Relation between the intrinsic and observed central engine activity time: implications for ultra-long GRBs

Abstract

The GRB central engine intrinsic activity time $T_{\mathrm{ce}}$ is usually described through either the $\gamma$-ray duration $T_{90}$ or through a generalized burst duration $t_{\mathrm{burst}}$ which includes both the $\gamma$-ray emission and (when present) an extended flaring X-ray plateau. Here, we define a more specific operational description of $T_{\mathrm{ce}}$, and within the framework of the internal-external shock model, we develop a numerical code to study the relationship between $T_{90}$ and $T_{\mathrm{ce}}$, as well as between $t_{\mathrm{burst}}$ and $T_{\mathrm{ce}}$, for different initial conditions. We find that when $T_{\mathrm{ce}}\lesssim 10^4$ s, late internal collisions or refreshed external collisions result in values of $T_{90}$ and $t_{\mathrm{burst}}$ larger than $T_{\mathrm{ce}}$, usually by factors of $2-3$. For $T_{\mathrm{ce}}\gtrsim 10^4$ s, the $t_{\mathrm{burst}}$ is always a good estimator for $T_{\mathrm{ce}}$, while $T_{90}$ can underpredict $T_{\mathrm{ce}}$ when the late central engine activity is moderate. We find a clear bimodal distribution for $T_{\mathrm{ce}}$, based on our simulations as well as on the observational data for $T_{90}$ and $t_{\mathrm{burst}}$. We suggest that $t_{\mathrm{burst}}$ is a reliable measure for defining "ultra-long" GRBs. Bursts with $T_{90}$ of order $10^3$ s need not belong to a special population, while bursts with $t_{\mathrm{burst}}>10^4$ s, where the late central engine activity is more moderate and shows up in X-rays, may represent a new population. These conclusions are insensitive to the initial conditions assumed in the models.

Accepted by ApJ

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Cited by in corpus (1)

• Relativistic MHD simulations of collision-induced magnetic dissipation in Poynting-flux-dominated jets/outflows