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A better device to detect ultraviolet light

Date:
October 4, 2013
Source:
American Institute of Physics (AIP)
Summary:
Researchers have developed a new photodiode that can detect in just milliseconds a certain type of high-energy ultraviolet light, called UVC, which is powerful enough to break the bonds of DNA and harm living creatures.
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FULL STORY

This is a crystal model of beta-Ga2O3.
Credit: Ishinomaki/S.Nakagomi

Researchers in Japan have developed a new photodiode that can detect in just milliseconds a certain type of high-energy ultraviolet light, called UVC, which is powerful enough to break the bonds of DNA and harm living creatures. The researchers describe their new device in the journal Applied Physics Letters.

Although this radiation doesn't normally reach Earth's surface, it can leak through to just below the hole in the ozone layer. Monitoring this radiation is a way of tracking the hole in the ozone layer, and photodiodes that measure UVC are also used as flame sensors and for communication in space.

Now, Shinji Nakagomi and colleagues at Ishinomaki Senshu University in Japan have built a new kind of photodiode that can detect the whole range of UVC light while remaining insensitive to visible light from the sun -- two features that have eluded designers of current devices. By being "solar blind," photodiodes are more sensitive to the UVC range and are thus more useful.

Building a Better Photodiode

Some photo detectors consist of vacuum tubes on sale, but they have short lifetimes and are relatively large and unwieldy. Today, many photodiodes are instead based on a so-called p-n junction, in which a semiconductor that carries positive charge (the absence of electrons called holes) is put in contact with the same semiconductor that instead carries negative charge (electrons). When light with sufficient energy (short wavelength) strikes atoms near the interface between the two semiconductors -- called p-type and n-type, respectively -- it generates mobile electrons and holes, boosting electrical current across the p-n junction and signaling the presence of light.

Other photodiodes made from materials like aluminum nitride and diamond are sensitive only to a limited range of UVC light. But recently, gallium oxide has shown promise because it's sensitive to the entire UVC range and is solar blind. The problem, however, is that it's difficult to make p-type gallium oxide.

Instead of a photodiode based on a conventional p-n junction, the researchers built one based on what's called a heterojunction, which is a p-n junction that incorporates two different semiconductors. The team used gallium oxide and silicon carbide, and found that their device responds quickly to UV light -- within milliseconds -- and has little dark current, which is the intrinsic electrical current that flows through the device even in the absence of light. Minimal dark current is important for a sensitive photodiode.

"The most important aspect about our device is that it is based on a heterojunction between gallium oxide and silicon carbide," said Nakagomi. "This gallium oxide and silicon carbide photodiode is promising for the detection of UV light."


Story Source:

The above post is reprinted from materials provided by American Institute of Physics (AIP). Note: Materials may be edited for content and length.


Journal Reference:

  1. Shinji Nakagomi, Toshihiro Momo, Syuhei Takahashi, Yoshihiro Kokubun. Deep ultraviolet photodiodes based on β-Ga2O3/SiC heterojunction. Applied Physics Letters, 2013; 103 (7): 072105 DOI: 10.1063/1.4818620

Cite This Page:

American Institute of Physics (AIP). "A better device to detect ultraviolet light." ScienceDaily. ScienceDaily, 4 October 2013. <www.sciencedaily.com/releases/2013/10/131004154347.htm>.
American Institute of Physics (AIP). (2013, October 4). A better device to detect ultraviolet light. ScienceDaily. Retrieved July 28, 2015 from www.sciencedaily.com/releases/2013/10/131004154347.htm
American Institute of Physics (AIP). "A better device to detect ultraviolet light." ScienceDaily. www.sciencedaily.com/releases/2013/10/131004154347.htm (accessed July 28, 2015).

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