24 July 2018

Material from PSI helps to check inconsistencies in the Big Bang theory

Media Releases Research Using Neutrons Matter and Material Particle Physics

Shortly after the Big Bang, radioactive atoms of the type beryllium-7, among others, came into being. Today, throughout the universe, they have long since decayed and do not occur naturally, in contrast to their decay product lithium. Now researchers at the Paul Scherrer Institute PSI have helped to better understand the first minutes of the universe: They collected artificially produced beryllium-7 and made it into a sample that could be investigated. The beryllium-7 was subsequently probed by researchers at CERN. The joint study by PSI, CERN, and 41 other research institutions addresses the so-called cosmological lithium problem: There is a marked discrepancy between the amount of lithium the Big Bang theory predicts should be in the universe and the amount of lithium actually observed. According to the present study, it now appears more likely that the cause of this cosmological lithium problem lies in the theoretical description of the origin of the universe. The scientific community will thus have to keep searching for a solution to the cosmological lithium problem. The researchers now published their results in the journal Physical Review Letters.

Researchers at the Paul Scherrer Institute have provided a hard-won puzzle piece towards a better understanding of the universe's origin: They were able to produce a sample of extremely rare and short-lived atoms of the isotope beryllium-7. Subsequently, at CERN, it was possible to probe this beryllium-7 – in practice, its interaction with neutrons – with far more precision than ever before.

Since through its radioactive decay beryllium-7 becomes lithium-7, studying it can help to crack a fundamental problem of the Big Bang theory: The theory predicts a three to four times greater amount of lithium in the universe than actual measurements show. This so-called cosmological lithium problem is one of the last great riddles of the current theory of the origin of the universe, because for all other elements produced shortly after the Big Bang, the theory conforms well to the measured data.

Virtually all of the present-day lithium-7 in the universe comes from the decayed beryllium-7 which in turn was formed shortly after the big bang. Thus the researchers were looking into the question of whether there might have been less beryllium in the beginning than previously believed, which could clear up the cosmological lithium problem. One of the last possibilities still open to be checked was the so-called neutron capture cross-section of beryllium-7. This value predicts the probability that a beryllium-7 atomic nucleus will capture a free neutron and subsequently decay.

The neutron capture cross-section of beryllium-7 was last measured, imprecisely by comparison, around 50 years ago, explains PSI researcher Dorothea Schumann, head of the Isotope and Target Chemistry research group. This key figure should now be investigated at CERN, more accurately than ever before. The beryllium-7 sample needed for this was provided by the PSI researchers.

Years of preparation and test runs

The production and measurement of the beryllium-7 sample was like a one-time theatre performance, for which the researchers had to do around three years of preparatory work and test runs. Beryllium-7 disappears so rapidly through radioactive decay that its quantity is reduced by half roughly every 53 days. Therefore everything had to be in position before the actual run at both PSI and CERN, as well as for transportation between the two institutions – so that as little time as possible would elapse between the production of the sample and the measurement.

The idea for the experiment arose in 2012. PSI researcher Schumann knew that she could extract the rare beryllium-7 from the cooling water of the Swiss Spallation Neutron Source SINQ, which is operated at PSI for experiments with neutron beams.

Here at PSI, with SINQ and the other large research facilities, we have unique sources for harvesting rare radioactive isotopes, Schumann says. For the researchers who operate and use these facilities, these isotopes are a by-product – but for many other research institutions, they are very useful and urgently needed. Like gold prospectors, Schumann and her research group extract these rare isotopes. And then we act as an interface to other researchers outside PSI who are interested in enriched samples of these isotopes.

CERN is interested

Researchers at CERN showed interest in obtaining a sample of beryllium-7. With it, they knew they could tackle the cosmological lithium problem, Schumann explains.

So Schumann and her team set about the preparations: Within PSI, Schumann made contact with the scientists and engineers who operate SINQ. A special filter system meeting the isotope researchers' specifications was connected to the cooling water of SINQ, which could collect material containing a suitable amount of beryllium-7 over a period of about three weeks. To the layperson, our filter can be thought of as being quite similar to the familiar household filter for tap water, says Stephan Heinitz, scientist in the research group of Schumann.

Then, among other things, the materials gathered in this way had to be chemically separated. This requires special expertise – which luckily we have in my research group, Schumann says. Nevertheless, this procedure took another week and had to be carried out, for protection against radiation from the material, in a so-called hot cell – a laboratory set up for the manipulation of radioactive materials.

A transport weight of 800 kilograms

From there, the concentrated sample of beryllium-7 had to be transferred into a suitable mount, and this in turn into an apparatus about the size of a cooking pot, which met specifications for use in the experimental setup at CERN. The apparatus as well as the radiation-proof containers for transferring the material – all of it was custom-made, relates Emilio Maugeri, another researcher in Schumann's group.

Finally, arrangements had to be organised and approved to transport a heavy load of radioactive materials from PSI to CERN.

The actual sample that we delivered to CERN contained only a few millionths of a gram of beryllium-7, Schumann explains. But the required shielding brought the transport weight up to 800 kilograms.

Within the critical time period, everything succeeded according to plan. The CERN researchers were able to carry out the experiment with the PSI sample and determine the thus-far insufficiently known neutron capture cross-section of beryllium-7.

The cosmological lithium problem remains unsolved

The CERN and PSI scientists and their collaborators from 41 other research institutions were especially interested in a particular decay path of beryllium-7: the probability of a process by which an atomic nucleus of beryllium-7 traps a free neutron – that is, an elementary particle with no net charge. At the same time one of the protons leaves the beryllium nucleus. Thus, since the nucleus now contains one less proton (and one more neutron), the beryllium atom transforms itself into an atom of the element lithium: It becomes lithium-7. The so-called neutron capture cross-section – that is, the probability of this entire process – depends on the energy that the free neutron has. Therefore the researchers took advantage of the possibility at CERN to vary the energy of the neutrons, and they made a measurement series for a wide range of neutron energies.

Yet these latest measurements of the neutron capture cross-section have not solved the cosmological lithium problem. As Schumann puts it: With the new measurements, the CERN researchers were able to determine the neutron capture cross-section so precisely that it now is clear: The cosmological lithium problem can't be solved in this way; it still persists. The scientific community will have to keep looking for an explanation.

Text: Paul Scherrer Institute/Laura Hennemann

About PSI

The Paul Scherrer Institute PSI develops, builds and operates large, complex research facilities and makes them available to the national and international research community. The institute's own key research priorities are in the fields of matter and materials, energy and environment and human health. PSI is committed to the training of future generations. Therefore about one quarter of our staff are post-docs, post-graduates or apprentices. Altogether PSI employs 2100 people, thus being the largest research institute in Switzerland. The annual budget amounts to approximately CHF 390 million. PSI is part of the ETH Domain, with the other members being the two Swiss Federal Institutes of Technology, ETH Zurich and EPFL Lausanne, as well as Eawag (Swiss Federal Institute of Aquatic Science and Technology), Empa (Swiss Federal Laboratories for Materials Science and Technology) and WSL (Swiss Federal Institute for Forest, Snow and Landscape Research).
(Last updated in May 2018)
Additional information
http://psi.ch/nNsY – „Astral matter from the Paul Scherrer Institute“ press release from 8 April 2014
http://psi.ch/SGEi – “Radioactive targets produced at PSI enable improving the Big Bang Theory” notice from 19 October 2016
Dr. Dorothea Schumann
Head of the research group Isotope and Target Chemistry
Paul Scherrer Institute, 5232 Villigen PSI, Switzerland
Telephone: +41 56 310 40 04
E-mail: dorothea.schumann@psi.ch [German, English]

Dr. Stephan Heinitz
Research group Isotope and Target Chemistry
Paul Scherrer Institute, 5232 Villigen PSI, Switzerland
Telephone: +41 56 310 45 83
E-mail: stephan.heinitz@psi.ch [German, English, Russian]

Dr. Emilio Maugeri
Research group Isotope and Target Chemistry
Paul Scherrer Institute, 5232 Villigen PSI, Switzerland
Telephone: +41 56 310 24 07
E-mail: emilio-andrea.maugeri@psi.ch [English, Italian, French]
Original Publication
The 7Be(n;p)7Li reaction and the Cosmological Lithium Problem: measurement of the cross section in a wide energy range at n_TOF (CERN)
L. Damone et al.
Physical Review Letters, 24 July 2018 (online)
DOI: 10.1103/PhysRevLett.121.042701