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Mad Scientist Camp (Opens in a new window)
PAN for Teachers (Opens in a new window)
MST Nuclear Astrophysics Course (Opens in a new window)
Art 2 Science Camp (Opens in a new window)
The Neutron Star Radius, And All That Jazz (Opens in a new window)
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
Young Scientists Study Group on Neutrino & Nuclear Physics for Nucleosynthesis & Chemical Evolution (Opens in a new window)
In China, the Jiangmen Underground Neutrino Observatory (JUNO) will be both searching for new physics and observing astrophysical neutrinos. The Jinping Underground Laboratory for Nuclear Astrophysics (JUNA) will be measuring key nuclear reactions for stellar evolution and nucleosynthesis.
Physics of Atomic Nuclei (Opens in a new window)
P-Process Workshop 2015: Status and Outlook (Opens in a new window)
Workshop on Binary Neutron Star Mergers (Opens in a new window)
The summer of 2015 will mark the onset of the first science run of 2nd-generation interferometric gravitational wave detectors and over the next years several such detectors will form a world-wide network. The most promising sources of gravitational waves for these instruments are mergers of compact binaries. In particular, the coalescences of binary neutron star systems are considered to be the most probable events. Through gravitational wave observations, the equation of state of high-density matter is expected to be significantly constrained.
GNASH: The anomalous metal-poor stars and convective-reactive nuclear astrophysics (Opens in a new window)
Nuclear Physics in Astrophysics VII: 28th EPS Nuclear Physics Divisional Conference (Opens in a new window)
Nuclear physics plays a central role in astrophysics as it accounts for the processes that govern the lives of stars and the creation of all elements beyond primordial hydrogen and helium. The energy released by nuclear reactions powers some of the most spectacular explosions in the Universe, which in turn contribute to the chemical evolution of our and other galaxies.
2015 JINA-CEE Frontiers in Nuclear Astrophysics (Opens in a new window)
Dear Nuclear Astrophysics Colleague,
We would like to invite you to participate in the JINA-CEE Frontiers in Nuclear Astrophysics Meeting to be held on March 23-25, 2015, at the James B. Henry Center for Executive Development, Michigan State University, 3535 Forest Road, Lansing, MI.
Science Alive (Opens in a new window)
IMSA Intersession PAN (Opens in a new window)
Mini-PAN (Opens in a new window)
A half-day event, this introduced more than 50 high school physics students in LCC’s Early College to the field of nuclear astrophysics. It included hands-on lessons regarding isotopes, nuclear reactions, and neutron capture. Graduate students gave brief explanations of their research and highlighted their own paths that led to JINA-CEE.
Physics of Atomic Nuclei (PAN) (Opens in a new window)
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.
The r-Process: Status and Challenges (Opens in a new window)
Recent developments in theory, simulations and observations have begun to shed new light on the origin of the heavy elements in the universe, especially those made by rapid neutron capture, the r-process. The workshop aims to bring together nuclear theorists, experimentalists, astrophysicists, and astronomers to discuss these advances and foster collaborations. A coordinated effort is critical to solving the grand challenge problem of pinning down the site(s) and understanding the possible diversity in the r-process.