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Activity Report 2010 - CNRS

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SCIENTIFIC REPORT<br />

FURTHER READING<br />

Nature 464, 1174-1177 (<strong>2010</strong>)<br />

Substrate-enhanced supercooling in<br />

AuSi eutectic droplets<br />

Astronomy and Astrophysics, 521, id.<br />

A29 (<strong>2010</strong>)<br />

NIKA: A millimeter-wave kinetic<br />

inductance camera<br />

In situ X-ray investigation<br />

of growing semiconductor<br />

nanowires<br />

“New comers” Project 2007: Tobias<br />

SCHÜLLI (ESRF & French CRG)<br />

Post-doctoral Fellow: Valentina CANTELLI<br />

Supercooled liquids are trapped in a<br />

metastable state even well below their<br />

freezing point, which can only be<br />

achieved in liquids that do not contain<br />

seeds that may trigger crystallization. It<br />

was during their studies, focused on the<br />

growth of semiconducting nanowires,<br />

that T. Schülli et al. discovered the<br />

unusual properties of a gold-silicon alloy,<br />

in contact with silicon (111) surface.<br />

(Fig.2)<br />

As they were observing the first stage of<br />

growth of nanowires, they saw that the<br />

metal-semiconductor alloy they used<br />

remained liquid at a much lower<br />

temperature than its crystallization point.<br />

The team studied what happened to the<br />

liquid in contact with a five-fold<br />

coordinated surface and then performed<br />

the control experiment with the same<br />

liquid exposed to three-fold and four-fold<br />

coordinated surfaces, which reduced the<br />

supercooling effect dramatically. This<br />

constituted the first experimental proof<br />

that pentagonal order is at the origin of<br />

supercooling.<br />

the solid–liquid interaction for the<br />

structure of the adjacent liquid layers.<br />

Such processes are crucial for present<br />

and future technologies, as fluidity and<br />

crystallization play a key part in soldering<br />

and casting, as well as in processing and<br />

controlling chemical reactions for<br />

microfluidic devices or during the<br />

vapour–liquid–solid growth of<br />

semiconductor nanowires.<br />

New generation of nanodetectors<br />

for astrophysics<br />

“New comers” Project 2007: Alessandro<br />

MONFARDINI (Institut Néel)<br />

Post-doctoral Fellow: Loren SWENSON<br />

The Néel IRAM KIDs Arrays (NIKA)<br />

project was kicked off in November 2008<br />

to develop a large mm-wave resident<br />

instrument at the 30-m IRAM<br />

radiotelescope on the Pico Veleta, near<br />

Granada (Spain). The main competitor to<br />

achieve this goal at IRAM is the GISMO<br />

collaboration led by the NASA Goddard<br />

Space Flight Center, focusing on<br />

superconducting TES (Transition Edge<br />

Sensors).<br />

An excellent post-doc (Loren SWENSON)<br />

was hired in July 2008 coming from Dr.<br />

Cleland’s famous group at the University<br />

of California Santa Barbara. A new<br />

dilution cryostat was developed, adapted<br />

for KIDs testing, when also started the<br />

designing/fabricating/testing of the first<br />

NbN resonators in collaboration with<br />

INAC (J.C. Villegier) and Olivier Buisson<br />

at the Institut Néel.<br />

In 2009, beginned the investigation of a<br />

particular KID concept known as LEKID<br />

(Lumped Element KID), allowing a purely<br />

planar design and a good optical<br />

coupling. Totally unexplored at that time,<br />

the potential of this new configuration for<br />

future large instruments operating in the<br />

mm-wave range was well appreciated.<br />

24<br />

Fig. 2: Droplet of a gold-silicon liquid alloy on<br />

a silicon (111) surface. Pentagonal clusters<br />

formed at the interface exhibit a denser<br />

structure compared to solid gold and prevent<br />

the liquid from crystallization at temperatures<br />

as low as 300 Kelvin below the solidification<br />

temperature. Graphics: M. Collignon<br />

It was therefore revealed that pentagonal<br />

atomic arrangements of Au atoms at this<br />

interface favour a lateral-ordering<br />

stabilization process of the liquid phase.<br />

This interface-enhanced stabilization of<br />

the liquid state shows the importance of<br />

Thanks to the rapid development of the<br />

project, a request for one week technical<br />

time at the 30-m telescope was made in<br />

September 2009. (To better understand<br />

the amplitude of the project, the<br />

approximate cost of one single hour time<br />

at Pico Veleta is estimated 1 k€.)<br />

The first run took place in October 2009,<br />

with very encouraging results. One could<br />

observe, for example, a number of faint<br />

galactic and extra-galactic sources.<br />

This LEKID array, used at the telescope,<br />

had been fabricated at the PTA-Grenoble<br />

platform.<br />

After the first light, and despite the small<br />

number of pixels (30-40) NIKA was<br />

already exhibiting better performances

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