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R-process Nucleosynthesis of Subminimal Neutron Star Explosions
Ist Teil von
The Astrophysical journal, 2023-10, Vol.956 (2), p.115
Ort / Verlag
Philadelphia: The American Astronomical Society
Erscheinungsjahr
2023
Link zum Volltext
Quelle
EZB Electronic Journals Library
Beschreibungen/Notizen
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 ∼4500 isotopes to study the nucleosynthesis and neutrino emission during the explosion. An electron antineutrino burst with a peak luminosity of ∼3 × 10
50
erg s
−1
is emitted while the ejecta is heated to ∼10
9
K. A robust
r
-process nucleosynthesis is realized in the ejecta. Lanthanides and heavy elements near the second and third
r
-process peaks are synthesized as end products of nucleosynthesis, suggesting that subminimal neutron star explosions could be an important source of solar chemical elements.