Black hole hyperaccretion inflow-outflow model. II. Long-duration gamma-ray bursts and supernova ${}^{56}\mathrm{Ni}$ bumps

Abstract

Long-duration gamma-ray bursts (LGRBs) associated with supernovae (SNe) are possibly born out of the death of a massive star. After the star collapses, a stellar-mass black hole (BH) is formed, surrounded by a hyperaccretion disk with outflows. Blandford-Znajek jets can be launched and then break out from the envelope to power LGRBs. The jet luminosity depends on the net inflow accretion rate at the inner radius of the disk. Furthermore, ${}^{56}\mathrm{Ni}$ synthesis should occur in the strong outflows from the accretion disk. The decay of ${}^{56}\mathrm{Ni}$ is considered to be the possible origin of SN bumps in the subsequent optical afterglows of LGRBs. If ${}^{56}\mathrm{Ni}$ originates entirely from the outflows, there is competition between the luminosities of LGRBs and those of the corresponding ${}^{56}\mathrm{Ni}$ bumps because of the material distribution between the disk inflows and outflows. In this paper, we investigated these two luminosities based on 15 cases of LGRB-SN in the framework of the BH hyperaccretion inflow-outflow model. Then, one can constrain the characteristics of the progenitor stars of these LGRBs. The results indicate that these LGRBs may originate from the low-metallicity ($Z\lesssim 10^{-2}{Z}_{\odot }$, where $Z$ and $Z_{\odot }$ are the metallicities of the stars and the Sun, respectively) stars or some massive solar-metallicity stars. For ultra-LGRBs (ULGRBs), such as GRB 111209A, most of the massive low-metallicity stars with $Z\lesssim 10^{-2}{Z}_{\odot }$ could be progenitors only if very strong outflows are launched from the disks. When the contributions of nucleosynthesis in the disk outflows are considered, there is no shortage of ${}^{56}\mathrm{Ni}$ mass for luminous SNe associated with ULGRBs.

arXiv comment9 pages, 1 table, 2 figures, accepted for publication in ApJ

References in corpus (79)

• Collapsars - Gamma-Ray Bursts and Explosions in "Failed Supernovae"
• How Massive Single Stars End their Life
• Binary interaction dominates the evolution of massive stars
• Discovery of the peculiar supernova 1998bw in the error box of GRB980425
• The Supernova -- Gamma-Ray Burst Connection
• Hot Accretion Flows Around Black Holes
• A very energetic supernova associated with the gamma-ray burst of 29 March 2003
• Gamma-Ray Bursts as the Death Throes of Massive Binary Stars
• Spectroscopic Discovery of the Supernova 2003dh Associated with GRB 030329
• Beaming in Gamma-Ray Bursts: Evidence for a Standard Energy Reservoir
• Hyper-Accreting Black Holes and Gamma-Ray Bursts
• The Proto-Magnetar Model for Gamma-Ray Bursts
• Observed Fractions of Core-Collapse Supernova Types and Initial Masses of their Single and Binary Progenitor Stars
• GRB Energetics and the GRB Hubble Diagram: Promises and Limitations
• Asymmetric Supernovae, Pulsars, Magnetars, and Gamma-Ray Bursts
• Neutrino trapping and accretion models for Gamma-Ray Bursts
• The death of massive stars - II. Observational constraints on the progenitors of type Ibc supernovae
• A very luminous magnetar-powered supernova associated with an ultra-long gamma-ray burst
• The Observer's Guide to the Gamma-Ray Burst-Supernova Connection
• A new population of ultra-long duration gamma-ray bursts
• GRB Radiative Efficiencies Derived from the Swift Data: GRBs vs. XRFs, Long vs. Short
• Numerical Simulation of Hot Accretion Flows (II): Nature, Origin, and Properties of Outflow and Their Possible Observational Applications
• Total and Jet Blandford-Znajek Power in Presence of Accretion Disk
• The Blandford-Znajek Process as a Centeral Engine for a Gamma Ray Burst
• The Broad-lined Type Ic SN 2003jd
• A Universal Scaling for the Energetics of Relativistic Jets From Black Hole Systems
• Photometry and Spectroscopy of GRB 030329 and Its Associated Supernova 2003dh: The First Two Months
• Common Envelope Evolution Leading to Supernovae with Dense Interaction
• Supernova Hosts for Gamma-Ray Burst Jets: Dynamical Constraints
• The Afterglow of GRB 130427A from 1 to 10^16 GHz
• Neutrino-Dominated Accretion and Supernovae
• r-Process Nucleosynthesis in Hot Accretion Disk Flows from Black Hole - Neutron Star Mergers
• Production of the entire range of r-process nuclides by black hole accretion disc outflows from neutron star mergers
• Nucleosynthesis in the Outflow from Gamma Ray Burst Accretion Disks
• Magnetized Relativistic Jets and Long-Duration GRBs from Magnetar Spindown during Core-Collapse Supernovae
• A new method for estimating the bolometric properties of Ibc SNe
• Powerful radiative jets in super-critical accretion disks around non-spinning black holes
• Hyper-accreting black hole as GRB central engine. I: Baryon loading in GRB jets
• Long Gamma-Ray Transients from Collapsars
• Neutrino-dominated accretion flows as the central engine of gamma-ray bursts
• Relativistic Jets and Long-Duration Gamma-ray Bursts from the Birth of Magnetars
• Structure and Luminosity of Neutrino-cooled Accretion Disks
• Activation of the Blandford-Znajek mechanism in collapsing stars
• Effects of Fall-Back Accretion on Proto-Magnetar Outflows in Gamma-Ray Bursts and Superluminous Supernovae
• How Long does a Burst Burst?
• Gamma Ray Bursts Are Observed Off-Axis
• Stellar explosions powered by the Blandford-Znajek mechanism
• Can Gamma-Ray Burst Jets Break Out the First Stars?
• Physical Properties and Evolutionary States of EA-type Eclipsing Binaries Observed by LAMOST
• The Merger of a Helium Star and a Black Hole: Gamma-Ray Bursts
• Blue Supergiant Model for Ultra-Long Gamma-Ray Burst with Superluminous-Supernova-Like Bump
• Nucleosynthesis in Outflows from the Inner Regions of Collapsars
• A statistical study of super-luminous supernovae in the magnetar engine model and implications for their connection with gamma-ray bursts and hypernovae
• Hyperaccreting Black Hole as Gamma-Ray Burst Central Engine. II. Temporal evolution of central engine parameters during Prompt and Afterglow Phases
• The "amplitude" parameter of Gamma-Ray Bursts and its implications for GRB classification
• Jet Luminosity of Gamma-ray Bursts: Blandford-Znajek Mechanism v.s. Neutrino Annihilation Process
• Discovery and redshift of an optical afterglow in 71 square degrees: iPTF13bxl and GRB 130702A
• Close Binary Progenitors of Long Gamma Ray Bursts
• Explosive Common-Envelope Ejection: Implications for Gamma-Ray Bursts and Low-Mass Black-Hole Binaries
• GRB 011121: A collimated outflow into wind-blown surroundings
• GRB 081007 and GRB 090424: the surrounding medium, outflows and supernovae
• Optical and near-infrared observations of SN 2013dx associated with GRB 130702A
• Black hole hyperaccretion inflow-outflow model. I. long and ultra-long gamma-ray bursts
• Issues in the Blandford-Znajek Process for GRB Inner Engine
• Ultra Long Gamma-Ray Bursts from the collapse of Blue Super Giant stars: an end-to-end simulation
• Evidence for jet launching close to the black hole in GRB 101219B - a Fermi GRB dominated by thermal emission
• Neutrino Interactions in the Outflow from Gamma-Ray Burst Accretion Disks
• A self-consistent analytical magnetar model: The luminosity of $\gamma$-ray burst supernovae is powered by radioactivity
• How Much Can ${}^{56}$Ni Be Synthesized by Magnetar Model for Long Gamma-ray Bursts and Hypernovae?
• Short Gamma-ray Bursts: the mass of the accretion disk and the initial radius of the outflow
• GRB 120422A: A Low-luminosity Gamma-ray Burst Driven by Central Engine
• GRB 140606B / iPTF14bfu: Detection of shock-breakout emission from a cosmological gamma-ray burst?
• Nucleosynthesis of Nickel-56 from Gamma-Ray Burst Accretion Disks
• Neutrino-cooled Accretion Model with Magnetic Coupling for X-ray Flares in GRBs
• The central engine of GRB 130831A and the energy breakdown of a relativistic explosion
• Self-gravity in neutrino-dominated accretion disks
• GRB 021211 as a Faint Analogue of GRB 990123: Exploring the Similarities and Differences in their Optical Afterglows
• The vertical composition of neutrino-dominated accretion disks in gamma-ray bursts
• Evolutions of stellar-mass black hole hyperaccretion systems in the center of gamma-ray bursts

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