Closure Relations for Electron-Positron Pair-Signatures in Gamma-Ray Bursts
arXiv:0708.1370 · doi:10.1086/527667
Abstract
We present recipes to diagnose the fireball of gamma-ray bursts (GRBs) by combining observations of electron-positron pair-signatures (the pair-annihilation line and the cutoff energy due to the pair-creation process). Our recipes are largely model-independent and extract information even from the non-detection of either pair-signature. We evaluate physical quantities such as the Lorentz factor, optical depth and pair-to-baryon ratio, only from the observable quantities. In particular, we can test whether the prompt emission of GRBs comes from the pair/baryonic photosphere or not. The future-coming Gamma-Ray Large Area Space Telescope (GLAST) satellite will provide us with good chances to use our recipes by detecting or non-detecting pair-signatures.
7 pages, 4 figures, accepted for publication in ApJ, with extended discussions. Conclusions unchanged
References in corpus (7)
- Gamma-Ray Bursts in the Swift Era
- GRB Radiative Efficiencies Derived from the Swift Data: GRBs vs. XRFs, Long vs. Short
- High Energy Neutrinos and Cosmic-Rays from Low-Luminosity Gamma-Ray Bursts?
- A new method of determining the initial size and Lorentz factor of gamma-ray burst fireballs using a thermal emission component
- Is the sky falling? Searching for stellar streams in the local Milky Way disc in the CORAVEL and RAVE surveys
- Unstable GRB photospheres and electron-positron annihilation lines
- Effects of Cosmic Infrared Background on High Energy Delayed Gamma-Rays from Gamma-Ray Bursts
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