论文标题
喷气引力波
Jet Gravitational Waves
论文作者
论文摘要
射流到相对论速度的加速会产生独特的记忆类型引力波(GW)信号:{\ it jet-gw}。我在这里讨论有关这些GWS性质的怨恨结果,并考虑它们在当前和拟议的检测器中的可检测性。古典来源是长而短的伽玛射线爆发,以及核心折叠超新星中的隐藏喷气机。从这些来源检测JET-GW将需要检测器,例如提议的BBO,Decigo和Lunar基于dectector的检测,这些检测器将在Decihz频段中运行。当前的LVK探测器如果足够不对称,可以从银河系SGR耀斑中检测到JET-GW。一旦检测到这些信号,就可以揭示有关喷气加速度和准确性的信息,否则无法探索。
The acceleration of a jet to relativistic velocities produces a unique memory type gravitational waves (GW) signal: {\it Jet-GW}. I discuss here resent result concerning properties of these GWs and consider their detectability in current and proposed detectors. Classical sources are long and short Gamma-ray bursts as well as hidden jets in core-collapse supernovae. Detection of jet-GWs from these sources will require detectors, such as the proposed BBO, DECIGO and lunar based detectors, that will operate in the deciHz band. The current LVK detectors could detect jet-GWs from a Galactic SGR flare if it is sufficiently asymmetric. Once detected these signals could reveal information concerning jet acceleration and collimation that cannot be explored otherwise.