涡旋与扭转磁场中的中微子振荡
Neutrino oscillations in vortex and twisting magnetic fields
AI总结：
本文基于左右对称模型推导涡旋与扭转磁场中的中微子演化方程，分析磁诱导共振转换，并指出高能太阳耀斑中ν_eL的显著损耗及利用相干弹性中微子-核散射望远镜观测的可能。
摘要：
本文在左右对称模型框架内研究了中微子流在涡旋磁场和扭转磁场中的行为。作为这些磁场的示例，我们讨论了耦合太阳黑子（CS's）的磁场，这些黑子是未来太阳耀斑的来源。预计中微子具有电荷半径、磁矩和无矢矩等多极矩。文中推导了类薛定谔形式的演化方程，并分析了所有由磁场诱导的共振转换。结果表明，在高能耀斑情形下，ν_eL中微子会因其共振吸收而发生显著损耗。本文还探讨了在基于相干弹性中微子-核散射反应工作的中微子望远镜上观测这一现象的可能性。
英文摘要：
The behavior of the neutrino flux in vortex and twisting magnetic fields is considered within the left-right symmetric model. By way of illustration of the magnetic fields we discuss the magnetic fields of the coupled sunspots (CS's) which are the sources of the future solar flares. It is expected that the neutrinos have such multipole moments as the charge radius, the magnetic and anapole moments. The evolution equation in the Schrodinger-like form is found and all magnetic-induced resonance conversions are analyzed. It is demonstrated that in the case of the high-energy flares the sizeable depletion of the $ν_{eL}$ neutrinos caused by their resonance absorptions takes place. Possibilities of observations of this phenomena are investigated at neutrino telescopes whose work is based on the reaction of the coherent elastic neutrino-nucleus scattering.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
