Binary-Stripped Stars as Core-Collapse Supernovae Progenitors

Abstract

Most massive stars experience binary interactions in their lifetimes that can alter both the surface and core structure of the stripped star with significant effects on their ultimate fate as core-collapse supernovae. However, core-collapse supernovae simulations to date have focused almost exclusively on the evolution of single stars. We present a systematic simulation study of single and binary-stripped stars with the same initial mass as candidates for core-collapse supernovae (11 - 21 M${}_{\odot }$). Generally, we find that binary-stripped stars core tend to be less compact, with a more prominent, deeper silicon/oxygen interface, and explode preferentially to the corresponding single stars of the same initial mass. Such a dichotomy of behavior between these two modes of evolution would have important implications for supernovae statistics, including the final neutron star masses, explosion energies, and nucleosynthetic yields. Binary-stripped remnants are also well poised to populate the possible mass gap between the heaviest neutron stars and the lightest black holes. Our work presents an improvement along two fronts, as we self-consistently account for the pre-collapse stellar evolution and the subsequent explosion outcome. Even so, our results emphasize the need for more detailed stellar evolutionary models to capture the sensitive nature of explosion outcome.

arXiv commentsubmitted to ApJ

References in corpus (96)

• The chemical composition of the Sun
• Modules for Experiments in Stellar Astrophysics (MESA)
• Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars
• Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions
• Binary interaction dominates the evolution of massive stars
• Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions
• GW190814: Gravitational Waves from the Coalescence of a 23 M${}_{\odot }$ Black Hole with a 2.6 M${}_{\odot }$ Compact Object
• Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation
• Mass-loss predictions for O and B stars as a function of metallicity
• Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar
• Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions
• Compact Remnant Mass Function: Dependence on the Explosion Mechanism and Metallicity
• Binary Population and Spectral Synthesis Version 2.1: construction, observational verification and new results
• Nearby Supernova Rates from the Lick Observatory Supernova Search. II. The Observed Luminosity Functions and Fractions of Supernovae in a Complete Sample
• Black Hole Formation in Failing Core-Collapse Supernovae
• Core-collapse supernova equations of state based on neutron star observations
• The Black Hole Mass Distribution in the Galaxy
• Mass Limits For Black Hole Formation
• The High Angular Resolution Multiplicity of Massive Stars
• The Mass Distribution of Stellar-Mass Black Holes
• The effect of massive binaries on stellar populations and supernova progenitors
• Physics of Core-Collapse Supernovae in Three Dimensions: a Sneak Preview
• Core-Collapse Supernova Explosion Theory
• Type Ib/c supernovae in binary systems I. Evolution and properties of the progenitor stars
• Perspectives on Core-Collapse Supernova Theory
• A two-parameter criterion for classifying the explodability of massive stars by the neutrino-driven mechanism
• The Neutron Star and Black Hole Initial Mass Function
• The Mass Distribution of Stellar Black Holes
• Bolometric light curves and explosion parameters of 38 stripped-envelope core-collapse supernovae
• The massive binary companion star to the progenitor of supernova 1993J
• The death of massive stars - II. Observational constraints on the progenitors of type Ibc supernovae
• The Compactness of Presupernova Stellar Cores
• Symmetry Parameter Constraints From A Lower Bound On The Neutron-Matter Energy
• The Overarching Framework of Core-Collapse Supernova Explosions as Revealed by 3D Fornax Simulations
• Exploring the relativistic regime with Newtonian hydrodynamics: An improved effective gravitational potential for supernova simulations
• High Resolution Study of Presupernova Compactness
• The Evolution of Massive Helium Stars Including Mass Loss
• A Simple Approach to the Supernova Progenitor-Explosion Connection
• Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae
• Core-collapse explosions of Wolf-Rayet stars and the connection to type IIb/Ib/Ic supernovae
• Three-Dimensional Simulations of Neutrino-Driven Core-Collapse Supernovae from Low-Mass Single and Binary Star Progenitors
• Revival of The Stalled Core-Collapse Supernova Shock Triggered by Precollapse Asphericity in the Progenitor Star
• Characterizing the Gravitational Wave Signal from Core-Collapse Supernovae
• The Carnegie Supernova Project I: analysis of stripped-envelope supernova light curves
• The Explosion of Helium Stars Evolved With Mass Loss
• A Successful 3D Core-Collapse Supernova Explosion Model
• Type Ib and IIb supernova progenitors in interacting binary systems
• Fornax: a Flexible Code for Multiphysics Astrophysical Simulations
• Rapidly evolving transients in the Dark Energy Survey
• The Progenitor Dependence of the Preexplosion Neutrino Emission in Core-Collapse Supernovae
• The Tarantula Massive Binary Monitoring: I. Observational campaign and OB-type spectroscopic binaries
• Ionizing spectra of stars that lose their envelope through interaction with a binary companion: role of metallicity
• Three-Dimensional Supernova Explosion Simulations of 9-, 10-, 11-, 12-, and 13-M${}_{\odot }$ Stars
• General Relativistic Three-Dimensional Multi-Group Neutrino Radiation-Hydrodynamics Simulations of Core-Collapse Supernovae
• Rotation-supported Neutrino-driven Supernova Explosions in Three Dimensions and the Critical Luminosity Condition
• Pre-supernova evolution, compact object masses and explosion properties of stripped binary stars
• Investigating the properties of stripped-envelope supernovae, what are the implications for their progenitors?
• A Systematic Survey of the Effects of Wind Mass Loss Algorithms on the Evolution of Single Massive Stars
• The Progenitor Dependence of Three-Dimensional Core-Collapse Supernovae
• Binary progenitor models of type IIb supernovae
• Systematic Features of Axisymmetric Neutrino-Driven Core-Collapse Supernova Models in Multiple Progenitors
• On Variations Of Pre-Supernova Model Properties
• Progenitor-dependent Explosion Dynamics in Self-consistent, Axisymmetric Simulations of Neutrino-driven Core-collapse Supernovae
• Electron-Capture and Low-Mass Iron-Core-Collapse Supernovae: New Neutrino-Radiation-Hydrodynamics Simulations
• Crucial Physical Dependencies of the Core-Collapse Supernova Mechanism
• Uncovering the Putative B-Star Binary Companion of the SN 1993J Progenitor
• A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary
• Magnetorotational Explosion of A Massive Star Supported by Neutrino Heating in General Relativistic Three Dimensional Simulations
• Temporal and Angular Variations of 3D Core-Collapse Supernova Emissions and their Physical Correlations
• Towards a Realistic Explosion Landscape for Binary Population Synthesis
• Revival of the Fittest: Exploding Core-Collapse Supernovae from 12 to 25 M${}_{\odot }$
• Three-Dimensional Core-Collapse Supernova Simulations with Multi-Dimensional Neutrino Transport Compared to the Ray-by-Ray-plus Approximation
• The Berkeley Sample of Stripped-Envelope Supernovae
• Sensitivity of the lower-edge of the pair instability black hole mass gap to the treatment of time dependent convection
• Massive donors in interacting binaries: effect of metallicity
• The Physics of the Neutrino Mechanism of Core-Collapse Supernovae
• Multi-D Simulations of Ultra-Stripped Supernovae to Shock Breakout
• The diverse lives of progenitors of hydrogen-rich core-collapse supernovae: the role of binary interaction
• A numerical model for multigroup radiation hydrodynamics
• The Birth Function for Black Holes and Neutron Stars in Close Binaries
• Predicting the Presence of Companions for Stripped-Envelope Supernovae: The Case of the Broad-Lined Type Ic SN 2002ap
• Supernova lightCURVE POPulation Synthesis I: including interacting binaries is key to understanding the diversity of type II supernova lightcurves
• Progenitors of Type IIb Supernovae: I. Evolutionary Pathways and Rates
• Gravitational Waves from Neutrino Asymmetries in Core-Collapse Supernovae
• Towards an Understanding of the Resolution Dependence of Core-Collapse Supernova Simulations
• Effects of winds on the leftover hydrogen in massive stars following Roche lobe overflow
• The presupernova core mass-radius relation of massive stars: understanding its formation and evolution
• Effect of binary evolution on the inferred initial and final core masses of hydrogen-rich, Type~II supernova progenitors
• Ultraviolet Detection of the Binary Companion to the Type IIb SN 2001ig
• Model Light Curves for Type Ib and Ic Supernovae
• Supernova 1987A: 3D Mixing and light curves for explosion models based on binary-merger progenitors
• Three-Dimensional Boltzmann-Hydro Code for core-collapse in massive stars III. A New method for momentum feedback from neutrino to matter
• Convective boundary mixing in a post-He core burning massive star model
• An Integral Condition for Core-Collapse Supernova Explosions
• The Antesonic Condition for the Explosion of Core-Collapse Supernovae I: Spherically Symmetric Polytropic Models: Stability & Wind Emergence
• Binaries at Low Metallicity: ranges for case A, B and C mass transfer

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