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GUPPY Nuclear Astrophysics Course (Opens in a new window)
This short course was for young students (grades 3-6) in GATE’s Gifted University for Parents and Precocious Students (GUPPY). It included a hands-on lesson on stellar nuclear reactions and a tour of the National Superconducting Cyclotron Laboratory.
GUPPY Nuclear Astrophysics Course (Opens in a new window)
This short course was for young students (grades 3-6) in GATE’s Gifted University for Parents and Precocious Students (GUPPY). It included a hands-on lesson on stellar nuclear reactions and a tour of the National Superconducting Cyclotron Laboratory.
Grandparents University Nuclear Lesson with Marbles (Opens in a new window)
This program invites MSU alumni to bring their grandchildren for three days of classes on campus. Participants used JINA-CEE’s “marble nuclei” model to learn about isotopes and nuclear reactions before touring the National Superconducting Cyclotron laboratory
Grandparents University Nuclear Lesson with Marbles (Opens in a new window)
This program invites MSU alumni to bring their grandchildren for three days of classes on campus. Participants used JINA-CEE’s “marble nuclei” model to learn about isotopes and nuclear reactions before touring the National Superconducting Cyclotron laboratory
Physics of Atomic Nuclei (Opens in a new window)
Physics of Atomic Nuclei (PAN) Program (Opens in a new window)
Physics of Atomic Nuclei (PAN) Program is a week long program at one of two world leading nuclear physics laboratories: Nuclear Science Laboratory located on the campus of the University of Notre Dame and the National Superconducting Cyclotron Laboratory located on the campus of Michigan State University. Learn nuclear astrophysics through lectures from faculty, and modern physics experiments. Read more.
NIC XV School (Opens in a new window)
Burst Environment, Reactions and Numerical Modelling Workshop 2018 (BERN18) (Opens in a new window)
There is a new impetus in efforts to reconcile thermonuclear burst observations and models, and also incorporate in more detail the nuclear physics inputs. At the same time, new experimental data is becoming available, that is challenging our existing understanding of burst physics.
2018 JINA-CEE Frontiers in Nuclear Astrophysics: Conference (Opens in a new window)
2018 JINA-CEE Frontiers in Nuclear Astrophysics: Junior Workshop (Opens in a new window)
The Junior Researcher Workshop is open to graduate students and postdocs and will be held on May 21-22 prior to the main conference. This portion of the meeting consists of students and postdoc research, as well as professional development workshops.
Summer school: Neutron star mergers for non-experts (Opens in a new window)
Recently a neutron star merger was observed with gravitational waves and electromagnetically at frequencies from radio to gamma rays. This single event GW170817 dramatically advances nuclear astrophysics and heralds an exciting new era in multi-messenger astronomy.
NS3 Nuclear Science Summer School (Opens in a new window)
NS3 is a summer school for undergraduate students that aims to introduce the participants to the field of nuclear science. NS3 will be hosted by Michigan State University (MSU) and will offer lectures and hands-on activities covering selected nuclear science topics. The school activities will take place at the National Superconducting Cyclotron Laboratory (NSCL) and will include lectures by local and visiting researchers, nuclear physics labs, a tour of the facility, discussions with graduate students and faculty, and more.
2018 NASA Laboratory Astrophysics Workshop (Opens in a new window)
The 2018 NASA Laboratory Astrophysics Workshop was held on April 8th through April 11th at the UGA Center for Continuing Education and Hotel. Available talks from the meeting can be found online.
Nuclear Astrophysics at Rings and Recoil Separators (NARRS2018) (Opens in a new window)
INT-JINA Topical Workshop (Opens in a new window)
Observation of gravitational waves (GWs), gamma-rays, x-rays, optical, infrared and radio waves from a neutron star (NS) merger event, now called GW170817, has the potential to revolutionize nuclear astrophysics. Data from this event has already provided strong hints that heavy elements are produced in NS mergers, and that these elements directly influence the observed optical and infra-red light curves. Properties of dense matter which was expected to play a key role also appear to be essential in interpreting the GW data.