Dynamics of neutrino-driven winds: inclusion of accurate weak interaction rates in strong magnetic fields

Abstract

Solving Newtonian steady-state wind equations with accurate weak interaction rates and magnetic fields (MFs) of young neutron stars considered, we study the dynamics and nucleosynthesis of neutrino-driven winds (NDWs) from proto neutron stars (PNSs). For a typical 1.4 M${}_{\odot }$ PNS model, we find the nucleosynthesis products are closely related to the luminosity of neutrinos and anti-neutrinos. The lower the luminosity is, the larger effect to the NDWs caused by weak interactions and MFs is. At a high anti-neutrino luminosity of typically $8\times 10^{51}$ erg s${}^{-1}$, neutrinos and anti-neutrinos dominate the processes in a NDW and the MFs hardly change the wind's properties. While at a low anti-neutrino luminosity of $10^{51}$ erg s${}^{-1}$ at the late stage of a NDW, the mass of product and nucleosynthesis are changed significantly in the strong MFs, they are less important than those in the early stage when the anti-neutrino luminosity is high. Therefore for the most models considered for the NDWs from PNSs, based on our calculations the influences of MFs and the net weak interactions on the nucleosynthesis is not significant.

8 pages, 3 figures, accepted for publication in RAA

References in corpus (5)

• Nucleosynthesis in Electron Capture Supernovae of AGB Stars
• Dynamical r-process studies within the neutrino-driven wind scenario and its sensitivity to the nuclear physics input
• Integrated Nucleosynthesis in Neutrino Driven Winds
• Influence of light nuclei on neutrino-driven supernova outflows
• Magnetic Field-Decay-Induced Electron Captures: a Strong Heat Source in Magnetar Crusts

Cited by in corpus (1)

• Singlet pairing gaps of neutrons and protons in hyperonic neutron stars