Nucleosynthesis of an $11.8M_{\odot }$ Supernova with 3D Simulation of the Inner Ejecta: Overall Yields and Implications for Short-Lived Radionuclides in the Early Solar System

Abstract

Based on a 3D supernova simulation of an $11.8M_{\odot }$ progenitor model with initial solar composition, we study the nucleosynthesis using tracers covering the innermost $0.1M_{\odot }$ of the ejecta. These ejecta are mostly proton-rich and contribute significant amounts of ${}^{45}$Sc and ${}^{64}$Zn. The production of heavier isotopes is sensitive to the electron fraction and hence the neutrino emission from the proto-neutron star. The yields of these isotopes are rather uncertain due to the approximate neutrino transport used in the simulation. In order to obtain the total yields for the whole supernova, we combine the results from the tracers with those for the outer layers from a suitable 1D model. Using the yields of short-lived radionuclides (SLRs), we explore the possibility that an $11.8M_{\odot }$ supernova might have triggered the formation of the solar system and provided some of the SLRs measured in meteorites. In particular, we discuss two new scenarios that can account for at least the data on ${}^{41}$Ca, ${}^{53}$Mn, and ${}^{60}$Fe without exceeding those on the other SLRs.

arXiv comment16 pages, 9 Figures, 4 Tables

References in corpus (52)

• The chemical composition of the Sun
• Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions
• Nucleosynthesis and Evolution of Massive Metal-Free Stars
• Nucleosynthesis in neutrino-driven winds: I. The physical conditions
• Presupernova evolution and explosive nucleosynthesis of rotating massive stars in the metallicity range -3 <=[Fe/H]<= 0
• Monte Carlo Study of Supernova Neutrino Spectra Formation
• Observed and Physical Properties of Core-Collapse Supernovae
• Physics of Core-Collapse Supernovae in Three Dimensions: a Sneak Preview
• Energy Input and Mass Redistribution by Supernovae in the Interstellar Medium
• A two-parameter criterion for classifying the explodability of massive stars by the neutrino-driven mechanism
• Nucleosynthesis in neutrino-driven winds: II. Implications for heavy element synthesis
• Three-dimensional core-collapse supernova simulated using a 15 $M_{\odot }$ progenitor
• The Overarching Framework of Core-Collapse Supernova Explosions as Revealed by 3D Fornax Simulations
• Charged-Particle Thermonuclear Reaction Rates: II. Tables and Graphs of Reaction Rates and Probability Density Functions
• Weak magnetism for antineutrinos in supernovae
• A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code for Core-Collapse Supernovae II. Relativistic Explosion Models of Core-Collapse Supernovae
• A Simple Approach to the Supernova Progenitor-Explosion Connection
• Non-Radial Instabilities and Progenitor Asphericities in Core-Collapse Supernovae
• Composition of the Innermost Core Collapse Supernova Ejecta
• Three-Dimensional Simulations of Neutrino-Driven Core-Collapse Supernovae from Low-Mass Single and Binary Star Progenitors
• The Status of Multi-Dimensional Core-Collapse Supernova Models
• A Successful 3D Core-Collapse Supernova Explosion Model
• Nucleosynthesis in the Innermost Ejecta of Neutrino-Drive Supernova Explosions in Two Dimensions
• High-resolution supernova neutrino spectra represented by a simple fit
• The Dynamics of Neutrino-Driven Supernova Explosions after Shock Revival in 2D and 3D
• Integrated Nucleosynthesis in Neutrino Driven Winds
• Hard X-ray emission lines from the decay of Ti-44 in the remnant of supernova 1987A
• Nucleosynthesis in the Hot Convective Bubble in Core-Collapse Supernovae
• Radioactive nuclei from cosmochronology to habitability
• On The Intrinsic Diversity of Type II-Plateau Supernovae
• Two Dimensional Core-Collapse Supernova Explosions Aided by General Relativity with Multidimensional Neutrino Transport
• Neutrino-Nucleus Reaction Cross Sections for Light Element Synthesis in Supernova Explosions
• The Nickel Mass Distribution of Normal Type II Supernovae
• Effects of neutrino oscillations on nucleosynthesis and neutrino signals for an 18 M supernova model
• New result for the neutron $\beta$-asymmetry parameter $A_0$ from UCNA
• Three-Dimensional Core-Collapse Supernova Simulations with Multi-Dimensional Neutrino Transport Compared to the Ray-by-Ray-plus Approximation
• PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry II: Explodability and Global Properties
• The light curve of SN 1987A revisited: constraining production masses of radioactive nuclides
• Supernova Neutrino Nucleosynthesis of Light Elements with Neutrino Oscillations
• Evidence for an aspherical Population III supernova explosion inferred from the hyper metal-poor star HE1327-2326
• Neutrino Emission as Diagnostics of Core-Collapse Supernovae
• Implications for Post-Processing Nucleosynthesis of Core-Collapse Supernova Models with Lagrangian Particles
• The $\nu$ process in the light of an improved understanding of supernova neutrino spectra
• Surround & Squash: The Interstellar Medium around Scorpius Centaurus OB2
• r-Process Nucleosynthesis in Shocked Surface Layers of O-Ne-Mg Cores
• Injection of Short-Lived Radionuclides into the Early Solar System from a Faint Supernova with Mixing-Fallback
• Uncertainties in Supernova Yields I: 1D Explosions
• Low 60Fe abundance in Semarkona and Sahara 99555
• Nucleosynthesis in 2D Core-Collapse Supernovae of 11.2 and 17.0 M${}_{\odot }$ Progenitors: Implications for Mo and Ru Production
• Evidence from stable isotopes and Be-10 for solar system formation triggered by a low-mass supernova
• Production of Mo and Ru isotopes in neutrino-driven winds: implications for solar abundances and presolar grains
• The $\nu$-process with fully time-dependent supernova neutrino emission spectra

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