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PUSHing Core-collapse Supernovae to Explosions in Spherical Symmetry. II. Explodability and Remnant Properties

Journal Article · · The Astrophysical Journal (Online)
 [1];  [2];  [2];  [3];  [4];  [3];  [5]
  1. GSI-Darmstadt (Germany); North Carolina State Univ., Raleigh, NC (United States); DOE/OSTI
  2. North Carolina State Univ., Raleigh, NC (United States)
  3. Univ. of Basel (Switzerland)
  4. Univ. of Parma (Italy); Univ. degli Studi di Milano (Italy)
  5. GSI-Darmstadt (Germany); Univ. of Basel (Switzerland)
+ Show Author Affiliations
In a previously presented proof-of-principle study, we established a parameterized spherically symmetric explosion method (PUSH) that can reproduce many features of core-collapse supernovae. The present paper goes beyond a specific application that is able to reproduce observational properties of SN 1987A and performs a systematic study of an extensive set of nonrotating, solar metallicity stellar progenitor models in the mass range from 10.8 to 120 M ⊙. This includes the transition from neutron stars to black holes as the final result of the collapse of massive stars, and the relation of the latter to supernovae, possibly faint supernovae, and failed supernovae. We discuss the explosion properties of all models and predict remnant mass distributions within this approach. The present paper provides the basis for extended nucleosynthesis predictions in a forthcoming paper to be employed in galactic evolution models.
Research Organization:
North Carolina State Univ., Raleigh, NC (United States)
Sponsoring Organization:
USDOE Office of Science (SC)
Grant/Contract Number:
SC0010263
OSTI ID:
1611370
Journal Information:
The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 1 Vol. 870; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English

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A critical assessment of turbulence models for 1D core-collapse supernova simulations journal June 2019
Enrichment of the Galactic disc with neutron capture elements: Sr journal February 2019
Early Chemical Evolution of Zn Driven by Magnetorotational Supernovae and the Pathway to the Solar Zn Composition journal August 2018
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Pristine IX: CFHT ESPaDOnS Spectroscopic Analysis of 115 Bright Metal-Poor Candidate Stars text January 2019
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Grids of stellar models with rotation: IV. Models from 1.7 to 120 journal June 2019
Missing red supergiants and carbon burning journal January 2020
Using failed supernovae to constrain the Galactic r-process element production journal May 2019
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One-, Two-, and Three-dimensional Simulations of Oxygen-shell Burning Just before the Core Collapse of Massive Stars journal August 2019
The Initial Mass–Final Luminosity Relation of Type II Supernova Progenitors: Hints of New Physics? journal August 2019
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Impact of the Rotation and Compactness of Progenitors on the Mass of Black Holes journal January 2020
PUSHing Core-collapse Supernovae to Explosions in Spherical Symmetry. IV. Explodability, Remnant Properties, and Nucleosynthesis Yields of Low-metallicity Stars journal January 2020
Is GW190425 Consistent with Being a Neutron Star–Black Hole Merger? journal February 2020
A Critical Assessment of Turbulence Models for 1D Core-Collapse Supernova Simulations text January 2019
One-, Two-, and Three-dimensional Simulations of Oxygen Shell Burning Just Before the Core-Collapse of Massive Stars text January 2019
New constraint from supernova explosions on light particles beyond the Standard Model text January 2019
Grids of stellar models with rotation IV. Models from 1.7 to 120 Msun at a metallicity Z = 0.0004 text January 2019
Galactic r-process abundance feature shaped by radial migration text January 2019
The initial mass-final luminosity relation of type II supernova progenitors. Hints of new physics? text January 2019

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