The origin of the GRB diversity in the internal shock model

F. Daigne; R. Mochkovitch

doi:10.1393/ncb/i2007-10280-3

The origin of the GRB diversity in the internal shock model

F. Daigne
, R. Mochkovitch

Institut d’Astrophysique de Paris

Research output: Contribution to journal › Article › peer-review

Abstract

Our knowledge of the GRB population has dramatically increased in the recent years. In addition to the "standard" bright cosmological GRBs observed by BATSE, Beppo-SAX and HETE2 have detected X-ray-rich GRBs, X-ray flashes, subenergetic GRBs and even a few "local" events (such as GRB 980425/SN1998bw). We describe how the internal shock model allows the existence of such a diversity in the GRB population.

Original language	English
Pages (from-to)	1465-1466
Number of pages	2
Journal	Nuovo Cimento della Societa Italiana di Fisica B
Volume	121
Issue number	12
DOIs	https://doi.org/10.1393/ncb/i2007-10280-3
Publication status	Published - 1 Dec 2006
Externally published	Yes

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AB - Our knowledge of the GRB population has dramatically increased in the recent years. In addition to the "standard" bright cosmological GRBs observed by BATSE, Beppo-SAX and HETE2 have detected X-ray-rich GRBs, X-ray flashes, subenergetic GRBs and even a few "local" events (such as GRB 980425/SN1998bw). We describe how the internal shock model allows the existence of such a diversity in the GRB population.

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The origin of the GRB diversity in the internal shock model

Abstract

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