Extra-galactic high-energy transients: event rate densities and luminosity functions
arXiv:1509.01592 · doi:10.1088/0004-637X/812/1/33
Abstract
Several types of extra-galactic high-energy transients have been discovered, which include high-luminosity and low-luminosity long-duration gamma-ray bursts (GRBs), short-duration GRBs, supernova shock breakouts (SBOs), and tidal disruption events (TDEs) without or with an associated relativistic jet. In this paper, we apply a unified method to systematically study the redshift-dependent event rate densities and the global luminosity functions (ignoring redshift evolution) of these transients. We introduce some empirical formulae for the redshift-dependent event rate densities for different types of transients, and derive the local specific event rate density, which also represents its global luminosity function. Long GRBs have a large enough sample to reveal features in the global luminosity function, which is best characterized as a triple power law. All the other transients are consistent with having a single power law luminosity function. The total event rate density depends on the minimum luminosity, and we obtain the following values in units of : for high-luminosity long GRBs above , for low-luminosity long GRBs above , , , and above for short GRBs with three different merger delay models (Gaussian, log-normal, and power law), above for SBOs, for normal TDEs above , and above for TDE jets as discovered by Swift. Intriguingly, the global luminosity functions of different kinds of transients, which cover over 12 orders of magnitude, are consistent with a single power law with an index of -1.6.
35 pages, 12 figures, accepted to ApJ
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