News | JINA-CEE, Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements

Nuclear experimentalists, theorists, and astrophysicists constrain reaction rates necessary for understanding how massive stars explode

          Nuclear experimentalists, theorists, and astrophys…
                      Jul 01, 2017

          JINA Newsletter (June 2017)
                      Jun 30, 2017

Advanced LIGO and the Origin of the r-Process

          Advanced LIGO and the Origin of the r-Process
                      Jun 08, 2017

          First CASPAR beam on the horizon
                      Jun 01, 2017

i-process Nucleosynthesis and Mass Retention Efficiency in He-shell Flash Evolution of Rapidly Accreting White Dwarfs

          i-process Nucleosynthesis and Mass Retention Effic…
                      May 22, 2017

Rp-process in X-ray Bursts May Produce Heavier Elements Faster

          Rp-process in X-ray Bursts May Produce Heavier Ele…
                      May 01, 2017

Following the Cosmic Evolution Of Pristine Gas

          Following the Cosmic Evolution Of Pristine Gas
                      May 01, 2017

A Lower Limit on the Heat Capacity of a Neutron Star Core

          A Lower Limit on the Heat Capacity of a Neutron St…
                      Apr 21, 2017

Fingerprinting Neutron Stars Through Thermonuclear Bursts

          Fingerprinting Neutron Stars Through Thermonuclear…
                      Apr 21, 2017

Neutrino Cooling in the Accreted Neutron Star Ocean

          Neutrino Cooling in the Accreted Neutron Star Ocea…
                      Apr 20, 2017

Impact of (α, n) reactions on weak r-process in neutrino-driven winds

          Impact of (α, n) reactions on weak r-process in ne…
                      Apr 19, 2017

          Portrait Theater Performances
                      Mar 23, 2017