Extra-galactic high-energy transients: event rate densities and luminosity functions

TL;DR

This paper systematically studies the event rate densities and luminosity functions of various extra-galactic high-energy transients, revealing unified properties and detailed rate estimates across different transient types and luminosity ranges.

Contribution

It introduces empirical formulas for redshift-dependent event rates and derives the global luminosity functions, highlighting a common power-law behavior across diverse transients.

Findings

Long GRBs have a triple power law luminosity function.

Other transients are consistent with a single power law luminosity function.

The total event rate densities vary significantly among transient types.

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 ${\rm Gpc^{-3}~yr^{-1}}$: $0.8^{+0.1}_{-0.1}$ for high-luminosity long GRBs above $ 10^{50}~{\rm erg~s^{-1}}$, $164^{+98}_{-65}$ for low-luminosity long GRBs above $5\times 10^{46}~{\rm erg~s^{-1}}$, $1.3^{+0.4}_{-0.3}$, $1.2^{+0.4}_{-0.3}$, and $3.3^{+1.0}_{-0.8}$ above $ 10^{50}~ {\rm erg~s^{-1}}$ for short GRBs with three different merger delay models (Gaussian, log-normal, and power law), $1.9^{+2.4}_{-1.2}\times 10^4$ above $ 10^{44}~{\rm erg~s^{-1}}$ for SBOs, $ 4.8^{+3.2}_{-2.1}\times10^2 $ for normal TDEs above $10^{44}~ {\rm erg~s^{-1}}$, and $0.03^{+0.04}_{-0.02}$ above $ 10^{48}~ {\rm erg~s^{-1}}$ 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.