论文标题
来自统一旋场的普朗克时代的量子磁单孔
Quantum magnetic monopoles at the Planck era from unified spinor fields
论文作者
论文摘要
我使用统一的旋转磁场（USF）来讨论在通货膨胀期间的磁性产生，作为来自大型带电载体玻色子的冷凝物的量子真空的激发。对于具有总能量$ m_p $的原始宇宙，对于用总planck磁性充电而创建的磁性单极$ q_m = q_p = q_p = \ pm e/\sqrtα$和总质量$ $ m_m $，它是在量化量化的动作后获得的。 \，m_m} {5 \，m_p} \ right）\，\ left（\ frac {e} {q_m} {q_m} \ right）^2 $。如果这些磁性单极具有总磁性电荷$ q_m = \ pm e $和一个小的质量$ m = m_m/n $，则可能会有大量的小量子磁性单极管，这可能是候选人以$ 30.97 \，\％的能量来解释planck Era the Intrordial Universe的$ 30.97 \，\％。还分析了Milli-Magnet带电的颗粒的情况。我们证明，质量小于$ 3.6 \ times 10^3 $ GEV的磁性单孔（mm）可以以非常小的费用为$ 10^{ - 14} \，E $，这是在Atlas和Moedal实验中进行搜索的量的含量。
I use Unified Spinor Fields (USF), to discuss the creation of magnetic monopoles during preinflation, as excitations of the quantum vacuum coming from a condensate of massive charged vector bosons. For a primordial universe with total energy $M_p$, and for magnetic monopoles created with a total Planck magnetic charge $q_M=q_P=\pm e/\sqrtα$ and a total mass $m_M$, it is obtained after quantisation of the action that the fine-structure constant is given by: $α= \frac{5}{6} \left(1- \frac{16 \,m_M}{5 \,M_p}\right) \,\left(\frac{e}{q_M}\right)^2$. If these magnetic monopoles were with total magnetic charge $q_M=\pm e$ and a small mass $m=m_M/n$, there would be a large number of small quantum magnetic monopoles which could be candidates to explain the presence of dark matter with a $30.97\,\%$ of the energy in the primordial universe at the Planck era. The case of milli-magnetically charged particles is also analysed. We demonstrate that magnetic monopoles (MM) with masses less than $3.6\times 10^3$ GeV, can exist with a very small charges of up to $10^{-14}\,e$, which are quantities of interest for searches to be performed in the ATLAS and MoEDAL experiments.
