论文标题
Pierre Auger Exotic Events和Axion Quark Nuggets
The Pierre Auger Exotic Events and Axion Quark Nuggets
论文作者
论文摘要
皮埃尔螺旋钻天文台报道了[1-3]观察到几种外来宇宙射线样事件,这些事件显然与雷暴有关。这些事件的大小比传统的宇宙射线事件大得多,并且它们具有非常不同的定时功能。观察到的现象的一种可能的性质仍然是积极研究和辩论的问题,因为这些异国情调事件的许多异常特征很难解释。特别是,这些外来事件的外观频率非常低(小于2个事件/年),与该地区常规雷击的典型速度形成鲜明对比。我们建议可以在所谓的斧头夸克掘金(AQN)暗物质模型中解释观察到的外来事件。这个想法是,由于大气分子沿其路径的电离,AQN可能在雷暴过程中触发并引发特殊而独特的雷击。相应的AQN诱导的照明闪光可能会显示一些特定的功能,而不是由典型和更频繁的常规闪光所共享的特定功能。我们通过证明观察结果[1-3](包括外观和时间持续时间的频率与观察结果一致)来支持这一建议。我们还评论了螺旋螺旋式异国情调的可能关系与望远镜阵列爆发和地面伽马射线闪光灯的关系。我们列出了AQN诱导的外来事件的许多特征(例如与这些事件同步的特定无线电脉冲),可以通过将来的实验直接测试。我们还建议使用分布式的声感应仪器来检测必须与螺旋螺旋式外来事件同步的声脉冲。
The Pierre Auger Observatory have reported [1-3] observation of several exotic cosmic ray -like events which apparently related to thunderstorms. These events are much larger in size than conventional cosmic ray events, and they have very distinct timing features. A possible nature of the observed phenomenon is still a matter of active research and debates as many unusual features of these exotic events are hard to explain. In particular, the frequency of appearance of these exotic events is very low (less than 2 events/year), in huge contrast with a typical rate of a conventional lightning strikes in the area. We propose that the observed exotic events can be explained within the so-called axion quark nugget (AQN) dark matter model. The idea is that the AQNs may trigger and initiate a special and unique class of lightning strikes during a thunderstorm as a result of ionization of the atmospheric molecules along its path. The corresponding AQN-induced lighting flashes may show some specific features not shared by typical and much more frequent conventional flashes. We support this proposal by demonstrating that the observations[1-3], including the frequency of appearance and time duration are consistent with observations. We also comment on possible relation of AUGER exotic events with the Telescope Array bursts and the terrestrial gamma ray flashes. We list a number of features of the AQN-induced exotic events (such as specific radio pulses synchronized with these events) which can be directly tested by future experiments. We also suggest to use distributed acoustic sensing instruments to detect the acoustic pulses which must be synchronized with AUGER exotic events.