Hydrogen transfer in excited pyrrole–ammonia clusters
Author(s) -
Olivier David,
C. DedonderLardeux,
Christophe Jouvet,
Hyuk Kang,
S. Martrenchard,
Takayuki Ebata,
Andrzej L. Sobolewski
Publication year - 2004
Publication title -
the journal of chemical physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.071
H-Index - 357
eISSN - 1089-7690
pISSN - 0021-9606
DOI - 10.1063/1.1704639
Subject(s) - chemistry , excited state , picosecond , cluster (spacecraft) , ionization , kinetic energy , reaction mechanism , ammonia , evaporation , atomic physics , kinetic isotope effect , reaction dynamics , photochemistry , deuterium , molecule , ion , physics , laser , organic chemistry , quantum mechanics , computer science , optics , thermodynamics , programming language , biochemistry , catalysis
The excited state hydrogen atom transfer reaction (ESHT) has been studied in pyrrole-ammonia clusters [PyH-(NH(3))(n)+hnu-->Py.+.NH(4)(NH(3))(n-1)]. The reaction is clearly evidenced through two-color R2P1 experiments using delayed ionization and presents a threshold around 235 nm (5.3 eV). The cluster dynamics has also been explored by picosecond time scale experiments. The clusters decay in the 10-30 ps range with lifetimes increasing with the cluster size. The appearance times for the reaction products are similar to the decay times of the parent clusters. Evaporation processes are also observed in competition with the reaction, and the cluster lifetime after evaporation is estimated to be around 10 ns. The kinetic energy of the reaction products is fairly large and the energy distribution seems quasi mono kinetic. These experimental results rule out the hypothesis that the reaction proceeds through a direct N-H bond rupture but rather imply the existence of a fairly long-lived intermediate state. Calculations performed at the CASSCF/CASMP2 level confirm the experimental observations, and provide some hints regarding the reaction mechanism.
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