Ideal Engine Durations For Gamma-Ray-Burst-Jet Launch
arXiv:1707.01056 · doi:10.1093/mnras/stx987
Abstract
Aiming to study GRB engine duration, we present numerical simulations to investigate collapsar jets. We consider typical explosion energy ( erg) but different engine durations, in the widest domain to date from 0.1 to 100 s. We employ an AMR 2D hydrodynamical code. Our results show that engine duration strongly influences jet nature. We show that the efficiency of launching and collimating relativistic outflow increases with engine duration, until the intermediate engine range where it is the highest, past this point to long engine range, the trend is slightly reversed; we call this point where acceleration and collimation are the highest "sweet spot" (10 -- 30 s). Moreover, jet energy flux shows that variability is also high in this duration domain. We argue that not all engine durations can produce the collimated, relativistic and variable long GRB-jets. Considering a typical progenitor and engine energy, we conclude that the ideal engine duration to reproduce a long GRB is 10 -- 30 s, where the launch of relativistic, collimated and variable jets is favored. We note that this duration domain makes a good link with Lazzati et al. (2013), which suggested that the bulk of BATSE's long GRBs is powered by 10 -- 20 s collapsar engines.
19 pages, 16 figures, 3 tables. Accepted for publication in MNRAS
References in corpus (18)
- An optical supernova associated with the X-ray flash XRF 060218
- The Galaxy Population Hosting Gamma-Ray Bursts
- GRB Radiative Efficiencies Derived from the Swift Data: GRBs vs. XRFs, Long vs. Short
- On the Rates of Gamma Ray Bursts and Type Ib/c Supernovae
- Relativistic MHD simulations of core-collapse GRB jets: 3D instabilities and magnetic dissipation
- Mass Fall-back and Accretion in the Central Engine of Gamma-Ray Bursts
- How much 56Ni can be produced in Core-Collapse Supernovae? : Evolution and Explosions of 30 - 100 Msun Stars
- Very high efficiency photospheric emission in long duration gamma-ray bursts
- SN 2006aj and the nature of low-luminosity gamma-ray bursts
- Aspherical Properties of Hydrodynamics and Nucleosynthesis in Jet-induced Supernovae
- Angular Energy Distribution of Collapsar-Jets
- Collimated Jet or Expanding Outflow: Possible Origins of GRBs and X-Ray Flashes
- Thermal Radiation from GRB Jets
- A Narrow Short-Duration GRB Jet from a Wide Central Engine
- Long-Term Evolution of Slowly Rotating Collapsar in Special Relativistic Magnetohydrodynamics
- Photospheric emission from long duration gamma-ray bursts powered by variable engines
- Models for Gamma-Ray Bursts and Diverse Transients
- Gamma-Ray Burst jet dynamics and their interaction with the progenitor star
Cited by in corpus (10)
- Jet Propagation in Expanding Medium for Gamma-Ray Bursts
- Jet Propagation in Neutron Star Mergers and GW170817
- The Optical/NIR afterglow of GRB 111209A: Complex yet not Unprecedented
- Gamma-ray burst afterglow blast waves
- Cocoon breakout and escape from the ejecta of neutron star mergers
- Cocoon cooling emission in neutron star mergers
- The large landscape of supernova, GRB and cocoon interactions
- A Monte Carlo Radiation Transfer Study of Photospheric Emission in Gamma Ray Bursts
- Three-dimensional numerical simulations of structured GRB jets
- Chemical stratification in a long gamma-ray burst cocoon and early-time spectral signatures of supernovae associated with gamma-ray bursts