Search

 

MediaMedia

Paris, 18 July 2012

The atomic nucleus : fissile liquid or molecule of life ?

A new view of the nucleus that unifies its liquid and molecule-like aspects has been put forward by a team from the Institut de Physique Nucléaire d'Orsay (Université Paris-Sud/CNRS) and from CEA (the French Atomic Energy Commission), in collaboration with the University of Zagreb. By making an analogy with neutron stars(1), the researchers have for the first time demonstrated one of the necessary conditions for the formation of molecule-like behavior within the atomic nucleus. Such molecule-like behavior makes it possible to understand the synthesis of elements that are key to the appearance of life. The work is published in Nature dated 19 July 2012.

The atomic nucleus is generally described as a drop of quantum liquid with a diameter of around a million billionth of a meter.  In particular, such liquid-like behavior explains nuclear fission, and applies especially to heavy nuclei, i.e. nuclei that contain a large number of nucleons (neutrons and protons).  On the other hand, light nuclei(2) can behave like tiny 'molecules', or clusters, made up of neutrons and protons within the nucleus.  This molecular aspect makes it possible to understand the stellar synthesis of carbon-12 and other heavier elements necessary for the appearance of life(3).

Until now, both the 'molecule-nucleus' and the 'liquid-nucleus' views coexisted.  Now, a team from the Institut de Physique Nucléaire d'Orsay (Université Paris-Sud/CNRS) and from CEA (the French Atomic Energy Commission), in collaboration with the University of Zagreb, proposes a unified view of these two aspects. By solving quantum physics equations on the scale of the nucleus (in particular the Schrödinger equation), the researchers have demonstrated that, although a light nucleus can show molecule-like behavior (tending towards the crystalline state), heavier nuclei take on a liquid-like behavior.  To establish this new theory, the physicists took inspiration from neutron stars(1). The deeper you go inside a neutron star, the more you pass from a crystalline medium to a liquid medium.  Thanks to this analogy, the physicists identified a mechanism of transition from the liquid to the crystalline state in the nucleus.  When the interactions between neutrons and protons are not strong enough to fix them within the nucleus, the latter is in a quantum-liquid type state where protons and neutrons are delocalized. Conversely, in a crystalline state, neutrons and protons are fixed at regular intervals within the nucleus. The nuclear molecule is interpreted as being an intermediate state between a quantum liquid and a crystal.  In the long term, the aim is to attain a unified understanding of the various states of the nucleus.

Fig 1

© Luc Petizon, IPN Orsay

Artist's impression showing the molecular states of the nucleus in a liquid.




Fig 2

© Jean-Paul Ebran/CEA

Probability density for the presence of neutrons and protons predicted for the neon-20 nucleus. It can be seen that this is not homogeneous: the neutrons and protons are distributed in clusters.



Notes:

(1) The core of a massive star that collapses during a supernova explosion becomes so dense that protons and neutrons combine, forming neutrons. The resulting body becomes a kind of giant atomic nucleus made up mostly of neutrons, which is what gives it its name.
(2) Such as oxygen-16 (16O), which contains 8 neutrons and 8 protons.
(3) For instance, the Hoyle state of carbon-12, key to nucleosynthesis, is described as a nuclear molecule made up of three alpha particles. An alpha particle is a cluster of two neutrons and two protons.

References:

“How atomic nuclei cluster”, J.-P. Ebran, Elias Khan, T Nikšić and D. Vretenar, Nature, 19 July 2012

Contact information:

Researchers l Elias Khan l T. 00.33 (0)1 69 15 71 73 l khan@ipno.in2p3.fr
Jean-Paul Ebran l T. 00.33 (0)1 69 26 67 54 l jean-paul.ebran@cea.fr

CNRS Press Office l Elsa Champion l T. 00.33 (0)1 44 96 43 90 l elsa.champion@cnrs-dir.fr


Top

Latest press releases

All disciplines

Back to homepageContactcredits