Electron anti-neutrinos at the Glashow resonance (GR, at $E_{{\overline{\nu }}_e}\sim 6.3$ PeV) have an enhanced probability to be detected. With three neutrinos detected by IceCube in the (1–2) PeV energy range at present, one would expect that about 1 to 4 GR ${\overline{\nu }}_e$ should have been detected. The high-energy ∼8.7 PeV muon neutrino detected by IceCube may not be a GR event. If so, we expect to detect 50 to 70 GR ${\overline{\nu }}_e$, then one would have a “missing Glashow-resonance problem”. This would suggest (1) that pγ interaction rather than pp interaction is the dominant channel to produce the observed IceCube high-energy neutrinos; (2) that multi-pion pγ interactions are suppressed; and (3) that the magnetic field and photon energy density in the pγ emission region is such that significant ${\mu }^{+}$ cooling occurs before decaying, yet ${\pi }^{+}$'s essentially do not cool before decaying.

电子反中微子在Glashow共振（GR，at ${Ë}_{{\overline{\nu }}_{Ë}}〜6.3$PeV）的概率更高。目前，IceCube在（1-2）PeV能量范围内检测到3个中微子，人们可以预期大约有1至4 GR${\overline{\nu }}_{Ë}$应该已经被检测到。IceCube检测到的高能量〜8.7 PeV的μ子中微子可能不是GR事件。如果是这样，我们预计将检测到50到70 GR${\overline{\nu }}_{Ë}$，那么就会有一个“缺少Glashow共振问题”。这表明（1）pγ相互作用而不是pp相互作用是产生观察到的IceCube高能中微子的主要渠道；（2）抑制了多pionpγ相互作用；（3）pγ发射区域的磁场和光子能量密度非常大${\mu }^{+}$ 冷却发生在腐烂之前 ${\pi }^{+}$在腐烂之前基本上不冷却。