Helmholtz Association

Heavy Elements

An der Ionenfalle SHIPTRAP wurde die Masse des künstlichen Elements 102, Nobelium, mit höchstmöglicher Präzision gemessen. Foto: GSI/G. Otto
The mass of the artificial element 102, nobelium, was measured with
utmost precision with the ion trap SHIPTRAP. Photo: GSI/G. Otto

The hitherto heaviest, officially acknowledged chemical element has the atomic number 112 and was discovered at the GSI Helmholtz Centre for Heavy Ion Research in Darmstadt. Since February 2010, it at last has a name: Copernicium, chemical symbol “Cn”, named for the astronomer Nikolaus Kopernikus. With this, the chemists’ union IUPAC accepted the name proposed by the international team of discoverers around the GSI researcher Sigurd Hofmann. In 1996, the team had targeted lead foils with a beam of zinc ions produced in the accelerator UNILAC. For a short moment, the atomic nuclei fused to form a new element – the element 112, which the scientists could identify in a highly sensitive verification process.

Copernicium is only an interim stage in the search for new elements. In doing so, the GSI focuses on various strategies. A new measuring apparatus called SHIPTRAP is capable of capturing and storing super heavy ions with a gas cell and a so-called Penning trap. Recently, one succeeded for the first time to capture ions of the elements 102(nobelium) and 103 (Lawrencium) and to measure their mass in detail. The researchers hope the same could be possible with even heavier kinds of atoms.

With another apparatus, the separator TASCA, the GSI experts recently verified another super heavy element, the element 114. The researchers could thereby reproduce a discovery from the Russian Dubna – raising the chances that the IUPAC officially acknowledges the as yet nameless element. “It is the hitherto heaviest kind of atom we have created in Darmstadt”, says GSI Department Head Dr. Fritz Peter Hessberger. “In the next few years, we will try to get to the elements 119 and 120.” An advance into absolute new territory, for these kinds of atoms still await their discovery.

Insights into Research: Structure of of Matter

A Look at the Cosmic Primeval Soup

Since March 2010, it operates according to routine – the Large Hadron Collider LHC in Geneva, the strongest accelerator of all times. Usually, it uses hydrogen nuclei (protons) to achieve new energy records. Yet as of autumn 2010, the 27 kilometre large ring is to collide the nuclei of lead atoms for the first time.

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Insights into Research: Structure of of Matter

Neutrino Hunt at the South Pole

It is the southern-most large-scale experiment of the world: “IceCube” is located at the South Pole and consists of around 5000 optical sensors, held on wire ropes and inserted up to 2.5 kilometres deep into the ice of the Antarctic.

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Einblicke in die Forschung: Struktur der Materie

Data at the End of the Tunnel

Just like Dr. Manuel Bibes and his colleagues from the French research organisation CNRS south of Paris, Dr. Sergio Valencia and Dr. Florian Kronast from the Helmholtz-Zentrum Berlin (HZB) für Materialien und Energie are classical basic researchers. And yet they show a way towards the development of fast starting computers with low energy consumption with their work on electric control of electron spins.

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Einblicke in die Forschung: Struktur der Materie

Magnetic Monopoles in Spin Ice

So far, magnetic monopoles have not raised any attention in nature. In contrast to electric charges, magnetic “charges” principally occur only as dipoles with a north and a south pole. Therefore, the discovery of magnetic monopoles in autumn 2009 constituted a sensation.

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Einblicke in die Forschung: Struktur der Materie

Flash Explores New States of Matter

Usually, it shimmers in a dull silver – simply typically aluminium. Yet given extreme circumstances, the light metal can become translucent, not for normal light, but for soft x-rays. This feature was discovered by an international team of physicists at the Research Centre DESY in Hamburg by way of the light source FLASH. Amongst other things, the result is of relevance for astrophysics and fusion research.

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09.01.2013