Author: Amir Shahmoradi
Abstract: It is proposed that the luminosity function, the rest-frame spectral correlations and distributions of cosmological Long-duration (Type-II) Gamma-Ray Bursts (LGRBs) may be very well described as multivariate log-normal distribution. This result is based on careful selection, analysis and modeling of LGRBs' temporal and spectral variables in the largest catalog of Gamma-Ray Bursts available to date: 2130 BATSE GRBs, while taking into account the detection threshold and possible selection effects. Constraints on the joint rest-frame distribution of the isotropic peak luminosity (Liso), total isotropic emission (Eiso), the time-integrated spectral peak energy (Epkz) and duration (T90z) of LGRBs are derived. The presented analysis provides evidence for a relatively large fraction of LGRBs that have been missed by BATSE detector with Eiso extending down to ∼1049 [erg] and observed spectral peak energies (Epk) as low as ∼ 5 [keV]. LGRBs with rest-frame duration T90z < 1 [s] or observer-frame duration T90 < 2 [s] appear to be rare events (<0.1% chance of occurrence). The model predicts a fairly strong but highly significant correlation (ρ = 0.58 ± 0.04) between Eiso & Epk of LGRBs. Also predicted are strong correlations of Liso & Eiso with T90z and moderate correlation between Liso & Epkz. The strength and significance of the correlations found, encourage the search for underlying mechanisms, though undermine their capabilities as probes of Dark Energy's equation of state at high redshifts. The presented analysis favors - but does not necessitate - a cosmic rate for BATSE LGRBs tracing metallicity evolution consistent with a cutoff ∼ 0.2 - 0.5, assuming no luminosity-redshift evolution. A comparison with the Short-hard (type-I) class of GRBs will be presented. It is argued that similar correlations are also likely present in the prompt emission of type-I GRBs, indicating a unified prompt emission mechanism for both classes of GRBs.