Absolute Rate, Evolving Luminosity function, and Evolving Jet Opening Angle Distribution for Long Gamma-Ray Bursts
arXiv:astro-ph/0509276 · doi:10.1143/PTP.114.983
Abstract
Using the luminosity function and the apparent GRB rate inferred from the spectral peak energy-luminosity relation, we investigate the absolute GRB formation rate, taking into account the effects of both the jet-luminosity evolution and the jet opening angle evolution. In the case that there is no jet opening angle evolution, the jet-corrected luminosity for high-redshift GRBs is much larger than typical values for low-z (z>~1) bursts. On the other hand, if the jet-luminosity does not evolve with time, the jet opening angle for high-z bursts should be much smaller than that for low-z GRBs. Therefore, it is preferable to take into account both evolution effects. We also estimate the local GRB event rate in a galaxy of ~10^{-7}-10^{-5}/yr.
11 pages, 6 figures, published in PTP
References in corpus (6)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Theories of Gamma-Ray Bursts
- The Fourth BATSE Gamma-Ray Burst Catalog (Revised)
- Probing the Cosmic Reionization History and Local Environment of Gamma-Ray Bursts through Radio Dispersion
- Are there cosmological evolution trends on Gamma-Ray Burst features?
- A possible observational evidence for angular distribution of opening half-angle of GRB jets
Cited by in corpus (7)
- The luminosity function and the rate of Swift's Gamma Ray Bursts
- Constraints on Type Ib/c and GRB Progenitors
- Collapse of rotating stars in the Universe and the cosmic gamma ray bursts
- Selection Effects on the Observed Redshift Dependence of GRB Jet Opening Angles
- Research on the redshift evolution of luminosity function and selection effect of GRBs
- Gravitational Wave Memory from the Relativistic Jet of Gamma-Ray Bursts
- GRBs luminosity function synthesized from \textit{Swift/BAT}, \textit{Fermi/GBM} and \textit{Konus-Wind} data