EU funding in the millions to study element formation in neutron star fusions — ERC Synergy Grant goes to international research team with GSI/FAIR participation
IMAGE: THIS ARTIST’S IMPRESSION SHOWS TWO TINY BUT VERY DENSE NEUTRON STARS AT THE POINT AT WHICH THEY MERGE AND EXPLODE AS A KILONOVA. view more
CREDIT: PICTURE: UNIVERSITY OF WARWICK/MARK GARLICK/ESO
The European Union has awarded a total of 11.3 million euros over a period of six years to the HEAVYMETAL research project, which aims to investigate the synthesis of chemical elements in neutron star mergers. Privatdozent Dr. Andreas Bauswein, a researcher in the Theory Department of the GSI Helmholtzzentrum für Schwerionenforschung in Darmstadt, is part of the four-member international team that receives the funding as part of an ERC Synergy Grant. At GSI, currently the international accelerator center FAIR (Facility for Antiproton and Ion Research) is under construction. In the future, states of matter as they occur in the interior of stars, stellar explosions and neutron star mergers will be studied in the laboratory at FAIR.
Neutron stars are remnants formed during stellar collapse in a supernova explosion. They have extremely strong gravitational fields, exceptionally intense magnetic fields, and consist of matter with very high density, making them important natural laboratories for fundamental physics. In binary systems consisting of two neutron stars, mergers of these extreme objects can occur: The two high-density stars collide at about 20% of the speed of light, leading to temperatures of several 100 billion kelvin. During the collision, considerable amounts of neutron-rich matter are expelled, in which heavy chemical elements such as silver, gold, platinum and many more are formed. The ejected matter evolves into a fireball, which is visible as a so-called kilonova.
“Kilonova science is emerging as a new field in astrophysics, offering an enormous discovery potential for understanding neutron stars, the origin of the heavy elements in particular, the physics of exotic heavy nuclei, and the phases of hot, ultra-dense, and exotic matter”, Bauswein explains his research focus. “The increasing sensitivity of gravitational wave detectors, also providing improved sky localisations for follow-up observations, and the next generation of telescopes, means that we expect an abundance of new kilonovae observations in the coming years. I look forward to exploring the research field in the best possible way together with my colleagues within the framework of the ERC Synergy Grant.”
The research project HEAVYMETAL (How Neutron Star Mergers make Heavy Elements) aims to make a big step in explaining kilonova explosions by spectroscopically dissecting their emissions and connecting them quantitatively to the physical properties of the neutron star merger. In doing so, HEAVYMETAL will probe the origin of the heavy elements, and delineate the nuclear and astrophysical pathways that created them — the so-called “r-process”. The research team will try to decipher the details of the observed spectra and use that information to gain unprecedented insight into the physical processes of the neutron star merger.
HEAVYMETAL brings together experts from different fields related to kilonova research who, by working together, can exploit synergies in the ambitious goal of explaining element synthesis: Andreas Bauswein and his team at GSI/FAIR have a long and high impact track record in connecting advanced hydrodynamical simulations to r-process nucleosynthesis, kilonova modelling and the properties of high-density matter. Already in 2017, Bauswein succeeded in securing an ERC Starting Grant of 1.5 million euros with his project GreatMoves on the simulation of neutron star mergers. In addition to Bauswein, Professor Darach Watson, University of Copenhagen, Denmark, Professor Padraig Dunne, University College Dublin, Ireland, and Dr. Stuart Sim, Queen's University, Belfast, UK, are also members of the research team funded by the ERC Synergy Grant.
Watson has been a key player in gaining and interpreting kilonova data and has worked in observational astronomy for two decades. Dunne is a leading experimental physicist in the area of laser plasma spectroscopy with a focus on laser plasmas of heavy elements. Sim is an expert in the modelling of radiation in explosive environments and in the development of codes designed to simulate detailed radiation-matter interactions and photon transport in rapidly expanding matter ejecta.
“We are very proud to have gained the support of the European Union for this cutting-edge research project,” says Professor Paolo Giubellino, Scientific Managing Director of GSI and FAIR. “International and interdisciplinary collaboration has always played a major role in our work. The implementation of many scientific projects is hardly conceivable without worldwide collaborations and the use of synergies between researchers. This starts with individual research areas such as the study of kilonovae in this group of experts and continues with the construction of our future research facility FAIR, which is being built in international collaboration between many researchers and nations.” FAIR is currently under construction in Darmstadt and will be connected to the GSI accelerator facility. In the future, it will be possible at FAIR to study states of matter similar to those occurring in the interior of stars, stellar explosions and neutron star mergers in the laboratory, which directly links to the HEAVYMETAL project.
ERC Synergy Grants are awarded by the European Union to research groups of two to a maximum of four scientists in any research area, exclusively on the basis of scientific excellence. The decisive factor for the grant is that the research in question cannot be carried out by the individual researchers alone, but only through joint cooperation.
Colorcoded is the density in the equatorial plane.
Matter is ejected from these violent collions expanding with several 10% the speed of light.
CREDIT
Simulation and visualization: G. Lioutas, GSI/FAIR
World-class research into Greenland's oldest ice and the Universe's densest stars win very large EU grants
Grant and Award AnnouncementIMAGE: THE GREEN2ICE TEAM. FROM THE LEFT: ANDERS SVENSSON, DORTHE DAHL-JENSEN, PIERRE-HENRI BLARD AND FRANÇOIS FRIPIAT (CREDIT: DORTHE DAHL-JENSEN) view more
CREDIT: DORTHE DAHL-JENSEN
When was Greenland actually green? And how does the Universe make gold, platinum and uranium? Researchers from the University of Copenhagen have just received 11.4 million euro to answer these big questions. The prestigious ERC Synergy grant from the European Research Council has been awarded, among others, to the ice physicists Dorthe Dahl-Jensen and Anders Svensson, and the astrophysicist Darach Watson.
The first ice cores were drilled in Greenland in 1955. But many an unsolved mystery remains in the oldest, deepest ice. For example, when was Greenland last carpeted by forest? And, when was the ice sheet formed? Niels Bohr Institute ice physicists will use a unique collection of old ice cores alongside freshly drilled ones to find answers from the past that will enlighten us about climatic change in the future.
"The answers ensconced in the oldest ice will point to the future and provide us with knowledge that is far more accurate than what we have today with regards to how much our oceans stand to rise and as to when the ice sheet will no longer be able to be saved. So, this isn't just exotic basic research, it is important knowledge about the ice sheet's robustness in the face of climate change," explains Professor Dorthe Dahl-Jensen of the Niels Bohr Institute.
Professor Dahl-Jensen heads GREEN2ICE, a large-scale research project that has just received a rare DKK 103 million (13.9 million euro) Synergy Grant from the European Research Council. Just over DKK 63 million (8.5 million euro) will go to the University of Copenhagen.
"This is a dream project for me - something I've been thinking about messing around with for many years. When we drill ice cores, we gain access to fascinating material from the depths, in the form of rocks, soil, small plant fossils and gases encased in air bubbles. These demonstrate that Greenland was once forested. By looking at these materials, we will be able to find out when this was, what type of forest existed and what sort of temperatures allowed for the forest to grow," explains Dorthe Dahl-Jensen.
Among other things, the researchers will be able to measure when gas in the small air bubbles in the ice was trapped. Other measurements will look at how long it has been since the stones found in the ice cores were shined upon by the sun.
Because the material is both rare and difficult to obtain, the researchers have stored it away in a freezer for many years, explains associate professor and ice physicist Anders Svensson, the other UCPH researcher involved with the project:
"We only have one chance. Indeed, the ice cores contain so little of this material and it can only be used once. That's what makes handling it is so risky and why we have never dared to do so until now, as methods have improved. But there is an enormous amount to gain if we succeed."
The experts' best guess as to when Greenland was last completely ice-free is about a million years ago. Using the new methods, the research team will test this hypothesis. Until now, it has only been possible to date ice back roughly 130,000 years.
In addition to Dorthe Dahl-Jensen and Anders Svensson, the GREEN2ICE research team consists of François Fripiat of the Université Libre de Bruxelles, Belgium and Pierre-Henri Blard from CNRS-Université de Lorraine, France. Other GREEN2ICE project partners are GEUS, DTU and the University of Manitoba.
An explosion of heavymetal
It's gold and platinum. It is tin and uranium. It is the vital iodine we have in our blood. It is the molybdenum that all living organisms need to use. The heavy elements are an important part of the world around us. However, it has always been a major mystery how these elements were created.
Research points to the heaviest elements in the periodic table being created in the gigantic explosion that occurs when two neutron stars collide – a phenomenon that only occurs once every 100,000 years in our galaxy. The only time the phenomenon has been observed in detail was in 2017. But how it happens physically has so far not been possible to answer.
The researchers in the second ambitious project for which the University of Copenhagen has received an ERC Synergy grant now aim to do just that. The HEAVYMETAL project has received almost DKK 84 million (11.3 million euro), of which almost 22 million kroner (2.9 million euro) has been awarded to Darach Watson from the Niels Bohr Institute, who leads the project.
“Neutron star collisions are a treasure trove of information that potentially allow us to answer some of the biggest open questions in physics and cosmology. First of all, about how a large number of the elements are created. But they have been extremely difficult to investigate. However, I believe it is possible with the outstanding team we have assembled here," says astrophysicist and associate professor Darach Watson.
The key is to decipher the spectroscopic data from the explosion, which was created during the neutron star collision in 2017. In this way, the research team will be able to see in detail the newly created heavy elements that are blown out in a radioactive fireball when neutron stars collide.
However, it first and foremost requires being able to model the very complex atomic structures of the heavy elements, which is extremely difficult.
"We expect to be able to measure both where and how the heavy elements are formed, how they are distributed, how much matter is ejected and more. We will dissect the explosion itself and then try to map in detail the nuclear physics of that process,” explains Darach Watson.
And it may also be possible to provide answers to several other important questions, such as how fast the Universe is expanding and how black holes are created.
HEAVYMETAL has assembled four different groups that work together as an international team of world-leading experts in each of their fields. In addition to Darach Watson who is the leader of the Copenhagen team, Andreas Bauswein leads the group at the GSI Helmholtzzentrum für Schwerionenforschung in Germany, Padraig Dunne the group from University College Dublin in Ireland, while Stuart Sim leads the Queen's University in Belfast, Northern Ireland group.
"For me, this is a dream team. Normally, as a researcher, you sit a lot by yourself. The fact that we can make such direct use of each other's different expertise will make a huge difference and really turbo-charge the research so that we can reach new results much faster," concludes Darach Watson.
Dorthe Dahl-Jensen
CREDIT
Emilie Thejll-Madsen
The four PIs of HEAVYMETAL (left to right): Darach Watson, Stuart Sim, Padraig Dunne, Andreas Bauswein
CREDIT
Darach Watson
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