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Download fileFluorescence in Rhoda- and Iridacyclopentadienes Neglecting the Spin–Orbit Coupling of the Heavy Atom: The Ligand Dominates
dataset
posted on 2014-07-07, 00:00 authored by Andreas Steffen, Karine Costuas, Abdou Boucekkine, Marie-Hélène Thibault, Andrew Beeby, Andrei
S. Batsanov, Azzam Charaf-Eddin, Denis Jacquemin, Jean-François Halet, Todd B. MarderWe present a detailed
photophysical study and theoretical analysis
of 2,5-bis(arylethynyl)rhodacyclopenta-2,4-dienes (1a–c and 2a–c)
and a 2,5-bis(arylethynyl)iridacyclopenta-2,4-diene (3). Despite the presence of heavy atoms, these systems display unusually
intense fluorescence from the S1 excited state and no phosphorescence
from T1. The S1 → T1 intersystem
crossing (ISC) is remarkably slow with a rate constant of 108 s–1 (i.e., on the nanosecond time scale). Traditionally,
for organometallic systems bearing 4d or 5d metals, ISC is 2–3
orders of magnitude faster. Emission lifetime measurements suggest
that the title compounds undergo S1 → T1 interconversion mainly via a thermally activated ISC channel above
233 K. The associated experimental activation energy is found to be
ΔHISC⧧ = 28 kJ mol–1 (2340
cm–1) for 1a, which is supported by
density functional theory (DFT) and time-dependent DFT calculations
[ΔHISC⧧(calc.) = 11 kJ mol–1 (920 cm–1) for 1a-H]. However, below
233 K a second, temperature-independent ISC process via spin–orbit
coupling occurs. The calculated lifetime for this S1 →
T1 ISC process is 1.1 s, indicating that although this
is the main path for triplet state formation upon photoexcitation
in common organometallic luminophores, it plays a minor role in our
Rh compounds. Thus, the organic π-chromophore ligand seems to
neglect the presence of the heavy rhodium or iridium atom, winning
control over the excited-state photophysical behavior. This is attributed
to a large energy separation of the ligand-centered highest occupied
molecular orbital (HOMO) and lowest unoccupied MO (LUMO) from the
metal-centered orbitals. The lowest excited states S1 and
T1 arise exclusively from a HOMO-to-LUMO transition. The
weak metal participation and the cumulenic distortion of the T1 state associated with a large S1–T1 energy separation favor an “organic-like” photophysical
behavior.