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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.
Journal ArticleDOI

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.
Journal ArticleDOI

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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Book

Gamma-Ray Bursts

TL;DR: In this paper, the present status of gamma-ray burst research is reviewed, with an emphasis on recent observations of their temporal, spectral, and global distribution properties, including the energy source and emission mechanism.
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Model-independent multivariable gamma-ray burst luminosity indicator and its possible cosmological implications

TL;DR: In this paper, a multivariable regression analysis is presented for a sample of 15 gamma-ray bursts (GRBs), where the observables used in the analysis include the isotropic gamma-rays energy (Eγ,iso), the peak energy of the νFν spectrum in the rest frame (E), and the rest-frame break time of the optical afterglow light curves (t).
Journal ArticleDOI

Gamma-Ray Bursts as a Probe of the Very High Redshift Universe

TL;DR: In this paper, it was shown that GRBs and their afterglows can be used as beacons to locate core collapse SNe at redshifts z > 1, and to study the properties of these SNe.
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