FRIB hosts summer school on neutron-star merger
The Facility for Rare Isotope Beams is hosting a summer school focused on the scientific discoveries resulting from the recent observation of a neutron-star merger.
The school runs until May 18 and is titled “Neutron star mergers for non-experts: GW170817 in the multi-messenger astronomy and FRIB eras.” It brings together graduate students, postdoctoral researchers and senior scientific experts working in nuclear physics, astrophysics, astronomy and related areas to discuss the impact of the merger on nuclear science and nuclear astrophysics.
“This is a unique and unprecedented opportunity to bring all these subfields of physics together,” said Charles Horowitz Indiana University professor and lead organizer.
Hosted by the FRIB Theory Alliance, a coalition of scientists from universities and national laboratories, this summer school has more than 80 attendees from around the world as well as over 20 zoom connections. Attendance is more than twice the originally expected number.
The observation of this merger provides additional information for nuclear astrophysics, and it signals a new era in multi-messenger astronomy. This summer school is designed to allow a broader audience to better appreciate the developments resulting from the observation of the merger. Lecturers at the summer school are from Columbia University, Indiana University, Princeton University, the Canadian Institute for Theoretical Astrophysics, Joint Institute for Nuclear Astrophysics – Center for the Evolution of the Elements (JINA-CEE) and Michigan State University.
For those who wish to participate online, the lectures are being livestreamed via Zoom: https://msu.zoom.us/j/656485558.
“This is a crash course covering the wide range of physics relevant to understanding neutron star mergers and gravitational wave event GW170817 in particular. This will help to give the students the tools they need to connect the science of FRIB to gravitational wave observations and, in the future, contribute to our understanding of the properties of neutron stars and the origin of the heavy elements in our galaxy,” said Luke Roberts, a lecturer at the school.
Filomena Nunes, FRIB Theory Alliance managing director, said that “there was a tremendous and worldwide response when we sent out the announcement of the school from truly passionate people who are now here learning more and sharing their excitement.”
Observing the neutron-star merger
In October 2017, the Gravitational Wave Laboratories LIGO and VIRGO announced the first observation of gravitational waves from the merger of two neutron stars on August 17, in an event called GW170817. Immediate follow-up observations with 70 observatories around the world revealed a short gamma-ray burst and a so-called “kilo-nova” associated with the same event.
A kilo-nova is the weeklong afterglow of a neutron star merger and is thought to be powered by the radioactive decay of rare isotopes produced and ejected during the merger.
GW170817 is a significant discovery with impact on nuclear astrophysics. It is the long-sought "smoking gun" observation that directly indicates a possible site for the rapid neutron capture process, or r-process, thought to be responsible for many of the heavy elements in nature.
The observations indicate that neutron star mergers occur frequently enough and eject enough material to be major nucleosynthesis sites. It is now more important than ever to understand the underlying nuclear physics to connect merger models with the new observations and to determine exactly which elements are produced in such events. In addition, the observations provide new information on the properties of neutron stars, which directly inform longstanding questions in nuclear science about the nature of nuclear matter.
MSU is establishing FRIB as a new scientific user facility for the Office of Nuclear Physics in the U.S. Department of Energy Office of Science. Under construction on campus and operated by MSU, FRIB will enable scientists to make discoveries about the properties of rare isotopes in order to better understand the physics of nuclei, nuclear astrophysics, fundamental interactions and applications for society, including in medicine, homeland security and industry.