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J.P. Flament, I. Baraldi, and F. Momicchioli, J. Phys. Chem. 1993, 97, 13358.
142.K. Akiyama, S. Tero-Kubota, and J. Higuchi, J. Am. Chem. Soc. 1998, 120, 8269.
143.See for reviews (a) H. Tomioka, Acc. Chem. Res. 1997, 30, 1315. (b) H. Tomioka, in Advances in Carbene Chemistry, Vol. 2, U. Brinker, Ed., JAI Press, Greenwich, CT, 1988, pp. 175–214.
144.See for reviews (a) D. Bourissou, O. Guerret, F. P. Gabbai, and G. Bertrand, Chem. Rev. 2000, 100, 39. (b) A. J. III., Arduengo, Acc. Chem. Res. 1999, 32, 913.
145.H. E. Zimmerman and D. H. Paskovich, J. Am. Chem. Soc. 1964, 86, 2149.
146.(a) M. Regitz, Angew. Chem., Int. Ed. Engl. 1991, 30, 674. (b) R. Dagani, Chem. Eng. News 1991, Jan. 28, 19; 1994, May 2, 20. (c) C. Heinemann, T. Mu¨ller, Y. Apeloig, and H. Schwartz, J. Am. Chem. Soc. 1996, 118, 2023. (d) C. Beohme and G. Frenking,
J.Am. Chem. Soc. 1996, 118, 2039. (e) W. Kirmse, Angen. Chem. Int. Ed. 2003, 42, 2117.
147.K. Hirai, K. Komatsu, and H. Tomioka, Chem. Lett. 1994, 503.
148.H. Tomioka, H. Okada, T. Watanabe, K. Banno, K. Komatsu, and K. Hirai, J. Am. Chem. Soc. 1997, 119, 1582.
149.H. Tomioka, H. Okada, T. Watanabe, and K. Hirai, Angew. Chem., Int. Ed. Engl. 1994, 33, 873.
150.V. R. Koch and G. J. Gleicher, J. Am. Chem. Soc. 1971, 93, 1657.
151.(a) H. Tomioka, H. Mizuno, H. Itakura, and K. Hirai, J. Chem. Soc., Chem. Commun. 1997, 2261. (b) H. Itakura, H. Mizuno, K. Hirai, and H. Tomioka, J. Org. Chem. 2000, 65, 8797.
152.M. Ballester, Acc. Chem. Res. 1985, 18, 380; Adv. Phys. Org. Chem. 1989, 25, 307, 321.
153.M. Ballester, J. Riera, J. Castafier, C. Badfa, and J. M. Monso´, J. Am. Chem. Soc. 1971, 93, 2115.
154.(a) H. Tomioka, K. Hirai, and C. Fujii, Acta Chem. Scand. 1993, 46, 680. (b) H. Tomioka,
K.Hirai, and T. Nakayama, J. Am. Chem. Soc. 1993, 115, 1285.
155.R. S. Rowland and R. Taylor, J. Phys. Chem. 1996, 100, 7384.
REFERENCES 461
156.S. C. Murov, I. Carmichael, and G. L. Hug, Handbook of Photochemistry, Marcel Dekker, New York, 1993.
157.(a) H. Tomioka, T. Watanabe, K. Hirai, K. Furukawa, T. Takui, and K. Itoh, J. Am. Chem. Soc. 1995, 117, 6376. (b) H. Tomioka, M. Hattori, and K. Hirai, J. Am. Chem. Soc. 1996, 118, 8723. (c) H. Tomioka, T. Watanabe, M. Hattori, N. Nomura, and K. Hirai, J. Am. Chem. Soc. 2002, 124, 474.
158.Reviews of triarylmethyls: (a) V. D. Sholle and E. G. Rozantsev, Russ. Chem. Rev. 1973, 42, 1011; (b) J. M. McBride, Tetrahedron 1974, 30, 2009.
159.S. T. Bowden and T. F. Watkins, J. Chem. Soc. 1940, 1249.
160.(a) C. S. Marvel, W. H. Rieger, and M. B. Mueller, J. Am. Chem. Soc. 1939, 61, 2769.
(b) C. S. Marvel, M. B. Mueller, C. M. Himel, and J. F. Kaplan, J. Am. Chem. Soc. 1939,
61, 2771.
161.A. Rajca and S. Utamupanya, J. Org. Chem. 1992, 113, 2552.
162.(a) J. A. Kerr, A. W. Kirk, B. V. O’Grady, and A. F. Trotman-Dickenson, Chem. Commun. 1967, 365. (b) G. O. Pritchard, J. T. Bryant, and R. L. Thommarson, J. Phys. Chem. 1965, 69, 2804. (c) J. A. Kerr, B. V. O’Grady, and A.-F. Trotman-Dickenson,
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164.K. Hirai and H. Tomioka, J. Am. Chem. Soc. 1999, 121, 10213.
165. The decay curve was analyzed in terms of second-order kinetics (2k=el ¼ 1:7 10 3 s 1) in our original paper (see Ref. 164) but we found that the curve was best analyzed as a sum of two exponential decays.
166.E. Wasserman, V. J. Kuck, W. A. Yager, R. S. Hutton, F. D. Greene, V. P. Abegg, and N. M. Weinshenker, J. Am. Chem. Soc. 1971, 93, 6355.
167.(a) H. Tomioka, J. Nakijima, H. Mizuno, E. Iiba, and K. Hirai, Can. J. Chem. 1999, 77, 1066. (b) H. Itakura, and H. Tomioka, Org. Lett. 2000, 2, 2995.
168.D. J. Astles, M. Girard, D. Griller, R. J. Kolt, and D. D. M. Wayner, J. Org. Chem. 1988, 53, 6053.
169.K. Hirai, Y. Nozaki, and H. Tomioka, to be published.
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173.K. Matsuda, N. Nakamura, K. Inoue, N. Koga, and H. Iwamura, Bull. Chem. Soc. Jpn. 1996, 69, 1483.
174.H. Tomioka, M. Hattori, K. Hirai, K. Sato, D. Shiomi, T. Takui, and K. Itoh, J. Am. Chem. Soc. 1998, 120, 1106.
175.K. Sonogashira, in Comprehensive Organic Synthesis, Vol. 3, B. M. Trast and I. Fleming, Eds., Pergamon Press, Oxford, 1991, pp. 521–549.
176.T. Takui, K. Sato, D. Shiomi, K. Itoh, T. Kaneko, E. Tsuchida, and H. Nishide, in Magnetism; A Supramolecular Function, O. Kahn, Ed., Kluwer Academic Publishers, Dordrecht, The Netherlands, 1996, pp. 249–280.
177.K. Matsuda, K. Takahashi, K. Inoue, N. Koga, and H. Iwamura, J. Am. Chem. Soc. 1995, 117, 5550.

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ATOMIC CARBON |
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3.6.3. Reaction of Carbon Atoms with Thiophene . . . . . . . . . . . . . . . . . |
485 |
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3.6.4. Reaction of Carbon Atoms with Furan . . . . . . . . . . . . . . . . . . . . . |
485 |
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3.6.5. C H Insertion versus Double-Bond Addition in the |
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Reaction of Carbon with Aromatics . . . . . . . . . . . . . . . . . . . . . . . |
486 |
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3.7. Deoxygenation by Atomic Carbon . . . . . . . . . . . . . . . . . . . . . . . . . . . . |
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3.7.1. Reaction of Carbon Atoms with Alcohols and Ethers. . . . . . . . . . . |
486 |
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3.7.2. The Formation of Carbenes by Carbon Atom Deoxygenation |
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of Carbonyl Compounds. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . |
488 |
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3.7.3. Phenylnitrene by the Deoxygenation of Nitrosobenzene . . . . . . . . . |
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3.8. Other Reactions of Carbon Atoms with Lone Pairs . . . . . . . . . . . . . . . . . |
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Molecular Beam Studies of Carbon Atom Reactions . . . . . . . . . . . . . . . . . . . |
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Conclusion and Outlook . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . |
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Suggested Reading . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . |
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References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . |
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1. HISTORICAL BACKGROUND AND SCOPE
Many of the intermediates in organic reactions derive their high reactivity from the fact that they involve low-valent forms of carbon that exhibit a thermodynamic drive to form a tetravalent carbon. In this connection, zero valent atomic carbon can be considered the ultimate in low valent carbon centered reactive intermediates. Much of the attraction of this fascinating species results from the fact that, in its drive to form four bonds, it often traverses other reactive species such as carbines, carbenes, and free radicals.
Many of the early studies of atomic carbon involved atoms generated in nuclear reactions with the pioneering work of Wolf1 and Wolfgang2,3 dominating in these investigations. This ‘‘hot atom chemistry’’ formed the basis of the important use of 11C in nuclear medicine. In 1966, Skell et al.4 developed the use of the carbon arc to generate and study the reactions of carbon atoms and published an impressive array of papers documenting new C atom reactions. Since that time, a variety of methods of producing and investigating C atom reactions has been reported. Although the chemistry of atomic carbon has been the subject of several reviews,1–6 the last of these appeared in 1980 and it is clearly time to review the progress that has been made in this important field since that time. While this chapter will concentrate on reactions that have been reported since 1980, earlier studies will be mentioned in order to compare reactivities of C atoms generated by various methods. Although atomic carbon has been identified as an extraterrestrial species7 and numerous studies of its rate of reaction with simple molecules under extraterrestrial conditions have been reported, this aspect of C atom chemistry will not be included. This chapter will concentrate on C atom reactions in which products and intermediates have been identified and will not consider kinetic studies in detail.

METHODS OF GENERATING ATOMIC CARBON |
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1.1. Energies and Spin States in Carbon Atom Reactions
The heats of formation (in kcal/mol) of several representative neutral carbon centered reactive intermediates are listed in Eq. 1. It is not surprising that the energies of these species are inversely proportional to the number of bonds to carbon, rendering C atoms both difficult to generate and highly reactive. The energetics are further complicated by the fact that the ground state of atomic carbon is a triplet [Cð3PÞ Hf ¼ 171 kcal/mol] with two metastable singlet excited states [Cð1DÞHf ¼ 201 kcal/mol] and [Cð1SÞ Hf ¼ 233 kcal/mol]. Since many of the C atom reactions that have been reported involve the 1D state, this species brings an additional 30 kcal of energy to its reactions. Thus, C atom reactions are usually highly exothermic and generate products with a great deal of excess energy. This exothermicity is especially interesting when the initial product of a C atom reaction is another reactive intermediate. For example, when a carbon inserts into a C H bond to generate a carbene, the carbene is formed with >100 kcal/mol of excess energy. Since carbenes are themselves high-energy species, it is unusual to generate them with so much excess energy and unique reactions are possible. Such considerations will be discussed in detail below.
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2. METHODS OF GENERATING ATOMIC CARBON
2.1. Nucleogenic Carbon and Nuclear Medicine
As mentioned above, the first studies of C atom reactions involved the generation of
this species by nuclear reactions. Reactions that have been used include
14N(n,p) 14C,8 12C(n,2n) 11C,9 12C(g,n) 11C,10 14N( p,a) 11C,11 12C( p,pn) 11C,12
10B(d,n) 11C,13 and 11B( p,n) 11C.13 Since yields in these nuclear reactions are low, only highly sensitive radiochromatographic techniques can be used to identify the products of the C atom reactions. The technique takes advantage of the fact that these reactions generate either 14C or 11C, both of which are radioactive. The fact that only products that retain the reacting C atom can be identified is a drawback to this method from a mechanistic standpoint. However, an impressive number of substrates has been investigated and products are generally similar to those from C atoms generated by other methods. The fact that reactions of these nucleogenic C atoms often generate products containing 11C has found considerable practical advantage in nuclear medicine.14 Since 11C is a positron emitter, it can be counted in the body with noninvasive positron emission tomography (PET) techniques. The use of 11C in nuclear medicine generally involves the production of a simple molecule such as 11CO, 11CO2, or 11CN . These labeled species are then incorporated