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This light-sensing camera may help detect extraterrestrial life, dark matter – Deccan Chronicle,

This light-sensing camera may help detect extraterrestrial life, dark matter – Deccan Chronicle,

Ever imagined a camera that can count photons, or particles of light and further aid in searching for chemical signs of life on other planets or dark matter? Well, this device is now a reality!

Researchers at the National Institute of Standards and Technology (NIST) have created one of the highest-performance cameras ever, composed of sensors that count single photons, or particles of light.

With more than 1, 000 sensors, or pixels, this camera might be of great help in future space-based telescopes searching for chemical signs of life on other planets, and in new instruments designed to search for the elusive “dark matter” believed to constitute most of the “stuff” in the universe.

Described in the journal Optics Express, it consists of sensors made from superconducting nanowires, which can detect single photons. Researchers used these detectors to demonstrate Einstein’s “spooky action at a distance,” for example.

Moreover, the nanowire detectors also have the lowest dark count rates of any type of photon sensor, meaning they don’t count false signals caused by noise rather than photons.

This feature is especially useful for dark-matter searches and space-based astronomy. But cameras with more pixels and larger physical dimensions than previously available are required for these applications, and they also need to detect light at the far end of the infrared band, with longer wavelengths than currently practical.

While it is small in size, a square measuring 1.6 millimeters on a side; it is packed with 1, 024 sensors ( (columns by) rows) to make high-resolution images.

The main challenge was to find a way to collate and obtain results from so many detectors without overheating. Researchers extended a “readout” architecture they previously demonstrated with a smaller camera of 64 sensors that adds up data from the rows and columns, a step toward meeting the requirements of NASA.

“My primary motivation for making the camera is NASA’s Origins Space Telescope project, which is looking into using these arrays for analyzing the chemical composition of planets orbiting stars outside of our solar system,” said Varun Verma, NIST electronics engineer.

Each chemical element in the planet’s atmosphere would absorb a unique set of colors, he pointed.

“The idea is to look at the absorption spectra of light passing through the edge of an exoplanet’s atmosphere as it transits in front of its parent star,” Verma explained.

“The absorption signatures tell you about the elements in the atmosphere, especially those that might give rise to life, such as water, oxygen and carbon dioxide. The signatures for these elements are in the mid- to far-infrared spectrum , and large-area single-photon counting detector arrays don’t yet exist for that region of the spectrum, so we received a small amount of funding from NASA to see if we could help solve that problem, “he continued.

Verma and colleagues achieved high fabrication success, with 99. 5 per cent of the sensors working properly . But detector efficiency at the desired wavelength is low. Boosting efficiency is the next challenge.

Other possible applications include like finding dark matter. Researchers around the world have been unable to find so-called weakly interacting massive particles (WIMPs) and are considering looking for dark matter with lower energy and mass.

Superconducting nanowire detectors offer promise for counting emissions of rare, low-energy dark matter and discriminating real signals from background noise.

Made in a complicated process at NIST’s Microfabrication Facility in Boulder, Colorado, detectors in the camera are fabricated on silicon wafers diced into chips. The nanowires, made of an alloy of tungsten and silicon, are about 3.5 millimeters long, 180 nanometers (nm) wide and 3 nm thick. The wiring is made of superconducting niobium.

The camera performance was measured by the Jet Propulsion Laboratory (JPL) at the California Institute of Technology in Pasadena, California.              

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