Skip to main content
ACS AuthorChoice logoLink to ACS AuthorChoice
. 2016 May 9;138(21):6707–6710. doi: 10.1021/jacs.6b03187

Solar-Driven Water Oxidation and Decoupled Hydrogen Production Mediated by an Electron-Coupled-Proton Buffer

Leanne G Bloor , Renata Solarska ‡,§, Krzysztof Bienkowski §, Pawel J Kulesza , Jan Augustynski §, Mark D Symes †,*, Leroy Cronin †,*
PMCID: PMC5033397  PMID: 27159121

Abstract

graphic file with name ja-2016-03187m_0005.jpg

Solar-to-hydrogen photoelectrochemical cells (PECs) have been proposed as a means of converting sunlight into H2 fuel. However, in traditional PECs, the oxygen evolution reaction and the hydrogen evolution reaction are coupled, and so the rate of both of these is limited by the photocurrents that can be generated from the solar flux. This in turn leads to slow rates of gas evolution that favor crossover of H2 into the O2 stream and vice versa, even through ostensibly impermeable membranes such as Nafion. Herein, we show that the use of the electron-coupled-proton buffer (ECPB) H3PMo12O40 allows solar-driven O2 evolution from water to proceed at rates of over 1 mA cm–2 on WO3 photoanodes without the need for any additional electrochemical bias. No H2 is produced in the PEC, and instead H3PMo12O40 is reduced to H5PMo12O40. If the reduced ECPB is subjected to a separate electrochemical reoxidation, then H2 is produced with full overall Faradaic efficiency.


The need to develop carbon-neutral energy sources is rapidly becoming an environmental and economic imperative.1 Solar power is an especially attractive option for this purpose, as it is both abundant and widely distributed geographically.2 Solar irradiation at the earth’s surface is inherently intermittent, due to both the weather and the diurnal cycle. This means that if solar power is to be effective as a multi-terawatt power source, then ways to store this energy to use at times when the sun is not shining must be found.3

The photoassisted electrolysis of water has been studied by numerous groups as a method by which solar energy could be stored as a fuel (H2).4 However, there remain several challenges to overcome before viable and cost-effective solar-to-hydrogen photoelectrochemical cells can be realized. First, solar power is diffuse, so that low current densities (∼10 mA cm–2 has been taken as a benchmark for a 10% efficient solar-to-fuels device under 1 Sun illumination)5 are standard, and even then these current densities are highly variable. Low current densities equate to slow gas production rates, and this can lead to extensive mixing of product gases, both in devices without a headspace separator6a and even in electrolyzers where “gas-impermeable” membranes such as Nafion are employed.6b6d At one extreme, this has the potential to produce explosive H2/O2 gas mixtures. In the less extreme case, where product gas crossover is slower, hydrogen permeating to the anode side of the cell is preferentially oxidized to protons and electrons, while oxygen on the cathode side is preferentially reduced to water. While these reactions prevent the buildup of dangerous headspace compositions, they consume energy and have a detrimental effect on overall solar-to-collected-hydrogen efficiencies.6 Gas crossover can be mitigated by using thicker membranes, but this in turn reduces efficiency by introducing greater ohmic resistance in the cell.6a,6c

A second challenge in the realization of a practical solar-to-hydrogen cell is how the hydrogen itself is harvested. Assuming a current density of 10 mA cm–2 for hydrogen production5 and a target of producing 500 g of H2 gas over the course of 8 h irradiation at 1 Sun,7 then an array of area ∼17 m2 is required (see Section SI-5 in the Supporting Information (SI) for calculation). This is possible in principle (see arguments advanced in ref (3b) and a functioning PEC system described in ref (4n)), but collecting H2 from such a high surface area array may be inefficient. Production of hydrogen at a point source would make effective use of any H2 evolution catalyst and would also facilitate pressurization for storage.

We previously reported the concept of the electron-coupled-proton buffer (ECPB), whereby the water oxidation and proton reduction half-reactions of water splitting can be completely decoupled in both space and time, Figure 1.8 Taking the example of phosphomolybdate ([PMo12O40]3–) as the ECPB, this decoupling can be described by the half-reactions:

graphic file with name ja-2016-03187m_m001.jpg 1a
graphic file with name ja-2016-03187m_m002.jpg 1b
graphic file with name ja-2016-03187m_m003.jpg 2

Figure 1.

Figure 1

Use of ECPBs allows the electrolysis of water to be split into two steps both spatially and temporally. Step 1 (blue lines) is the oxidation of water concomitant with reduction of the ECPB, and step 2 (red lines) is reoxidation of the ECPB with concomitant hydrogen evolution. Previously, both steps have been driven electrochemically,8a,8b and an electrochemical step 1 followed by a catalytic release of H2 in step 2 has been demonstrated.8c Herein, we show that step 1 can be performed in a PEC, with an electrochemical step 2.

In our original work,8a both of the necessary energy inputs for eqs 1a/1b and 2 were provided purely electrochemically. However, we hypothesized that such a system would be amenable to a combined photoelectrochemical cycle, whereby eqs 1a and 1b would be driven in a PEC without a bias voltage and eq 2 would be driven electrochemically (with a bias voltage). Herein, we demonstrate the feasibility of such a system by using a WO3 photoanode in a PEC to drive the simultaneous oxidation of water to O2 and reduction of [PMo12O40]3– to [PMo12O40]5– without the need for any additional electrical bias. Current densities of over 1 mA cm–2 were achieved under simulated solar irradiation with high Faradaic efficiency for oxygen production, but without any detectable hydrogen production during irradiation (and hence no danger of the product gases mixing). The reduced phosphomolybdate could subsequently be reoxidized electrochemically to regenerate [PMo12O40]3– and produce hydrogen with full Faradaic efficiency.

A general schematic of the photoelectrochemical cell for O2 evolution and reduction of the ECPB is given in Figure 2. Tungsten trioxide was chosen as the photoanode because it is stable under the pH conditions used in this work (pH 0.1) and because its band gap straddles both water oxidation onset (ca. +1.2 V vs NHE) and the reduction potential of [PMo12O40]3– (ca. +0.6 V vs NHE)8a at this pH.9 An airtight cell was thus constructed according to Figure 2, using a 1 cm2 WO3 photoanode (prepared on an FTO substrate by a literature procedure)10 in contact with 1 M methanesulfonic acid (pH 0.1) in one compartment and phosphomolybdic acid (H3PMo12O40, 0.5 M in water) in the other compartment in contact with a large area carbon felt electrode. The two chambers were separated by a Nafion membrane, and an electrical connection was established between the photoanode and carbon felt cathode through a potentiostat. The reference and counter electrode leads of this potentiostat were both connected to the cathode to give a floating reference (or two-electrode) configuration, across which fixed bias voltages could be applied in a controlled fashion (see SI for a full description of the experimental setup). It is important to note that although the ECPB is highly colored, it is retained in the cathode compartment by the membrane such that the photoanode is immersed in a transparent solution containing 1 M methanesulfonic acid only. Hence there is no attenuation of the irradiation reaching the photoanode by the ECPB.

Figure 2.

Figure 2

General schematic of the photoelectrochemical cell configuration used to drive water oxidation and concomitant reduction of the ECPB at zero bias. FTO = fluorine-doped tin oxide on glass. The reduction of the ECPB at the cathode is shown as being coupled to protonation as suggested by our previous results (see ref (8a)).

Figure 3 (top) shows a chopped-light experiment in which the applied bias voltage between the photoanode and cathode was fixed at 0 V (i.e., no external bias), and the photoanode was irradiated periodically with simulated solar light (AM 1.5) at 1 Sun intensity. These results indicated that current densities of well over 1 mA cm–2 could be obtained at 0 V bias in this system under illumination, with the current density falling to zero when the light was turned off (Figure 3a, red line). These results were conducted without any compensation for resistance, which was found to be around 14 Ω. Control experiments with an identical setup but using a bare FTO electrode without WO3 (Figure 3a, black line) or with an FTO-WO3 electrode but with only 1 M methanesulfonic in the cathode compartment (blue line) indicated that both the WO3 photoanode and the ECPB were essential for observing photocurrent under these conditions.

Figure 3.

Figure 3

(A) Chopped light experiment in a two-electrode configuration at 0 V bias, according to the cell setup in Figure 2 (red line). Black line: with H3PMo12O40 but using only FTO as the anode. Blue line: with a WO3-FTO anode, but using no ECPB. (B) Chopped light experiment in a two-electrode configuration, as above, but with the bias potential varied from 0 to 0.5 V at a rate of 1 mV/s. Expansions of the low current areas of both these graphs (so that the blue and black traces can be seen more clearly) are given in Figures S2 and S3.

Figure 3 (bottom) shows a chopped light experiment obtained under the same conditions as the red trace in Figure 3a, but this time with the bias voltage being swept from 0 to 0.5 V at a rate of 1 mV/s (a sweep over a wider range of potentials is shown in Figures S4 and S5). Hence if modest bias voltages are applied, current densities approaching 2.5 mA cm–2 can be obtained. These current densities compare favorably with photocurrents obtained in three-electrode configurations with WO3 photoanodes at low pH, for which maximum current densities under high anodic bias normally plateau at ∼1 mA cm–2.10,11

During the chopped light experiments described above, bubbling was observed at the anode, while the cathode compartment turned from yellow (characteristic of [PMo12O40]3–) to blue (indicating reduction to [PMo12O40]5–). In order to determine the nature of any gases produced in either compartment, irradiation at 1 Sun and AM 1.5 was conducted at 0 V bias, while the headspaces of the anode and cathode chambers were investigated by gas chromatography and fluorescence probe spectroscopy (see SI for details). Gas chromatography indicated that oxygen gas was present in the anode headspace, but no hydrogen gas could be detected in either compartment headspace, suggesting that complete decoupling of the water oxidation and proton reduction reactions had occurred in this step. Quantification of the amount of oxygen evolved was possible using an O2 fluorescence-quench probe, and comparison with the total charge passed during irradiation indicated that the Faradaic efficiency for oxygen production by photolytic water splitting was 84% (±6%), see Figure 4.

Figure 4.

Figure 4

Comparison of the amount of O2 expected in the cell headspace on the basis of the charge passed (black dashed line) and O2 detected in the cell headspace by fluorescence-quench measurements (red line). Bubbles collected on the anode and were periodically dislodged by shaking, accounting for the increments observed in the measured O2 signal.

These results suggest that solar-driven water oxidation can be coupled to reduction of [PMo12O40]3– to give a reduced ECPB without simultaneous hydrogen evolution, such that gas mixing in a working device could be kept to a minimum (even at current densities under irradiation on the order of only 1 mA cm–2).

Our previous work8a demonstrated that the reduced form of the ECPB ([PMo12O40]5–) is stable with respect to reoxidation in air on the time scale of hours-to-days and gives clean reconversion to [PMo12O40]3– with concomitant H2 evolution (at 100% Faradaic yield) when oxidized electrochemically at modest bias voltages. Hence, in order to demonstrate the feasibility of the second main advantage of this approach (generation of hydrogen by reoxidation of the ECPB in a separate device to the solar-harvesting array), we reoxidized the [PMo12O40]5– produced during water oxidation electrochemically in a cell containing the reduced [PMo12O40]5– buffer in one compartment and 1 M methanesulfonic acid in the other at +0.75 V vs Ag/AgCl (see section SI-6 in the SI). Complete reoxidation was gauged by achieving a low steady-state background current and by return of the ECPB to its original yellow color. Comparison of the charge passed during reoxidation and the amount of hydrogen evolved revealed full Faradaic efficiency for decoupled H2 production. The charge passed during reoxidation was also identical to the charge passed during initial reduction of the ECPB during the photodriven water oxidation step. Hence this ECPB makes a good mediator for potential solar-to-hydrogen applications, greatly reducing gas crossover and allowing O2 and H2 to be generated at different rates and at different times on account of these two processes being electrochemically decoupled. A rough estimation of the overall efficiency of this system (energy in vs energy out) gives a figure of between 1 and 2% (see SI).

In summary, we have demonstrated that a combined solar-electrochemical system that uses an ECPB to decouple the half reactions of water splitting is feasible. The potential benefits of this approach include reduced gas mixing at low current densities (due to decoupling of the half-reactions), the potential for hydrogen to be generated more rapidly than the oxygen (i.e., at a rate which is not limited by the solar flux), and the ability to generate the hydrogen at a time and place distinct from the large surface-area solar-harvesting array (for ease of collection and pressurization, and for the most effective use of the electrochemical cell and its components). A further benefit may include the ability to use membranes other than Nafion in the large area array, as the gas permeability of the membrane is less of an issue if oxygen evolution and hydrogen evolution are decoupled (the separator need only prevent the ECPB from accessing the anode compartment). Cheaper separators are highly desirable if large area arrays are to be made affordable, and one such cheap candidate material for this role is cellulose, which we have already demonstrated performs similarly to Nafion in decoupled water splitting mediated by [PMo12O40]3–.8a Certain key challenges still remain in this approach (especially regarding increasing the current densities for water oxidation), and efforts toward improving this system are currently underway in our laboratories.

Acknowledgments

This work was supported by the EPSRC (grants nos. EP/J015156/1; EP/L023652/1; EP/I033459/1; EP/J015156/1; EP/K023004/1; EP/L023652/1), and EC grant 318671 (MICREAGENTS). L.C. thanks the Royal Society/Wolfson Foundation for a Merit Award and the ERC for an Advanced Grant (ERC-ADG, 670467 SMART-POM). M.D.S. acknowledges the University of Glasgow for a Kelvin Smith Research Fellowship. P.J.K. was supported in part by National Research Council, Poland under Maestro Project. The datasets underpinning this work can be obtained by contacting L.C.

Supporting Information Available

The Supporting Information is available free of charge on the ACS Publications website at DOI: 10.1021/jacs.6b03187.

  • Experimental details and data (PDF)

The authors declare no competing financial interest.

Supplementary Material

ja6b03187_si_001.pdf (386.3KB, pdf)

References

  1. a Cai Y.; Judd K. L.; Lenton T. M.; Lontzek T. S.; Narita D. Proc. Natl. Acad. Sci. U. S. A. 2015, 112, 4606. 10.1073/pnas.1503890112. [DOI] [PMC free article] [PubMed] [Google Scholar]; b Rogelj J.; McCollum D. L.; Reisinger A.; Meinshausen M.; Riahi K. Nature 2013, 493, 79. 10.1038/nature11787. [DOI] [PubMed] [Google Scholar]; c Schaeffer M.; Kram T.; Meinshausen M.; van Vuuren D. P.; Hare W. L. Proc. Natl. Acad. Sci. U. S. A. 2008, 105, 20621. 10.1073/pnas.0802416106. [DOI] [Google Scholar]
  2. a Lewis N. S.; Nocera D. G. Proc. Natl. Acad. Sci. U. S. A. 2006, 103, 15729. 10.1073/pnas.0603395103. [DOI] [PMC free article] [PubMed] [Google Scholar]; b Blankenship R. E.; Tiede D. M.; Barber J.; Brudvig G. W.; Fleming G.; Ghirardi M.; Gunner M. R.; Junge W.; Kramer D. M.; Melis A.; Moore T. A.; Moser C. C.; Nocera D. G.; Nozik A. J.; Ort D. R.; Parson W. W.; Prince R. C.; Sayre R. T. Science 2011, 332, 805. 10.1126/science.1200165. [DOI] [PubMed] [Google Scholar]
  3. a Cook T. R.; Dogutan D. K.; Reece S. Y.; Surendranath Y.; Teets T. S.; Nocera D. G. Chem. Rev. 2010, 110, 6474. 10.1021/cr100246c. [DOI] [PubMed] [Google Scholar]; b Armaroli N.; Balzani V. Chem. - Eur. J. 2016, 22, 32. 10.1002/chem.201503580. [DOI] [PubMed] [Google Scholar]
  4. See, for example:; a Symes M. D.; Cronin L. In Materials for a Sustainable Future; Letcher T. M., Scott J. L., Eds.; RSC Publishing: Cambridge, 2012; pp 592–614. [Google Scholar]; b Joya K. S.; de Groot H. J. M. ChemSusChem 2014, 7, 73. 10.1002/cssc.201300981. [DOI] [PubMed] [Google Scholar]; c Joya K. S.; Joya Y. F.; Ocakoglu K.; van de Krol R. Angew. Chem., Int. Ed. 2013, 52, 10426. 10.1002/anie.201300136. [DOI] [PubMed] [Google Scholar]; d Tachibana Y.; Vayssieres L.; Durrant J. R. Nat. Photonics 2012, 6, 511. 10.1038/nphoton.2012.175. [DOI] [Google Scholar]; e Concepcion J. J.; House R. L.; Papanikolas J. M.; Meyer T. J. Proc. Natl. Acad. Sci. U. S. A. 2012, 109, 15560. 10.1073/pnas.1212254109. [DOI] [PMC free article] [PubMed] [Google Scholar]; f Rocheleau R. E.; Miller E. L.; Misra A. Energy Fuels 1998, 12, 3. 10.1021/ef9701347. [DOI] [Google Scholar]; g Yamada Y.; Matsuki N.; Ohmori T.; Mametsuka H.; Kondo M.; Matsuda A.; Suzuki E. Int. J. Hydrogen Energy 2003, 28, 1167. 10.1016/S0360-3199(02)00280-X. [DOI] [Google Scholar]; h Reece S. Y.; Hamel J. A.; Sung K.; Jarvi T. D.; Esswein A. J.; Pijpers J. J. H.; Nocera D. G. Science 2011, 334, 645. 10.1126/science.1209816. [DOI] [PubMed] [Google Scholar]; i Khaselev O.; Turner J. A. Science 1998, 280, 425. 10.1126/science.280.5362.425. [DOI] [PubMed] [Google Scholar]; j Licht S.; Wang B.; Mukerji S.; Soga T.; Umeno M.; Tributsch H. J. Phys. Chem. B 2000, 104, 8920. 10.1021/jp002083b. [DOI] [Google Scholar]; k Abdi F. F.; Han L.; Smets A. H. M.; Zeman M.; Dam B.; van de Krol R. Nat. Commun. 2013, 4, 2195. 10.1038/ncomms3195. [DOI] [PubMed] [Google Scholar]; l Brillet J.; Yum J.-H.; Cornuz M.; Hisatomi T.; Solarska R.; Augustynski J.; Grätzel M.; Sivula K. Nat. Photonics 2012, 6, 824. 10.1038/nphoton.2012.265. [DOI] [Google Scholar]; m Chen Y.; Sun K.; Audesirk H.; Xiang C.; Lewis N. S. Energy Environ. Sci. 2015, 8, 1736. 10.1039/C5EE00311C. [DOI] [Google Scholar]; n Sathre R.; Scown C. D.; Morrow W. R.; Stevens J. C.; Sharp I. D.; Ager J. W.; Walczak K.; Houle F. A.; Greenblatt J. B. Energy Environ. Sci. 2014, 7, 3264. 10.1039/C4EE01019A. [DOI] [Google Scholar]; o Roger I.; Symes M. D. J. Mater. Chem. A 2016, 4, 6724. 10.1039/C5TA09423B. [DOI] [Google Scholar]
  5. McCrory C. C. L.; Jung S.; Ferrer I. M.; Chatman S. M.; Peters J. C.; Jaramillo T. F. J. Am. Chem. Soc. 2015, 137, 4347. 10.1021/ja510442p. [DOI] [PubMed] [Google Scholar]
  6. a Jin J.; Walczak K.; Singh M. R.; Karp C.; Lewis N. S.; Xiang C. Energy Environ. Sci. 2014, 7, 3371. 10.1039/C4EE01824A. [DOI] [Google Scholar]; b Barbir F. Sol. Energy 2005, 78, 661. 10.1016/j.solener.2004.09.003. [DOI] [Google Scholar]; c Schalenbach M.; Carmo M.; Fritz D. L.; Mergel J.; Stolten D. Int. J. Hydrogen Energy 2013, 38, 14921. 10.1016/j.ijhydene.2013.09.013. [DOI] [Google Scholar]; d Chandesris M.; Médeau V.; Guillet N.; Chelghoum S.; Thoby D.; Fouda-Onana F. Int. J. Hydrogen Energy 2015, 40, 1353. 10.1016/j.ijhydene.2014.11.111. [DOI] [Google Scholar]; e Berger A.; Segalman R. A.; Newman J. Energy Environ. Sci. 2014, 7, 1468. 10.1039/C3EE43807D. [DOI] [Google Scholar]
  7. Ivy J.Summary of Electrocatalytic Hydrogen Production, Milestone Completion Report; National Renewable Energy Laboratory: Golden, CO, 2004.
  8. a Symes M. D.; Cronin L. Nat. Chem. 2013, 5, 403. 10.1038/nchem.1621. [DOI] [PubMed] [Google Scholar]; b Rausch B.; Symes M. D.; Cronin L. J. Am. Chem. Soc. 2013, 135, 13656. 10.1021/ja4071893. [DOI] [PubMed] [Google Scholar]; c Rausch B.; Symes M. D.; Chisholm G.; Cronin L. Science 2014, 345, 1326. 10.1126/science.1257443. [DOI] [PubMed] [Google Scholar]
  9. a Darwent J. R.; Mills A. J. Chem. Soc., Faraday Trans. 2 1982, 78, 359. 10.1039/f29827800359. [DOI] [Google Scholar]; b Grätzel M. Nature 2001, 414, 338. 10.1038/35104607. [DOI] [PubMed] [Google Scholar]; c Wang F.; Di Valentin C.; Pacchioni G. J. Phys. Chem. C 2012, 116, 8901. 10.1021/jp300867j. [DOI] [Google Scholar]; d Coridan R. H.; Shaner M.; Wiggenhorn C.; Brunschwig B. S.; Lewis N. S. J. Phys. Chem. C 2013, 117, 6949. 10.1021/jp311947x. [DOI] [Google Scholar]; e Huang Z.-F.; Song J.; Pan L.; Zhang X.; Wang L.; Zou J.-J. Adv. Mater. 2015, 27, 5309. 10.1002/adma.201501217. [DOI] [PubMed] [Google Scholar]
  10. a Santato C.; Ulmann M.; Augustynski J. J. Phys. Chem. B 2001, 105, 936. 10.1021/jp002232q. [DOI] [PubMed] [Google Scholar]; b Santato C.; Odziemkowski M.; Ulmann M.; Augustynski J. J. Am. Chem. Soc. 2001, 123, 10639. 10.1021/ja011315x. [DOI] [PubMed] [Google Scholar]; c Solarska R.; Bienkowski K.; Zoladek S.; Majcher A.; Stefaniuk T.; Kulesza P. J.; Augustynski J. Angew. Chem., Int. Ed. 2014, 53, 14196. 10.1002/anie.201408374. [DOI] [PubMed] [Google Scholar]
  11. See, for example:; a Hodes G.; Cahen D.; Manassen J. Nature 1976, 260, 312. 10.1038/260312a0. [DOI] [Google Scholar]; b Miller E. L.; Paluselli D.; Marsen B.; Rocheleau R. E. Sol. Energy Mater. Sol. Cells 2005, 88, 131. 10.1016/j.solmat.2004.07.058. [DOI] [Google Scholar]; c Miller E. L.; Marsen B.; Cole B.; Lum M. Electrochem. Solid-State Lett. 2006, 9, G248. 10.1149/1.2201994. [DOI] [Google Scholar]; d Hill J. C.; Choi K.-S. J. Phys. Chem. C 2012, 116, 7612. 10.1021/jp209909b. [DOI] [Google Scholar]; e de Respinis M.; De Temmerman G.; Tanyeli I.; van de Sanden M. C. M.; Doerner R. P.; Baldwin M. J.; van de Krol R. ACS Appl. Mater. Interfaces 2013, 5, 7621. 10.1021/am401936q. [DOI] [PubMed] [Google Scholar]; f Spurgeon J. M.; Velazquez J. M.; McDowell M. T. Phys. Chem. Chem. Phys. 2014, 16, 3623. 10.1039/c3cp55527e. [DOI] [PubMed] [Google Scholar]; g Walczak K.; Chen Y.; Karp C.; Beeman J. W.; Shaner M.; Spurgeon J.; Sharp I. D.; Amashukeli X.; West W.; Jin J.; Lewis N. S.; Xiang C. ChemSusChem 2015, 8, 544. 10.1002/cssc.201402896. [DOI] [PubMed] [Google Scholar]; h Bignozzi C. A.; Caramori S.; Cristino V.; Argazzi R.; Meda L.; Tacca A. Chem. Soc. Rev. 2013, 42, 2228. 10.1039/C2CS35373C. [DOI] [PubMed] [Google Scholar]; i Wang N.; Wang D.; Li M.; Shi J.; Li C. Nanoscale 2014, 6, 2061. 10.1039/c3nr05601e. [DOI] [PubMed] [Google Scholar]; j Miseki Y.; Kusama H.; Sugihara H.; Sayama K. J. Phys. Chem. Lett. 2010, 1, 1196. 10.1021/jz100233w. [DOI] [Google Scholar]

Associated Data

This section collects any data citations, data availability statements, or supplementary materials included in this article.

Supplementary Materials

ja6b03187_si_001.pdf (386.3KB, pdf)

Articles from Journal of the American Chemical Society are provided here courtesy of American Chemical Society

RESOURCES