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R-Matrix Workshop on Methods and Applications (Opens in a new window)
We would like to invite you to participate in a JINA-CEE sponsored workshop on all things R-matrix that will be held June 27 to July 1, 2016, in Santa Fe, New Mexico, USA.
Niigata School on Nuclear Astrophysics (NIC XIV School) (Opens in a new window)
The NIC School will take place at Niigata University, about 10 km from the NIC-XIV Symposium site from 13-17 June 2016, preceding the NIC-XIV Symposium. Lectures, presented by internationally recognized experts, will cover various areas of research in nuclear astrophysics, from theories to experiments and observations.
The r-Process Nucleosynthesis: Connecting FRIB with the Cosmos (Opens in a new window)
This is an exciting time for the study of r-process nucleosynthesis. Astrophysical simulations of neutron star mergers and core collapse supernovae are making rapid progress, and locating attractive sites for the r-process.
Neutron Stars in the Multi-Messenger Era (Opens in a new window)
This international symposium aims to bring theorists and observers together to assess the current state of knowledge, and to identify areas in which more theoretical work is needed to enable interpretation and extraction of information from observations. Additional goals are to inform observers and experimenters regarding complementary efforts, and to promote new collaborations to undertake in-depth investigations. Because of the breadth of physics and astrophysics needed to describe neutron stars, frontier efforts that are necessarily multidisciplinary are required.
JINA-CEE Satellite Workshop on Experiments for X-ray Burst Nucleosynthesis (Opens in a new window)
The workshop will focus on fostering collaborations, sharing of resources, and new experimental initiatives aimed at improving our understanding of X-ray bursts and will give the opportunity to bring the community together to discuss the uncertainties in X-ray burst nucleosynthesis, the availability of current and future resources, and how to utilize resources more effectively to address uncertainties in X-ray bursts.
2016 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 29-31, 2016, at the Gillespie Conference Center, 53995 SR 933, South Bend, IN 46637.
NuPECC Long Range Plan Town Meeting in Nuclear Astrophysics (Opens in a new window)
The purpose of this meeting is to collect ideas for the preparation of the next NuPECC long range plan in Nuclear Astrophysics.
Electron Capture Supernovae and Super-AGB Stars (Opens in a new window)
This Joint Institute for Nuclear Astrophysics (JINA) workshop aims to bring together Australian and international experts from stellar evolution, supernova theory, stellar spectroscopy, hydrodynamics, and nuclear physics with expected topics including:
Nucleosynthesis Away From Stability (Opens in a new window)
The workshop "Nucleosynthesis away from stability" addresses reaction rates and nucleosynthesis of radioactive species, and implications for GCE. The goal of the workshop is to document the present state of knowledge, identify key open questions, and coordinate efforts in experiments, simulations and observations.
2015 Low Energy Community Meeting (Opens in a new window)
The 2015 Low Energy Community Meeting was held in East Lansing Michigan on the Campus of Michigan State University.
Google Hangout for JINA-CEE (Opens in a new window)
NSF-funded Physics Frontiers Centers (PFCs) are pushing the frontiers of science across the disciplines of physics.
The Neutron Star Radius, And All That Jazz (Opens in a new window)
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.
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.