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Steric Effects for Proton, Hydrogen-Atom, and Hydride Transfer Reactions with Geometric Isomers of NADH-Model Ruthenium
Complexes
Brian W. Cohen,† Dmitry E. Polyansky,*,† Patrick Achord,† Diane Cabelli,†
James T. Muckerman,† Koji Tanaka,§ Randolph P. Thummel,‡ Ruifa Zong,‡ and Etsuko Fujita*,†
† Chemistry Department, Brookhaven National Laboratory, Upton, New York 11973-5000, USA § Institute for Molecular Science, 5-1 Higashiyama, Myodaiji, Okazaki, Aichi 444-8787, Japan
‡ Department of Chemistry, University of Houston, Houston TX 77204-5003, USA
Supporting Information
Electronic Supplementary Material (ESI) for Faraday DiscussionsThis journal is © The Royal Society of Chemistry 2011
Figure S1. Cyclic voltammogram of [Ru(2)]2+ in CH3CN versus SCE.
E1/22•–/2 = 0.75 V
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Assignments of the absorption bands of [Ru(2)]2+
Peak Percent Transition 528 nm (2.3 eV) 0.2 HOMO-2 → LUMO MLCT 0.21 HOMO-1 → LUMO MLCT 436 nm (2.8 eV) 0.35 HOMO-2 → LUMO+1 MLCT 0.08 HOMO-1 → LUMO+2 MLCT 355 nm (3.5 eV) 0.08 HOMO-4 → LUMO →* 0.12 HOMO-2 → LUMO+3 MLCT 0.15 HOMO-1 → LUMO+4 MLCT
HOMO-4 HOMO-3 HOMO-2 HOMO-1
HOMO LUMO LUMO+1 LUMO+2
LUMO+3 LUMO+4
Figure S2. Calculated spectrum, assignment of absorption bands and the frontier orbitals of [Ru(2)]2+.
Electronic Supplementary Material (ESI) for Faraday DiscussionsThis journal is © The Royal Society of Chemistry 2011
Figure S3. The bimolecular rate constant of quenching the excited state of [Ru(2)]2+ by DABCO in acetonitrile.
Electronic Supplementary Material (ESI) for Faraday DiscussionsThis journal is © The Royal Society of Chemistry 2011
300 400 500 600 700 800 900 1000 1100
0.00
0.25
0.50
0.75
1.00
Abs
Wavelength, nm
Figure S4. UV-vis-NIR absorption spectra of stepwise reduction of [Ru(2)]2+ (black) to [Ru(2•–)]+ (green) by Na/Hg amalgam in CH3CN.
400 600 800 1000 1200
0.0
0.5
1.0
Ab
sorb
anc
e (
a.u
.)
Wavelength (nm)
Figure S5. UV-vis-NIR spectra of photochemical formation of [Ru(2•–)]+ (red) from [Ru(2)]2+ (black) in CH3CN/NEt3. The blue spectrum measured after an addition of 10 eq. of HClO4 to the [Ru(2•–)]+ solution indicates formation of a 1:1 mixture of [Ru(2)]2+ and [Ru(2HH)]2+.
Electronic Supplementary Material (ESI) for Faraday DiscussionsThis journal is © The Royal Society of Chemistry 2011
[Ru(2)]2+ [Ru(2•–)]+
[Ru(2H•)]2+ [Ru(2HH)]2+
[Ru(2H)]3+ Possible conformer of [Ru(2H)]24+
Electronic Supplementary Material (ESI) for Faraday DiscussionsThis journal is © The Royal Society of Chemistry 2011
Figure S6. Calculated structures of [Ru(2)]2+, [Ru(2•–)]+, [Ru(2H•)]2+, [Ru(2HH)]2+, [Ru(2H)]3+ and a possible isomer of [Ru(2H)]2
4+. The red line indicates an internal hydrogen bond between the protonated N atom and a coordinated N of the bpy ligand.
Figure S7. Calculated Mulliken atomic spin densities in [Ru(2•)]+ and protonated [Ru(2H•)]2+.
Figure S8. 1H NMR spectra of [Ru(2HH)]2+ photochemically (top) and chemically (bottom) produced in CD3CN. Impurities due to photodecomposition are labeled (*).
**
Electronic Supplementary Material (ESI) for Faraday DiscussionsThis journal is © The Royal Society of Chemistry 2011
640 660 680 700 720 740 760 780 800 820 840
0
1000
2000
3000
4000
5000
6000
7000
Em
issi
on in
tens
ity,
coun
ts
Wavelength, nm
0 mM 10 mM 23 mM 43 mM
Figure S9. Uncorrected emission spectra of [Ru(1)]2+ in CH3CN (excitation at 528 nm) in the presence of different concentrations of H2Q.
0.00 0.01 0.02 0.03 0.04 0.050.9
1.0
1.1
1.2
1.3
1.4
1.5
1.6
1.7
1.8
I 0/I
[H2Q], M
Figure S10. The plot of I0/I vs. concentration of H2Q, where I0 is the emission intensity in the absence of H2Q. The red line is the linear fit with the slope = 16.3 M-1.
Electronic Supplementary Material (ESI) for Faraday DiscussionsThis journal is © The Royal Society of Chemistry 2011
0.00 0.01 0.02 0.03 0.04 0.05 0.06
1.00
1.05
1.10
1.15
1.20
1.25
1.30
H2Q
D2Q
0/
[H2Q] or [D
2Q], M
Figure S11. The bimolecular rate constant of reaction of H2Q and D2Q with *[Ru(1)]2+ in CH3CN. Kinetic isotope effect (KIE) was found to be kH/kD = 6.2.
0.00 0.01 0.02 0.03 0.04 0.05 0.06 0.070.98
1.00
1.02
1.04
1.06
1.08
1.10
1.12
1.14
1.16
0/
[2,5-tBu2H
2Q], M
Figure S12. The bimolecular rate constant of reaction of H2Q(But)2 with *[Ru(1)]2+ in CH3CN.
Electronic Supplementary Material (ESI) for Faraday DiscussionsThis journal is © The Royal Society of Chemistry 2011
0.00 0.02 0.04 0.06 0.08 0.10 0.120.00
0.25
0.50
0.75
1.00
1.25
1.50
1.75
2.00
(kob
s, s-1
) x
103
[Ph3C+], M
Figure S13. Observed rate of the formation of 626 nm band in the reaction between [Ru(1HH)]2+
and the excess of triphenyl carbenium cation in acetonitrile plotted vs. concentration of [Ph3C]+.
The rate constant obtained from the linear fit was 1.5 10-2 M-1 s-1.
300 400 500 600 700 800
0
1
2
3
Abs
Wavelength, nm
Figure S14. UV-vis spectra of the product of the reaction between [Ru(1HH)]2+ and [Ph3C]+ in methylene chloride (black); [Ru(1H)]3+ in water pH = 1.
Electronic Supplementary Material (ESI) for Faraday DiscussionsThis journal is © The Royal Society of Chemistry 2011
300 400 500 600 700 800
0
1
2
3
Abs
Wavelength, nm
Figure S15. UV-vis spectra of the product of the reaction between [Ru(1HH)]2+ and [Ph3C]+ in methylene chloride after addition of triethylamine (black); [Ru(1)]2+ in water pH = 7.
Figure S16. 1H NMR of reaction mixture of [Ru(2HH)]2+ and [Ph3C]+ in CD3CN, showing the formation of Ph3CH (5.6 ppm) in a 1:1 ratio with [Ru(2)]2+. Characteristic peaks are integrated at 5.6 for Ph3CH and 9.07, 8.84-8.80, and 6.78 ppm for [Ru(2)]2+.
Electronic Supplementary Material (ESI) for Faraday DiscussionsThis journal is © The Royal Society of Chemistry 2011
200 250 300 350 400 450 500 550 600 650 700 750 8000.0
0.5
1.0
1.5
2.0
2.5
Abs
orba
nce
Wavelength (nm)
Figure S17. UV-vis spectra of [Ru(2)]2+ before (red) and after (black) photochemical reduction, hydride donation, and purification in CH3CN.
Electronic Supplementary Material (ESI) for Faraday DiscussionsThis journal is © The Royal Society of Chemistry 2011
Figure S18. 1H NMR of [Ru(2)]2+ starting material (bottom) and after photochemical reduction, hydride donation, and purification (top) in CD3CN.
Electronic Supplementary Material (ESI) for Faraday DiscussionsThis journal is © The Royal Society of Chemistry 2011
Figure S19. The bimolecular rate constant of hydride donation from [Ru(2HH)]2+ to [Ph3C]+ in CH3CN.
Electronic Supplementary Material (ESI) for Faraday DiscussionsThis journal is © The Royal Society of Chemistry 2011
Table S1. Computed Geometrical Parameters of Ru(2) Species.
[Ru(2)]2+ [Ru(2•–)]+ [Ru(2H•)]2+ [Ru(2H)]3+ [Ru(2HH)]2+
Ru–N pyridyl 2.085 2.094 2.091 2.081 2.088
Ru–N pbn 2.157 2.141 2.166 2.159 2.171
Ru–N bpy1 (tr) 2.101 2.091 2.122 2.126 2.118
Ru–N bpy1 2.095 2.083 2.096 2.101 2.095
Ru–N bpy2 (tr) 2.089 2.092 2.090 2.085 2.088
Ru–N bpy2 2.092 2.081 2.091 2.096 2.090
C9–H 1.092 1.089 1.087 1.088 1.097, 1.102
N10–H n/a n/a 1.016 1.021 1.009
C5–C12 1.407 1.424 1.430 1.398 1.513
C12–C13 1.453 1.445 1.431 1.436 1.402
C13–N10 1.369 1.382 1.404 1.370 1.409
C9–C12 1.407 1.398 1.409 1.405 1.514
C11–C12 1.453 1.467 1.449 1.427 1.420
C11–N10 1.347 1.350 1.375 1.354 1.366
N1–C11–C12–C9 179.97 179.99 179.44 179.69 176.82
N bpy···H n/a n/a 2.069 2.036 2.083
N10–N bpy n/a n/a 3.047 3.035 3.066
N10–H···N bpy n/a n/a 163.9 165.5 163.9
N N
N [Ru]
2+
101
11 14
129
13
Electronic Supplementary Material (ESI) for Faraday DiscussionsThis journal is © The Royal Society of Chemistry 2011