Kinetic energy releases (KERs) in unimolecular fragmentations of singly and multiply charged ions provide information concerning ion structures, reaction energetics and dynamics. This topic is reviewed covering both early and more recent developments. The subtopics discussed are as follows: (1) introduction and historical background; (2) ion dissociation and kinetic energy release: kinematics; potential energy surfaces; (3) the kinetic energy release distribution (KERD); (4) metastable peak observations: measurements on magnetic sector and time-of-flight instruments; energy selected results by photoelectron photoion coincidence (PEPICO); (5) extracting KERDs from metastable peak shapes; (6) ion structure determination and reaction mechanisms: singly and multiply charged ions; biomolecules and fullerenes; (7) theoretical approaches: phase space theory (PST), orbiting transition state (OTS)/PST, finite heat bath theory (FHBT) and the maximum entropy method; (8) exit channel interactions; (9) general trends: time and energy dependences; (10) thermochemistry: organometallic reactions, proton-bound clusters, fullerenes; and (11) the efficiency of phase space sampling.
An in-line double mass spectrometer has been employed to determine reaction rate coefficients and excitation functions for several types of negative ion reactions involving ozone. The interactions studied include electron transfer reactions, such as, M−+O3→M+O3− (where M−=O−, OH−, F−, Cl−, Br−, I−, S−, SH−, Cl−2, C2H−, NO2−, and CO3−) and particle transfer reactions, such as MO−+O2→M+O3− (where MO−=O2−, NO2−, NO3−, CO3−). Translational energy thresholds have been determined for those reactions which are endothermic by applying exact Doppler corrections for the thermal motion of the neutral as well as corrections for the translational energy distribution of the projecticle ions. These experiments place a lower limit of 2.26+0.04−0.06 eV on the electron affinity of ozone. This value is in excellent agreement with the value computed from the bond dissociation energy of O3− in its most stable configuration, D00(O−–O2) =1.80 eV, as deduced from measurements of the translational energy thresholds for the collisional dissociation process, O−3+M→O−+O2+M, where M=He, Ar. Further implications of these experiments with respect to the structure, thermochemistry, and excited states of O−3 are discussed.
Unimolecular fragmentations of the anthracene and phenanthrene
radical cations
C14H10
•+ were
studied by
time-resolved photoionization in the vacuum UV, RRKM/QET calculations,
and MS/MS with electron
ionization. The primary reactions observed are parallel
H•, H2, C2H2,
C3H3
•, and
C4H2 losses, as well as two
consecutive H• losses from
C14H9
+ and
C12H8
•+,
respectively. Appearance energies were determined for
the
microsecond and millisecond time ranges. Activation parameters
were deduced for the reactions. The H•
and C2H2 loss reactions are characterized by
loose transition states. The following heats of formation
were
deduced: ΔH
f0°
(C14H9
+, anthracenyl) = 282.0
± 3.0 kcal/mol,
ΔH
f0°(C14H9
+,
phenanthrenyl) = 276.4 ±
3.0 kcal/mol and
ΔH
f0°(C12H8
•+,
biphenylene) ≤ 281.7 ± 3.0 kcal/mol. The C−H bond energies in
the
anthracene and phenanthrene radical cations are 4.38 ± 0.08 and 3.92
± 0.10 eV, respectively. The role of
isomerization of the parent radical cations prior to dissociation will
be discussed.
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