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Titlebook: Gamma-Ray Bursts; The brightest explos Gilbert Vedrenne,Jean-Luc Atteia Book 2009 Springer-Verlag Berlin Heidelberg 2009 Cosmology.Universe

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发表于 2025-3-21 20:08:15 | 显示全部楼层 |阅读模式
书目名称Gamma-Ray Bursts
副标题The brightest explos
编辑Gilbert Vedrenne,Jean-Luc Atteia
视频video
概述First book to provide a complete overview of the GRB story at the research level.Explains to the reader the importance of GRBs in the context of modern astrophysics and cosmology.Details the discovery
丛书名称Springer Praxis Books
图书封面Titlebook: Gamma-Ray Bursts; The brightest explos Gilbert Vedrenne,Jean-Luc Atteia Book 2009 Springer-Verlag Berlin Heidelberg 2009 Cosmology.Universe
描述Since their discovery was first announced in 1973, gamma-ray bursts (GRBs) have been among the most fascination objects in the universe. While the initial mystery has gone, the fascination continues, sustained by the close connection linking GRBs with some of the most fundamental topics in modern astrophysics and cosmology. Both authors have been active in GRB observations for over two decades and have produced an outstanding account on both the history and the perspectives of GRB research.
出版日期Book 2009
关键词Cosmology; Universe; astrophysics; gamma-ray bursts; stellar explosions; supernovae
版次1
doihttps://doi.org/10.1007/978-3-540-39088-6
isbn_softcover978-3-642-07254-3
isbn_ebook978-3-540-39088-6
copyrightSpringer-Verlag Berlin Heidelberg 2009
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发表于 2025-3-21 22:51:48 | 显示全部楼层
The BATSE decade,ed to study GRBs. BATSE consisted of eight pairs of NaI detectors. Each pair included a Large Area Detector (LAD) and a Spectroscopy Detector (SD). The area of a Large Area Detector was 2000 cm.. With a sensitivity 5 to 10 times better than previous GRB detectors, BATSE detected an average of 1 GRB
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BeppoSAX and the afterglow era,bout the mission and its instruments. In the introduction to this chapter, it is important to mention the remarkable work done by the scientific and technical teams, which were strongly motivated by two researchers, E. Costa and F. Frontera. These two reseachers were very excited by the GRB mystery
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,Gamma-ray bursts—fireballs and blastwaves, the main properties of gamma-ray bursts with standard physics applied to somewhat ‘exotic’ objects. In this chapter we outline the most popular model to explain GRBs and their afterglows. This model, with its basic ingredients, has very often been called the standard model.
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Early afterglows: the Swift revolution,ontributed to a better knowledge of GRBs. In particular, these observations contributed to a better appreciation of the connection between the GRB prompt emission and the afterglow. Swift has brought various surprises: the complex behavior of the early X-ray afterglow (., .), the frequent faintness
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Progenitors,ts have made it possible to measure the isotropic equivalent energies emitted by GRBs in gamma-rays. These energies reach 10. to 10. erg. As most GRBs are probably collimated with typical opening angles between 1° and 20°, the true energy is clustered around 10. to 10. ergs which must be liberated i
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https://doi.org/10.1007/978-3-540-39088-6Cosmology; Universe; astrophysics; gamma-ray bursts; stellar explosions; supernovae
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