论文标题
高能中微子瞬变和多门徒天文学的未来
High-energy neutrino transients and the future of multi-messenger astronomy
论文作者
论文摘要
最近发现高能天体中性中微子的发现，以及一致的电磁和中微子发射的最初暗示，是多门徒天文学时代的开始。由于它们的高功率，预计瞬态源将通过增强的粒子加速和相互作用提供观察到的能量天线的很大一部分。在这里，我们回顾了从瞬态天体物理来源以及当前和即将到来的实验景观中中微子排放的理论期望，突出了发现和指定其可检测性的最有希望的渠道。
The recent discovery of high-energy astrophysical neutrinos and first hints of coincident electromagnetic and neutrino emission herald the beginning of the era of multi-messenger astronomy. Due to their high power, transient sources are expected to supply a significant fraction of the observed energetic astroparticles, through enhanced particle acceleration and interactions. Here, we review theoretical expectations of neutrino emission from transient astrophysical sources and the current and upcoming experimental landscape, highlighting the most promising channels for discovery and specifying their detectability.
