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Pressure dependency for heavy isotope enhancement in ozone formation
Author(s) -
Thiemens Mark H.,
Jackson Teresa
Publication year - 1990
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/gl017i006p00717
Subject(s) - ozone , isotope , kinetic energy , kinetic isotope effect , chemistry , analytical chemistry (journal) , materials science , environmental chemistry , atomic physics , physics , deuterium , organic chemistry , nuclear physics , quantum mechanics
It has previously been shown that a 18 O, 17 O mass independent isotopic enrichment accompanies O 3 formation. Precise definition of the mechanism has proven difficult and further experimental characterization of the mediating parameters is needed. The potential role of activated complex lifetime is determined by measuring the effect of pressure in the region where third body kinetic fall‐off is known to occur (∼ 4 atmospheres). In the pressure region ∼ 8 to 45 atmospheres, the 18 O, 17 O enrichment decreases by nearly 84‰. For pressures between 45 to 66 atmospheres (1.6 × 10 21 molecules cm −3 ), the enhancement decreases by only 6‰ and is absent (δ 18 O = O) at 56 atmospheres. For pressures 56 to 87 atm, the product ozone is depleted in 18 O in a nearly mass dependent fashion. The decrease in O 3 ‐ 18 O enrichment with pressure initiates at a significantly lower pressure than expected, based upon the known reaction order pressure dependency. At present, no theoretical model quantitatively accounts for the observations.