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Title: A MAD Model for Gamma-Ray Burst Variability

Journal Article · · Monthly Notices of the Royal Astronomical Society

Here we present a model for the temporal variability of long gamma-ray bursts during the prompt phase (the highly variable first 100 seconds or so), in the context of a magnet- ically arrested disk (MAD) around a black hole. In this state, sufficient magnetic flux is held on to the black hole such that it stalls the accretion near the inner region of the disk. The system transitions in and out of the MAD state, which we relate to the vari- able luminosity of the GRB during the prompt phase, with a characteristic timescale defined by the free fall time in the region over which the accretion is arrested. We present simple analytic estimates of the relevant energetics and timescales, and com- pare them to gamma-ray burst observations. In particular, we show how this model can reproduce the characteristic one second time scale that emerges from various analyses of the prompt emission light curve. Finally, we also discuss how our model can accommodate the potentially physically important correlation between a burst quiescent time and the duration of its subsequent pulse (Ramirez-Ruiz & Merloni 2001).

Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE National Nuclear Security Administration (NNSA)
Grant/Contract Number:
AC52-06NA25396
OSTI ID:
1338734
Report Number(s):
LA-UR-15-29635
Journal Information:
Monthly Notices of the Royal Astronomical Society, Vol. 461, Issue 1; ISSN 0035-8711
Publisher:
Royal Astronomical SocietyCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 12 works
Citation information provided by
Web of Science

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Cited By (9)

An MAD explanation for the correlation between bulk Lorentz factor and minimum variability time-scale journal April 2018
Constraints on gamma-ray burst inner engines in a Blandford–Znajek framework journal February 2019
Accretion into Black Hole, and Formation of Magnetically Arrested Accretion Disks journal June 2019
Constraining the Environmental Properties of FRB 131104 Using the Unified Dynamical Afterglow Model journal July 2018
Time-reversed Gamma-Ray Burst Light-curve Characteristics as Transitions between Subluminal and Superluminal Motion journal September 2019
Viscous Evolution of Magnetized Clumps: A Source for X-Ray Flares in Gamma-Ray Bursts journal January 2020
CDF-S XT1 and XT2: White Dwarf Tidal Disruption Events by Intermediate-mass Black Holes? journal October 2019
CDF-S XT1 and XT2: White Dwarf Tidal Disruption Events by Intermediate-Mass Black Holes? text January 2019
Accretion into black hole, and formation of magnetically arrested accretion disks preprint January 2019

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