论文标题
从径向影响地球上搜索磁化夸克nugget暗物质的结果
Results of search for magnetized quark-nugget dark matter from radial impacts on Earth
论文作者
论文摘要
磁化夸克掘金（MQN）是最近提出的与标准模型以及Tatsumi在磁铁中的Quark-Nugget核心理论一致的深色候选者。先前的出版物已经涵盖了它们在早期宇宙中的形成，在巨大的质量衰减之前，将它们的磁力衰减，通过磁磁磁与正常物质的相互作用，以及首先观察一致的MQN，即几乎切入的影响，限制了其表面磁场的表面磁场b_o b_o b_o b_o b_o b_o b_o tattatsumi的值为0.1至10.0 ttt to new ttt to new tt to new ttt to new ttt to new ttt to new 1.65 tt +/1.65 tt。 MQN质量分布和相互作用横截面在很大程度上取决于B_O。它们的磁粘着比几何尺寸大得多，并且可能导致足够的能量沉积以形成非恒星陨石坑，这大约每年报告。我们报告了水饱和泥炭，软沉积物和花岗岩中MQN能量沉积的计算机模拟，并报告了发掘这种火山口的结果。观测值和MQN影响的流体动力模拟之间的五个一致性支持了与MQN暗物质一致的第二个观察结果，并提出了一种合格其他MQN事件的方法。结果还将B_O冗余地限制在大于0.4 tt。
Magnetized Quark Nuggets (MQNs) are a recently proposed dark-matter candidate consistent with the Standard Model and with Tatsumi's theory of quark-nugget cores in magnetars. Previous publications have covered their formation in the early universe, aggregation into a broad mass distribution before they can decay by the weak force, interaction with normal matter through their magnetopause, and first observation consistent MQNs, i.e. a nearly tangential impact limiting their surface-magnetic-field parameter B_o from Tatsumi's values of 0.1 to 10.0 TT to new value of 1.65 TT +/- 21%. The MQN mass distribution and interaction cross section depend strongly on B_o. Their magnetopause is much larger than their geometric dimensions and can cause sufficient energy deposition to form non-meteorite craters, which are reported approximately annually. We report computer simulations of the MQN energy deposition in water-saturated peat, soft sediments, and granite and report results from excavating such a crater. Five points of agreement between observations and hydrodynamic simulations of an MQN impact support this second observation consistent with MQN dark matter and suggest a method for qualifying additional MQN events. The results also redundantly constrain B_o to greater than 0.4 TT.
