2015MNRAS.453.2982D


Query : 2015MNRAS.453.2982D

2015MNRAS.453.2982D - Mon. Not. R. Astron. Soc., 453, 2982-2991 (2015/November-1)

Self-organized criticality in a two-dimensional cellular automaton model of a magnetic flux tube with background flow.

DANILA B., HARKO T. and MOCANU G.

Abstract (from CDS):

We investigate the transition to self-organized criticality in a two-dimensional model of a flux tube with a background flow. The magnetic induction equation, represented by a partial differential equation with a stochastic source term, is discretized and implemented on a two-dimensional cellular automaton. The energy released by the automaton during one relaxation event is the magnetic energy. As a result of the simulations, we obtain the time evolution of the energy release, of the system control parameter, of the event lifetime distribution and of the event size distribution, respectively, and we establish that a self-organized critical state is indeed reached by the system. Moreover, energetic initial impulses in the magnetohydrodynamic flow can lead to one-dimensional signatures in the magnetic two-dimensional system, once the self-organized critical regime is established. The applications of the model for the study of gamma-ray bursts (GRBs) is briefly considered, and it is shown that some astrophysical parameters of the bursts, like the light curves, the maximum released energy and the number of peaks in the light curve can be reproduced and explained, at least on a qualitative level, by working in a framework in which the systems settles in a self-organized critical state via magnetic reconnection processes in the magnetized GRB fireball.

Abstract Copyright: © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2015)

Journal keyword(s): magnetic reconnection - MHD - gamma-ray burst: general

Simbad objects: 9

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Number of rows : 9
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 Fermi bn101126198 gB 05 39 -22.6           ~ 18 0
2 Fermi bn120119170 gB 08 00 06.940 -09 04 53.83           ~ 193 0
3 Fermi bn100919884 gB 10 53 +06.0           ~ 10 0
4 SN 2013dx SN* 14 29 14.77 +15 46 26.6           ~ 178 0
5 Fermi bn140919636 gB 14 46 08.96 -32 10 34.7           ~ 19 0
6 Fermi bn091209001 gB 17 24 +38.3           ~ 11 0
7 PSR J1808-2024 Psr 18 08 39.32 -20 24 40.1           ~ 1316 2
8 HD 226868 HXB 19 58 21.6757355952 +35 12 05.784512688 9.38 9.72 8.91 8.42   O9.7Iabpvar 4590 0
9 GRB 080805 gB 20 56 55.30 -62 25 58.8           ~ 102 0

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