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 ...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展开更多
高精力天体物理学是在当代的天体物理学的最活跃的分支之一。它学习射出 X 光检查和光线光子的天体物理学的目标，例如增大中子星的超级巨大、星尺寸的黑洞，和各种各样的种类。与许多卫星转菠、基于地面的观察设备的操作，高精力天体...高精力天体物理学是在当代的天体物理学的最活跃的分支之一。它学习射出 X 光检查和光线光子的天体物理学的目标，例如增大中子星的超级巨大、星尺寸的黑洞，和各种各样的种类。与许多卫星转菠、基于地面的观察设备的操作，高精力天体物理学在过去的十年喜欢快速的开发。这块地将继续在来十年很快进展，这被预见，与在高精力的中微子和重力的波浪隧道的天体物理学的来源的可能的开创性的发现。当它站在 2013，物理的边疆的这期特刊被奉献给高精力天体物理学的领域的系统的调查。展开更多
文摘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
文摘高精力天体物理学是在当代的天体物理学的最活跃的分支之一。它学习射出 X 光检查和光线光子的天体物理学的目标，例如增大中子星的超级巨大、星尺寸的黑洞，和各种各样的种类。与许多卫星转菠、基于地面的观察设备的操作，高精力天体物理学在过去的十年喜欢快速的开发。这块地将继续在来十年很快进展，这被预见，与在高精力的中微子和重力的波浪隧道的天体物理学的来源的可能的开创性的发现。当它站在 2013，物理的边疆的这期特刊被奉献给高精力天体物理学的领域的系统的调查。
