into contact with surface charge polarities of solvent (Ps(σ)). The μs(σ′) is the chemical potential of contacting surface segments σ′. The factor aeff represents the surface area of contacting segments. The Emisfit term represents electrostatic misfit energy between a pair of surface polarities of σ and σ′. This gives the contribution of the local interaction between σ and σ′ surface polarities originated from electrostatics. The EHB accounts for the additional stabilization due to hydrogen bonding, which arises when two strongly and opposite surface polarities contact and is not included in Emisfit. Thus, the μs(σ) is computed taking into account the chemical potential of the environment, the distribution of surface polarities and pairwise electrostatic and hydrogen-bond interactions between surface polarities. The van der Waals interaction can be added to the solutions reference energy. Pseudo chemical potential of compound Xi can be determined by integrating of μs(σ) over the compound as follows.

 
image file: d5cp02239h-t9.tif(18)

In the eqn (18), the size and shape differences of the molecule in the system and volume dependent term μXC,S are taken account. From σ-potential, the activity coefficient of arbitrary mixture (γXS) is calculated as in eqn (19).

 
image file: d5cp02239h-t10.tif(19)
Where μXX is the reference state of the pure compound.

Excess enthalpy of a fluid mixture (HE) can be predicted using COSMO-RS via summing the contribution of each component as shown in eqn (20)–(22).29,41

 
image file: d5cp02239h-t11.tif(20)
where HEi is excess enthalpy of component i, xi is mole fraction of component i, Hi is enthalpy of mixture, and H0i enthalpy of pure component i. COSMO-RS calculates HE from sum of hydrogen bonding (HE(HB), van der Waals HE(vdW) and electrostatic contribution (HE(MF)) to excess enthalpy (eqn (21)) which originates from microscopic interaction energies.
 
HE = HE(HB) + HE(vdW) + HE(MF) (21)

Combining eqn (20) and (21) results eqn (22).

 
image file: d5cp02239h-t12.tif(22)

Thus, COSMO-RS predicts excess enthalpy of the mixtures via molecular-level interactions present between two different molecules.

In this work, we used COSMOtherm 2024 software42 with BP_TZVP_24.ctd parameterization, while σ-profiles were obtained from the COSMObase2023 database. We chose to use σ-profiles, which were calculated using the TZVPD-FINE basis set because this predicts LLE more likely compared to the TZVP basis set.25 Here, the TZVP basis set did not predict LLE in the case of the MeOH + DMC + [Emim][MeSO3] mixture. Also, the COSMOtherm manual stated that the prediction of isobaric VLE for mixtures including ionic liquids is not feasible.41 However, COSMO-RS predictions for isobaric VLE of H2O + [Emim][MeSO3] and MeOH + [Emim][MeSO3] resulted in reasonable predictions. Thus, these isobaric predictions were analyzed in this work. Since COSMO-RS modelling was performed by modelling [Emim][MeSO3] as individual ions, the composition and activity coefficient of the COSMO-RS predictions should be converted to match the mole fraction definition usually used in the context of ILs.40,41 We performed this conversion for VLE and LLE predictions.

4. Results and discussion

4.1 Experimental binodal curves and tie line data

Experimental results for LLE for DMC + MeOH + [Emim][MeSO3] and DMC + H2O + [Emim][MeSO3] mixtures at 293.15 K and at atmospheric pressure are shown in Tables 2–4. It was observed that the LLE of DMC + MeOH + [Emim][MeSO3] mixture also included H2O, which was quantified. However, the mass fraction of H2O was small enough to consider this a ternary mixture of DMC + MeOH + [Emim][MeSO3]. The composition of one liquid phase was almost pure DMC for both mixtures. However, the composition of the second liquid phase was different. In the DMC + H2O + [Emim][MeSO3] mixture, the composition of the second phase included a wide range of H2O and [Emim][MeSO3]. Interestingly, we observed that top and bottom liquid phases were reversed for two measured tie-lines, as shown in Table 4. In the mixture of DMC + MeOH + [Emim][MeSO3], the second phase was present only with low mass fraction values for MeOH.
Table 2 Experimental binodal compositions in weight fractions for the DMC + MeOH + [Emim][MeSO3] system at T = 293.15 K and 101 kPa pressure
T/K = 293.15
DMC + MeOH + [Emim][MeSO3] DMC + H2O + [Emim][MeSO3]
WMeOH W[Emim][MeSO3] WDMC W[Emim][MeSO3]
Expanded uncertainties are: UT = 0.4 K, UP = 20 kPa and Uwi = 0.04.
0.0314 0.0624 0.978 0.013
0.0433 0.11751 0.963 0.007
0.0568 0.1967 0.273 0.713
0.0722 0.2796 0.243 0.729
0.061 0.37941 0.242 0.729
0.0523 0.47013 0.200 0.741
0.031 0.58038 0.194 0.755
0.0249 0.6002 0.184 0.745
    0.142 0.757
    0.137 0.769
    0.120 0.182
    0.118 0.140
    0.118 0.081
    0.115 0.186
    0.115 0.098
    0.106 0.273
    0.105 0.266
    0.095 0.724
    0.081 0.463
    0.080 0.376
    0.079 0.388
    0.076 0.520
    0.067 0.681
    0.065 0.654
    0.065 0.567


Table 3 Experimental tie lines compositions in weight fractions for the DMC + MeOH + H2O + [Emim][MeSO3] mixture at T = 293.15 K and 101 kPa pressure
Feed sample Top phase: DMC-rich phase Bottom phase: [Emim][MeSO3]-rich phase
W[Emim][MeSO3] WMeOH WDMC W[Emim][MeSO3] WMeOH WDMC WH2O W[Emim][MeSO3] WMeOH WDMC WH2O
Expanded uncertainties are: UwMeOH = 0.004, UwDMC = 0.048, image file: d5cp02239h-t13.tif and image file: d5cp02239h-t14.tif, UT = 0.4 K, UP = 20 kPa.
0.2674 0.0413 0.6912 0 0.0106 0.9855 0.0040 0.3961 0.0558 0.5416 0.0065
0.3220 0.0328 0.6452 0 0.0068 0.9889 0.0043 0.4763 0.0445 0.4725 0.0067
0.3777 0.0288 0.5935 0 0.0052 0.9852 0.0096 0.5066 0.0371 0.4471 0.0091
0.4422 0.0142 0.5435 0.0006 0.0022 0.9920 0.0052 0.5907 0.0180 0.3741 0.0171


Table 4 Experimental tie lines compositions in weight fractions for the DMC + H2O + [Emim][MeSO3] mixture at T = 293.15 K and 101 kPa pressure
Feed sample Top phase: DMC-rich phase Bottom phase: [Emim][MeSO3]-rich phase
WH2O WDMC W[Emim][MeSO3] WH2O WDMC W[Emim][MeSO3] WH2O WDMC W[Emim][MeSO3]
Expanded uncertainties are image file: d5cp02239h-t15.tif, UwDMC = 0.049, UwMeOH = 0.004 and image file: d5cp02239h-t16.tif, UT = 0.4 K, UP = 20 kPa.
0.1024 0.4038 0.4938 0.0056 0.9688 0.0256 0.1484 0.0978 0.7538
0.1930 0.4064 0.4006 0.0101 0.9784 0.0114 0.3010 0.0641 0.6350
0.3009 0.4020 0.2971 0.0174 0.9795 0.0031 0.4677 0.0726 0.4597
0.3974 0.4050 0.1976 0.0244 0.9721 0.0035 0.6409 0.0930 0.2661
0.0568 0.3945 0.5486 0.0017 0.9983 0 0.0850 0.1683 0.7467
0.4047 0.3926 0.2027 0.0231 0.9769 0 0.6602 0.0895 0.2503

Feed sample Top phase: [Emim][MeSO3]-rich phase Bottom phase: DMC-rich phase
WH2O WDMC W[Emim][MeSO3] WH2O WDMC W[Emim][MeSO3] WH2O WDMC W[Emim][MeSO3]
0.4968 0.3971 0.1061 0.7992 0.1058 0.0950 0.0270 0.9730 0
0.5489 0.3949 0.0562 0.8834 0.1140 0.0026 0.0287 0.9713 0


4.2 Modelling results

4.2.1 Binary mixtures. Binary phase equilibrium data were used in this work for NRTL parameter regression. Thus, the ability of NRTL and COSMO-RS was compared as a part of evaluating the modelling ability of both models. Experimental data and average absolute deviation (AAD) of boiling point temperature and liquid phase composition for VLE and LLE systems are shown in Table 5 and illustrated in Fig. 2. The NRTL model accurately described all binary phase equilibrium systems. Accuracy of NRTL was highest for VLE of mixtures not including [Emim][MeSO3], and lowest for mixtures which includes [Emim][MeSO3] and for DMC + H2O mixture. Similarly, the accuracy of COSMO-RS was highest for non-[Emim][MeSO3] including systems (except for MeOH + DMC mixture), and it has more deviation from experimental data for [Emim][MeSO3] including systems. In the case of the LLE of [Emim][MeSO3] and DMC, the experimental data suggest a marginal decrease in the DMC mole fraction with increasing temperature, although this trend may be affected by measurement uncertainty. In contrast, both NRLT and COSMO-RS predict an opposite trend. For NRTL, the deviation arises from the regression including all binary and ternary phase equilibria, which provide overall good accuracy despite this in the LLE case. COSMO-RS shows a similar but larger deviation. This model may underestimate repulsive interaction between DMC and [Emim][MeSO3] and over predicts their temperature dependence. Interestingly, COSMO-RS predictions for vapor–liquid–liquid equilibrium (VLLE) of DMC + H2O mixture were more accurate than NRTL correlation despite parameter regression. Thus, COSMO-RS could give qualitatively and, for a few mixtures, also quantitatively correct predictions for the studied binary systems.
Table 5 The accuracy of NRTL and COSMO-RS for studied binary mixtures
Mixture/system Type AAD (K) NRTL AAD (K) COSMO-RS Ref.
a image file: d5cp02239h-t17.tifb image file: d5cp02239h-t18.tifc image file: d5cp02239h-t19.tif
MeOH + H2O VLE 0.6a 0.9a 43
MeOH + DMC VLE 0.3a 2.2a 20
H2O + [Emim][MeSO3] VLE 2.7a 2.7a 20
MeOH + [Emim][MeSO3] VLE 2.5a 6.1a 20
DMC + H2O VLE 5.6a 1.6a 44
DMC + H2O LLE 0.02b 0.07b 16
DMC + [Emim][MeSO3] LLE 0.005c 0.3c 20



image file: d5cp02239h-f2.tif
Fig. 2 NRTL and COSMO-RS results for binary systems: (a) MeOH + H2O, (b) MeOH + DMC, (c) H2O + [Emim][MeSO3], (d) MeOH + [Emim][MeSO3], (e) DMC + H2O, and (f) DMC + [Emim][MeSO3].
4.2.2 Ternary liquid–liquid equilibria. LLE for DMC + H2O + [Emim][MeSO3] and DMC + MeOH + [Emim][MeSO3] mixtures are shown in Fig. 3. These were modelled using NRTL and COSMO-RS. The resulting NRTL parameter regression is shown in Table 6. The root mean square deviation (RMSD) of the NRTL model for LLE of DMC + H2O + [Emim][MeSO3] was 0.013, and for DMC + MeOH + [Emim][MeSO3] was 0.030. Thus, NRTL can model these ternary LLE with high precision. We also estimated the consistency of the NRTL parameters for both mixtures,37 which are shown in Fig. S2 and S3. According to the software used for this test,38 these parameters were consistent.
image file: d5cp02239h-f3.tif
Fig. 3 LLE diagram for DMC + H2O + [Emim][MeSO3] (a) and (b) and DMC + MeOH + [Emim][MeSO3] (c) and (d) mixtures at 293.15 K and 101.3 kPa. NRTL results are shown in (a) and (c), while COSMO-RS results are in (b) and (d).
Table 6 NRTL parameters for different mixtures in this work, τij = aij + bij/T (K)
ij aij aji bij bji α RMSD
DMC (1) + H2O (2) + [Emim][MeSO3] (3) 0.013
1–2 −2.693 −1.448 1072.812 1357.798 0.2  
1–3 15.759 −3.114 −2479.746 490.206 0.2  
2–3 −36.584 1.813 13[thin space (1/6-em)]258.792 −1533.285 0.3  
 
DMC (1) + MeOH (2) + [Emim][MeSO3] (3) + H2O (4) 0.030
1–2 28.112 −30.932 −9298.03 10[thin space (1/6-em)]722.694 0.3  
1–3 15.759 −3.114 −2479.746 490.206 0.2  
2–3 −21.044 93.461 5295.157 −28[thin space (1/6-em)]933.843 0.3  
2–4 15.048 −3.978 −4759 1208.97 0.3  


The COSMO-RS predictions were qualitatively accurate as shown in Fig. 3. For the DMC + H2O + [Emim][MeSO3] mixture, COSMO-RS could predict quantitatively that the composition of one liquid phase is almost pure DMC. COSMO-RS prediction of the second liquid phase in the range of w[Emim][MeSO3] < 0.5 was surprisingly accurate, but in the range of w[Emim][MeSO3] > 0.5, predictions started to deviate from experimental data. Despite this, COSMO-RS has a qualitatively accurate trend for the second liquid phase. COSMO-RS could only predict the ternary LLE of DMC + MeOH + [Emim][MeSO3] mixture when TZVPD-FINE parameterization was used. This parameterization is more likely to predict LLE split than the TZVP parameterization,25 which might explain this result. COSMO-RS prediction for LLE of DMC + MeOH + [Emim][MeSO3] was similar as in the case of DMC + H2O + [Emim][MeSO3] mixture. Thus, it could predict the overall shape of the LLE phase envelope, but not LLE behavior quantitatively.

4.2.3 Molecular interactions. One benefit of COSMO-RS is the ability to describe interactions at the molecular level from the chemical potential corresponding to the σ-profile (μ(σ)),23 while interactions within binary mixtures can be estimated from excess enthalpy predictions (HE).29 COSMO-RS can predict the contribution of electrostatics (HE(MF)), hydrogen bonding (HE(MF)), and van der Waals (HE(vdW)) interactions to HE, giving insight into interactions within mixtures. The screened surface charge (σ-surface) reflects the polarity of a component in a liquid-like phase. The σ-surface for each component investigated in this study is shown in Fig. 4.
image file: d5cp02239h-f4.tif
Fig. 4 The σ-surface for H2O, MeOH, DMC, [MeSO3] and [Emim]+ components. The c0 and c1 are lowest and second lowest energy conformation of molecule.

The μ(σ) plots for all studied components are shown in Fig. 5, where μ(σ) describes the affinity of a component or mixture to a specific surface polarity (σ). Values of σ in the range of σ < −0.8 e/nm2 describe the affinity towards hydrogen bond donor (HBD). The affinity towards non-polar surface charge is described in the range of −0.8 e/nm2 < σ < 0.8 e/nm2, while charge σ > 0.8 e/nm2 describes the tendency to interact with hydrogen bond acceptor (HBA). Negative μ(σ) describes a favorable interaction, whereas positive μ(σ) an unfavorable one.


image file: d5cp02239h-f5.tif
Fig. 5 Chemical potential of the σ-profile segments (a) and zoom in figure (b).

MeOH shows favorable interaction with HBD (σ < −1.75 e/nm2), slight repulsion from non-polar to HBA polarity, and favorable interactions again at σ > 2 e/nm2 polarity. This behavior suggests that the oxygen in the MeOH will interact more strongly with positively charged species (e.g., polar hydrogens) than with negatively charged ones (e.g., oxygens). The methyl group of MeOH enhances affinity for nonpolar species, as reflected by the lower μ(σ) in the nonpolar region compared to H2O.

H2O starts to have increasing affinity for both HBD and HBA at σ < −1.5 e/nm2 and σ > 1.25 e/nm2 polarity, respectively. The polarity of −1.5 e/nm2 < σ < 1.25 e/nm2 has more unfavorable interactions than in the case of MeOH. H2O interacts more strongly with HBA and almost as strongly with HBD than MeOH since H2O has two polar hydrogens and an electron-rich oxygen. At the same time, the weaker affinity for nonpolar regions is attributed to the lack of nonpolar character.

DMC has favorable interaction with HBD in the range of σ < −2 e/nm2, while DMC has slightly unfavorable interaction over the range −2 e/nm2 < σ < 1 e/nm2. The magnitude of unfavorable interactions increases in the range of σ > 1 e/nm2. DMC has a similar affinity towards non-polarity as MeOH. The μ(σ) plot can be explained by DMC's electron-rich oxygen in the carbonyl group, which can interact with HBD but has a strong repulsive interaction with HBA. The presence of two methyl groups in DMC might provide a similar affinity to non-polar character as MeOH. Thus, the LLE split between DMC and H2O may be attributed to H2O poor ability to interact with non-polar character while DMC has more favorable interaction with non-polar character. Also, H2O has stronger affinity towards HBD and HBA and DMC has unfavorable affinity towards HBA and less strong affinity towards HBD than H2O. However, MeOH contains a methyl group that increases its affinity towards non-polar character sufficiently to prevent LLE split between MeOH and DMC.

[Emim] cation has the most unfavorable affinity towards HBD (σ < −0.8 e/nm2), while affinity increases almost linearly up to σ = 0. Affinity to HBA polarity increases dramatically when σ > 2 e/nm2. This increase might be due to the positive polarity of the cation, which highly favors HBA and disfavors HBD interactions. [Emim]–cation has a polar hydrogen between two nitrogen atoms as seen in the Fig. 4, which can interact with HBA and thus amplify affinity towards HBA.

[MeSO3] anion has highly favorable interactions with HBD (σ < −0.8 e/nm2). From the HBD region, affinity decreases roughly linearly in the range of σ > −3 e/nm2. However, favorable affinity changes to unfavorable in non-polar region, and [MeSO3] anion has unfavorable interaction with HBA (σ > 0.8 e/nm2). This might be due to the sulfonate group, which has three electron-rich oxygens that can strongly interact with HBD (e.g., polar hydrogens) while disfavoring interactions with HBA (e.g., oxygens). The methyl group might increase slightly affinity towards non-polarity.

The μ(σ) plot of [Emim][MeSO3] (50[thin space (1/6-em)]:[thin space (1/6-em)]50 mixture of [Emim] cation and [MeSO3] anion) has characteristics from μ(σ) plots of anion and cation. It has favorable interactions with HBD (σ < −1.5 e/nm2) while favorable interactions with HBA occurs in more positively polar characteristics, roughly from σ > 2 e/nm2. This might indicate that [Emim][MeSO3] interacts more easily with HBD, probably through the three electron-rich oxygen atoms in the sulfonate group. Cation needs even more polar HBA for favorable interaction, indicating that [Emim] cation hydrogens are weakly polar (except one as seen in Fig. 4).

The LLE split between [Emim][MeSO3] and DMC might be due to multiple reasons. First, DMC has more unfavorable interactions with HBA than [Emim][MeSO3]. This might be due to lack of polar hydrogens in DMC while [Emim] cation has at least one polar hydrogen. Second, DMC has more favorable interactions towards non-polar character roughly in the range of −1 < σ < 0 while DMC has high amount of this polarity according the σ-profile (Fig. 1). [Emim][MeSO3] has strong affinity towards HBD and highly polar HBA. This might indicate that [Emim][MeSO3] interacts strongly with polar hydrogens presents in H2O and MeOH.

The interactions between molecules in a mixture can be estimated from HE. These predictions and the LLE envelope for DMC + H2O + [Emim][MeSO3] are shown in Fig. 6. According to HE (Fig. 6a), [Emim][MeSO3]–H2O interaction is attractive while [Emim][MeSO3]–DMC and DMC–H2O interactions are repulsive. Hydrogen bonding HE(HB) (Fig. 6c) is the key driver for the interactions. This is attractive to [Emim][MeSO3]–H2O and repulsive to H2O–DMC interactions. Electrostatic interactions HE(MF) (Fig. 6b) explains mainly the repulsive [Emim][MeSO3]–DMC interactions. The HE(vdW) only makes a minor contribution to these interactions. All interactions that COSMO-RS predicts might not be possible in reality since LLE constrains the compositions that a liquid mixture may have in phase equilibrium conditions. The hypothetical compositions in two liquid phase regions are shown using grey surface in Fig. 6–8.


image file: d5cp02239h-f6.tif
Fig. 6 Contour plot of COSMO-RS predicted excess enthalpy for H2O + DMC + [Emim][MeSO3] mixture at 293.15 K (a). The contribution of electrostatic (b), hydrogen bonding (c) and van der Waals (d) interactions to excess enthalpy. The dashed line represents 0 excess enthalpy, ■ is experimental binodal measured in this work, grey surface is LLE envelope estimated from binodal measurements.

image file: d5cp02239h-f7.tif
Fig. 7 Contour plot of COSMO-RS predicted excess enthalpy for MeOH + DMC + [Emim][MeSO3] mixture at 293.15 K (a). The contribution of electrostatic (b), hydrogen bonding (c) and van der Waals (d) interactions to excess enthalpy. Dashed line represents 0 excess enthalpy, ▲ is experimental binodal measured in this work, grey surface is LLE envelope estimated from binodal measurements.

image file: d5cp02239h-f8.tif
Fig. 8 Contour plot of COSMO-RS predicted Gibbs free energy of mixing for H2O + DMC + [Emim][MeSO3] (a) and MeOH + DMC + [Emim][MeSO3] (b) mixtures at 293.15 K. ■ is experimental bidonal for H2O + DMC + [Emim][MeSO3] mixture, ▲ is experimental bidonal for MeOH + DMC + [Emim][MeSO3] mixture, and grey surface is LLE envelope estimated from binodal measurements.

HE and the LLE envelope for DMC + MeOH + [Emim][MeSO3] are shown in Fig. 7. This predicts that [Emim][MeSO3]–MeOH has favorable interactions while [Emim][MeSO3]–DMC and MeOH–DMC have repulsive interactions. The interactions are similar with the DMC + H2O + [Emim][MeSO3] mixture, but the strength of interactions is generally lower. Hydrogen bonding HE(HB) (Fig. 7c) behavior explains mostly the favorable and unfavorable interactions, while electrostatic behavior (Fig. 7b) has a minor effect on the interactions (except for [Emim][MeSO3]–DMC interactions), and the HE(vdW) (Fig. 7d) does not have a substantial contribution. Thus, the hydrogen bonding between [Emim][MeSO3]–H2O or MeOH explains most of these interactions, while electrostatic repulsion has a significant contribution to [Emim][MeSO3]–DMC interactions.

The LLE tie lines can be defined from the surface of Gibbs energy of mixing (Gm). The contour plots of Gm for H2O + DMC + [Emim][MeSO3] and MeOH + DMC + [Emim][MeSO3] systems are displayed in the Fig. 8. For both mixtures, the Gm plots follow the trend from HE plots. This indicates that the minimum and maximum of the Gm plots originate from the interactions. Minimums are close to molar composition, where interactions are most favorable, and maximums are close to composition, where interactions are unfavorable. Molecular-level interactions can explain this behavior. μ(σ) analysis indicates that H2O and MeOH can form hydrogen bonding interactions with [Emim][MeSO3]. [Emim][MeSO3] has a strong affinity to HBD (polar hydrogens) and more polar HBA (electron-rich oxygens). At the same time, H2O and MeOH can provide both HBD and HBA. Stronger interaction with H2O might originate from two polar hydrogens. DMC has strong repulsion with HBA, while [MeSO3] anion provides electron-rich oxygens, thus explaining the strong repulsion.

5. Conclusion

In this work, ternary LLE of DMC + H2O + [Emim][MeSO3] and MeOH + DMC + [Emim][MeSO3] was measured at 293.15 K, and measurements were modelled using NRTL and COSMO-RS. Parameters for the NRTL model were regressed utilizing VLE and LLE data from binary mixtures and ternary LLE measurements involving all studied components. COSMO-RS was used to give insight into interaction at the molecular level by calculating the chemical potential corresponding to the σ-profile and predicting excess enthalpies with the contribution of electrostatic, hydrogen bonding, and van der Waals interactions. The Gibbs energy of mixing was predicted to give insight into LLE behavior.

The accuracy of NRTL was higher than COSMO-RS for modelling phase equilibria for binary mixtures, except for VLLE of the DMC + H2O mixture. NRTL also resulted in higher accuracy for modelling measured ternary LLE mixtures with RMSD values of 0.013 and 0.030 for DMC + H2O + [Emim][MeSO3] and MeOH + DMC + [Emim][MeSO3] mixtures, respectively. COSMO-RS was able to predict ternary LLE qualitatively and partly with quantitative accuracy.

The COSMO-RS can provide detailed insight into molecular-level interactions. According to the calculated chemical potential corresponding to the σ-profile, [Emim][MeSO3] has a high affinity towards hydrogen bond donors (HBD) and can have high affinity towards hydrogen bond acceptors (HBA), if polarity is high enough. This can be explained by three electron-rich oxygens in [MeSO3] anion and polar hydrogen in [Emim] cation. DMC exhibits unfavorable interactions with HBA, which can be explained by the lack of polar hydrogens. Both H2O and MeOH have an affinity towards HBD and HBA, while H2O has a stronger affinity towards HBA due to its two polar hydrogens. The predicted excess enthalpy indicates that [Emim][MeSO3]–H2O and [Emim][MeSO3]–MeOH have favorable interactions where the hydrogen bonding contribution is the main driver for interactions. The unfavorable [Emim][MeSO3]–DMC was explained from electrostatic repulsion, which can be connected to repulsion between [MeSO3] anion and DMC oxygens. The calculated Gibbs energy of mixing indicated that these interactions significantly contribute to LLE behavior.

Author contributions

Juho-Pekka Laakso: conceptualization, methodology, investigation, writing – original draft, writing – review & editing. Behnaz Asadzadeh: conceptualization, methodology, validation, writing – original draft, writing – review & editing. Petri Uusi-Kyyny: conceptualization, writing – review & editing, funding, acquisition. Ville Alopaeus: supervision, writing – review & editing.

Conflicts of interest

The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.

List of symbols

Abbrevitations

CASChemical Abstract Service
H2OWater
DMCDimethyl carbonate
[Emim][MeSO3]1-Ethyl-3-methylimidazolium methanesulfonate
LLELiquid–liquid equilibrium
VLEVapor–liquid equilibrium
VLLEVapor–liquid–liquid equilibrium
NRTLNon-random two-liquid
COSMO-RSConductor-like Screening Model
CO2Carbon dioxide
ILIonic liquid
HBAHydrogen bonding acceptor
HBDHydrogen bonding donor
TZVPTriple-zeta valence polarization
TZVPD-FINETriple-zeta valence with polarization and diffuse functions
RMSDRoot mean square deviation
SO3Sulfonate group
AADAverage absolute deviation

Symbols

FResponse factor
ASurface area of gas chromatography signal
mMass
ucCombined uncertainty
UCombined expanded uncertainty
fFunction
fFugacity
yMole fraction of vapor phase
xMole fraction of liquid phase
γActivity coefficient
PPressure
nNumber of measurements
αNon-randomness constant for binary ij interactions in NRTL model
τ, a, b, c, d, e, f, GDimensionless interaction parameters in NRTL model
P(σ)Sigma profile
ASurface area of molecule
EmisfitEnergy component for misfit interactions
EvdWEnergy component for van der Waals interactions
EHBEnergy component for hydrogen bonding interactions
σSurface polarization charge density for a molecule
αEffective interaction parameter or scaling factor for damping polar interactions
aeffEffective surface area in COSMO-RS model
τvdWParameter related to van der Waals damping factor for interactions
cHBCoefficient representing the strength of hydrogen bonding interactions
σdonorCharge density or potential related to the hydrogen bond donor site
σHBSigma profile specific to hydrogen bonding interactions
σacceptorCharge density or potential related to the hydrogen bond acceptor site
μs(σ)Chemical potential specific to surface segment for a solvent
RUniversal gas constant
TTemperature
μ(σ)Chemical potential specific to surface segment
HETotal excess enthalpy
HE(vdW)Contribution of van der Waals interaction to excess enthalpy
HE(MF)Contribution of misfit (electrostatic) interactions to excess enthalpy
HE(HB)Contribution of hydrogen bonding to excess enthalpy
GmGibbs energy of mixing
wWeight fraction
c0Conformation of a molecule structure at the lowest energy level
c1Conformation of a molecule structure at a second lowest energy level

Subscript

iComponent i
jComponent j
sSolvent

Data availability

The data supporting this article have been included as part of the SI. The supplementary information file includes the settings for Agilent 7890B gas chromatography, the equations for calculating the uncertainty of measurements, the vapor pressure correlation for [Emim][MeSO3] and the results of NRTL consistency tests. See DOI: https://doi.org/10.1039/d5cp02239h.

Acknowledgements

This work was supported by Academy of Finland, project “in situ equilibrium shifting in CO2 utilization reactions by novel absorbents (CO2 shift)” project number 351113. The authors wish to acknowledge CSC – IT Center for Science, Finland, for computational resources.

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