R-process Nucleosynthesis of Subminimal Neutron Star Explosions
arXiv:2211.14023 · doi:10.3847/1538-4357/acf570
Abstract
We show that a minimum-mass neutron star undergoes delayed explosion after mass removal from its surface. We couple the Newtonian hydrodynamics to a nuclear reaction network of isotopes to study the nucleosynthesis and neutrino emission during the explosion. An electron antineutrino burst with a peak luminosity of erg s is emitted while the ejecta is heated to K. A robust -process nucleosynthesis is realized in the ejecta. Lanthanides and heavy elements near the second and third -process peaks are synthesized as end products of nucleosynthesis, suggesting that subminimal neutron star explosions could be an important source of solar chemical elements.
14 pages, 18 figures, published version
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