Page 3: Research news on Stellar nucleosynthesis

Stellar nucleosynthesis is the research area concerned with the nuclear processes by which chemical elements are formed and transformed within stars and related astrophysical environments. It encompasses hydrogen burning (pp-chains, CNO cycles), helium burning, advanced hydrostatic burning stages (carbon, neon, oxygen, silicon burning), and explosive nucleosynthesis in supernovae and neutron-star-related events. The field integrates nuclear reaction theory and measurements, stellar structure and evolution modeling, and observational constraints from stellar spectra and isotopic abundances. A central focus is quantifying reaction rates and yields to explain the origin and distribution of isotopes in the cosmos and to constrain models of stellar evolution and galactic chemical evolution.

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 ...

Cosmic ray research helps unravel lithium-7 origin

The origin of lithium (Li), the third element of the periodic table, has long been shrouded in mystery. This element, commonly found in cosmic rays as two stable isotopes, 6Li and 7Li, is crucial to understanding the origins ...

Flares from magnetized stars can forge planets' worth of gold

Astronomers have discovered a previously unknown birthplace of some of the universe's rarest elements: a giant flare unleashed by a supermagnetized star. The astronomers calculated that such flares could be responsible for ...

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 ...

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