Population III Gamma-Ray Bursts and Breakout Criteria for Accretion-Powered Jets

Abstract

We investigate the propagation of accretion-powered jets in various types of massive stars such as Wolf-Rayet stars, light Population III (Pop III) stars, and massive Pop III stars, all of which are the progenitor candidates of Gamma-Ray Bursts (GRBs). We perform two dimensional axisymmetric simulations of relativistic hydrodynamics taking into account both the envelope collapse and the jet propagation (i.e., the negative feedback of the jet on the accretion). Based on our hydrodynamic simulations, we show for the first time that the accretion-powered jet can potentially break out relativistically from the outer layers of Pop III progenitors. In our simulations, the accretion rate is estimated by the mass flux going through the inner boundary, and the jet is injected with a fixed accretion-to-jet conversion efficiency $\eta$. By varying the efficiency $\eta$ and opening angle ${\theta }_{op}$ for more than 40 models, we find that the jet can make a relativistic breakout from all types of progenitors for GRBs if a simple condition $\eta \gtrsim 10^{-4}({\theta }_{op}/8^{\circ }{)}^2$ is satisfied, which is consistent with analytical estimates. Otherwise no explosion or some failed spherical explosions occur.

50 pages, 20 figures, accepted to ApJ

References in corpus (21)

• Shapiro delay measurement of a two solar mass neutron star
• The Proto-Magnetar Model for Gamma-Ray Bursts
• Protostellar Feedback Halts the Growth of the First Stars in the Universe
• Measured Metallicities at the Sites of Nearby Broad-Lined Type Ic Supernovae and Implications for the SN-GRB Connection
• The Formation of the First Stars II. Radiative Feedback Processes and Implications for the Initial Mass Function
• Mass Fall-back and Accretion in the Central Engine of Gamma-Ray Bursts
• Very high efficiency photospheric emission in long duration gamma-ray bursts
• Rotation Speed of the First Stars
• The Connection between Gamma-Ray Bursts and Extremely Metal-Poor Stars: Black Hole-forming Supernovae with Relativistic Jets
• Population III.1 and III.2 gamma-Ray Bursts: Constraints on the event rate for future radio and X-ray surveys
• Jet propagations, breakouts and photospheric emissions in collapsing massive progenitors of long duration gamma ray bursts
• Angular Energy Distribution of Collapsar-Jets
• Can Gamma-Ray Burst Jets Break Out the First Stars?
• Population III GRB Afterglows: Constraints on Stellar Masses and External Medium Densities
• Formation of black hole and accretion disk in a massive high-entropy stellar core collapse
• Collimated Jet or Expanding Outflow: Possible Origins of GRBs and X-Ray Flashes
• Thermal Radiation from GRB Jets
• General Relativistic Hydrodynamic Simulations and Linear Analysis of the Standing Accretion Shock Instability around a Black Hole
• Low angular momentum accretion in the collapsar: how long can a long GRB be?
• Impact of Rotation on Neutrino Emission and Relic Neutrino Background from Population III Stars
• Gamma-Ray Burst without Baryonic and Magnetic Load?

Cited by in corpus (37)

• The Physics of Gamma-Ray Bursts and Relativistic Jets
• Formation of the First Stars
• Jet collimation in the ejecta of double neutron star merger: new canonical picture of short gamma-ray bursts
• Titans of the Early Universe: The Prato Statement on the Origin of the First Supermassive Black Holes
• Opening Angles of Collapsar Jets
• Relativistic supernovae have shorter-lived central engines or more extended progenitors: the case of SN\,2012ap
• Finding the First Cosmic Explosions I: Pair-Instability Supernovae
• Blue Supergiant Model for Ultra-Long Gamma-Ray Burst with Superluminous-Supernova-Like Bump
• On the Cosmological Evolution of Long Gamma-ray Burst Properties
• Finding the First Cosmic Explosions II: Core-Collapse Supernovae
• Supermassive Population III Supernovae and the Birth of the First Quasars
• Probing the stellar initial mass function with high-$z$ supernovae
• Ultra Long Gamma-Ray Bursts from the collapse of Blue Super Giant stars: an end-to-end simulation
• Luminous supernova-like UV/optical/infrared transients associated with ultra-long gamma-ray bursts from metal-poor blue supergiants
• Long Duration X-Ray Flash and X-Ray Rich Gamma Ray Burst from Low Mass Population III Star
• Can direct collapse black holes launch gamma-ray bursts and grow to supermassive black holes?
• Illuminating the Primeval Universe with Type IIn Supernovae
• Are Ultra-Long Gamma-Ray Bursts Caused by Blue Supergiant Collapsars, Newborn Magnetars, or White Dwarf Tidal Disruption Events?
• The First Gamma-Ray Bursts in the Universe
• SN 2016coi (ASASSN-16fp): an energetic H-stripped core-collapse supernova from a massive stellar progenitor with large mass loss
• Population III Hypernovae
• Numerical models of blackbody-dominated gamma-ray bursts -- II. Emission properties
• Gamma-ray bursts and Population III stars
• Jet-powered supernovae of $\sim 10^5{M}_{\odot }$ population III stars are observable by $Euclid$, $WFIRST$, $WISH$, and $JWST$
• Numerical models of blackbody-dominated gamma-ray bursts -- I. Hydrodynamics and the origin of the thermal emission
• The Potential for Detecting Gamma-Ray Burst Afterglows from Population III Stars with the Next Generation of Infrared Telescopes
• Can we quickly flag Ultra-long Gamma-Ray Bursts?
• Can very massive Population III stars produce a super-collapsar?
• The First Billion Years project: gamma-ray bursts at z>5
• Searching for the first stars with the Gaia mission
• A Study of Primordial Very Massive Star Evolution. II. Stellar Rotation and Gamma-Ray Burst Progenitors
• Black hole hyperaccretion in collapsars. III. GRB timescale
• The propagation of neutrino-driven jets in Wolf-Rayet stars
• On the Anti-Correlation between Duration and Redshift in Gamma-ray Bursts
• Hard X-ray Spectral Investigations of Gamma-ray Bursts, 120521C and 130606A, at High-redshift z~6
• Evolution of jets driven by relativistic radiation hydrodynamics as Long and Low Luminosity GRBs
• A new era of sub-millimeter GRB afterglow follow-ups with the Greenland Telescope