Active-Sterile Neutrino Oscillations in Neutrino-driven Winds: Implications for Nucleosynthesis

A protoneutron star produced in a core-collapse supernova (CCSN) drives a wind by its intense neutrino emission. We implement active-sterile neutrino oscillations in a steady-state model of this neutrino-driven wind to study their effects on the dynamics and nucleosynthesis of the wind in a self-con...

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Veröffentlicht in:	The Astrophysical journal 2019-08, Vol.880 (2), p.81
Hauptverfasser:	Xiong, Zewei, Wu, Meng-Ru, Qian, Yong-Zhong
Format:	Artikel
Sprache:	eng
Schlagworte:	abundances – stars: mass-loss – stars: neutron – supernovae: general Astronomy & Astrophysics ASTRONOMY AND ASTROPHYSICS Astrophysics Neutrinos neutrinos – nuclear reactions Nuclear fusion nuclear reactions, nucleosynthesis, abundances nucleosynthesis Oscillations stars: mass-loss stars: neutron Steady state models Stellar winds Supernova supernovae: general Wind Wind effects Wind speed Wind velocities Zirconium isotopes
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