Thursday 30 November 2017

Deducing the properties of a new form of diamond

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Earlier this year, amorphous diamond was synthesized for the first time using a technique involving high pressures, moderately high temperatures and a tiny amount of glassy carbon as starting material. A father-son team at Clemson University has now successfully calculated a number of basic physical properties for this new substance, including elastic constants and related quantities.
via Science Daily

How to produce the purest argon ever?

ARIA’s modules are being leak-tested at CERN before travelling to Sardinia, Italy. The top, bottom and one standard column module have now been lined up horizontally to test their alignment. (Image: J. Ordan/CERN)

Producing the purest argon ever made is no mean feat, in fact it needs a column 26 metres taller than the Eiffel Tower.

CERN is part of a project, called ARIA, to construct a 350-metre-tall distillation tower that will be used to purify liquid argon for scientific and, in a second phase, medical use.

The full tower, composed of 28 identical modules plus a top (condenser) and a bottom (re-boiler) special module, will be installed in a disused mine site in Sardinia, Italy.

The project is was initiated to supply the purest argon possible to the international dark matter experiment DarkSide at INFN’s Gran Sasso National Laboratories. DarkSide is a dual-phase liquid-argon time-projection chamber that aims to detect the possible passage of a dark matter particle in the form of a Weakly Interacting Massive Particle (WIMP) when it hits the argon nuclei contained in the detector. Since this WIMP-nuclei interaction is predicted to be extremely rare, the detector must contain only the purest argon possible, so as not to accidentally produce a spurious signal.

ARIA has been designed to produce this extra-pure argon. Atmospheric argon contains many “impurities” such as water, oxygen, krypton and argon-39, an isotope of argon, which are all sources of unwanted signals. Argon from underground sources is already depleted from the argon-39 isotope by a factor of 1400, but this is still not enough for dark-matter research. ARIA is designed to purify underground argon by a further factor of 100.

For more information, read this article.


via CERN: Updates for the general public
https://home.cern/about/updates/2017/11/how-produce-purest-argon-ever

A very special run for the LHCb experiment

The LHCb detector in open configuration. (Image: Anna Pantelia/CERN)

For the first time, the LHCb experiment at CERN has collected data simultaneously in collider and in fixed-target modes. With this, the LHCb special run is even more special.

The past two weeks have been devoted to special runs of the Large Hadron Collider (LHC), at the end of the LHC 2017 proton run and before the winter shutdown. One run involved proton collisions at an energy of 5.02 TeV, mainly to set a reference to compare with lead-ion collision data. What was exceptional this year is that a tiny quantity of neon gas was injected into the beam pipe near the LHCb experiment’s interaction point. This allowed physicists to collect proton-neon at the same time as proton-proton collision data.

When (noble) gases are injected into the beam pipe to collide with protons, the LHCb experiment is in “fixed-target” mode, in contrast to the standard “collider” mode. But unlike traditional fixed target experiments, where the beam of accelerated particles is directed at a dense solid or liquid target, here LHC protons are colliding with a handful of neon nuclei injected near the collision point and floating in the beam pipe. These nuclei slightly pollute the almost perfect LHC vacuum, but the conditions they create – where pressure is in the order of 10-7 millibar – are still considered to be typical of ultra-high vacuum environments.

There are two main reasons to collect proton-gas collision data at the LHC. On one hand, these data help understand nuclear effects (i.e. depending on the type of nuclei involved in the collisions), affecting the production of specific types of particles (J/ψ and D0 mesons), whose suppressed production is considered to be the hallmark of the quark-gluon plasma. The quark-gluon plasma is the state in which the matter filling the universe a few millionths of a second after the Big Bang was , when protons and neutrons had not yet formed, composed of quarks not binding together and then free to move on their own.  

On the other hand, proton-neon interactions are important to also study cosmic rays – highly energetic particles, mostly protons, coming from outside the Solar System – when they collide with nuclei in the Earth’s atmosphere. Neon is one of the components of the Earth’s atmosphere and it is very similar in terms of nuclear size to the much more abundant nitrogen and oxygen.

This gas-injection technique was originally designed to measure the brightness of the accelerator's beams, but its potential was quickly recognised by the LHCb physicists and it is now also being used for dedicated physics measurements. In 2015 and 2016, the LHCb experiment already performed special proton-helium, proton-neon and proton-argon runs. In October this year, for eight hours only, the LHC accelerated and collided xenon nuclei, allowing the four large LHC experiments to record xenon-xenon collisions for the first time.

This recent 11-day proton-neon run will allow physicists to collect a dataset that is 100 times larger than all proton-neon collision data collected until now at the LHC, and the first results of the analyses are foreseen for next year.

Find out more on the LHCb website


via CERN: Updates for the general public
https://home.cern/about/updates/2017/11/very-special-run-lhcb-experiment