Thursday, 4 May 2017

Upscaling high-quality graphene devices

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Researchers have succeeded in upscaling high-quality graphene devices to the 100-micron scale and beyond. By perfecting CVD graphene production, transfer and patterning processes, scientists from the University of Hamburg and Graphenea manage to observe the quantum Hall effect in devices longer than 100 micrometers, with electronic properties on par with micromechanically exfoliated devices.

The work by Timothy Lyon and co-authors, published in Applied Physics Letters, started from graphene grown by chemical vapor deposition (CVD) on a copper substrate. CVD is the most successful technique for producing large-area high-quality graphene for high-tech applications. However, graphene on metal is not useful for applications in electronics, thus the material is usually transferred onto another substrate before use. The transfer process has proven to be a tough nut to crack, in many cases leading to cracks, defects, and chemical impurities that reduce the quality of the graphene.

In this most recent advance, researchers optimized every step of the transfer and patterning processes, resulting in large-area graphene of unprecedented quality. Transfer from copper was performed in eight consecutive steps, with three more steps needed to produce electrical contacts. Although the copper is removed with a standard etching solution, the bottom side of the graphene is cleaned with two reactive chemical etching steps to remove organic and inorganic contaminants. Also at other steps of the process, such as polymer removal, standard chemicals are replaced by carefully chosen ones in order to avoid graphene damage.

Figure: Graphene devices and measurement.

The optimized processing results in tear-free graphene on the desired Si/SiO2 substrate. Further processing is done to implement metallic contacts for electrical measurements. The electrical performance of the devices is measured in vacuum and at low temperature, revealing multiple quantum Hall levels. The quantum Hall effect on large scales opens the way to use graphene for universal electrical resistance standard measurements, hopefully leading to more precise measures of electron charge and the Planck constant.

The graphene devices have their charge neutrality point near zero gate voltage, which indicates very high material purity. Perhaps most importantly, the measured carrier mobility is as high as 3760 cm2/(Vs), which unambiguously shows that CVD graphene is an excellent candidate for electronic applications. Upscaling high-quality graphene device production beyond 100 microns is essential for commercial production. The authors of the research envisage such devices to find uses in THz-emitters, thermo-power couplers, and possibly flexible thin-film sensors.


via Graphenea

High temperature step-by-step process makes graphene from ethene

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An international team of scientists has developed a new way to produce single-layer graphene from a simple precursor: ethene -- also known as ethylene -- the smallest alkene molecule, which contains just two atoms of carbon.
via Science Daily

A lot of galaxies need guarding

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Like the quirky characters in the upcoming film Guardians of the Galaxy Vol. 2, the Hubble Space Telescope has some amazing superpowers, specifically when it comes to observing galaxies across time and space. One stunning example is galaxy cluster Abell 370, which contains a vast assortment of several hundred galaxies tied together by the mutual pull of gravity. That's a lot of galaxies to be guarding, and just in this one cluster!
via Science Daily
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A Lot of Galaxies Need Guarding in This NASA Hubble View


Power of Massive Galaxy Cluster Harnessed to Probe Remote Galaxies in Early Universe
Like the quirky characters in the upcoming film Guardians of the Galaxy Vol. 2, NASA's Hubble Space Telescope has some amazing superpowers, specifically when it comes to observing galaxies across time and space. One stunning example is galaxy cluster Abell 370, which contains a vast assortment of several hundred galaxies tied together by the mutual pull of gravity. That's a lot of galaxies to be guarding, and just in this one cluster! Photographed in a combination of visible and near-infrared light, the immense cluster is a rich mix of galaxy shapes. Entangled among the galaxies are mysterious-looking arcs of blue light. These are actually distorted images of remote galaxies behind the cluster. These far-flung galaxies are too faint for Hubble to see directly. Instead, the gravity of the cluster acts as a huge lens in space, magnifying and stretching images of background galaxies like a funhouse mirror. Abell 370 is located approximately 4 billion light-years away in the constellation Cetus, the Sea Monster. It is the last of six galaxy clusters imaged in the recently concluded Frontier Fields project — an ambitious, community-developed collaboration among NASA's Great Observatories and other telescopes that harnessed the power of massive galaxy clusters and probed the earliest stages of galaxy development.


via Hubble - News feed
http://hubblesite.org/news_release/news/2017-20

The Perseus Cluster Waves

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The cosmic swirl and slosh of giant waves in an enormous reservoir of glowing hot gas are traced in this enhanced X-ray image from the Chandra Observatory. The frame spans over 1 million light-years across the center of the nearby Perseus Galaxy Cluster, some 240 million light-years distant. Like other clusters of galaxies, most of the observable mass in the Perseus cluster is in the form of the cluster-filling gas. With temperatures in the tens of millions of degrees, the gas glows brightly in X-rays. Computer simulations can reproduce details of the structures sloshing through the Perseus cluster's X-ray hot gas, including the remarkable concave bay seen below and left of center. About 200,000 light-years across, twice the size of the Milky Way, the bay's formation indicates that Perseus itself was likely grazed by a smaller galaxy cluster billions of years ago.

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