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Title: Relativistic MHD simulations of collision-induced magnetic dissipation in poynting-flux-dominated jets/outflows

Journal Article · · The Astrophysical Journal (Online)
ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [3];  [2]
  1. Univ. of Nevada, Las Vegas, NV (United States); Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
  2. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
  3. Univ. of Nevada, Las Vegas, NV (United States)

We perform 3D relativistic ideal MHD simulations to study the collisions between high-σ (Poynting- ux-dominated) blobs which contain both poloidal and toroidal magnetic field components. This is meant to mimic the interactions inside a highly variable Poynting- ux-dominated jet. We discover a significant electromagnetic field (EMF) energy dissipation with an Alfvenic rate with the efficiency around 35%. Detailed analyses show that this dissipation is mostly facilitated by the collision-induced magnetic reconnection. Additional resolution and parameter studies show a robust result that the relative EMF energy dissipation efficiency is nearly independent of the numerical resolution or most physical parameters in the relevant parameter range. The reconnection outflows in our simulation can potentially form the multi-orientation relativistic mini-jets as needed for several analytical models. We also find a linear relationship between the σ values before and after the major EMF energy dissipation process. In conclusion, our results give support to the proposed astrophysical models that invoke signi cant magnetic energy dissipation in Poynting- ux-dominated jets, such as the internal collision-induced magnetic reconnection and turbulence (ICMART) model for GRBs, and reconnection triggered mini-jets model for AGNs.

Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE Office of Science (SC), Fusion Energy Sciences (FES)
Grant/Contract Number:
AC52-06NA25396; NNX15AK85G; NNX14AF85G
OSTI ID:
1254837
Report Number(s):
LA-UR-15-20564
Journal Information:
The Astrophysical Journal (Online), Vol. 805, Issue 2; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 38 works
Citation information provided by
Web of Science

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Relativistic MHD simulations of core-collapse GRB jets: 3D instabilities and magnetic dissipation journal December 2015
A long-lived neutron star merger remnant in GW170817: constraints and clues from X-ray observations journal November 2018
An HLLC Riemann solver for resistive relativistic magnetohydrodynamics journal February 2018
Internal shocks in microquasar jets with a continuous Lorentz factor modulation journal March 2018
Synchrotron Origin of the Typical grb band Function—A case Study of grb 130606b journal January 2016
Toward an Understanding of grb Prompt Emission Mechanism. i. the Origin of Spectral lags journal July 2016
External Shock in a Multi-bursting Gamma-Ray Burst: Energy Injection Phase Induced by the Later Launched Ejecta journal January 2018
On the Synchrotron Spectrum of GRB Prompt Emission journal January 2018
Gamma-Ray Burst Jet Breaks Revisited journal June 2018
Gamma-Ray Burst Optical Afterglows with Two-component Jets: Polarization Evolution Revisited journal June 2018
A Comprehensive Analysis of Fermi Gamma-Ray Burst Data. IV. Spectral Lag and its Relation to E p Evolution journal October 2018
Toward an Understanding of GRB Prompt Emission Mechanism. II. Patterns of Peak Energy Evolution and Their Connection to Spectral Lags journal December 2018
On the Broadband Synchrotron Spectra of Pulsar Wind Nebulae journal February 2019
Gamma-Ray Bursts Induced by Turbulent Reconnection journal September 2019
“Double-tracking” Characteristics of the Spectral Evolution of GRB 131231A: Synchrotron Origin? journal October 2019
Thermal Components in Gamma-Ray Bursts. I. How Do They Affect Nonthermal Spectral Parameters? journal November 2019
Adiabatic Non-resonant Acceleration in Magnetic Turbulence and Hard Spectra of Gamma-Ray Bursts journal September 2017
Synchrotron Origin of the Typical GRB Band Function - A Case Study of GRB 130606B text January 2015
Relativistic MHD simulations of core-collapse GRB jets: 3D instabilities and magnetic dissipation text January 2015
Towards an understanding of GRB prompt emission mechanism: I. The origin of spectral lags text January 2015
Particle Acceleration during Magnetic Reconnection in a Low-beta Pair Plasma text January 2016
Adiabatic non-resonant acceleration in magnetic turbulence and hard spectra of gamma-ray bursts text January 2017
On the synchrotron spectrum of GRB prompt emission text January 2017
External Shock in a Multi-Bursting Gamma-ray Burst: Energy Injection Phase induced by the Later Launched Ejecta text January 2017
Toward an understanding of GRB prompt emission mechanism: II. Patterns of peak energy evolution and their connection to spectral lags text January 2018
On the broad-band synchrotron spectra of pulsar wind nebulae text January 2018
Thermal Components in Gamma-ray Bursts. I. How Do They Affect Non-Thermal Spectral Parameters? text January 2019
3D Turbulent Reconnection: Theory, Tests and Astrophysical Implications text January 2020