Gamma-ray bursts and their links with supernovae and cosmology

Gamma-ray bursts are the most luminous explosions in the Universe, whose origin and mechanism are the focus of intense interest. They appear connected to su- pernova remnants from massive stars or the merger of their remnants, and their bright- ness makes them temporarily detectable out to the largest distances yet explored in the universe. After pioneering breakthroughs from space and ground experiments, their study is entering a new phase with observations from the recently launched Fermi satellite, as well as the prospect of detections or limits from large neutrino and gravitational wave detectors. The interplay between such observations and theoretical models of gamma-ray bursts is reviewed, and cosmology. as well as their connections to supernovae

Gamma-ray bursts in the swift-Fermi era

Gamma 光线爆炸(GRB ) 在在宇宙的最强烈的出现之中。他们是强大的爆炸，对高 redshift，和思维到可见是黑洞出生的签名。他们是高度发光的事件并且提供远宇宙的优秀探针。GRB 研究极大地从斯威夫特，费密和一个活跃紧跟的社区与结果在过去的 10 年进展了。在这评论，我们调查在这些最近的观察和迅速的 GRB 排放和随后的晚霞的理论模型之间的相互影响。