A new application of the traditional Fenton process to gold cyanide synthesis using acetonitrile as a cyanide source

Wuzhong Yia, Xiaoqing Yanb, Renhong Li*ab, Jian-Qiang Wangc, Shihui Zoua, Liping Xiaoa, Hisayoshi Kobayashid and Jie Fan*a
aKey Lab of Applied Chemistry of Zhejiang Province, Department of Chemistry, Zhejiang University, Hangzhou 310027, China. E-mail: jfan@zju.edu.cn
bKey Lab of Advanced Textile Materials and Manufacturing Technology, Ministry of Education of China, Zhejiang Sci-Tech University, Hangzhou 310018, China. E-mail: lirenhong@zju.edu.cn
cShanghai Synchrotron Radiation Facility, Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Shanghai 201204, China
dDepartment of Chemistry and Materials Technology, Kyoto Institute of Technology, Matsugasaki, Sakyo-ku, Kyoto, Japan

Received 13th January 2016 , Accepted 26th January 2016

First published on 28th January 2016


Abstract

Previous cyanation processes always involved the use of hypertoxic CN ions or UV-light, which is health-risky and energy-wasting. For the purpose of environment-friendly chemistry, we introduced a general Fenton-reaction synthesis of metal cyanide solids using acetonitrile as a green cyanide source. This Fenton-improved cyanation method gets rid of CN ions and UV-light efficiently, which is green and facile.


Metal cyanides (MCs) have a variety of applications in many industrially important processes, such as metallurgy, electroplating, plastics, medicine, pesticides, dyeing, and rubber manufacturing.1–5 The conventional preparation of MCs,6–11 however, always utilize highly toxic NaCN, KCN or HCN as cyanide sources,12 which could potentially threaten humans and the environment even when handled with extreme caution. For the purpose of green chemistry, efforts have been made to find alternative hypotoxic cyanide sources and green ways to produce MCs. Radical-involved cyaniding processes thus came into being.13,14 The radical-involved processes replace CN with ˙CN, which not only exclude the toxicity from free cyanide anions, but greatly enrich the cyanide sources, such as acetonitrile (MeCN).

MeCN is conventionally treated as an inert cyanating agent because of its stable C–CN bond (133 kcal mol−1) and has been widely used as polar aprotic solvent in organic synthesis and purification.15,16 However, our recently publications showed that a photo-induced hydroxyl radical (˙OH) is able to activate the C–CN bond of MeCN to make it a good cyanide source for the production of MCs.13 Combining electron paramagnetic resonance (EPR) experiments with DFT calculations, we find that the hydroxyl radical (˙OH) is likely to be the initiator of this photo-assisted cyanation process. It could initiate the reaction in two reasonable pathways. (I) ˙OH would abstract one H atom from MeCN to yield a ˙CH2CN intermediate, and ˙CN would be produced during the chain propagation process. AuCN would be formed through the combination of ˙CN radicals and AuNPs. (II) ˙OH would attack AuNPs directly to form AuOH intermediates, which would react with nitrile to yield AuCN. ˙OH is indispensable in both reaction routes. To rule out the possible effect of UV irradiation and further identify the role of ˙OH, a UV-absent process to produce ˙OH is desired, which drew our attention to Fenton’s reagent.

Fenton’s reagent, an aqueous mixture of Fe2+ and H2O2, is believed to function as an oxidizing agent through the formation of ˙OH (Fe2+ + H2O2 → Fe3+ + ˙OH + OH).17–19 The strong oxidizing ability of ˙OH makes it a powerful agent in the treatment of toxic organic pollutants including benzene, nitrobenzene and phenols.20–23 While efforts have been made to improve the performance of Fenton’s reagent for the degradation of organic pollutants, applications of Fenton’s reagent in other aspects are rare, especially in non-aqueous systems.

In this paper, Fenton’s reagent is adopted as an ˙OH source to conduct the cyanation of metal nanoparticles. The controllable production of ˙OH as well as the simple and mild reaction conditions make it a perfect tool to investigate the role of ˙OH in the cyanation process. The experimental results indicate that this Fenton-improved cyanation (FIC) method could effectively exclude the toxicity from free cyanide anions. Compared to our previously reported photo-assisted cyanation process, the FIC process avoids the use of UV-irradiation and is thus more energy-saving and more feasible for the large-scale industrial production of MCs. Unlike traditional Fenton processes, which are usually conducted in acidic aqueous solution, the FIC process takes place in MeCN solution, which provides a possibility for Fenton’s reagent to be used in organic synthesis.

In our previous publication, ˙OH radicals were generated in solution through UV-assisted autoxidation of benzaldehyde. The complex mechanism, uncontrollable radical composition and concentration limited our basic understanding of the intrinsic activity of ˙OH radicals in the cyanation of AuNPs, although EPR experiments and DFT calculations provided us with a qualitative description. Benefiting from the well-investigated Fenton process,24–26 herein, the concentration of ˙OH radical is tuned by adjusting the dosage of Fe2+. Typically, ˙OH radicals were produced by mixing 200 μl of 30% H2O2 with X mg of FeSO4·7H2O (X = 0, 1, 2, 5, 10, 50) in 4 mL of MeCN under air under stirring at 30 °C. 60 mg of 5.0 wt% AuNPs/SiO2 was added into the solution as the reaction substrate. After reacting for several hours, the solid product was obtained by centrifuging and washing twice with deionized water before drying in a vacuum oven at 60 °C overnight and X-ray diffraction was employed to determine the conversion of Au to AuCN. The control experiments suggest that the conversion could take place only in the presence of both FeSO4·7H2O and H2O2, implying the indispensable role of the ˙OH radical. Besides, the complete cyanation of 60 mg of 5.0 wt% AuNPs/SiO2 could be achieved within 4 h only if the addition of FeSO4·7H2O was above 10 mg. The diffraction peaks at 2θ = 17.4°, 30.4°, 35.3°, 47.3°, 53.4°, 57.2° and 63.2° could be well indexed to the (001), (100), (002), (102), (110), (111) and (200) plane reflections of a hexagonal AuCN crystal (JCPDS card number: 11-0307). When the addition of FeSO4·7H2O is below 10 mg, visible peaks at 2θ = 38.1°, 44.4° and 64.6°, corresponding to (111), (200), and (220) of Au (JCPDS: 04-0784) are detected, suggesting the presence of unreacted Au. The gradually disappearing Au peaks shown in Fig. 1a, along with the decreased time for the complete conversion of AuNPs to AuCN (Fig. 1b), indicating that the cyanation reaction rate is determined by the amount of FeSO4·7H2O, i.e. the concentration of ˙OH. It is surprising to find that no other by-products, such as Fe7(CN)18 (Prussian blue), have been observed in the FIC reaction system despite the presence of a large amount of iron salts (Fig. S1). This observation indirectly excludes the existence of toxic CN anions in our reaction system and argues for the radical nature of the FIC process. Besides, only CO2 and O2 were detected via GC-TCD in the gas-phase of the FIC system, which further confirmed the green nature of the FIC method.


image file: c6ra01025c-f1.tif
Fig. 1 (a) XRD patterns of the solid products obtained using the FIC method after a 4 h reaction with different dosages of FeSO4·7H2O and (b) the required time for the full conversion of AuNPs to AuCN with the corresponding FeSO4·7H2O addition.

The radical reaction nature of the FIC system was further verified via the in situ room-temperature electron paramagnetic resonance (EPR) spin-trapping technique. As shown in Fig. S2, only one group in the EPR signal (black squares) emerged from the quaternary system containing the DMPO spin-trapping reagent, H2O2, Fe2+ and the MeCN solvent, and was made of hydroxyl radicals (DMPO–˙OH, αN = αβH = 12.5 G). In contrast to the system without AuNPs, the present reaction system exhibited two groups with weak EPR signals, which can be ascribed to DMPO–˙CN (black dots) and DMPO–˙H (black triangle) species at the beginning. However, these weak signals quickly disappeared within just one minute, which is greatly different from the photo-assisted cyanation process with ˙CN radicals all along the reaction. Two causes may count for this difference: (I) compared with the photo-assisted cyanation process, the FIC process is milder, leading to a lower ˙CN concentration which is hard to detect; (II) without the assistance of UV-light, it is difficult to cleave the C–C bond in MeCN to release ˙CN under the attack of ˙OH directly. Namely, this FIC process prefers to undergo the pathway with the AuOH intermediate rather than the pathway with the ˙CN intermediate.

The reaction process was monitored by detecting the solid product at different reaction times (Fig. S3). The reaction extent of Au to AuCN is determined via XRD where the variation of the Au/AuCN ratio suggests the conversion. Consistent with this, the colour of the suspension changes from wine red to grass green, as shown in Fig. S4. On the other hand, the plasmon band for the AuNPs initially centred at 558 cm−1 blue-shifts to 542 cm−1 in the first 10 min, which correlates mostly with the size decrease of the AuNPs. As the time went on, more AuNPs were transformed to AuCN, which has a visible absorption band centered at 592 cm−1, resulting in a red-shift.

Meanwhile, a notable shape transition can be seen over the period of the cyanation process. Before reaction, the AuNPs are smooth spheres supported on silica, presenting rounded edges (Fig. S5). After 0.5 h of reaction, these rounded edges become rough with some tiny grains around the AuNPs under the attack of the ˙OH and/or ˙CN radicals. These grains are undoubtedly AuCN oligomers owing to the appearance of their corresponding XRD peaks and the remarkable colour change (Fig. S4). As a function of the reaction time, all AuNPs are cleaved into small clusters and gradually changed to AuCN oligomers. However, it is hard to obtain the lattice fringes of AuCN oligomers owing to their easy reduction under a strong electron beam.

It is reported that ˙OH in Fenton’s reagent could quickly dissolve gold from a mechanically polished gold surface to give a much smoother surface.27 Coupling this with the TEM results, we assumed that this FIC process was a surface attacking reaction, and thus the particle size may heavily affect the FIC reaction rate. To confirm this, AuNPs of 9.5 nm and 13.3 nm obtained upon calcination at 600 °C and 800 °C, respectively, were used for tests. The former fully converted to AuCN within 6 h, 2 h longer than for 5.7 nm AuNPs obtained upon calcination at 450 °C. However, the AuNPs of 13.3 nm only could be partially transformed even after 24 h of reaction with a size of unreacted AuNPs larger than 20 nm. The results of the size-dependence experiments implied that this FIC process was a size sensitive reaction: the AuNPs with a size smaller than 10 nm could be transformed to AuCN at a fast rate while the AuNPs over 20 nm transformed at a very slow rate.

The FT-IR analysis provides us with more information on the order and connectivity within MC chains. As shown in Fig. 2a, only one band (2230 cm−1) corresponding to the stretching vibration of the C[triple bond, length as m-dash]N bond (νC[triple bond, length as m-dash]N) in the wavenumber range of 2400 to 2100 cm−1 is found, demonstrating that the as-produced AuCN is only comprised of Au⋯CN⋯Au chains without the presence of Fe⋯CN for which νC[triple bond, length as m-dash]N is centred at 2070 cm−1.9,28 The existence of a single C[triple bond, length as m-dash]N environment in the compound is further confirmed via the observation of only one νAu–CN stretching frequency, which occurs at 669 cm−1. Meanwhile, XPS and ICP-AES analyses were also adopted to detect the content of iron in a washed AuCN sample, and only a negligible amount of iron was observed, further ensuring the purity of the as prepared AuCN. In addition, compared with AuNPs, the Au 4f XPS binding energies of the AuCN samples shift from 87.7 to 88.9 eV for the Au 4f5/2 signals and from 84.1 to 85.3 eV for the Au 4f7/2 signals (Fig. 2b). The 1.2 eV up-shift of the Au 4f peaks as well as the appearance of the N 1s peak (Fig. 2b, inset) further confirm the formation of AuCN species.


image file: c6ra01025c-f2.tif
Fig. 2 (a) FT-IR spectra and (b) XPS of the Au 4f and N 1s (inset) peaks of Au/SiO2 and AuCN/SiO2 obtained via the FIC process.

The unique structure of as-prepared AuCN was further demonstrated using extended X-ray absorption fine structure (EXAFS) and X-ray absorption near edge structure (XANES) analyses. As displayed in Fig. 3a, the XANES spectra indicate that Au is oxidized based on the intensity of the “white line” at 11[thin space (1/6-em)]924 eV compared with Au foil, which is in consistent with the XPS results. In the Fourier transforms (r space) of the EXAFS data for AuCN (Fig. 3b), there is one prominent peak at ∼1.56 Å from the Au–C/N contribution. The other two peaks at ∼2.25 Å and ∼2.61 Å are from the Au–Au contribution, as also revealed in Au foil. The best fit for the fine structure indicates that the average coordination number is ca. 2.4 for the Au–C/N model at a distance of 1.96 Å, and ca. 3.9 for the Au–C–N or Au–N–C models at 3.14 Å (Table S1).


image file: c6ra01025c-f3.tif
Fig. 3 (a) XANES patterns and (b) Fourier transforms (r space) of the EXAFS analysis.

The similarity between Fenton-like reagents (a mixture of other transition metal ions with H2O2) and Fenton’s reagent further enlarges the possibilities of our FIC process. Utilizing Cu2+/H2O2 as a ˙OH provider, we successfully prepared AuxCu1−xCN (0.5 ≤ x ≤ 1, the x value depends on the concentration of Cu2+ and the reaction time). It is interesting that no CuCN phase was detected via XRD and FT-IR characterization in our sample (Fig. S6). In addition, the fact that only one νC[triple bond, length as m-dash]N frequency at 2210 cm−1 is observed in the FT-IR spectrum indicates the strict alternation of the metal atoms, i.e., Au⋯Cu⋯Au⋯Cu, together with cyanide ordering.9 It is likely that partial Cu2+ was reduced to Cu0 NPs by H2O2,29 which coupled with ˙CN and inserted into AuCN chains to form AuxCu1−xCN. A 10 h reaction between 17 mg of Cu(NO3)2·3H2O, 200 μl of H2O2 and 60 mg of 5 wt% AuNPs/SiO2 produced a substrate formulated as Au0.5Cu0.5CN, the XRD peaks of which (2 theta = 17.9, 30.2, 35.4, 36.2, 47.8, 53.9, and 57.2) matched well with the reference.9 AgCN and AuxAg1−xCN can also be obtained by wholly or partially replacing AuNPs with AgNPs or AgNO3 (Fig. S7).

In summary, we have demonstrated a simple way to synthesize metal cyanides and mixed metal cyanides. By using Fenton’s reagent and acetonitrile, harmful UV-light and toxic cyanide ions can be avoided efficiently, making it feasible for the large-scale industrial production of MCs. Besides, the important role that ˙OH played in the cyanation process was identified without the effects of UV-light, and provided an efficient proof for our hypothesis in photo-assisted cyanation. It is the first time that the conventional Fenton reagent was utilized in the synthesis of metal cyanides, opening a door for the application of Fenton’s reagent in synthetic chemistry. Furthermore, this facile green method provides a possibility to replace conventional metallurgical technology.

The XAFS research described in this paper was performed at the HXMA beamline of the CLS, which is supported by the CFI, NSERC, NRC, CIHR, the University of Saskatchewan, the Government of Saskatchewan, and Western Economic Diversification Canada. We are grateful for the financial support from the NSFC (21222307, 21373181, 21403197 and 21503189), the Fundamental Research Funds for the Central Universities (2014XZZX003-02), Zhejiang Provincial Natural Science Foundation of China (LY15B030009), and the China Postdoctoral Science Foundation (2014M550333 and 2015T80636).

Notes and references

  1. M. J. Katz, K. Sakai and D. B. Leznoff, Chem. Soc. Rev., 2008, 37, 1884–1895 RSC.
  2. O. S. Wenger, Chem. Rev., 2013, 113, 3686–3733 CrossRef CAS PubMed.
  3. X. Roy, L. K. Thompson, N. Coombs and M. J. MacLachlan, Angew. Chem., 2008, 47, 511–514 CrossRef CAS PubMed.
  4. T. D. Harris, C. Coulon, R. Clerac and J. R. Long, J. Am. Chem. Soc., 2011, 133, 123–130 CrossRef CAS PubMed.
  5. C. F. Shaw, Chem. Rev., 1999, 99, 2589–2600 CrossRef CAS.
  6. R. S. Bradley, D. C. Munro and P. N. Spencer, Trans. Faraday Soc., 1969, 65, 1920–1926 RSC.
  7. H. J. Barber, A. Schonberg and A. Mustafa, J. Chem. Soc., 1943, 79–80 RSC.
  8. Q. Fu, H. Saltsburg and M. Flytzani-Stephanopoulos, Science, 2003, 301, 935–938 CrossRef CAS PubMed.
  9. A. M. Chippindale, S. J. Hibble, E. J. Bilbe, E. Marelli, A. C. Hannon, C. Allain, R. Pansu and F. Hartl, J. Am. Chem. Soc., 2012, 134, 16387–16400 CrossRef CAS PubMed.
  10. S. Kroeker, R. E. Wasylishen and J. V. Hanna, J. Am. Chem. Soc., 1999, 121, 1582–1590 CrossRef CAS.
  11. M. Schrinner, M. Ballauff, Y. Talmon, Y. Kauffmann, J. Thun, M. Moller and J. Breu, Science, 2009, 323, 617–620 CrossRef CAS PubMed.
  12. T. F. Huzar, T. George and J. M. Cross, Expert Rev. Respir. Med., 2013, 7, 159–170 CrossRef CAS PubMed.
  13. R. H. Li, H. Kobayashi, J. W. Tong, X. Q. Yan, Y. Tang, S. H. Zou, J. B. Jin, W. Z. Yi and J. Fan, J. Am. Chem. Soc., 2012, 134, 18286–18294 CrossRef CAS PubMed.
  14. S. Zou, R. Li, H. Kobayashi, J. Liu and J. Fan, Chem. Commun., 2013, 49, 1906–1908 RSC.
  15. J. Kim, H. J. Kim and S. Chang, Angew. Chem., 2012, 51, 11948–11959 CrossRef CAS PubMed.
  16. D. S. Marlin, M. M. Olmstead and P. K. Mascharak, Angew. Chem., 2001, 40, 4752–4754 CrossRef CAS.
  17. H. J. H. Fenton, J. Chem. Soc., Trans., 1894, 65, 899–910 RSC.
  18. F. Haber and J. Weiss, Proc. R. Soc. London, Ser. A, 1934, 147, 332–351 CrossRef CAS.
  19. C. Walling, Acc. Chem. Res., 1975, 8, 125–131 CrossRef CAS.
  20. I. Hua and M. R. Hoffmann, Environ. Sci. Technol., 1997, 31, 2237–2243 CrossRef CAS.
  21. B. N. Aronstein, R. A. Lawal and A. Maka, Environ. Toxicol. Chem., 1994, 13, 1719–1726 CrossRef CAS.
  22. E. Brillas, I. Sires and M. A. Oturan, Chem. Rev., 2009, 109, 6570–6631 CrossRef CAS PubMed.
  23. A. D. Bokare and W. Choi, J. Hazard. Mater., 2014, 275, 121–135 CrossRef CAS PubMed.
  24. M. S. Lucas and J. A. Peres, Dyes Pigm., 2006, 71, 236–244 CrossRef CAS.
  25. Y. W. Kang and K.-Y. Hwang, Water Res., 2000, 34, 2786–2790 CrossRef CAS.
  26. A. Babuponnusami and K. Muthukumar, J. Environ. Chem. Eng., 2014, 2, 557–572 CrossRef CAS.
  27. A. M. Nowicka, U. Hasse, M. Hermes and F. Scholz, Angew. Chem., 2010, 49, 1061–1063 CrossRef CAS PubMed.
  28. P. J. Kulesza, M. A. Malik, A. Denca and J. Strojek, Anal. Chem., 1996, 68, 2442–2446 CrossRef CAS.
  29. X. Liao, R. Li, Z. Li, X. Sun, Z. Wang and J. Liu, New J. Chem., 2015, 39, 5240–5248 RSC.

Footnote

Electronic supplementary information (ESI) available: Details of experimental procedures of preparation and characterization of catalysts and catalytic data. See DOI: 10.1039/c5ra01025c

This journal is © The Royal Society of Chemistry 2016
Click here to see how this site uses Cookies. View our privacy policy here.