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.

The Rubin Observatory will rapidly detect more supernovae

In our galaxy, a supernova explodes about once or twice each century. But historical astronomical records show that the last Milky Way core-collapse supernova seen by humans was about 1,000 years ago. That means we've missed ...

Possible 'superkilonova' exploded not once but twice

When the most massive stars reach the ends of their lives, they blow up in spectacular supernova explosions, which seed the universe with heavy elements such as carbon and iron. Another type of explosion—the kilonova—occurs ...

Forget stardust—it was star ice all along

Carl Sagan famously said that "We're all made of star stuff." But he didn't elaborate on how that actually happened. Yes, many of the molecules in our bodies could only have been created in massive supernovae explosions—hence ...

Heaviest tin isotopes provide insights into element synthesis

An international team of researchers, led by scientists from GSI/FAIR in Darmstadt, Germany, has studied r-process nucleosynthesis in measurements conducted at the Canadian research center TRIUMF in Vancouver. At the center ...

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