Slow Electron Making More Efficient Radiation Emission.
Dong-Sing Wuu1, Sin-Liang Ou2, Ching-Ho Tien3
1Department of Materials Science and Engineering, National Chung Hsing University, Taichung, 40227, Taiwan, R.O.C.. dsw@nchu.edu.tw.
Scientific Reports
|March 22, 2018
Summary
This study introduces an electron-retarding n-electrode (ERN) for InGaN blue light-emitting diodes (LEDs). The ERN improves efficiency by slowing electrons, enhancing radiation emission and optoelectronic performance.
Area of Science:
- Materials Science
- Optoelectronics
- Semiconductor Physics
Background:
- Electron mobility significantly exceeds hole mobility in conventional emitting devices, leading to increased non-recombination rates.
- This imbalance hinders the overall efficiency of light-emitting devices.
Purpose of the Study:
- To enhance the efficiency of Indium Gallium Nitride (InGaN) blue light-emitting diodes (LEDs) by addressing the electron-hole mobility mismatch.
- To demonstrate an electron-retarding n-electrode (ERN) to slow electron transport and improve radiation emission.
Main Methods:
- An electron-retarding n-electrode (ERN) was fabricated on the n-GaN layer of InGaN blue LEDs.
- Pulsed-laser deposited cobalt-doped Zinc Oxide (ZnO) film was utilized as the ERN material, meeting requirements for Ohmic contact, dilute magnetic doping, and electrical conductivity.
- The performance of LEDs with and without the ERN was compared.
Main Results:
- The 120-nm-thick ERN/n-GaN achieved a significant electron retarding of 19.9% compared to n-GaN.
- LEDs incorporating the ERN exhibited increased output power (246.7 mW vs. 212.9 mW) and wall-plug efficiency (18.2% vs. 15.1%) at 350 mA.
- Efficient electron filling in quantum wells due to the ERN led to an enlarged bandgap and a blue-shift in emission wavelength.
Conclusions:
- The developed ERN technique effectively mitigates the electron-hole velocity difference, improving optoelectronic performance.
- The cobalt-doped ZnO ERN demonstrates suitability for enhancing InGaN blue LEDs.
- This approach offers a viable solution for boosting the efficiency of light-emitting devices.
Related Concept Videos
Emission Spectra
76.6K
When solids, liquids, or condensed gases are heated sufficiently, they radiate some of the excess energy as light. Photons produced in this manner have a range of energies, and thereby produce a continuous spectrum in which an unbroken series of wavelengths is present.
76.6K
Biological Effects of Radiation
18.1K
All radioactive nuclides emit high-energy particles or electromagnetic waves. When this radiation encounters living cells, it can cause heating, break chemical bonds, or ionize molecules. The most serious biological damage results when these radioactive emissions fragment or ionize molecules. For example, α and β particles emitted from nuclear decay reactions possess much higher energies than ordinary chemical bond energies. When these particles strike and penetrate matter, they...
18.1K
Gene Evolution - Fast or Slow?
8.2K
The genomes of eukaryotes are punctuated by long stretches of sequence which do not code for proteins or RNAs. Although some of these regions do contain crucial regulatory sequences, the vast majority of this DNA serves no known function. Typically, these regions of the genome are the ones in which the fastest change, in evolutionary terms, is observed, because there is typically little to no selection pressure acting on these regions to preserve their sequences.
In contrast, regions which code...
In contrast, regions which code...
8.2K
Gene Evolution - Fast or Slow?
3.7K
3.7K
Radiation: Applications
1.8K
The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
The average...
1.8K
Absorption of Radiation
1.3K
The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
1.3K


