Page 2: Research news on Explosive nucleosynthesis

Explosive nucleosynthesis is a research area in nuclear astrophysics that investigates the production of chemical elements and isotopes in environments where rapid energy release drives nonequilibrium nuclear reactions, typically associated with stellar explosions such as core-collapse and thermonuclear supernovae, novae, and neutron star mergers. It focuses on reaction networks under extreme temperatures, densities, and dynamic timescales, including rapid neutron capture (r-process), rapid proton capture (rp-process), and explosive silicon and oxygen burning. The field integrates nuclear reaction cross sections, equation-of-state physics, hydrodynamic simulations, and observational abundance patterns to constrain explosion mechanisms and the origin of heavy elements in the universe.

Learning more about supernovae through stardust

Most of the diverse elements in the universe come from supernovae. We are, quite literally, made of the dust of those long-dead stars and other astrophysical processes. But the details of how it all comes about are something ...

How a nearby supernova left its mark on Earth life

When a massive star explodes as a supernova, it does more than release an extraordinary amount of energy. Supernovae explosions are responsible for creating some of the heavy elements, including iron, which is blasted out ...

New insights on the role of nucleon exchange in nuclear fusion

Low-energy nuclear fusion reactions can potentially provide clean energy. In stars, low-energy fusion reactions during the stages of carbon and oxygen burning are critical to stellar evolution. These reactions also offer ...

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