We would like to invite you to participate in the Joint CNA (Center for Nuclear Astrophysics, Shanghai Jiao Tong University) and JINA-CEE (The Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements) Winter School on  Nuclear Astrophysics to be held onDecember 12-17, 2016, at the Shanghai Jiao Tong University in Shanghai, China.

We will be holding a JINA-CEE/TRIUMF Satellite Workshop on Recoil Separators for Nuclear Astrophysics on Tues 11th and Wed 12th October, 2016, at the TRIUMF laboratory in Vancouver, Canada.

The Workshop is funded by JINA-CEE and TRIUMF.

The focus of the school will be the understanding and application of nuclear reaction networks to astrophysical models for systems such as novae, x-ray bursts (rp-process) and neutron star mergers (r-process). The reaction network employed will be the public NucNet code published by Prof. Bradley Meyer, of Clemson University.

The Torino Workshops series started in Torino in 1995 and 11 workshops have been held so far in different parts of the world. The 12th workshop will be held jointly with the biannual CSFK Astromineralogy Workshop IV, which started in Budapest in 2010.

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.
 

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.

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.

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.

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.

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.
 

The purpose of this meeting is to collect ideas for the preparation of the next NuPECC long range plan in Nuclear Astrophysics.

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:

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. 

The 2015 Low Energy Community Meeting was held in East Lansing Michigan on the Campus of Michigan State University.

NSF-funded Physics Frontiers Centers (PFCs) are pushing the frontiers of science across the disciplines of physics.

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.