Supporting Information Solving the 170-Year-Old Mystery About Red-Violet and Blue Transient Intermediates in the Gmelin Reaction Yin Gao, Abouzar Toubaei, Xianqi Kong, and Gang Wu*[a] chem_201503353_sm_miscellaneous_information.pdf Supporting Information Solving the 170 Year Old Mystery about Red-Violet and Blue Transient Intermediates in Gmelin Reaction Yin Gao, Abouzar Toubaei, Xianqi Kong, and Gang Wu* Department of Chemistry, Queen’s University, 90 Bader Lane, Kingston, Ontario, Canada K7L 3N6 E-mail: [email protected] 1. Experimental details Materials. All chemicals were obtained from Sigma-Aldrich unless stated otherwise: sodium nitroprusside (SNP, Na2[Fe(CN)5NO]·2H2O), sodium hydroxide (NaOH), 15N-labeled sodium nitrite (Na15NO2, 98% 15N), 17O-labeled water (H217O, 41.1% 17O, purchased from CortecNet), ethylenediaminetetraacetic acid (EDTA, C10H16N2O8), sodium carbonate (Na2CO3), sodium bicarbonate (NaHCO3), sodium chloride (NaCl), potassium cyanide (KCN), and ionexchange resin (Amberlite IR-120, strongly acidic form). Synthesis of 15N- and 17O-labelled SNPs. 15N-labeled SNP (Na2[FeII(CN)5(15NO)]·2H2O) was prepared in aqueous solution by mixing commercial SNP (260 mg) with 1.1 molar equivalents of NaOH and 5 molar equivalents of Na15NO2. The reaction mixture was kept at room temperature for 10 min, followed by addition of 285 µL of 4 M acetic acid. The reaction solution was concentrated to a paste on a rotary evaporator. The residual material was redissolved in 2 mL of 4 M acetic acid and the solvent was evaporated on a rotary evaporator. This process was repeated once. The obtained solid was treated with 1,4-dioxane (4 mL). The solid materials were collected by filtration, washed with ethanol (2 × 3 mL), and then dried under vacuum (153 mg, yield 59%). The 15N enrichment level in the final product was about 80%. 15N NMR (50.6 MHz, D2O): 371 ppm (referencing to liquid NH3); 13C NMR (125.6 MHz, D2O): 134.81 ppm (Ceq) and 132.84 ppm (Cax). 17O-labeled SNP (Na2[FeII(CN)5(N17O)]·2H2O) was prepared by mixing 265 mg of commercial SNP and 35.6 mg of NaOH in 300 µL of H217O (41.1% 17 O, purchased from CortectNet). A few grains of Amberlite IR-120 (strongly acidic form) were gradually added to the reaction mixture and the progress of this reaction was monitored via 17O NMR spectroscopy. The addition of the acidic resin was stopped once the reaction reached equilibrium, in order to maximize the formation of [FeII(CN)5(N17O)]2-. The mixture was then 1 treated with 1,4-dioxane (4 mL). The precipitates were then collected via filtration and dried under vacuum. The 17O-enrichment level of the product was determined to be 20% by 17O NMR. 17 O NMR (67.7 MHz, D2O): 419 ppm (referencing to water), 13C NMR (125.6 MHz, D2O): 134.81 ppm (Ceq) and 132.84 ppm (Cax). Synthesis of Na2S2. Na2S2 was prepared from the reaction between Na2S and sulfur under the anaerobic condition. To 10 mL oxygen free deionized water (which was degassed under Ar for 20 min) was transferred 10.84 g sodium sulfide nonahydrate (Na2S⋅9H2O). The solution was bubbled with N2 for 10 min while heating to 90°C until all Na2S were dissolved. 1.2 molar equivalent sulfur (1.75 g) was then added into the Na2S solution. After sulfur was fully dissolved, the reaction mixture was kept at 75 °C under N2 for 1 hr. After cooling to room temperature, the orange-red solution was frozen with liquid N2 and then lyophilized to obtain the yellow solid of Na2S2. 2. Characterization of the blue product from reaction between NP and Na2S2 45567*45528*9:;*<*=5567*45528*:&>9>*?'*@>A* !#,-.# (#,-.#(!#/01# $#,-.#$!#/01# )#,-.#)!#/01# '#,-.#)!#/01# $"!# ()#,-.#)!#/01# !"#$%&%'('%)"% ("'# ("&# !"#$%"&'()* ("%# ("$# ("!# !"'# !"&# !"%# !"$# !"!# $!!# )!!# %!!# *!!# &!!# +!!# +&,)-)'./0*1'23* Figure S1. UV-vis spectra (0.1 mm pathlength) of the reaction solution containing 25 mM NP and 75 mM Na2S2 in aqueous solution (pH 11). The inset shows the blue color of the initial reaction solution. 2 3. Quantum mechanical computations All quantum chemical calculations were performed on Sun SPARC Enterprise M9000 servers at the High Performance Computing Virtual Laboratory (HPCVL) of Queen’s University. Each of the servers consists of 64 quad-core 2.52 GHz sparc64 VII processors with 8 GB of RAM per core (2TB of total memory). Geometry optimizations and NMR parameters calculations were carried out with Gaussian 09.1 The B3LYP hybrid functional was used, together with the Watchers2 all-electron basis set (14s11p6d3f)→[8s6p4d1f] for the Fe atom and 6-311++G(3df,3pd) basis set for other atoms. Solvation effects in aqueous solution were evaluated using the integral equation formalism polarizable continuum model (IEFPCM)3-9 as implemented in Gaussian 09. The following σref values were used in converting the computed magnetic shielding constants (σ) to chemical shifts (δ): 15N, 264.5 ppm;10 17O, 287.5 ppm.11 For 13 C chemical shifts, we used σref = 156 ppm, which was based on the computed magnetic shielding for the reference compound [Fe(CN)6]4– and its experimental 13C chemical shift, δ = 177.0 ppm. Table S1. Computed and experimental NMR chemical shifts for FeII complexes, nitrite and nitrate. Compound [Fe(CN)5N(O)S]4– Method G09 Exp δ(17O)/ppm 1245 1027 [Fe(CN)5N(O)SS]4– G09 Exp 1078 939 [Fe(CN)5N(O)SH]3– G09 [Fe(CN)5N(O)SSH]3– δ(15N)/ppm 881 700 δ(13Cax)/ppm 167.0 NA δ(13Ceq)/ppm 175.6 174.7 785 630 164.8 NA 172.3 173.5 965 724 148.2 159.3 G09 856 642 148.1 156.4 [Fe(CN)5NO2]4– G09 Exp 723 690 664 555 184.0 172.9 177.1 175.2 [Fe(CN)5N(O)OH]3– G09 695(N=O) 466 (N-O-H) 571 150.2 152.1 [Fe(CN)5NO]2– G09 Exp 392 419 449 371 117.4 132.3 122.3 134.5 NO2– G09 Exp 724 661 685 609 NO3– G09 Exp 427 405 422 367 NA: Not available. 3 Table S2. Comparison of experimental and computed (TD-DFT) UV-vis absorption bands for [SNO]–, [SSNO]–, [Fe(CN)5N(O)S]4– and [Fe(CN)5N(O)S]4–. Compound Method λmax(nm) [SNO]– TD-DFT Exp.12 TD-DFT Exp.12 TD-DFT Exp. TD-DFT Exp. 296 325 383 448 446 540 480 570 [SSNO]– [Fe(CN)5N(O)S]4– [Fe(CN)5N(O)SS]4– Oscillator strength (f) 0.06 Transition (%) HOMO-2 → LUMO (65%) 0.08 HOMO → LUMO (72%) 0.12 HOMO-2 → LUMO (91%) 0.20 HOMO → LUMO (88%) Figure S2. Molecular orbitals that contribute to the UV-vis absorption bands shown in Table S2 for (a) [SNO]–, (b) [SSNO]–, (c) [Fe(CN)5N(O)S]4– and (d) [Fe(CN)5N(O)SS]4– 4 4. Aqueous-phase pKa calculations Aqueous-phase pKa values were calculated using the thermodynamic cycle shown in Figure S3 and the integral equation formalism polarizable continuum model (IEFPCM).3-9 The generally accepted experimental-theoretical values for Ggas(H+) and ΔGS(H+) are –6.2813 and –265.9 kcal/mol.14 pKa = –log Ka pKa = ΔGº/ln 10RT, where ΔGº = ΔGaq According to Figure S2, ΔGaq can be calculated in the following fashion: ΔGaq = ΔGgas + ΔGS (H+) + ΔGS (A–) – ΔGS (HA) ΔGgas = Ggas(A–) + Ggas (H+) – Ggas (HA) In this work, we used the following equation to convert the ΔGgas reference state (24.46 L at 298.15 K) from 1 atm to 1 M: ΔGgas(1M) = ΔGgas(1atm) + RT ln(24.46) Thus, the pKa values can be calculated using the following equation: pKa = [Ggas(A–) – Ggas (HA) + ΔGS (A–) – ΔGS (HA) – 270.29]/1.3644 "Ggas A!gas AHgas !"Gs(AH) + H+gas "Gs(A!) "Gs(H+) "Gaq AHaq A!aq + H+aq Figure S3. Thermodynamic cycle used in pKa calculations. Because it is still a challenge to calculate absolute pKa values to a high degree of accuracy, it is a common practice that a “calibration” process is performed for a class of closely related 5 compounds. To this end, we first computed pKa values for a set of compounds containing -OH and -SH functional groups with known experimental pKa values (the “calibration compounds” shown in Table S3), in order to establish a correlation between pKa (calc.) and pKa(exp). Then we can apply this correlation to predict the pKa values for the compounds in question (the “unknown compounds in Table S3). The pKa calibration plot is shown in Figure S4. Table S3. Computed aqueous pKa values for “calibration compounds” and “unknown compounds”. pKa (calc.) pKa (exp) Calibration compounds Nitrous acid Formic acid Acrylic acid Phenol H2 O H2 S HSCN CH3OH CH3SH HNCO 3.5 7.6 9.7 17.4 31.0 11.7 -5.9 30.9 17.3 9.1 3.3 3.8 4.3 10 15.7 7 -1.28 15.5 10.4 3.73 Unknown compounds cis-HSNO trans-HSNO HSSNO trans-nitrous acid 3.5 4.1 0.2 4.2 2.6a 2.9a 1.0a 2.9a a Predicted values using pKa(exp) = pKa(calc) × 0.4776 + 0.9; see Figure S4. 6 20 y = 0.4776x + 0.9293 R² = 0.97218 pKa(exp) 10 0 -20 -10 0 -10 10 20 30 40 pKa(cal) Figure S4. Correlation between pKa(exp) and pKa(cal) for the “calibration compounds” shown in Table S3. 7 5. FTIR characterization 2051.8 1254.3 a !4 14N 805.6 " 15N 2055.8 !"#$%&#'()% !"#$%&#'()% 1358.3 ! 4!"#$"%&' !"#$"%(' 2200 1800 1600 1400 1200 1000 800 600 400 b22002000 2000 1800 1600 1400 1200 1000 800 600 400 !"#$%&#'()% N!"#$"%&' " 151200 N!"#$"%(' 1000 800 2200 2000 1800 1600 141400 2045.6 1295.1 600 400 1254.3 "#'% c 2000 1800 1600! 1400 2200 1200 1000 800 4 600 400 "#$&% 14N " 15N 2200 2000 1800 1600 1400 1200 1000 800 600 400 "#$% 2200 2000 1800 1600 1400 1200 1000 800 600 400 "#'% 2200 2000 1800 1600 1400 1200 1000 800 600 !"#$%&#'()% 1935.5 2200 2000 1800 1600 1400 1200 1000 800 600 "#"&% 2141.5 660.8 d !4 400 400 "#$&% "% "#$% 14N !"#"&% " 15N "#"&% 2200 2000 1800 1600 1400 1200 1000 800 600 400 2200 20001800 18001600 1600 1400 1200 1000800800 2200 2000 1400 1200 1000 600600 400400 ()*+),$% ()*+),-% -1 "% (cm 1000 )1000 800 2200 2000 1600 2200 2000 1800 1800 wavenumber 1600 1400 1400 1200 1200 800 600 600 400 400 !"#$% !"#"&% !"#$% 4– 4– 4– Figure ATR-FTIR of 800 a) [Fe(CN) 5N(O)S] , b) [Fe(CN)5N(O)SS] , c) [Fe(CN)5NO2] and d) 2200 2000S5. 1800 1600 1400 spectra 1200 1000 600 400 ()*+),$% ()*+),-% 2– [Fe(CN)5NO] (NP) in aqueous solution. The 14N-15N difference spectra (red traces) are also displayed. Note that, because the 15N labeling level in the complexes is only 60%, the 14N-15N difference peak is not perfectly anti-symmetric. The spectral noise in the region below 600 cm–1 is the artifact from ATR measurement. 6. References (1) Gaussian 09, Revision D.01, Frisch, M. J.; Trucks, G. W.; Schlegel, H. B.; Scuseria, G. E.; Robb, M. A.; Cheeseman, J. R.; Scalmani, G.; Barone, V.; Mennucci, B.; Petersson, G. A.; Nakatsuji, H.; Caricato, M.; Li, X.; Hratchian, H. P.; Izmaylov, A. F.; Bloino, J.; Zheng, G.; Sonnenberg, J. L.; Hada, M.; Ehara, M.; Toyota, K.; Fukuda, R.; Hasegawa, J.; Ishida, M.; Nakajima, T.; Honda, Y.; Kitao, O.; Nakai, H.; Vreven, T.; Montgomery, J. A., Jr.; Peralta, J. E.; Ogliaro, F.; Bearpark, M.; Heyd, J. J.; Brothers, E.; Kudin, K. N.; Staroverov, V. N.; Kobayashi, R.; Normand, J.; Raghavachari, K.; Rendell, A.; Burant, J. C.; Iyengar, S. S.; Tomasi, J.; Cossi, M.; Rega, N.; Millam, J. M.; Klene, M.; Knox, J. E.; Cross, J. B.; Bakken, V.; Adamo, C.; Jaramillo, J.; Gomperts, R.; Stratmann, R. E.; Yazyev, O.; Austin, A. J.; Cammi, R.; Pomelli, C.; 8 Ochterski, J. W.; Martin, R. L.; Morokuma, K.; Zakrzewski, V. G.; Voth, G. A.; Salvador, P.; Dannenberg, J. J.; Dapprich, S.; Daniels, A. D.; Farkas, Ö.; Foresman, J. B.; Ortiz, J. V.; Cioslowski, J.; Fox, D. J. Gaussian, Inc., Wallingford CT, 2009. (2) Wachters, A. J. H. J. Chem. Phys. 1970, 52, 1033. (3) Miertus, S.; Scrocco, E;. Tomasi, J. Chem. Phys. 1981, 55, 117-129. (4) Miertus, S.; Tomasi, J. Chem. Phys. 1982, 65, 239-245. (5) Cossi, M.; Barone, V.; Cammi, R.; Tomasi, J. Chem. Phys. Lett. 1996, 255, 327-335. (6) Cances, M. T.; Mennucci, V.; Tomasi, J. J. Chem. Phys. 1997, 107, 3032-3041. (7) Barone, V.; Cossi, M.; Mennucci, B.; Tomasi, J. J. Chem. Phys. 1997, 107, 3210-3221. (8) Cossi, M. T.; Barone, V.; Mennucci, B.; Tomasi, J. Chem. Phys. Lett. 1998, 286, 253-260. (9) Barone, V.; Cossi, M.; Tomasi, J. J. Comput. Chem. 1998, 19, 404-417. (10) Jameson, C. J.; Jameson, A. K.; Oppusunggu, D.; Wille, S.; Burrell, P. M.; Mason, J. J. Chem. Phys. 1981, 74, 81-88. (11) Wasylishen, R. E.; Bryce, D. L. J. Chem. Phys. 2002, 117, 10061-10066. (12) Cortese-Krott, M. M.; Fernandez, B. O.; Santos, J. L. T.; Mergia, E.; Grman, M.; Nagy, P.; Kelm, M.; Butler, A.; Feelisch, M. Redox. Biol. 2014, 2, 234-244. (13) Liptak, M. D.; Shields, G. C. J. Am. Chem. Soc. 2001, 123, 7314-7319. (14) Camaioni D.M.; Schwerdtfeger, C.A. J. Phys. Chem. A 2005, 109, 10795-10797. 9
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