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Gamma-Ray Bursts in the Swift Era

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TLDR
In this article, the authors review the rapid observational and theoretical progress in this dynamical research field during the first two-year of the Swift mission, focusing on how observational breakthroughs have revolutionized our understanding of the physical origins of GRBs.
Abstract
Since the successful launch of NASA's dedicated gamma-ray burst (GRB) mission, Swift, the study of cosmological GRBs has entered a new era. Here I review the rapid observational and theoretical progress in this dynamical research field during the first two-year of the Swift mission, focusing on how observational breakthroughs have revolutionized our understanding of the physical origins of GRBs. Besides summarizing how Swift helps to solve some pre-Swift mysteries, I also list some outstanding problems raised by the Swift observations. An outlook of GRB science in the future, especially in the GLAST era, is briefly discussed.

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Dark Energy

TL;DR: A survey of theoretical models and some aspects of numerical studies for dark energy can be found in this paper, where the authors review the problem of dark energy, including a survey of the theoretical models.
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The physics of gamma-ray bursts & relativistic jets

TL;DR: A comprehensive review of major developments in our understanding of gamma-ray bursts, with particular focus on the discoveries made within the last fifteen years when their true nature was uncovered, can be found in this paper.
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The Physics of Gamma-Ray Bursts and Relativistic Jets

TL;DR: A comprehensive review of major developments in the understanding of gamma-ray bursts can be found in this article, with particular focus on the discoveries made within the last fifteen years when their true nature was uncovered.
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The strongest cosmic magnets: soft gamma-ray repeaters and anomalous X-ray pulsars

Abstract: Two classes of X-ray pulsars, the anomalous X-ray pulsars and the soft gamma-ray repeaters, have been recognized in the last decade as the most promising candidates for being magnetars: isolated neutron stars powered by magnetic energy. I review the observational properties of these objects, focussing on the most recent results, and their interpretation in the magnetar model. Alternative explanations, in particular those based on accretion from residual disks, are also considered. The possible relations between these sources and other classes of neutron stars and astrophysical objects are also discussed.
References
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Journal ArticleDOI

Collapse of Neutron Stars to Black Holes in Binary Systems: A Model for Short Gamma-Ray Bursts

TL;DR: In this article, the authors proposed a short gamma-ray burst (SGRB) model, where the mass of a white dwarf-neutron star coalescence in a low-mass binary system is enough to exceed the critical mass of the neutron star and trigger its collapse to a black hole.
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BeppoSAX confirmation of beamed afterglow emission from GRB 990510

TL;DR: In this paper, the authors compare the prompt X-ray (2{10 keV) emission of GRB 990510 measured by the BeppoSAX Wide Field Cameras (WFC) during the burst to the Xray afterglow detected by the Narrow Field Instruments (NFI).
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Properties of X-ray rich gamma ray bursts and X-ray flashes detected with BeppoSAX and Hete-2

TL;DR: In this article, the spectrum of the prompt emission and the X-ray and optical afterglow fluxes of 54 X-Ray Rich Gamma Ray Burst (XRRs) and X Ray Flashes (XRFs), observed by BeppoSAX and HETE-2, were compared with classical Gamma Ray Bursts.
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Constraining the Origin of TeV Photons from Gamma-Ray Bursts with Delayed MeV-GeV Emission Formed by Interaction with Cosmic Infrared/Microwave Background Photons

TL;DR: In this paper, it has been suggested that electromagnetic cascade of very high-energy gamma-rays from gamma-ray bursts (GRBs) in the infrared/microwave background can produce delayed MeV-GeV photons.
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