论文标题
重新审视脉冲星死亡线 - I.几乎真空差距
Pulsar death line revisited -- I. Almost vacuum gap
论文作者
论文摘要
在本文中，这是一系列专门针对无线电脉冲星死亡线进行详细分析的论文中的第一本，我们考虑了在足够长的脉冲星周期中产生次级颗粒的可能性。到此，我们重新考虑了内部间隙上磁极盖上次生等离子体产生的潜在降低。我们的研究使得有可能完善产生次级血浆的条件，例如次级颗粒的产生及其空间分布的多样性。我们的研究还可以进一步定量分析次级等离子体生成对所有参数的可能性，包括磁轴与旋转轴的倾斜角，极盖大小和磁场几何形状。
In this paper, which is the first in a series of papers devoted to a detailed analysis of the death line of radio pulsars, we consider a possibility of producing secondary particles at a sufficiently long pulsar period P. To this end, we reconsidered the potential drop necessary for secondary plasma generation in the inner gap over magnetic polar caps. Our research made it possible to refine the conditions for generating secondary plasma, such as the multiplicity of the production of secondary particles and their spatial distribution. Our research also made it possible to further quantitatively analyse the dependence of the possibility of secondary plasma generation on all parameters, including the inclination angle of the magnetic axis to the rotation axis, the polar cap size and the magnetic field geometry.
