paper

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

References in corpus (11)

Cited by in corpus (2)