Q-NONTHERMAL-PARTICLE-TRANSPORT · provisional_seed
宇宙线、gamma-ray binaries、星系弥散gamma射线、非热射电/X-ray及中微子产生。
仅报告瞬变探测且无粒子机制或输运约束。
决定高能反馈、弥散背景和多信使源解释是否一致。
The jet driven by S140 IRS1 offers a viable particle acceleration site, yielding injection timescales and maximum particle energies consistent with theoretical expectations, whereas stellar winds are energetically disfavored.
deterministic_keyword_v1_1 · confidence=0.59
Theoretical studies and recent observations suggest that the winds of massive stars could be sources of Galactic cosmic rays.
deterministic_keyword_v1 · confidence=0.67
Galaxy clusters are among the most massive gravitationally bound systems in the Universe and are considered major reservoirs of high-energy cosmic rays, yet no conclusive γ-ray detection from them has been achieved.
deterministic_keyword_v1 · confidence=0.63
We therefore propose a hybrid model that combines inverse Compton emission from PWN electrons with hadronic interactions between escaped cosmic rays and a nearby molecular cloud.
deterministic_keyword_v1 · confidence=0.71