![]() |
|
![]() |

Triplet Emitters and
Control of Emission Properties
Hartmut Yersin
Institut für Physikalische Chemie, Universität Regensburg
D-93040 Regensburg, Germany
E-mail: hartmut.yersin@chemie.uni-regensburg.de
Abstract
Essential photophysical properties of organometallic triplet emitters depend systematically on the metal participation in the triplet states and on the effective spin-orbit coupling. These factors control the amount of zero-field splitting (ZFS) of the triplet state into substates. Increase of ZFS corresponds to higher metal character in the triplet state. Higher metal character reduces the energy difference between excited singlet and triplet states, enhances the singlet-triplet intersystem crossing rate, lowers the emission decay time, changes the vibrational satellite structure, decreases the excited state geometry change, leads to a stronger electronic coupling between the ligands etc.. These effects are discussed by referring to well characterized compounds. Based on the new ordering scheme presented for triplet emitter materials, a controlled development of compounds with pre-defined photophysical properties becomes possible.
1. Ordering scheme for organometallic triplet emitters
Many
photophysical properties of the lowest excited triplet states and the
corresponding transitions of organometallic compounds are essentially
determined by the extent of metal participation in the wavefunctions.
This metal participation does not only alter the spatial extension of
the wavefunctions, but it also induces significant mixtures of singlet
and triplet states by spin-orbit coupling (SOC) which is mainly carried
by the metal orbitals. It is of interest to develop an understanding
how these effects influence the photophysical properties of emitter
materials. Indeed, this is possible. Moreover, it can be shown that a
simple ordering scheme can be helpful in this respect. [1-5]
Specifically, the energy splitting of the triplet state into substates,
the zero-field splitting (ZFS) measured in cm-1,
can be utilized, since this parameter displays the importance of metal
character and SOC for the respective triplet state.
The
amount of ZFS is usually determined spectroscopically. Nevertheless, it
is instructive to visualize that it is dominantly controlled by
specific interactions. For example, the splitting of a pure 3ππ*
state which is not metal-perturbed is only given by spin-spin
interactions (e.g. see [6-8]). In this situation, the ZFS is of the
order of 0.1 cm-1.
However, if 3MLCT
and 1MLCT
states are in proximity (MLCT = metal-to-ligand charge transfer), the
substates of these latter states will interact due to SOC with the
substates of the 3ππ*
term. This can lead to a significant triplet splitting in particular,
when 5d orbitals are involved in the 1,3MLCT
states. As consequence, the ZFS can increase by more than three orders
of magnitude, for example, up to
Fig. 1: Ordering scheme for organometallic triplet emitters according to the amount of zero-field splitting (ZFS) of the emissive triplet state. This splitting reflects the size of metal participation (MLCT and/or d-orbital character) and spin-orbit coupling in the corresponding wavefunctions. The diagrams at the bottom show energy levels of the relevant frontier molecular orbitals for the different compounds. For detailes see text. (Compare [5] and for the Ir(III) compounds [13-15].)
Fig.
1
shows a sequence of a series of compounds which are arranged according
to an increasing ZFS of the emissive triplet state. The ZFS values of
most of the compounds have been determined from highly resolved optical
spectra. [1-5] (References for the individual compounds are given in
[5].) Only for Ir(ppy)3
[13] and Ir(ppy)2(CO)(Cl)
[14] such resolved spectra were not yet obtainable, and therefore the
information was determined indirectly from the temperature dependence
of the emission decay time.
The
low-lying electronic states of the compounds shown in Fig. 1 have to be
assigned to different types of frontier orbital transitions. Thus, the
lowest triplets of [Rh(bpy)3]3+
and [Pt(bpy)2]2+
are characterized as ligand centered 3LC(3ππ*)
states with very small metal admixtures and those of
2. Photophysical properties of triplet emitters controlled by metal participation
The energy splitting (ZFS) of a triplet state into substates displays the importance of metal character and spin-orbit coupling for this state. The ZFS value varies by more than a factor of 2000 (Fig. 1). Thus, essential changes of photophysical properties are expected to occur. Several important trends will be discussed in the following subsections. This is carried out on a qualitative and introductory basis. (Fig. 2) For comparison, properties of typical organic molecules (ππ* emitters) are also referred to.
2.1 Singlet-triplet splitting
Organic molecules exhibit S1 – T1 splittings being typically of the order of 104 cm-1 (Fig. 2) for states which stem from a ππ* configuration and for molecules of similar sizes like those shown as ligands in Fig. 1. The ΔE(S1-T1) splitting is essentially given by the exchange interaction and is a consequence of electron-electron interaction. For an organo-metallic compound, such as Pd(thpy)2, one finds a value of 5418 cm-1 [5]. The emissive triplet of this compound has been classified experimentally [5, 16-18] and later also by CASPT2 ab initio calculations [19] as being mainly of LC(ππ*) character with a small MLCT(4dπ*) admixture. Therefore, the compound is found at the left hand side of the ordering scheme of Fig. 1. [5] On the other hand, for Pt(thpy)2 with a significant MLCT(5dπ*) admixture to the LC(ππ*) state [4, 5], the amount of ΔE(S1-T1) is reduced to 3278 cm-1 [5]. (Fig. 2) Obviously, enhancing of metal character in the corresponding wavefunctions increasingly reduces the ΔE(S1-T1) value. Due to the higher metal character, the electronic wavefunctions extend over a larger spatial region of the complex. This is connected to an on average larger spatial separation between the interacting electrons. Thus, electron-electron interaction and also exchange interaction are reduced. This explains both the lowering of the S1 state and the reduction of ΔE(S1-T1) for compounds with higher metal character.
Fig. 2: Photophysical properties of a representative organic molecule compared to two organo-transition-metal emitters. The emissive triplets of Pd(thpy)2 and Pt(thpy)2 exhibit small and significant MLCT admixtures to the LC(ππ*) states, respectively. The positions of the compounds in the ordering scheme and the molecular structures are found in Fig. 1. Photophysical properties of Pd(thpy)2 and Pt(thpy)2 are discussed in detail in [5]. lig. vibr. = ligand vibrations, M-L vibr. = metal-ligand vibration.
2.2. Inter-system crossing
After excitation of the singlet state S1
either optically or by electron-hole recombination, the organic
molecule can exhibit an efficient fluorescence (S1→
S0
emission) with a time constant of the order of 1 ns. In competition to
this process, ISC can at least principally depopulate the S1
state. However, the time constant of τ(ISC)
is often much
larger (order of 10 to 100 ns) than the radiative decay constant of the
S1
state and thus ISC does not effectively quench the
fluorescence. (Fig. 2) On the other hand, in transition metal
complexes, the ISC time is drastically reduced due to singlet-triplet
mixing induced by SOC and due to the reduction of the energy separation
ΔE(S1-T1).
Further, due to this latter effect, the number of vibrational quanta
which are responsible for the deactivation is reduced and thus the ISC
process becomes even more probable. For example, already for a
compound, such as Pd(thpy)2,
with a relatively small metal participation in the wavefunction of the T1
state and a halved ΔE(S1-T1)
value, ISC is by four to five orders of magnitude faster (800 ps [5])
than in usual organic compounds with 1ππ*
and 3ππ*
states. For Pt(thpy)2
with a higher metal participation, the process is again much faster
(τ(ISC)
≈ 50 fs [5]). (Fig. 2)
In
conclusion, the process of inter-system crossing in organometallic
compounds with transition metal ions is fast and efficient for all
compounds shown in Fig. 1. The quantum efficiency for this process is
often nearly one. Therefore, an emission from the S1
state is not observable. This property is the basis of the triplet
harvesting effect in OLEDs which are based on triplet emitters. [33]
2.3. Phosphorescence decay time
In pure
organic molecules, the S0(π2)
↔ T1(ππ*)
transition is usually strongly forbidden. The radiative decay time can
be of the order of 10 s. [20] On the other hand, non-radiative
processes are mostly much faster. Thus, phosphorescence from the T1
state is normally totally quenched at ambient temperature. With
increasing SOC, the radiative decay time of the T1
→ S0
transition is reduced and thus the radiative path can compete
with the non-radiative one. Interestingly, already a relatively small 3MLCT/1MLCT
admixture to the 3LC(ππ*)
state increases the S0
↔ T1
transition probability drastically. For example, for Pd(thpy)2
the radiative decay time is reduced to be of the order of 1
ms. For Pt(thpy)2
with a significant MLCT admixture to the lowest 3LC
state, it is even reduced by six to seven orders of magnitude as
compared to the organic emitters, and one finds a radiative decay time
of the order of 1 μs. (Fig. 2) For completeness, it is remarked
that the values given refer to an average radiative decay of the
triplet, since the different triplet substates exhibit distinctly
different decay properties (e.g. see the following sub-section and
[5]).
In
summary, for organometallic compounds the transition probability
between the T1
and the S0
states can be tuned by several orders of magnitude as compared to
organic emitters. This is mainly induced by an increase of spin-orbit
coupling. Thus, the radiative processes can well compete with the
non-radiative ones. Consequently, organo-transition-metal compounds can
exhibit efficient emissions (phosphorescence) and therefore are well
suited as emitter materials for OLEDs.
2.4. Zero-field splitting
Triplet
states split generally into substates. This is also valid for purely
organic molecules. However, for these one finds only small values of
ZFS of the order of 0.1 cm-1
which result from spin-spin coupling between the electrons in the π
and π*
orbitals, respectively (e.g. see
[6-8]). On the other hand, in organo-transition-metal compounds SOC
will modify the triplet states’ properties by mixing in
higher lying states of singlet and triplet character. Already small
admixtures have drastic consequences. For example, one finds an
increase of the ISC rate (see above) and of the phosphorescence decay
rate (see previous subsection) by orders of magnitude, although the ZFS
is not yet distinctly altered. [5] Well studied examples with this
behavior are [Rh(bpy)3]3+
and Pd(qol)2 (=Pdq2).
[7, 21, 22]
Higher
metal participation and larger SOC lead to distinct ZFSs as has already
been discussed and depicted in Fig. 1. Importantly, the individual
triplet substates can have very different photophysical properties with
regard to radiative decay rates, vibronic coupling, coupling to the
environment, emission quantum yields, population and relaxation
dynamics due to spin-lattice relaxation, sensitivity with respect to
symmetry changes, etc.. [1-5, 7, 13, 14, 16-18, 21-25] At ambient
temperature, the individual properties are largely smeared out and one
finds mostly only an averaged behavior. Nevertheless, the individual
triplet substates still determine the overall emission properties.
2.5. Emission band structure and vibrational satellites
At
ambient temperature, the phosphorescence of organometallic compounds
consists usually of superimposed spectra, which stem from the different
triplet substates (see previous subsection, Fig. 2). An individual
spectrum which results from one specific substate is composed of a
transition at the electronic origin (0-0 transition), a large number of
vibrational satellites, and of in part overlapping low-energy
satellites which involve librations of the complex in its environment.
Moreover, all of these individual transitions are smeared out by
inhomogeneity effects. Thus, at ambient temperature normally only a
broad-band emission results. Sometimes residual, moderately resolved
structures occur, which often stem from overlapping vibrational
satellites (not necessarily from progressions). Interestingly, at low
temperature and under suitable conditions, these structures
can be well resolved and characterized. [1-5, 15-18, 21-32] From this
kind of investigations it follows that also the vibrational satellite
structure is influenced by metal praticipation in the electronic
states. [29] Specifically, the spectra of compounds with electronic
transitions of mainly LC(ππ*)
character (small metal participation) are largely determined
by satellites corresponding to ligand vibrations (fundamentals,
combinations, progressions). However, with increasing metal
participation, low-energy vibrational satellites of metal-ligand
character grow in additionally (up to about 600 cm-1
from the electronic origin). [29] (Fig. 2) Thus, the maximum of the
unresolved emission spectrum shifts towards the electronic 0-0
transition.
To
summarize, metal participation in the emitting state leads to a slight
blue shift of the unresolved emission maximum as compared to an LC
spectrum with the same 0-0 transition energy. Moreover, the occurrence
of additional low-energy metal-ligand vibrational satellites causes a
further smearing out of the spectrum. In particular, the slight
spectral shift might be of interest for fine-tuning of the emission
color.
2.6. Electronic charge distribution and excited state reorganization
The
singlet-triplet transitions of compounds with small metal character,
situated on the left hand side of Fig. 1, are localized to one of the
ligands, even if the formal symmetry of the complex would allow a
delocalization over all of the ligands. This has been proven for
[Rh(bpy)3]3+
[21] and
oreover,
since the metal character or MLCT contribution in the triplet state, if
sufficiently large, can induce a ligand-ligand coupling that
delocalizes the excited state wavefunction, the metal
contribution will also affect the geometry change that follows an
excitation. For the localized situation in the compounds mentioned
above, one finds a maximum Huang-Rhys parameter [5] of S = 0.3, while
for the compounds with delocalized triplets, this
characteristic parameter is by a factor of three to four
smaller. [2, 5] Geometry changes or reorganization effects
which occur upon excitation of the emissive triplet states are small
for nearly all of the complexes investigated (in rigid matrices). But
still, it can be concluded that the reorganization effects are further
minimized for those organometallic compounds with high metal
participation in the triplet states (complexes at the right hand side
of Fig. 1). The emissive states of these compounds exhibit a weaker
coupling to the environment and therefore represent good
candidates for OLED emitter materials with high emission quantum yields.
3. Conclusion
On the basis of a detailed knowledge about the photophysical properties of organo-transition-metal emitters, clear trends are elucidated for triplet emitters. This leads to the possibility to control important factors, such as metal participation and spin-orbit coupling in the triplet states, by chemical variation. Thus, the controlled development of compounds with predefined photophysical properties will be achievable. Specifically, increase of metal participation and SOC is displayed in a growing zero-field splitting of the triplet into substates. This parameter can be determined experimentally. The corresponding ZFS values of the compounds discussed in this investigation vary by more than a factor of 2000. In particular, increasing metal character lowers the energy of the excited singlet, reduces the energy separation between the excited singlet and triplet states, enhances the intersystem crossing rate from the lowest excited singlet to the lowest triplet, lowers the emission decay time by increasing the corresponding radiative rate, changes the vibrational satellite structure and thus the spectral distribution of the emission band, decreases the excited state reorganization energy, etc.. This promising new concept can, for example, usefully be applied to develop new triplet emitter materials for more efficient OLEDs. [33]
4. References
| 1. | Yersin H., Humbs W., Strasser J.; Coord. Chem. Rev. 1997, 159, 325 |
| 2. | Yersin H., Humbs W., Strasser J.; Top. Curr. Chem. 1997, 191, 153 |
| 3. | Yersin H., Strasser J.; J. Luminescence 1997, 72-74, 462 |
| 4. | Yersin H., Humbs W.; Inorg. Chem. 1999, 38, 5820 |
| 5. | Yersin H., Donges D.;&xnbsp; Top. Curr. Chem. 2001, 214, 81 |
| 6. | Lumb M. D. (ed); Luminescence Spectroscopy, Academic Press, London 1978 |
| 7. | Glasbeeek M.; Top. Curr. Chem. 2001, 213, 95 |
| 8. | Azumi T., Miki H.; Top. Curr. Chem. 1997, 191, 1 |
| 9. | Komada Y., Yamauchi S., Hirota N.; J. Phys. Chem. 1986, 90, 6425 |
| 10. | Ikeda S., Yamamoto S., Nozaki K., Ikeyama T., Azumi T., Burt J.A., Crosby G.A.; J. Phys. Chem. 1991, 95, 8538 |
| 11. | Colombo M.G., Hauser A., Güdel H.U.; Top. Curr. Chem. 1994, 171, 143 |
| 12. | Funayama T., Kato M., Kosugi H., Yagi M., Higuchi J., Yamauchi S.; Bull. Chem. Soc. Jpn. 2000, 73, 1541 |
| 13. | Finkenzeller W.J., Yersin H.; Chem. Phys. Lett. 2003, 377, 299 |
| 14. | Finkenzeller W.J., Stoessel P., Yersin H.; Chem. Phys. Lett. 2004, 397, 289 |
| 15. | Hay P.J.; J. Phys. Chem. A 2002, 106, 1634 |
| 16. | Yersin H., Schützenmeier S., Wiedenhofer H., von Zelewsky A.; J. Phys. Chem. 1993, 97, 13496 |
| 17. | Schmidt J., Wiedenhofer H., von Zelewsky A., Yersin H.; J. Phys. Chem. 1995, 99, 226 |
| 18. | Glasbeek M., Sitters R., van Veldhofen E., von Zelewsky A., Humbs W., Yersin H.; Inorg. Chem. 1998, 37, 5159 |
| 19. | Pierloot K., Ceulemans A., Merchán M., Serrano-Andrés L.; J. Phys. Chem. A 2000, 104, 4374 |
| 20. | Turro N.; Modern molecular photochemistry. Benjamin/Cummings Publ., Menlo Park, California, USA 1978 |
| 21. | Humbs W., Yersin H.; Inorg. Chem. 1996, 35, 2220 |
| 22. | Yersin H., Donges D., Nagle J.K., Sitters R., Glasbeek M.; Inorg. Chem. 2000, 39, 770 |
| 23. | Yersin H., Strasser J.; Coord. Chem. Rev. 2000, 208, 331 |
| 24. | Strasser J., Homeier H.H.H., Yersin H.; Chem. Phys. 2000, 255, 301 |
| 25. | Yersin H., Donges D., Humbs W., Strasser J., Sitters R., Glasbeek M.; Inorg. Chem. 2002, 41, 4915 |
| 26. | Wiedenhofer H., Schützenmeier S., von Zelewsky A.; Yersin H.; J. Phys. Chem. 1995, 99, 13385 |
| 27. | Yersin H., Kratzer C.; Coord. Chem. Rev. 2002, 229, 75 |
| 28. | Yersin H., Kratzer C.; Chem. Phys. Lett. 2002, 362, 365 |
| 29. | Yersin H., Huber P., Wiedenhofer H.; Coord. Chem. Rev. 1994, 132, 35 |
| 30. | Humbs W., Yersin H.; Inorg. Chim. Acta. 1997, 265, 139 |
| 31. | Braun D., Huber P., Wudy J., Schmidt J., Yersin H.; J. Phys. Chem. 1994, 98, 8044 |
| 32. | Huber P., Yersin H.; J. Phys. Chem. 1993, 97, 12705 |
| 33. | Yersin H.; Top. Curr. Chem. 2004, 241, 1 |