6528
M. Hmadeh et al. / Tetrahedron 64 (2008) 6522–6529
Special care was taken to ensure that complete equilibration was
attained. Absorption spectra versus pH were recorded using a Var-
ian CARY 50 spectrophotometer fitted with HELLMA optical fibers
(HELLMA, 041.002-UV) and an immersion probe made of quartz
suprazil (HELLMA, 661.500-QX).
thank the French Ministry of Research and Education for granting
them a Ph.D. fellowship.
Supplementary data
Supplementary data associated with this article can be found in
4.4. Fluorescence titration
An aliquot of 40 mL of 6 (5.25ꢄ10ꢁ6 M) was introduced into
a jacketed cell (METROHM 6.1414.150) maintained at 25.0(2) ꢃC by
the flow of a HAAKE FJ thermostat. The solution was continuously
de-oxygenated by bubbling with oxygen-free argon. The initial pH
was adjusted at 0.85 with concentrated perchloric acid, and the
titration of 6 was carried out by addition of known volumes of
a tetrametylammonium hydroxide solution (0.1 M). An aliquot
(2 mL) was taken after each addition of base, and a fluorescence
emission spectrum (250–700 nm) was recorded versus pH with
1 cm quartz optical cell (HELLMA, 110-QS) on a PERKIN-ELMER LS-
50B spectrofluorimeter maintained at 25.0(2) ꢃC by the flow of
a HAAKE FJ thermostat. The excitation wavelength was 250ꢅ1 nm,
and the excitation and emission slit widths were set at 5 nm. The
absorbance at the excitation wavelength (lexcꢆ250 nm) was kept
lower than 0.1 to minimize reabsorption processes and to keep it
constant throughout the fluorescence titration. The light source
was a pulsed xenon flash lamp with a pulse width at half peak
References and notes
1. Vogel, A. I. Practical Organic Chemistry, 5th ed.; Longman: London, 1991; p 49.
2. (a) Vaisman, B.; Konijin, A. M.; Fibach, E. Acta Haematol. 1999, 101, 135–139; (b)
Jing, Y.; Nakajo, S.; Xia, L.; Nakaya, K.; Fang, Q.; Waxman, S.; Han, R. Leuk. Res.
1999, 23, 43–50; (c) Liu, L.; Yulan, Z.; Qian, X. Dyes Pigments 2004, 60, 17–21.
3. Mesulam, M. M. J. Histochem. Cytochem. 1978, 26, 106–117.
4. (a) Standefer, J. S.; Vanderjagt, D. Clin. Chem. 1977, 23, 749–751; (b) Thomas,
P. D.; Poznanzki, M. J. Anal. Biochem. 1990, 188, 228–232; (c) Williams, K. J.;
Rosenstein, R.; Smith, R. P. Clin. Chim. Acta 1985, 145, 113–118.
´
5. (a) Bissell, R. A.; Cordova, E.; Kaifer, A. E.; Stoddart, J. F. Nature 1994, 369, 133–
137; (b) Ballardini, R.; Balzani, V.; Gandolfi, M. T.; Prodi, L.; Venturi, M.; Philip,
D.; Ricketts, H. G.; Stoddart, J. F. Angew. Chem., Int. Ed. Engl. 1993, 32, 1301–1303.
6. (a) Fa´ber, R.; Mielke, G. F.; Rapta, P.; Stasko, A.; Nuyken, O. Collect. Czech. Chem.
ˇ
Commun. 2000, 65, 1403–1418; (b) Zhang, S. T.; Zhao, J. M.; Zhan, Y. Q.; Wu, Y.;
Zhou, Y. C.; Ding, X. M.; Hou, X. Y. Appl. Phys. Lett. 2004, 84, 2916–2918.
7. D’Eramo, F.; Are´valo, A. H.; Silber, J. J.; Sereno, L. J. Braz. Chem. Soc. 1994, 5, 213–
218.
8. (a) Siri, O.; Braunstein, P.; Taquet, J. P.; Collin, J. P.; Welter, R. Dalton Trans. 2007,
1481–1483; (b) Elhabiri, M.; Siri, O.; Sornosa Tent, A.; Albrecht-Gary, A. M.;
Braunstein, P. Chem.dEur. J. 2004, 10, 134–141; (c) Taquet, J. P.; Siri, O.;
Braunstein, P.; Welter, R. Inorg. Chem. 2006, 45, 4668–4676; (d) Siri, O.; Taquet,
J. P.; Collin, J. P.; Rohmer, M. M.; Benard, M.; Braunstein, P. Chem.dEur. J. 2005,
11, 7247–7253; (e) Siri, O.; Braunstein, P. Chem. Commun. 2000, 2223–2224; (f)
Siri, O.; Braunstein, P.; Rohmer, M. M.; Be´nard, M.; Welter, R. J. Am. Chem. Soc.
2003, 125, 13793–13803.
height <10 ms and power equivalent to 20 kW.
4.5. Refinement of the data
9. (a) Brooks, S. J.; Gale, P. A.; Light, M. E. CrystEngComm 2005, 7, 586–591; (b)
Kalisz, M.; Novak, M. A.; de Amorim, H. S.; Sinnecker, J. P.; Vaz, M. G. F. J. Magn.
Magn. Mater. 2005, 294, e51–e55.
10. Khramov, D. M.; Boydston, A. J.; Bielawski, C. W. Org. Lett. 2005, 8, 1831–1834.
11. Gehrhus, B.; Hitchcock, P. B.; Lappert, M. F. Z. Anorg. Allg. Chem. 2005, 631, 1383–
1386.
12. (a) Estela, J. M.; Far, M.; Cerda, V. Thermochim. Acta 1989, 153, 143–164; (b)
Reartes, G. B.; Liberman, S. J.; Blesa, M. A. Talanta 1987, 34, 1039–1042.
13. Glab, S.; Hulanicki, A. Talanta 1974, 21, 679–681.
14. Perlemutter-Hayman, B. Acc. Chem. Res. 1986, 19, 90–96.
15. McClelland, R. A.; Ren, D.; D’Sa, R.; Ahmed, A. R. Can. J. Chem. 2000, 78, 1178–
1185.
The spectrophotometric and potentiometric data were pro-
cessed with the SPECFIT program, which adjusts the stability con-
stants and the corresponding molar extinction coefficients
(Mꢁ1 cmꢁ1) of the species at equilibrium. SPECFIT47–50 uses factor
analysis to reduce the absorbance matrix and to extract the ei-
genvalues prior to the multiwavelength fit of the reduced data set
according to the Marquardt algorithm.51,52 Distribution curves of
the various species were calculated using the Haltafall program.53
Origin 5.0 was used to process the analytical results.54 For the sake
of simplicity, charges are omitted in all the chemical equilibria. The
16. Berlman, I. B. J. Chem. Phys. 1970, 52, 5616–5621.
17. Du, H.; Fuh, R. A.; Li, J.; Corkan, A.; Lindsey, J. S. Photochem. Photobiol. 1998, 68,
141–142.
errors are given as 3
s
with
s
¼standard deviation.
18. Shizuka, H.; Nakamura, M.; Morita, T. J. Phys. Chem. 1979, 83, 2019–2024.
19. Jaffe, H. H.; Orchin, M. Theory and Applications of Ultraviolet Spectroscopy;
Wiley: New York, NY, 1962.
20. (a) Arulmozhiraja, S.; Fujii, T. J. Chem. Phys. 2001, 115, 10589–10594; (b)
Tachikawa, H.; Kawabata, H. J. Phys. Chem. B 2003,107,1113–1119; (c) Nori-Sharh,
D.; Asadzadeh, S.; Ghjanizadeh, F. R.; Deyhimi, F.; Mohammadpour, M.; Jameh-
Bozorghi, S. J. Mol. Struct. (Theochem) 2005, 717, 41–51; (d) Mantas, A.; Deretey,
E.; Ferretti, F. H.; Estrada, M.; Csizmadia, I. G. J. Mol. Struct. (Theochem) 2000,
504, 77–103.
21. (a) Clark, G. L.; Pickett, L. W. J. Am. Chem. Soc. 1931, 53, 167–177; (b) Trotter, J.
Acta Crystallogr. 1961, 14, 1135–1140; (c) Hargreaves, A.; Hasan-Rizvi, S. Acta
Crystallogr. 1962, 15, 365–373; (d) Robertson, G. B. Nature 1961, 191, 593–594;
(e) Charbonneau, G. P.; Delugeard, Y. Acta Crystallogr., Sect. B 1976, 32, 1420–
1423; (f) Gustar, K.; Suhnel, J.; Wild, U. P. Helv. Chim. Acta 1978, 61, 2100–2107;
(g) Charbonneau, G. P.; Delugeard, Y. Acta Crystallogr., Sect. B 1977, 33, 1586–
1588; (h) Baudour, J. L. Meth. Struct. Anal. Modulated Struct. Quasicrystals 1991,
383–390.
22. Dobrzycki, L.; Wozniak, K. CrystEngComm 2006, 8, 780–783.
23. Parthasarathi, R.; Padmanabhan, J.; Sarkar, U.; Maiti, B.; Subramanian, V.;
Chattaraj, P. K. Internet Electron. J. Mol. Des. 2003, 2, 798–813.
24. Wagner, P. J. J. Am. Chem. Soc. 1967, 89, 2820–2825.
25. (a) Bhattacharyya, K.; Chowdhury, M. Chem. Rev. 1993, 93, 507–535; (b) The
Exciplex; Gordon, M., Ware, W. R., Eds.; Academic: New York, NY, 1975.
26. Braslavsky, S. E. Pure Appl. Chem. 2007, 79, 293–465.
27. Eisenthal, K. B. Laser Chem. 1983, 3, 145–162.
28. Bencini, A.; Bianchi, A.; Lodeiros, C.; Masotti, A.; Parola, A. J.; Pina, F.; Seixas de
Melo, J.; Valtancoli, B. Chem. Commun. 2000, 1639–1640.
29. de Silva, A. P.; Gunaratne, H. Q. N.; Gunnlaugsson, T.; Huxley, A. J. M.; McCoy,
C. P.; Rademacher, J. T.; Rice, T. E. Chem. Rev. 1997, 97, 1515–1566.
30. Simeonov, A.; Matsushita, M.; Juban, E. A.; Thompson, E. H. Z.; Hoffman, T. Z.;
Beuscher, A. E., IV; Taylor, M. J.; Wirsching, P.; Rettig, W.; McCusker, J. K.; Ste-
vens, R. C.; Millar, D. P.; Schultz, P. G.; Lerner, R. A.; Janda, K. D. Science 2000,
290, 307–313.
4.6. Photophysics
Emission spectra were collected on a PERKIN-ELMER LS-50B
luminescence spectrophotometer with solutions of absorbance
smaller than 0.1 at wavelength >lexc in order to avoid errors due to
the inner filter effect. Absorption spectra were also measured along
the fluorescence titration by using a Varian CARY 300 spectro-
photometer. Fluorescence quantum yields were determined rela-
tive to fluorescent standard quinine sulfate (Fabs¼0.546, 0.5 M
H2SO4) with possibility of correcting for differences between the
refractive index of the reference nr, and the sample solutions ns
using the expression:
R
Isð
l
l
Þ ꢄ Dr ꢄ n2s
Þ ꢄ Ds ꢄ n2r
R
4f ð Þ
4f ð Þ
s
¼
r
Irð
The indices s and r denote sample and reference, respectively. The
integrals over I represent areas of the corrected emission spectra, D
is the optical density at the wavelength of excitation.
Acknowledgements
This work has been supported by the Centre National de la
Recherche Scientifique (UMR 7177 and UMR 6114). M.H. and H.T.
31. Abad, S.; Pischel, U.; Miranda, M. A. J. Phys. Chem. A 2005, 109, 2711–2717.