I. Wiater, J. G. P. Born, R. Louw
FULL PAPER
[23]
[24]
R. B. Woodward, R. Hoffmann, The Conservation of Orbital
Symmetry, Acad. Press, 1970, chapter 7.
Physical and Chemical Aspects of Combustion (Eds.: F. L.
Dryer, R. F. Sawyer), Gordon and Breach, 1997, chapters 1
and 4.
Some samples were concentrated by solvent evaporation with a
gentle stream of N2, to allow better measurement of trace products.
Synthesis of 2-Phenoxyphenol: 2-Phenoxyphenol was prepared ac-
cording to the procedure described in ref.[38] A comparable amount
of DD was formed. The product mixture was liquefied in toluene,
treated with 10% KOH and extracted with water. This extract was
acidified with diluted HCl, extracted with toluene and checked by
GC-MS. Toluene was gently evaporated with a stream of N2. The
crystalline product was dissolved in n-pentane and was kept at –20
°C for a few days for recrystallisation. The purity of the sample
used in the slow combustion with benzene was checked by GC to
be 99% (1% of DD).
[25]
[26]
[27]
[28]
P. Mulder, R. Louw, J. Chem. Soc., Perkin Trans. 2 1986,
1541–1550.
Z. Tao, Z. Li, Int. J. Chem. Kinet. 1999, 31, 65–72 and refer-
ences cited therein.
Thermochemical Data of Organic Compounds (Eds.: J. B. Ped-
ley, R. D. Naylor, S. P. Kirby), Chapman and Hall, NY, 1986.
This approach means that the C–OH bond strengths in A and
C are taken to be identical to that in phenol. Likewise,
∆Hf0298 of hydroxy-biphenyl should be ca. 0 kcal/mol. Remark-
ably, the NIST compilation,[10] based on the original French
paper,[37] advocates ϩ8.5 for the p-isomer and 4 kcal/mol for
ortho-hydroxybiphenyl. The idea that these C–OH bonds are
much (4–8.5 kcal) weaker than in phenol and the idea that the
para form should be no less than 4 kcal destabilized relative to
ortho form must be in error.
[1]
Beilsteins Handbuch der Organischen Chemie 1933, XVII, 71.
[2]
R. Cypres, B. Bettens, Tetrahedron 1975, 31, 359–365.
[3]
J. G. P. Born, R. Louw, P. Mulder, Chemosphere 1989, 19,
401–406.
J. G. P. Born, Ph. D. Thesis 1992, Leiden University (in En-
glish).
I. W. C. E. Arends, R. Louw, P. Mulder, J. Phys. Chem. 1993,
97, 7914–7925.
Ref.[10] advances that ∆Hf0298 (IV) ϭ –17 ± 3 kcal/mol, so
roughly only 6 kcal greater than that of phenol. As will be ex-
plained in more detail elsewhere,[30] this cannot be correct. One
argument is that it would make VI about 5 kcal more stable
than allyl phenyl ether, with the consequence that, contrary to
observation,[32] the gas-phase Claisen rearrangement should
also proceed in an inert environment (enolisation of VI occur-
ring after cooling and condensing the reactant vapours). An-
other reason for rejecting this is that the value of –17 kcal/
mol for IV is very much lower than that calculated from group
additivity, from cyclohexadiene (25) and the increment for Cϭ
O replacing –CH2–, i.e., –25, hence 0 kcal/mol; it is unrealistic
to have an additional delocalization energy of more than
15 kcal/mol in this dienone system.
[29]
[4]
[5]
[6]
H. H. Grotheer, R. Louw, 26th Symp.(Int.) on Combustion
1996, 2405–2411.
[7]
S. S. Sidhu, L. Maqsud, B. Dellinger, G. Mascolo, Comb. and
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[8]
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[9]
W. M. Shaub, W. Tsang, Environ.Sci. Technol. 1983, 17, 721–
730.
[10]
NIST Chemistry WebBook (Ed.: W. G. Mallard), NIST Stand-
[30]
[31]
[32]
[33]
R. Louw, D. Santoro, (to be) submitted to J. Phys. Chem.
R. Weber, H.-P. Hagenmaier, Chemosphere 1999, 38, 529–549.
R. Louw, Recl. Trav. Chim. Pays-Bas 1971, 90, 1119–1122.
ard Reference, Database 69 – November 1998 Release, Na-
tional Institute of Standards and Technology, Gaithersburg,
MD, 1998.
[11]
With ∆Hf0298 values of –1 kcal/mol for PhO–CH2–CHϭCH2,
and ϩ7 kcal/mol for VI, and accepting rate parameters for the
forward reaction: log A/s–1 ϭ 11, Ea ϭ 32, those for the reversal
of VI to starting compound will be log A ഠ 11 and E ϭ
24 kcal/mol. At 800 K this means k ഠ 104.4 s–1. The vapour of
added acetic acid could make the ‘‘rate constant’’ for competi-
tive enolisation equal to or larger than this.
D. M. Chipman, R. Liu, X. Zhou, P. Pulay, J. Chem. Phys.
1994, 100, 5023–5035.
[12]
Y. Qin, R. A. Wheeler, J. Chem. Phys. 1995, 102, 1689–1698.
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[14]
M. F. R. Mulcahy, D. J. Williams, Aust. J. Chem. 1965, 18,
20–38.
[34]
[35]
[36]
[15]
P. Frank, J. Herzler, T. Just, C. Wahl, Symp. Int. Combust. Proc.
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[16]
M. Foti, K. U. Ingold, J. Lusztyk, J. Am. Chem. Soc. 1994,
P. M. Sommeling, P. Mulder, R. Louw, D. V. Avila, J. Lusztyk,
K. U. Ingold, J. Phys. Chem. 1993, 97, 8361–8364.
116, 9440–9447.
[17]
W. A. Waters, C. Wickham-Jones, J. Chem. Soc. 1951, 812–823.
Without detailing the thermochemistry, reaction (a) is ca.
47 kcal endothermic, while the reactions by (b)–(d) are associ-
ated with activation barriers of some 35 kcal/mol. While scis-
sion (a) will have an Arrhenius A value of ca. 1015 s–1, the other
are intramolecular additions with much lower A values, e.g.,
1010 s–1. As a result, (a) can effectively compete with (b)–(d),
the more so at higher temperatures.
G. Bertholon, M. Giray, R. Perrin, M.-F. Vincent-Falaquet-
Bernet, Bull. Soc. Chim. France 1971, 9, 3180.
E. Klarmann, L. W. Gates, V. A. Shternov, J. Am. Chem. Soc.
[18] [18a] R. F. Moore, W. A. Waters, J. Chem. Soc. 1954, 243–246. –
[18b]
E. C. Horswill, K. U. Ingold, Can. J. Chem. 1966, 44 (3),
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[19]
Comprehensive Organic Chemistry, Vol. 5 (Ed.: E. Haslam),
Pergamon Press, New York, 1979, Ch. 29, pp. 956–957.
[20]
D. Wang, I. György, K. Hildenbrand, C. von Sonntag, J. Chem.
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[38]
[39]
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[21]
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1435.
[22]
1932, 54, 1204–1211.
The standard heats of formation are –18 kcal/mol for anisole
and approximately –30 kcal/mol for o- and p-cresol. The
‘‘keto’’ structures of the latter make them some 15 kcal/mol less
stable;[33] their heats of formation and hence methyl–R bond
strengths are close to that of anisole.
P. Franchi, M. Lucarini, G. F. Pedulli, L. Valgimigli, B. Lunelli
J. Am. Chem. Soc. 1999, 121, 507–514.
Received June 18, 1999
[O99364]
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