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Wednesday August 5, 2015

Nano-sized Electronic Circuit Promises Bright View of Early Universe

News Release
Thursday July 10, 2008

Nano-sized Electronic Circuit Promises Bright View of Early Universe

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N.J. – A newly developed
nano-sized electronic device is an important step toward helping astronomers
see invisible light dating from the creation of the universe. This invisible
light makes up 98% of the light emitted since the “big bang,” and may provide
insights into the earliest stages of star and galaxy formation almost 14
billion years ago.

Credit: Carl Blesch
Physics Prof. Michael Gershenson with laboratory equipment used to fabricate ultra-sensitive, nano-sized infrared light detector.

The tiny, new circuit, developed by physicsts at Rutgers University,
NASA’s Jet Propulsion Laboratory in Pasadena, Calif., and the State University of New York at Buffalo, is 100 times
smaller than the thickness of a human hair. It is sensitive to faint traces of
light in the far-infrared spectrum (longest of the infrared wavelengths), well
beyond the colors humans see.

“In the expanding universe, the earliest stars move away from
us at a speed approaching the speed of light,” said Michael
Gershenson, professor of physics at Rutgers
and one of the lead investigators. “As a result, their light is strongly
red-shifted when it reaches us, appearing infrared.”

Because the Earth’s atmosphere strongly absorbs far-infrared
light, Earth-based radiotelescopes cannot detect the very faint light emitted
by these stars. So scientists are proposing a new generation of space
telescopes to gather this light. Yet to take full advantage of space-borne
telescopes, detectors that capture the light will have to be far more sensitive
than any that exist today.

Detectors of infrared and submillimeter waves, known as
bolometers, measure the heat generated when they absorb photons, or units of
light. Today’s infrared bolometer technology is mature and has reached the
limit of its performance.

“The device we built,
which we call a hot-electron nanobolometer, is potentially 100 times more
sensitive than existing bolometers,” Gershenson said. “It is also faster to
react to the light that hits it.”

The research team is publishing a description of the
experimental device in an upcoming issue of the journal Nature Nanotechnology.
The journal’s website posted an electronic copy of the paper this week at: The team is led by Gershenson and
Boris Karasik of the Jet Propulsion Laboratory (JPL), a NASA center managed by
the California Institute of Technology (CalTech). Most of the fabrication and
measurement work was done at Rutgers by graduate student Jian Wei, now a
post-doctoral associate at the Northwestern
University; postdoctoral
researcher David Olaya, now with the National Institute of Standards and
Technology; and postdoctoral researcher Sergey Pereverzev, now with JPL and
CalTech. The theoretical support for this research was provided by Andrei
Sergeev of the State University of New York at Buffalo.

Made of titanium and niobium metals, the novel device is
about 500 nanometers long and 100 nanometers wide. The physicists built it
using thin-film and nanolithography techniques similar to those used in
computer chip fabrication. The device operates at very cold temperatures –
about 459 degrees below zero Fahrenheit, or one-tenth of one degree above
absolute zero on the Kelvin scale.

Photons striking the nanodetector heat electrons in the
titanium section, which is thermally isolated from the environment by
superconducting niobium leads. By detecting the infinitesimal amount of heat
generated in the titanium section, one can measure the light energy absorbed by
the detector. The device can detect as little as a single photon of far
infrared light.

“With this single detector, we have demonstrated a proof of
concept,” said Gershenson. “The final goal is to build and test an array of 100
by 100 photodetectors, which is a very difficult engineering job.” Rutgers took the lead on fabrication and electrical
characterization of the single detector, and JPL will take the lead on the
optical characterization of the detector and developing detector arrays.

Gershenson expects the detector technology to be useful for
exploring the early universe when satellite-based far-infrared telescopes start
flying 10 to 20 years from now. “That will make our new technology useful for
examining stars and star clusters at the farthest reaches of the universe,” he

Media Contact: Carl Blesch
732-932-7084, ext. 616

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