How heavy elements come about in the universe

How heavy elements come about in the universe
For the first time, the fusion of hydrogen and xenon was able to be investigated at the same temperatures as occur in stellar explosions using an ion storage ring. Credit: Mario Weigand

Heavy elements are produced during stellar explosion or on the surfaces of neutron stars through the capture of hydrogen nuclei (protons). This occurs at extremely high temperatures, but at relatively low energies. An international research team headed by Goethe University has now succeeded in investigating the capture of protons at the storage ring of the GSI Helmholtzzentrum für Schwerionenforschung.

As the scientists report in the current issue of Physical Review Letters, their goal was to determine more precisely the probability for a capture in astrophysical scenarios. As Dr. Jan Glorius from the GSI atomic physics research department explains, they were faced with two challenges in this endeavour: "The reactions are most probable under astrophysical circumstances in an energy range called the Gamow window. In this range, nuclei tend to be somewhat slow, making them difficult to obtain in the required intensity. In addition, the —the probability of proton capture—decreases rapidly with energy. Until now, it has been almost impossible to create the right conditions in a laboratory for these kinds of reactions."

René Reifarth, Professor for experimental astrophysics at Goethe University suggested a solution as early as 10 years ago: The low energies within the Gamow window range can be reached more precisely when the heavy reaction partner circulates in an accelerator in which it interacts with a stationary proton gas. He achieved initial successes in September 2015 with a group of Heimholtz early career researchers. Since then, his team has gained excellent support from Professor Yuri Litvinov, who leads the EU-funded research project ASTRUm at GSI.

In the experiment, the international team first produced xenon ions. They were decelerated in the experimental storage ring ESR and caused to interact with protons. This resulted in reactions in which the xenon nuclei captured a proton and were transformed into heavier caesium—a process like that which occurs in astrophysical scenarios.

"The experiment makes a decisive contribution to advancing our understanding of in the cosmos," says René Reifarth. "Thanks to the high-performance accelerator facility at GSI, we were able to improve the experimental technique for decelerating the heavy reaction partner. We now have more exact knowledge of the area in which the reaction rates occur, which until now had only been theoretically predicted. This allows us to more precisely model the production of elements in the universe."


Explore further

Measurements yield precise atomic masses for nuclear reactions in the stars

More information: J. Glorius et al, Approaching the Gamow Window with Stored Ions: Direct Measurement of Xe124(p,γ) in the ESR Storage Ring, Physical Review Letters (2019). DOI: 10.1103/PhysRevLett.122.092701
Journal information: Physical Review Letters

Citation: How heavy elements come about in the universe (2019, March 19) retrieved 24 June 2019 from https://phys.org/news/2019-03-heavy-elements-universe.html
This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no part may be reproduced without the written permission. The content is provided for information purposes only.
233 shares

Feedback to editors

User comments

Mar 19, 2019
The extreme release of energy in astrophysical objects is accompanied by outflows, sometimes superluminal. It is important that these phenomena are observed on the scales from stars to galaxies, setting off a unity of explosive processes. But the nature of the central engines remains unclear. In our model all these phenomena have a common nature and the central engines are elastons.
https://www.acade...nization

Mar 19, 2019
Excellent! This experimental data will allow us to understand the conditions in supernovae and neutron stars that formed these elements.

Mar 20, 2019
To my mind after the formation of electron proton and neutron the heavy noble elements took the form as He, Ne Ar, Kr, Xe Rn and one more. Rn was the first and He was the last. Rest is for experiment.

Mar 20, 2019
This kind of basic research in nuclear 'chemistry' is essential. We seem in this akin to our first forays into chemistry in the 1800's Russians seem to be ahead of us, but that may be an illusion as we hide a lot in order to benefit big business here and maybe other places. The Russians seem more interested in getting the job done so the benefits can be applied to space exploration and civilian power purposes to heat cities sprawled out over vast territories not now served by maybe a continental grid system.

Please sign in to add a comment. Registration is free, and takes less than a minute. Read more