Pre-collapse Properties of Superluminous Supernovae and Long Gamma-Ray Burst Progenitor Models

Abstract

We analyze the properties of 42 rapidly rotating, low metallicity, quasi-chemically homogeneously evolving stellar models in the mass range between 4 and 45 ${\mathrm{M}}_{\odot }$ at the time of core collapse. Such models were proposed as progenitors for both superluminous supernovae (SLSNe) and long duration gamma-ray bursts (lGRBs), and the Type Ic-BL supernovae (SNe) that are associated with them. Our findings suggest that whether these models produce a magnetar driven SLSN explosion or a near-critically rotating black hole (BH) is not a monotonic function of the initial mass. Rather, their explodability varies non-monotonically depending on the late core evolution, once chemical homogeneity is broken. Using different explodability criteria we find that our models have a clear preference to produce SLSNe at lower masses, and lGRBs at higher masses; but find several exceptions, expecting lGRBs to form from stars as low as 10 ${\mathrm{M}}_{\odot }$, and SLSNe with progenitors as massive as 30 ${\mathrm{M}}_{\odot }$. In general, our models reproduce the predicted angular momenta, ejecta masses and magnetic field strengths at core collapse inferred for SLSNe and lGRBs, and suggest significant interaction with their circumstellar medium, particularly for explosions with low ejecta mass.

Accepted for publication in ApJ. 17 pages, 11 figures, 2 tables

References in corpus (17)

• The NumPy array: a structure for efficient numerical computation
• Modules for Experiments in Stellar Astrophysics (MESA)
• Pulsational Pair-Instability Supernovae
• Observational constraints on the progenitors of core-collapse supernovae : the case for missing high mass stars
• Mind the gap: The location of the lower edge of the pair instability supernovae black hole mass gap
• The magnetar model for Type I superluminous supernovae I: Bayesian analysis of the full multicolour light curve sample with MOSFiT
• Rotational mixing in massive binaries: detached short-period systems
• Binary star progenitors of long gamma-ray bursts
• Spectroscopy of superluminous supernova host galaxies. A preference of hydrogen-poor events for extreme emission line galaxies
• Rotation-supported Neutrino-driven Supernova Explosions in Three Dimensions and the Critical Luminosity Condition
• Gamma-Ray Bursts from tidally spun-up Wolf-Rayet stars?
• Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity
• Are LGRBs biased tracers of star formation? Clues from the host galaxies of the $Swift$/BAT6 complete sample of bright LGRBs III: Stellar masses, star formation rates and metallicities at $z>1$
• Numerical simulations of the magnetorotational instability in protoneutron stars: I. Influence of buoyancy
• The circumstellar medium around a rapidly rotating, chemically homogeneously evolving, possible gamma-ray burst progenitor
• Magnetohydrodynamic Turbulence Powered by Magnetorotational Instability in Nascent Proto-Neutron Stars
• Taking stock of SLSN and LGRB host galaxy comparison using a complete sample of LGRBs

Cited by in corpus (32)

• Different to the core: the pre-supernova structures of massive single and binary-stripped stars
• The spins of compact objects born from helium stars in binary systems
• Magnetorotational core collapse of possible GRB progenitors. IV. A wider range of progenitors
• Superluminous supernovae: an explosive decade
• Three dimensional magnetorotational core-collapse supernova explosions of a 39 solar mass progenitor star
• The chemical signature of jet-driven hypernovae
• A synthetic population of Wolf-Rayet stars in the LMC based on detailed single and binary star evolution models
• Stripped-envelope stars in different metallicity environments. II. Type I supernovae and compact remnants
• 3D Simulations of Strongly Magnetised Non-Rotating Supernovae: Explosion Dynamics and Remnant Properties
• 3D Simulations of Oxygen Shell Burning with and without Magnetic Fields
• A three-dimensional hydrodynamics simulation of oxygen-shell burning in the final evolution of a fast-rotating massive star
• Stripped-Envelope Stars in Different Metallicity Environments I. Evolutionary Phases, Classification and Populations
• The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities
• Evaluating chemically homogeneous evolution in stellar binaries: Electromagnetic implications -- Ionizing photons, SLSN-I, GRB, Ic-BL
• The effects of surface fossil magnetic fields on massive star evolution: III. The case of $\tau$ Sco
• Modeling overcontact binaries, I. The effect of tidal deformation
• Modeling contact binaries, II. The effect of energy transfer
• Long-duration Gamma-ray Burst Progenitors and Magnetar Formation
• Density Profiles of Collapsed Rotating Massive Stars Favor Long Gamma-Ray Bursts
• Modeling contact binaries, III. Properties of a population of close, massive binaries
• Neutrino-driven massive stellar explosions in 3D fostered by magnetic fields via turbulent $\alpha$-effect
• The effects of rotation, metallicity and magnetic field on the islands of failed supernovae
• A model of anisotropic winds from rotating stars for evolutionary calculations
• Progenitors of Long-Duration Gamma-ray Bursts
• Metal-enriched Pair-instability supernovae: Effects of rotation
• Variety of disk wind-driven explosions in massive rotating stars
• Are binary black hole mergers and long gamma-ray bursts drawn from the same black hole population?
• The drastic impact of Eddington-limit induced mass ejections on massive star populations
• The magnetic, spectroscopic, and photometric variability of the Wolf-Rayet star WR55
• Detailed evolutionary models of massive contact binaries: I. Model grids and synthetic populations for the Magellanic Clouds
• The influence of rotation and metallicity on the explodability of massive stars
• A Black Hole is Born: 3D GRMHD Simulation of Black Hole Formation from Core-Collapse