Global Nuclear Energy Initiative at LBNL
Above (left) Silicon Telescope for Reaction Studies (STARS)Above (right) Clover detectors (gamma rays) for light charged particles
Above (left) Silicon Telescope for Reaction Studies (STARS)Above (right) Clover detectors (gamma rays) for light charged particles
Scientists have new insights into factors that determine how twin neutron stars—stars with the same mass but different sizes and compositions—can coexist.
Theoretical calculations enable more accurate determination of reaction rates for modelling primordial lithium-6 abundance and massive stars’ lifecycle.
Signup for the Office of Science’s GovDelivery email service, and check the box for the Nuclear Physics Program in your subscriber preferences.
Subscribe