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Emission editor

1. Overview

The Emission editor allows you to control how light is generated within active layers of your device, both for photoluminescence (PL) and electroluminescence (EL). Only electrically active layers can emit light. Open the editor by clicking Emission parameters in the left-hand menu of the Device structure tab. You can then enable or disable emission for each active layer using the toggle at the top left of the editor window.

2. Parameters

When emission is enabled, the following options are available:

OghmaNano main window showing how to open the Emission editor via the Emission parameters icon.
OghmaNano main simulation window β€” open the Emission editor from the left-hand panel via the Emission parameters icon.
Luminescence editor with options for experimental spectra, free-to-free emission, free-to-trap emission, and ray tracing settings.
Emission editor with experimental emission spectra enabled. Options include free-to-free emission, free-to-trap emission, emission efficiency, and ray tracing setup.

If Use experimental emission spectra is disabled, additional fields appear to let you specify photon generation efficiencies for different recombination/trapping channels:

Each value ranges from 0.0–1.0 and specifies the fraction of recombination events that produce photons. This allows modelling of more complex radiative and non-radiative recombination pathways, e.g. trap-mediated emission relevant in infrared or defect spectroscopy.

Emission editor with experimental spectra disabled, showing extended photon generation efficiency parameters for recombination and trapping events.
Emission editor with experimental spectra disabled β€” extended options appear for defining photon generation efficiency of different recombination/trapping processes.

3. Ray tracing

The bottom section configures angular sampling for ray tracing of emitted photons:

Together, these parameters define the angular distribution of rays sampled on a sphere around the emitting layer. For example, with 180 theta steps (0–360Β°) and 25 phi steps (0–360Β°), the simulation samples a full spherical distribution of emission directions.