TheEp−Eisorelation and the internal shock model

2014/12/18 by R. Mochkovitch, L. Nava
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Computational astrophysics #Emission spectrum #Gamma-ray bursts and supernovae #Internal heating #Pulsars and Gravitational Waves Research #Shock (circulatory) #Shock wave #astro-ph.HE

paper · pdf · doi:10.1051/0004-6361/201424490

published as A&A 577, A31 (2015) · 7 pages, 4 figures

arxiv created 2014/12/18 · openalex publication_date 2015/02/20 · arxiv updated 2015/04/29 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. The validity of the Ep − Eiso correlation in gamma-ray bursts and the possibility of explaining the prompt emission with internal shocks are highly debated questions.

Citations

• Gamma-ray bursts from internal shocks in a relativistic wind: temporal and spectral properties
• Dissipative Photosphere Models of Gamma‐Ray Bursts and X‐Ray Flashes
• A COMPLETE SAMPLE OF BRIGHTSWIFTLONG GAMMA-RAY BURSTS. I. SAMPLE PRESENTATION, LUMINOSITY FUNCTION AND EVOLUTION
• Low-luminosity gamma-ray bursts as a distinct GRB population: a firmer case from multiple criteria constraints
• Synchrotron emission in the fast cooling regime: which spectra can be explained?
• Peak Energy Clustering and Efficiency in Compact Objects
• Peak energy of the prompt emission of long gamma-ray bursts versus their fluence and peak flux
• GAMMA-RAY BURST PROMPT EMISSION LIGHT CURVES AND POWER DENSITY SPECTRA IN THE ICMART MODEL
• Constraints on cold magnetized shocks in gamma-ray bursts