Exploring the central engines of gamma-ray bursts from prompt light curves

Le résumé fourni par la source

Hyperaccreting stellar-mass black hole systems are leading candidates for the central engines of gamma-ray bursts (GRBs). Their jets are thought to be powered by either the Blandford–Znajek (BZ) process or neutrino-dominated accretion flows (NDAFs), but discriminating between these mechanisms remains challenging. To address this, we proposed using the luminosity decay slope (d) of GRB light curves to distinguish between the BZ and NDAF mechanisms, thereby linking the light-curve morphology to the central engine physics. By analysing 85 single-peaked GRBs with fast-rise, exponential-decay (FRED) profiles observed by Swift/BAT using 64 ms background-subtracted light curves, we fitted the decay slope (d) with the empirical Kocevski–Ryde–Liang (KRL) function and compared the results with theoretical predictions for the BZ (d ≈ 1.67) and the NDAF (d ≈ 3.7–7.8) mechanisms. We find that the decay slope (d) can differentiate central engine mechanisms, with 15 GRBs consistent with the BZ mechanism and 22 supporting the NDAF mechanism. However, most events exhibit slopes within the range 2 < d < 4, suggesting a hybrid of mechanisms, with NDAF being dominant.

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