Exciton Simulation¶
Opto-electronic processes are defined in the kMC simulation to model OLED emission. In this example, a phosphorescent emitter is considered. Loss processes are included using both Dexter and Förster mechanisms.
Create Materials¶
To construct the OLED device stack, we will create an electron transport layer, a hole transport layer and a host-guest emitter. This requires the definition of 4 materials.
Phosphorescent Dye¶
Ir(ppy)3 is used as the phosphorescent dye. We will select the corresponding template when creating a new material.
On the Electronic tab, we specify a HOMO level of -5.27 eV and a LUMO level of -1.86 eV. A Gaussian broadening is enabled by default.
Several material-specific parameters are specified to describe exciton generation and emission. These parameters are set on the Excitonic tab of the material editor.
We will set a singlet binding energy of 0.75 eV and a triplet binding energy of 1 eV. By enabling the option to link the singlet and triplet binding energies, the exciton energy levels will be computed automatically based on the exciton binding energy and the HOMO/LUMO levels.
An energy level broadening is defined for the exciton levels, just as we did for the polaron levels, accounting for the variations in molecular parameters due to the inhomogeneous environment of the layer. A Gaussian broadening is used, this time with a width of 0.05 eV.
To describe Dexter-type exciton diffusion, Dexter transfer parameters are specified. We choose a prefactor of 1, with a decay length of 0.3 nm.
Note
The rates of transfer processes is specified in normalized units. I.e. the true prefactor is multiplied by a normalization factor. This time unit is specified in the parameter set.
This decomposition allows us to write the material parameters using convenient factors.
In contrast, the radiative processes are provided in natural units, without normalization. These parameters specify the real frequency in the input, with normalization applied internally by Bumblebee.
By selecting the phosphorescent material template, the singlet fractions will have been set to 0, such that the exciton generation products will exclusively be triplets.
An intersystem crossing rate of \(10^{10}\,\textrm{s}^{-1}\) will be specified. The reverse intersystem crossing rate is set to 0. This allows any singlets obtained through e.g. exciton transport to be irreversibly converted to triplets.
The radiative decay rate of the triplet excitons is set to \(6.1\cdot{}10^{5}\,\textrm{s}^{-1}\). The non-radiative decay rate is set to \(1.9\cdot{}10^{4}\,\textrm{s}^{-1}\). The photoluminescent and electroluminescent quantum yields of the dye are now reported to provide an indication of the molecular emitter efficiency.
Note
Förster processes will be configured in the stack editor. Because Förster transfer describes a dipolar process, the rate parameters exhibit strong variations with molecular environment. The stack editor allows definition of custom rates for inter-layer transfer processes, and allows definition of multiple intra-layer Förster processes to account for more complex rate expressions.
Host¶
CBP is used as a host material. Select the appropriate template when creating a new material entry.
We use a HOMO level of -6.08 eV and a LUMO level of -1.75 eV. A Gaussian broadening is enabled by default. For the excitons, we use a singlet binding energy of 1 eV and a triplet binding energy of 1.7 eV. For Dexter-type exciton transfer, a prefactor of 0.95 is used along with a decay length of 0.3.
The singlet-triplet generation ratio will be set to 0.25 (corresponding to a statistical 1:3 distribution of singlet and triplet excitons).
Thermalization losses during exciton transport from the dye through the host are included by setting the non-radiative decay rates to \(10^{5}\,\textrm{s}^{-1}\) for singlets and \(10^{4}\,\textrm{s}^{-1}\) for triplets. The radiative decay rates are set to 0.
Electron Transport Layer¶
TPBi is used as an electron transport layer. Select the Transport layer when creating a new material.
We use a HOMO level of -6.2 eV and a LUMO level of -1.7 eV. For the excitons, we use a singlet binding energy of 0.75 eV and a triplet binding energy of 1 eV. For Dexter-type exciton transfer, a prefactor of 1 is used along with a decay length of 0.3.
To mimic the effect of an exciton diffusion barrier in the stack, a non-radiative decay rate of \(10^{8}\,\textrm{s}^{-1}\) is specified for both excitons.
Hole Transport Layer¶
TAPC is used as the hole transport layer. We use a HOMO level of -5.5 eV and a LUMO level of -0.96 eV. For the excitons, we use a singlet binding energy of 1 eV and a triplet binding energy of 1.59 eV. For Dexter-type exciton transfer, a prefactor of 1 is used along with a decay length of 0.3. A non-radiative decay rate of \(10^{8}\,\textrm{s}^{-1}\) is specified for both excitons.
Create Compositions¶
We will create a host-guest mixture containing 0.9 CBP and 0.1 Ir(ppy)3.
Create a Stack¶
We start by composing the stack layers. We use a 20 nm TAPC hole transport layer, a 30 nm host-guest layer in the center and a 20 nm TPBi electron transport layer.
The stack editor now allows us to define the Förster radii. Förster rates are defined for various processes, including diffusion, quenching and annihilation. Because the Förster rates depend on the molecular environment, separate reactions have to be specified for each pair of materials. To streamline this process, the web interface provides the option to automatically configure the most common processes for the current stack. The mechanisms that are included are based on the material templates.
For this tutorial, we will use the default Förster interactions. This will include the triplet diffusion, triplet quenching and exciton annihilation reactions.
For illustration purposes, we will use the manual option to add singlet quenching to our list of reactions. Selecting the option Add Förster Interaction will open a new menu.
We select Ir(ppy)3 as the donor material, i.e. the material containing the singlet. We then select all 4 materials as possible acceptors. In the list of processes, we select both singlet-electron and singlet-hole quenching. We will specify a Förster radius of 1 nm. Clicking the Generate button will now automatically configure both quenching reactions for each donor-acceptor pair. Each of these processes will have the same Förster radius by default. Selecting the radius of a specific reaction allows you to change the value. Here, we will use a 1.5 nm radius for the quenching reactions inside Ir(ppy)3. Select the Save button to add the reactions to the stack.
Note
For inter-layer Dexter transport, the rate constants are obtained as a geometric average of the layer parameters. Custom parameters can be specified for individual layer pairs to overrule this behavior.
Create a Parameter Set¶
We will use the single voltage point template to create the parameter set. We select our stack and set a default voltage of 5 V. The maximum number of simulation steps will be set at 1.000.000.000.
Excitonic processes are included in the simulation by enabling the exciton module. The single voltage point template includes this option by default. You can check the module configuration by navigating to the Modules tab.
Starting the Simulation¶
A voltage sweep can be performed to investigate the roll-off in device efficiency at higher voltages. We select a voltage range from 3 to 6 V and select 7 voltage points. A single disorder instance can be selected to decrease the simulation runtime.
If you wish to limit the computational time required for this tutorial, you can perform the single voltage point simulation instead. This will use the 5 V default chosen in the parameter set.
Simulation Output¶
The distribution of carriers over the stack layers can be viewed in the Profiles section of the Sweep Report panel.
A summary of the excitonic process frequencies is provided in the OLED Report section, along with the current-voltage characteristics and device efficiency.