研究方向 · 研究方向详情
英文标题：Dense Environments and Multi-messenger Transients
科学问题
致密环境如何重塑瞬变外流，并将能量重新分配到中微子、光子和引力波通道？
English question: How do dense environments reshape transient outflows and redistribute their energy across neutrino, photon, and gravitational-wave channels?
这个研究方向追踪周围介质如何在信号到达观测者之前改变外流。它保持物理链条清晰：环境约束改变喷流动力学，激波加速粒子，微观相互作用产生信使，而面向探测器的可观测量仍与模型推导的推断目标分开。
Zhu 等人 2021 是这一背景中的编辑锚点，因为其受阻的 AGN 吸积盘喷流分化出中微子和光子信号，同时为短 GRB 通道保留了预测的引力波对应体。锚点只负责组织本页，不表示一个首要科学类别。
This Research Line follows how a surrounding medium changes an outflow before the signal reaches an observer. It keeps the physical chain explicit: environmental confinement changes jet dynamics, shocks accelerate particles, microscopic interactions produce messengers, and detector-facing observables remain separate from model-derived inference targets.
Zhu et al. 2021 is the Editorial Anchor for this context because its choked AGN-disk jet branches into neutrino and photon signals while retaining a predicted gravitational-wave counterpart for the short-GRB channel. The anchor organizes this page; it does not claim a primary scientific class.
英文原题：High-energy neutrino signatures of embedded GRB jets in AGN disks: a dynamic jet-propagation framework
阅读角色：前沿、方法 · 该方向的编辑锚点
这项工作提供了在致密 AGN 吸积盘环境中描述喷流传播和中微子产生的动态模型前沿。
English note: This Work provides a dynamic-model frontier account of jet propagation and neutrino production in a dense AGN-disk environment.
英文原题：Propagation of GRB Relativistic Jets in AGN Disks and Its Implication for GRB Detection
阅读角色：基础、前沿 · 该方向的编辑锚点
这项工作提供了在致密 AGN 吸积盘中喷流传播、准直和受阻的解析框架，把传统包层理论拓展至致密盘环境。
English note: This Work provides the analytical jet propagation and choking framework in dense AGN disks connecting stellar envelope models to AGN-embedded multi-messenger transients.
英文原题：High-energy Neutrinos from Choked Gamma-Ray Bursts in Active Galactic Nucleus Accretion Disks
阅读角色：基础、前沿 · 该方向的编辑锚点
这项工作提供了从嵌入式受阻喷流追踪到中微子、光子和引力波分支的 V0.1 基础。
English note: This Work supplies the V0.1 foundation for tracing an embedded choked jet into distinct neutrino, photon, and gravitational-wave branches.