The Maximum Isotropic Equivalent Energy Of Gamma Ray Bursts

Abstract

The canonball model, which unifies cosmic ray bursts (CRBs) and gamma ray bursts (GRBs), is used to predict the maximum isotropic equivalent gamma ray energy release in a GRB. The predicted maximum is based on the observed knee around 1 TeV in the energy spectrum of Galactic cosmic ray electrons, and on the Amati correlation in GRBs. Both were predicted by the cannonball model of CRBs and GRBs before their empirical discoveries. The predicted maximum agrees well with that concluded from up to date GRB observations.

arXiv commentExpanded version, 4 figures

References in corpus (18)

• Collapsars - Gamma-Ray Bursts and Explosions in "Failed Supernovae"
• Intrinsic spectra and energetics of BeppoSAX Gamma-Ray Bursts with known redshifts
• Discovery of the X-Ray Afterglow of the Gamma-Ray Burst of February 28 1997
• The energy spectrum of cosmic-ray electrons at TeV energies
• Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons
• Probing the ATIC peak in the cosmic-ray electron spectrum with H.E.S.S
• The Ep,i - Eiso correlation in GRBs: updated observational status, re-analysis and main implications
• The DArk Matter Particle Explorer mission
• Extended Measurement of the Cosmic-Ray Electron and Positron Spectrum from 11 GeV to 4.8 TeV with the Calorimetric Electron Telescope on the International Space Station
• Extremely energetic Fermi Gamma-Ray Bursts obey spectral energy correlations
• Addressing the circularity problem in the $E_{\text{p}}-E_{\text{iso}}$ correlation of Gamma-Ray Bursts
• Gamma Ray Bursts from Minijets
• Towards a complete theory of Gamma Ray Bursts
• The Konus-Wind catalog of gamma-ray bursts with known redshifts. II. Waiting mode bursts simultaneously detected by Swift/BAT
• A theory of Cosmic Rays
• A blast from the infant Universe: the very high-z GRB 210905A
• The Cosmic-Ray Spectra: News on their Knees
• Origin Of The Cosmic Ray Positrons Observed Near Earth- Meson Decay Or Dark Matter Decay?

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• Properties of the extremely energetic GRB~221009A from Konus-WIND and SRG/ART-XC observations
• GRB minimum variability timescale with Insight-HXMT and Swift: implications for progenitor models, dissipation physics and GRB classifications
• GRB 221009A and the Apparently Most Energetic Gamma-Ray Bursts
• Time domain astrophysics with transient sources. Delay estimate via Cross Correlation Function techniques