论文标题
宇宙强体光谱中的Gluon冷凝效应
The gluon condensation effect in the cosmic hadron spectra
论文作者
论文摘要
宇宙质子和核 - 光谱的硬化是通过使用Gluon冷凝（GC）模型来解释的，该模型指出，质子中的大量纤维可能在高能阈值附近凝结。结果表明，GC效应是一系列异常的天体物理现象的共同起源，包括伽马射线光谱中的破碎幂律，正电子和电子谱的过量以及质子和细胞核谱的硬化。
Hardening of cosmic proton- and nuclei-spectra is explained by using the gluon condensation (GC) model, which states that a large amount of gluons in proton may condense near the high energy threshold. The results present the GC-effect as common origin of a series of anomalous astrophysical phenomena including the broken power-law in gamma-ray spectra, the excess in positron- and electron-spectra and hardening of proton- and nuclei-spectra.
