2017
DOI: 10.1007/s11214-017-0366-4
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Gamma-Ray Bursts and Fast Transients

Abstract: The current status of observations and theoretical models of gamma-ray bursts and some other related transients, including ultra-long bursts and tidal disruption events, is reviewed. We consider the impact of multi-wavelength data on the formulation and development of theoretical models for the prompt and afterglow emission including the standard fireball model utilizing internal shocks and external shocks, photospheric emission, the role of the magnetic field and hadronic processes. In addition, we discuss so… Show more

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Cited by 24 publications
(12 citation statements)
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“…Achromatic jet-breaks have been observed in optical/IR, however they often do not coincide with breaks observed in X-rays, indicating that our knowledge of the afterglows emission is still limited, and questioning if the jet-angle and collimated energy that have been estimated are right. Even if from the theoretical side many explanations (energy injections, double jet, structured jets) have been proposed to interpret the afterglow emission from IR/optical to X-rays, more multi-frequency observations are necessary (see, e.g., Willingale & Mészáros, 2017). Compared to today, the larger number of THESEUS GRBs and the more sensitive spectra observed with XGIS will allow us to better understand the nature of the afterglow and of the central engine of GRBs.…”
Section: Grb Physics Progenitors and Cosmologymentioning
confidence: 99%
“…Achromatic jet-breaks have been observed in optical/IR, however they often do not coincide with breaks observed in X-rays, indicating that our knowledge of the afterglows emission is still limited, and questioning if the jet-angle and collimated energy that have been estimated are right. Even if from the theoretical side many explanations (energy injections, double jet, structured jets) have been proposed to interpret the afterglow emission from IR/optical to X-rays, more multi-frequency observations are necessary (see, e.g., Willingale & Mészáros, 2017). Compared to today, the larger number of THESEUS GRBs and the more sensitive spectra observed with XGIS will allow us to better understand the nature of the afterglow and of the central engine of GRBs.…”
Section: Grb Physics Progenitors and Cosmologymentioning
confidence: 99%
“…Thanks to the BeppoSAX mission that discovered GRB afterglows and the Neil Gehrels Swift observatory that initiated the systematic study of the early afterglow, we have a very consolidated knowledge of the temporal and spectral behaviour of the low energy (<10 keV) afterglow (see, e.g., [32,77]). However, due to the limited sensitivity of the current instrumentation, at higher energies the afterglow temporal and spectral behaviour is an almost uncharted territory.…”
Section: Hard X-ray Spectrum and Polarisation Of Grb Afterglowsmentioning
confidence: 99%
“…Gamma-ray bursts (GRBs) are the most energetic explosions in the universe and are not only extremely interesting phenomena in astrophysics but also important for multi-messenger astrophysics with gravitational waves and cosmic-ray particles [87]. GRBs happen every day, in any place in the sky, and last only a few tens of seconds.…”
Section: Observation Of Prompt Photons From Gamma-ray Burstsmentioning
confidence: 99%