Photoactive chromium(III) complexes saw a conceptual
breakthrough
with the discovery of the prototypical molecular ruby mer-[Cr(ddpd)2]3+ (ddpd = N,N′-dimethyl-N,N′-dipyridin-2-ylpyridine-2,6-diamine), which shows intense
long-lived near-infrared (NIR) phosphorescence from metal-centered
spin-flip states. In contrast to the numerous studies on chromium(III)
photophysics, only 10 luminescent molybdenum(III) complexes have been
reported so far. Here, we present the synthesis and characterization
of mer-MoX3(ddpd) (1, X =
Cl; 2, X = Br) and cisfac-[Mo(ddpd)2]3+ (cisfac-[3]
3+
), an isomeric heavy homologue of the prototypical
molecular ruby. For cisfac-[3]
3+
, we found strong zero-field splitting using magnetic
susceptibility measurements and electron paramagnetic resonance spectroscopy.
Electronic spectra covering the spin-forbidden transitions show that
the spin-flip states in mer-1, mer-2, and cisfac-[3]
3+
are much lower in energy than those in
comparable chromium(III) compounds. While all three complexes show
weak spin-flip phosphorescence in NIR-II, the emission of cisfac-[3]
3+
peaking
at 1550 nm is particularly low in energy. Femtosecond transient absorption
spectroscopy reveals a short excited-state lifetime of 1.4 ns, 6 orders
of magnitude shorter than that of mer-[Cr(ddpd)2]3+. Using density functional theory and ab initio multireference calculations, we break down the
reasons for this disparity and derive principles for the design of
future stable photoactive molybdenum(III) complexes.