An international research team has for the first time combined data from heavy ion experiments, gravitational wave measurements and other astronomical observations using advanced theoretical modeling to more precisely constrain the properties of nuclear matter as it can be found inside neutron stars. The results were published in the journal Nature.
Throughout the universe, neutron stars are born in supernova explosions that mark the end of the life of massive stars. Sometimes neutron stars are linked in binary systems and will eventually collide with each other. These high energies, astrophysical phenomena present such extreme conditions that they produce most of the heavy elements, such as silver and gold. Therefore, neutron stars and their collisions are unique laboratories for studying the properties of matter at densities far beyond the densities inside atomic nuclei. Heavy ion collision experiments conducted with particle accelerators are a complementary means of producing and probing matter at high density and under extreme conditions.
New insights into the fundamental interactions at play in nuclear matter
“Combining insights from nuclear theory, nuclear experiments and astrophysical observations is essential to shed light on the properties of neutron-rich matter across the full density range probed in neutron stars,” said Sabrina Huth, from the Institute of Nuclear Physics of the Technical University of Darmstadt, which is one of the main authors of the publication. Peter TH Pang, another lead author from the Institute of Gravitational and Subatomic Physics (GRASP) at Utrecht University, added: “We find that the stresses from gold ion collisions with particle accelerators show remarkable consistency with astrophysical observations, even if they are obtained with completely different methods.”
Recent advances in multi-messenger astronomy have provided the international research team, made up of researchers from Germany, the Netherlands, the United States and Sweden, with new insights into fundamental interactions at stake in nuclear material. In an interdisciplinary effort, the researchers included the information obtained during heavy ion collisions in a framework combining astronomical observations powerful electromagnetic signals, gravitational wave measurements and astrophysical calculations with Nuclear physics calculations. Their systematic study combines all of these individual disciplines for the first time, indicating higher pressure at intermediate densities in neutron stars.
Heavy ion collision data included
The authors incorporated information from the gold ion collision experiments carried out at GSI Helmholtzzentrum für Schwerionenforschung in Darmstadt as well as at Brookhaven National Laboratory and Lawrence Berkeley National Laboratory in the United States in their multi-step procedure which analyzes the constraints of nuclear theory and astrophysical observations, including measurements of mass of neutron stars through radio observations, information from the Neutron Star Interior Composition Explorer (NICER) mission on the International Space Station (ISS), and multi-messenger observations of binary neutron star mergers.
Nuclear theorists Sabrina Huth and Achim Schwenk of the Technical University of Darmstadt and Ingo Tews of Los Alamos National Laboratory have played a key role in translating information obtained from heavy ion collisions into matter of neutron stars , necessary to integrate the astrophysical constraints.
The inclusion of heavy ion collision data in the analyzes added constraints in the density region where nuclear theory and astrophysical observations are less sensitive. This helped provide a more complete understanding of dense matter. In the future, improved constraints of heavy ion collisions may play an important role in linking nuclear theory and astrophysical observations by providing complementary information. This is especially true for experiments that probe higher densities, and reducing experimental uncertainties has great potential to provide new constraints for the properties of neutron stars. New information from either side can easily be included in the framework to further enhance the understanding of dense matter in years to come.
Sabrina Huth et al, Constraining neutron star matter with microscopic and macroscopic collisions, Nature (2022). DOI: 10.1038/s41586-022-04750-w
Technical University Darmstadt
Quote: New insights into neutron star matter (June 8, 2022) Retrieved June 9, 2022 from https://phys.org/news/2022-06-insights-neutron-star.html
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