Cristina
Antuña-Nieto
,
Elena
Rodríguez
,
M. Antonia
López-Antón
,
Roberto
García
* and
M. Rosa
Martínez-Tarazona
Instituto de Ciencia y Tecnología del Carbono, INCAR-CSIC, C/Francisco Pintado Fe, 26, 33011 Oviedo, Spain. E-mail: robo@incar.csic.es; Fax: +34 985 297662; Tel: +34 985 119090
First published on 25th June 2020
Mercury has been the focus of environmental concern and scientific research for decades due to the risks associated with its use, release and emission. An international agreement established in 2017 during the UN Minamata Convention highlighted the need for innovative approaches and technology to tackle these problems. The use of regenerable sorbents for mercury removal in the gas phase is a possible solution that can avoid the generation of new mercury-contaminated waste. However, to make significant progress in this field, it is necessary to develop efficient, economic and environmentally friendly sorbents, for which, a good understanding of the mechanism of adsorption in this type of process is needed. In this study, several kinetic models were applied to determine the rate-controlling step in the adsorption process of elemental mercury by regenerable sorbents based on gold. Three diffusional models (Weber and Morris, Bangham and pseudo-first order models) and two adsorptive models (pseudo-second order and Elovich models) were tested. The results of this study show that external diffusion from the gaseous phase to the sorbent particles is the rate-limiting step. The complexity of the process is also reflected in the results obtained, which indicate that pore diffusion plays a significant role over most of the mass transfer zone, while adsorption itself becomes determinant only when the saturation of the sorbent is near.
Presumably, significant cuts in CO2 emissions will be reached by 2050, due to energy policies and the application of carbon capture and storage (CCS) strategies.2 In such CCS technologies, the presence of elemental mercury (Hg0) in gases enriched in CO2 is not only an environmental risk but also a technological problem: it needs to be controlled in the compression stage,3 which is carried out, in many cases, in cryogenic aluminum plate fin exchangers. If the Hg0 reaches these heat exchangers, it can form an amalgam with Al, which may cause deterioration or even destruction of the installation. The final part of the CCS process, the storage of CO2 in geological environments, is also negatively affected by the presence of Hg, not only due to the reduction of the volume occupied by CO2, but also as a result of some chemical reactions that could decrease its injectivity.4
Hg0 is significantly difficult to capture even by using the most advanced technologies already developed for industrial gases. This problem is being addressed through the development of specific sorbents.5–7 By using regenerable sorbents, the mercury that is retained may be desorbed and condensed to be confined and isolated. The sorbents studied so far for this purpose are mainly metal oxides and porous solids impregnated with noble metals such as gold, silver, palladium and platinum.8–16
The sorbents based on metal oxides have the ability to capture mercury and other trace elements at high temperatures (200–400 °C), and have even been tested for the retention of toxic metals in gasification processes.17,18 Studies carried out with regenerable sorbents based on manganese oxide showed a good capability for mercury capture up to 300 °C and were completely regenerated at 500 °C.14 No decrease in mercury retention capacity over repeated cycles of mercury adsorption/desorption was observed. Metal oxides and composites have also been evaluated as regenerable sorbents for the treatment of gaseous steams generated in industrial processes such as energy generation or non-ferrous metal smelting.15,16 They capture elemental mercury by catalytic oxidation and adsorption with great efficiency and can be regenerated by thermal decomposition.
On the other hand, the regenerable materials loaded with noble metals (Au, Ag, Cu, Pd or Pt),8,11,14,19–21 are able to retain elemental mercury by amalgamation between the metal and the mercury, both in an elemental state.9,10,22 Subsequently, the amalgam can be decomposed by heating at 450 °C to detach and recover the mercury, leaving the sorbent ready for the next adsorption cycle.
Regenerable sorbents based on activated carbon foams impregnated with nanodispersed gold, developed and tested for gaseous Hg0 capture, are the focus of this work.23 Activated carbon foams offer enhanced mechanical strength and easy manageability, which makes it possible to manufacture carbon structures of any monolithic shape. Furthermore, the physical and chemical characteristics of their surfaces can be modified to meet the needs of any particular industrial adsorption process.
The adsorption process surely depends on the capacity of sorbents to retain pollutants, but also on the adsorption kinetics.24–27 A number of kinetic models have been studied to describe heavy metal adsorption processes, mainly from the liquid phase,28,29 and most of them by means of batch experiments. Pseudo-first-order, pseudo-second-order and Elovich equations have been used most often.30–35
There is only a limited amount of information available in the literature on the adsorption kinetics of gas-phase mercury,26,36 and the pseudo-second order model appears to be the most accurate to describe the process, indicating the rate-limiting influence of the adsorption itself; however, the good behaviour of other models suggests that the whole process is complex, and that the diffusion of the sorbate to and into the sorbent may also pose a significant influence.
This study attempts to improve the current level of understanding of the adsorption of elemental mercury in a new kind of sorbent, by applying several simplified kinetic models, namely Weber and Morris (intraparticle diffusion), Bangham, pseudo-first order, pseudo-second order and Elovich models. The models are applied to the experimental data obtained from the capture of Hg0 in the gas phase by adsorption with gold-impregnated activated carbon foams, which have proven to capture mercury with 100% capacity over several adsorption–desorption cycles.23
CF500 | CF800 | |
---|---|---|
Surface area (SBET, m2 g−1) | 880 | 738 |
Micro-porosity volume (VDR-N2, cm3 g−1) | 0.36 | 0.28 |
Narrow porosity volume (VDR-CO2, cm3 g−1) | 0.30 | 0.19 |
True density (ρHe, g cm−3) | 1.52 | 1.91 |
Apparent density (ρHg, g cm−3) | 0.42 | 0.31 |
Open porosity (s, %) | 72.3 | 83.7 |
Total pore volume (VHg, cm3 g−1) | 1.71 | 2.69 |
The activated carbon foams were impregnated with 1, 2, 3, 4 and 5 wt% Au, following the THPC (tetrakis(hydroxymethyl)-phosphonium chloride) method, which is based on the formation of Au colloids. The detailed procedure has been previously reported.23,38 The actual amount of Au loaded in the sorbent is determined by analysing the Au in the solution, after the foam impregnation, by inductively coupled plasma mass spectrometry (ICP-MS). The sorbents prepared with Au contents of 1 to 5 wt% were labelled CF500-1%, CF500-2%, CF500-3%, CF500-4% and CF500-5% and CF800-1%, CF800-2%, CF800-3%, CF800-4% and CF800-5%.
The average size of the Au particles in the Au-loaded carbon foams, estimated using SEM and TEM,23 increases with Au-loading, from 5 nm in CF500-1% to 23 nm in CF500-5%, and from 16 nm in CF800-1% to 116 nm in CF800-5%. The deposited Au in the surface is in its elemental state as demonstrated via XPS analysis, by the presence of two Au 4f peaks corresponding to the binding energy of metallic Au (84.0 eV and 87.7 eV) in the XPS spectrum.23 It was observed that the loading of elemental Au on the activated carbon foam does not exert a significant influence on the surface area and pore diameter of the adsorbent, as it was previously reported.39
The laboratory scale device used for the retention of Hg was described in previous works.23,39 A general schematic is depicted in Fig. 1. The gas composition used in the experiments was 80% CO2 and 20% N2, with 100 μg m−3 of Hg0 being incorporated to the gas stream. The sorbent was kept at 40–50 °C and the total volume of the gas flow through it was 500 mL min−1. Hg0 was monitored at the exit of the sorbent bed, using a continuous elemental mercury analyser (VM 3000). In the case of an eventual oxidation of elemental mercury,40,41 the Hg2+ originated would be captured with a Dowex® 1 × 8 ion exchanger resin. The total amount of Hg retained in the sorbent and the Hg2+ captured in the resin were analysed using a mercury analyser (Advanced Mercury Analyser, AMA 254).
To study the kinetics of the adsorption process, the interval taken into consideration is the mass transfer zone, beginning just at the breakthrough time (considered as zero time), when the period of 100% Hg adsorption ends. The cumulative adsorbed mercury curves in this mass transfer zone after breakthrough for the studied adsorbents are shown in Fig. 2. In general, it can be observed that an increasing concentration of Au in the adsorbent gives rise to slower adsorption rates (longer times needed for saturation) and higher amounts of Hg captured. The latter does not mean a higher capacity of the adsorbent for mercury capture, but suggests that a higher amount of Au has remained untouched in the zone of 100% adsorption (before the breakthrough point). This therefore means a lower efficiency of the sorbent. The adsorption capacity of these Au-loaded carbon foams has been studied previously by the authors,23 and has been proven to be influenced by the amount, dispersion and particle size of the elemental Au incorporated, and by the chemical nature of the carbon foam surface.
Fig. 2 Cumulative Hg0 captured by Au-impregnated carbon foams after the breakthrough time: (a) Au-loaded CF500 samples; (b) Au-loaded CF800 samples. |
Adsorption on the surface of a porous material is considered to take place via three steps:29,43,44 (i) diffusion through the fluid surrounding the solid particles to the external surface of the adsorbent, controlled by external mass transfer, (ii) diffusion through the fluid within the pores of the sorbent particles to the sorption sites, in a pore diffusion mechanism, and (iii) adsorption at the active sites on the surface of the sorbent.
The mechanism of adsorption can be described by various mathematical models, with approaches that differ according to which step is considered as the rate-limiting one. The deviation between the calculated and experimental data are expressed by correlation coefficient R2 and the sum of squares due to error (SSE), which will be used in this study for model comparison. The kinetic models may be roughly classified as diffusional and adsorption models.
qt = kidt1/2 + θ |
This model contemplates the adsorption process as controlled by external mass transfer (boundary layer diffusion) and internal pore diffusion.49 Among multiple stages of adsorption, the process can be considered as controlled by intra-particle diffusion only if the plot of qtversus t1/2 produces a straight line.45
Fig. S4 and S5 (ESI†) display the cumulative capture of Hg with different Au loadings of the carbon foams and the corresponding curves derived from the Weber and Morris model. The kinetic parameters obtained for the adsorption curves of the ten sorbents tested are listed in Tables 2 and 3. The values of R2 are rather low, revealing poor fits between the experimental curves and the theoretical ones derived from the model. The value of the constant kid, on the other hand, increases with the increasing amount of Au loaded in the carbon foams, according to the evolution of the cumulated Hg0 in the mass transfer zone.
CF500-1% | CF500-2% | CF500-3% | CF500-4% | CF500-5% | ||
---|---|---|---|---|---|---|
Weber and Morris | SSE | 1942 | 3005 | 6816 | 28830 | 281100 |
R 2 | 0.9496 | 0.9478 | 0.9359 | 0.9278 | 0.9077 | |
k id (mg g−1 min−1/2) | 3.214 | 3.912 | 4.300 | 5.006 | 9.226 | |
θ (mg g−1) | 1.509 × 10−12 | 3.439 × 10−13 | 2.742 × 10−12 | 0.000083 | 9.784 | |
Bangham | SSE | 1345 | 2956 | 6787 | 27270 | 247800 |
R 2 | 0.9651 | 0.9487 | 0.9362 | 0.9317 | 0.9186 | |
k (mg g−1 s−α) | 1.916 | 3.494 | 4.568 | 6.370 | 14.95 | |
α | 0.5989 | 0.5206 | 0.4891 | 0.4604 | 0.432 | |
Pseudo-first order | SSE | 270.4 | 313.8 | 821.6 | 1947 | 18960 |
R 2 | 0.9930 | 0.9946 | 0.9923 | 0.9951 | 0.9938 | |
q e (μg g−1) | 62.57 | 77.41 | 83.89 | 124.4 | 282.7 | |
k 1 (min−1) | 0.007006 | 0.007136 | 0.007593 | 0.004876 | 0.003669 | |
Pseudo-second order | SSE | 445.6 | 757.4 | 1918 | 6293 | 58010 |
R 2 | 0.9884 | 0.9869 | 0.9820 | 0.9842 | 0.9810 | |
q e (μg g−1) | 91.81 | 106.7 | 113.0 | 163.6 | 364.1 | |
k 2 (g μg−1 s−1) | 5.648 × 10−5 | 5.527 × 10−5 | 5.812 × 10−5 | 2.703 × 10−5 | 9.56 × 10−6 | |
Elovich | SSE | 638.7 | 1318 | 3291 | 12450 | 117800 |
R 2 | 0.9834 | 0.9771 | 0.9691 | 0.9688 | 0.9613 | |
α (μg g−1 s−1) | 0.5278 | 0.7478 | 0.9152 | 0.9310 | 1.7057 | |
β (g μg−1) | 0.0316 | 0.0300 | 0.0296 | 0.0213 | 0.0100 |
CF800-1% | CF800-2% | CF800-3% | CF800-4% | CF800-5% | ||
---|---|---|---|---|---|---|
Weber and Morris | SSE | 3311 | 4160 | 19400 | 10420 | 64260 |
R 2 | 0.9486 | 0.9410 | 0.9454 | 0.9528 | 0.9402 | |
k id (mg g−1 min−1/2) | 2.897 | 2.912 | 5.235 | 3.957 | 6.634 | |
θ (mg g−1) | 1.157 × 10−12 | 0.008725 | 2.386 × 10−10 | 7.371 × 10−8 | 3.496 × 10−9 | |
Bangham | SSE | 2142 | 3920 | 8052 | 10420 | 20970 |
R 2 | 0.9668 | 0.9444 | 0.9773 | 0.9528 | 0.9805 | |
k (mg g−1 s−α) | 1.547 | 3.632 | 2.090 | 3.933 | 2.173 | |
α | 0.6084 | 0.4630 | 0.6525 | 0.5010 | 0.6765 | |
Pseudo-first order | SSE | 356.3 | 146.1 | 1319 | 522.4 | 3903 |
R 2 | 0.9945 | 0.9979 | 0.9963 | 0.9976 | 0.9964 | |
q e (μg g−1) | 75.14 | 68.48 | 166.4 | 108.4 | 258.5 | |
k 1 (min−1) | 0.003942 | 0.005398 | 0.002625 | 0.003796 | 0.001762 | |
Pseudo-second order | SSE | 629.1 | 696.1 | 2238 | 1931 | 6102 |
R 2 | 0.9902 | 0.9901 | 0.9937 | 0.9913 | 0.9943 | |
q e (μg g−1) | 110.9 | 90.18 | 249.0 | 146.8 | 400.6 | |
k 2 (g μg−1 s−1) | 2.603 × 10−5 | 5.432 × 10−5 | 7.598 × 10−6 | 2.212 × 10−5 | 2.996 × 10−6 | |
Elovich | SSE | 937.3 | 1587 | 3218 | 4053 | 8493 |
R 2 | 0.9855 | 0.9774 | 0.9909 | 0.9816 | 0.9921 | |
α (μg g−1 s−1) | 0.3526 | 0.5694 | 0.4980 | 0.5822 | 0.5086 | |
β (g μg−1) | 0.0259 | 0.0386 | 0.0108 | 0.0225 | 0.0066 |
The plots corresponding to the linear form of the model are shown in Fig. 3. Again, the correlation coefficients (R2) obtained are low, indicating a poor description of the process of adsorption of Hg0 by the Au-loaded activated carbon foams, and that the intra-particle diffusion is hardly the adsorption rate-controlling step.
qt = ktα |
The kinetic coefficients indicate correlations slightly better than those observed with the Weber and Morris model (Tables 2 and 3). However, the plots show that the correlations are far from the experimental results (Fig. S6 and S7, ESI†). According to these results, the present Hg adsorption process is not determined by the diffusion of the adsorbate inside the sorbent particles.
The model can also be represented by a linear equation:50,51
qe = qt(1 − e−k1t) |
ln(qe − qt) = lnqe − k1t |
With this model, the estimated values of the accumulated concentration of Hg0 in the sorbents in equilibrium (qe) increases from 62.57 and 75.14 μg g−1 for CF500-1% and CF800-1%, to 282.7 and 258.5 μg g−1 for CF500-5% and CF800-5%, respectively (Tables 2 and 3). The adsorption constant provided by the model ranges from 1.762 × 10−3 s−1 (CF800-5%, Table 3) to 7.593 × 10−3 s−1 (CF500-3%, Table 2).
Fig. 5 displays the plots corresponding to the linear equation of the first-order model. They show good correlation coefficients, especially in the case of adsorbent CF800-2% (R2 = 0.9989). The correlations are similar to or better than those of the Bangham model. The correlation also becomes worse as saturation approaches. These results, together with those of the non-linear plots (Fig. S8 and S9, ESI†) indicate that the mass transfer between the adsorbate and the adsorption sites plays a significant role in the process of adsorption of Hg by Au-loaded activated carbon foams. The pseudo-first order equation accurately predicts the initial period of adsorption57–59 and, for that reason, fast Hg0 adsorption processes can be better adjusted to pseudo-first order kinetics.53
Good correlations are also obtained with this model for the experimental data (Fig. S10 and S11, ESI,† and Tables 2 and 3). However, the values of R2 are slightly lower and the values of SSE are slightly higher than those of the pseudo-first order model indicating that the latter reflects the mechanism of adsorption more accurately in this particular case.
The plots corresponding to the linear equation of the model are displayed in Fig. 6. The best match with the experimental results is that of sample CF800-2%, and the worst corresponds to CF800-1%. It is evident that the distribution of the experimental results is closer to a straight line as adsorption time increases, suggesting that the adsorption, presumably by Hg–Au amalgamation, become the limiting step as the adsorption process proceeds and approaches the saturation of the sorbent.
The non-linear and linear plots in Fig. S12 and S13 (ESI†) and Fig. 7 and the values in Tables 2 and 3 indicate a worse correlation than those observed for the pseudo-first order and the pseudo-second order models.
When the non-linear correlations are considered, the pseudo-first order and Bangham models provide the best matches, and so it is the external diffusion that controls the global adsorption process from the beginning to the point where the sorbent is saturated. The linear plots support this assertion, but they also show that: (i) the Bangham model matches the experimental results in the first stages of the process and only deviates from them when the sorbent is close to the saturation point, and (ii) the pseudo-second order model approaches the experimental results more closely in the last stages of the process, including the saturation of the sorbent. The results confirm that, although external diffusion seems to control the entire process, pore diffusion is also determinant in the initial stages, whereas adsorption acquires importance towards the end, when saturation of the sorbent is imminent.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/d0nj00898b |
This journal is © The Royal Society of Chemistry and the Centre National de la Recherche Scientifique 2020 |