Trapped fireshell (halo) of photons and pairs around black-hole horizon: Source for ultra-high-energy particles
黑洞视界附近被捕获的光子-正负电子对火壳(晕):超高能粒子之源
We study the Compton-rocket effect of strong radiation force accelerating electrons in an opaque fireshell (or fire spot) of dense photons and electron-positron pairs, whose temperature is spatially inhomogeneous and exceeds the electron mass. We find the possibility of the charged-particle acceleration and the avalanche runaway process, leading to a non-trivial probability of ultra-high-energy (UHE) electrons and protons, which subsequently produce very-high-energy (VHE) photons and neutrinos. In a simplified one-dimensional model, we qualitatively show such peculiar dynamics using the fireball, Gamma-Ray Burst central engine, whose inner part inflows and forms a gravitationally trapped fireshell (halo) around the horizon of a black hole. The fireshell is metastable, cooling via UHE particle emissions and blackbody radiation. We calculate the UHE particle luminosity varying in time, and discuss the peculiar features of such produced UHE particles, which lead to VHE particles, in connection with possible numerical simulations, observations and experiments.
展开 ▾在不透明辐射流体中,Klein-Nishina 截面随粒子能量升高而下降,使逃逸概率非零,从而形成超高能电子-质子雪崩;该机制由微观局部辐射力梯度驱动,不依赖源的宏观对称性。
GRB 火球模型历来聚焦向外膨胀的外流部分 Rees+ 1992,而广义相对论流体研究显示火球内区可被引力捕获为视界附近的致密光子-正负电子对晕 Ruffini+ 2003,作者此前也把这类引力热灾变结构同喷流/火球形成联系起来 Xue 2021 Xue 2025。本文把 O'Dell 1981 的 Compton-rocket 辐射力推广到温度超过电子质量的完全不透明辐射流体,指出 Klein-Nishina 截面随能量下降可触发电子-质子雪崩逃逸,给出超高能粒子的非零产生概率。该机制与 Faure+ 2024 等粒子模拟研究形成互补,未来需三维数值模拟和完整散射截面来验证逃逸动力学,并可推广至双星并合、活动星系核、早期宇宙及强激光实验。
预印本 2025-12-03 · 刊出 2026-05-27 · 收录 2026-08-20