scispace - formally typeset
Open AccessJournal ArticleDOI

Gamma-Ray Bursts in the Swift Era

Reads0
Chats0
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.

read more

Citations
More filters
Journal ArticleDOI

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.
Journal ArticleDOI

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
More filters
Journal ArticleDOI

Swift identification of dark gamma-ray bursts

TL;DR: In this article, the authors present an optical flux vs. X-ray flux diagram for all known gamma-ray bursts (GRBs) for which an Xray afterglow has been detected, and propose an operational definition of dark bursts as those bursts that are optically subluminous with respect to the fireball model.
Journal ArticleDOI

Is thermal emission in gamma-ray bursts ubiquitous?

TL;DR: In this article, a hybrid model with a thermal and a non-thermal component was proposed to explain the gamma-ray burst spectral evolution, and the authors showed that the thermal component is the key emission process determining the spectral evolution.
Journal ArticleDOI

Gamma‐ray burst efficiency and possible physical processes shaping the early afterglow

TL;DR: In this article, the authors re-examine the estimates of kinetic energy in GRB afterglows and show that the efficiency of converting the kinetic energy into gamma-rays is moderate and does not challenge the standard internal shock model.
Journal ArticleDOI

Particle Acceleration in Relativistic Jets due to Weibel Instability

TL;DR: In this article, the Weibel instability created in the collisionless shock front accelerates particles perpendicular and parallel to the jet propagation direction, which contributes to the electron s transverse deflection behind the jet head.
Journal ArticleDOI

Implications of the Lag-Luminosity Relationship for Unified Gamma-Ray Burst Paradigms

TL;DR: In this paper, a cross-correlation methodology was used to estimate spectral lags for 1429 long (T90 > 2 s) BATSE gamma-ray bursts (GRBs) with peak flux Fp > 0.25 photons cm-2 s-1, near to the BATSE trigger threshold.
Related Papers (5)

The Swift Gamma-Ray Burst Mission

Neil Gehrels, +77 more