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Gamma-ray bursts and cosmology
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 2007I review the current status of the use of gamma-ray bursts (GRBs) as probes of the early Universe and cosmology. I describe the promise of long GRBs as probes of the high redshift ( z >4) and very high redshift ( z >5) Universe, and several key scientific results that have come from ...
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1991
We summarize the observed features of γ-ray bursts, with particular emphasis on the cyclotron lines seen in their spectra. We then discuss the theory of cyclotron resonant scattering, and compare the theoretical and observed line spectra. Finally, we mention some implications.
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We summarize the observed features of γ-ray bursts, with particular emphasis on the cyclotron lines seen in their spectra. We then discuss the theory of cyclotron resonant scattering, and compare the theoretical and observed line spectra. Finally, we mention some implications.
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On the origin of gamma-ray bursts
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 2008Gamma-ray bursts are the most energetic explosions in the Universe, occurring at cosmological distances. The initial phase of the emission from these bursts is predominantly of gamma rays and stems from a highly relativistic outflow. The nature of this emission is still under debate.
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The theory of gamma-ray bursts
AIP Conference Proceedings, 1984A γ-ray burst occurs when a strongly magnetic neutron star experiences either a thermonuclear explosion in degenerate material accumulated over a long period of time or the sudden, greatly super-Eddington accretion of matter. Certain aspects of the thermonuclear model are briefly reviewed and special attention is devoted to mechanisms for producing the
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Swift observations of gamma-ray bursts
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 2007Since its launch on 20 November 2004, the Swift mission has been detecting approximately 100 gamma-ray bursts (GRBs) each year, and immediately (within approx. 90 s) starting simultaneous X-ray and UV/optical observations of the afterglow.
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Revisiting the luminosity and redshift distributions of long gamma-ray bursts
Monthly Notices of the Royal Astronomical Society, 2021Jun-Jie Wei, Houdun Zeng, Xue-Feng Wu
exaly
The Ep,i–Eiso correlation: type I gamma-ray bursts and the new classification method
Monthly Notices of the Royal Astronomical Society, 2020P Yu Minaev
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Synchrotron self-compton emission in the two-component jet model for gamma-ray bursts
Journal of High Energy Astrophysics, 2023Yuri Sato, Kohta Murase, Yutaka Ohira
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Distinction of groups of gamma-ray bursts in the BATSE catalog through fuzzy clustering
Astronomy and Computing, 2021Soumita Modak
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