论文标题
伽马射线脉冲星对距离的通量的依赖性：第二次费米目录中数据的非参数分析
Dependence of the flux of gamma-ray pulsars on distance: A nonparametric analysis of the data in the second FERMI catalogue
论文作者
论文摘要
脉冲星的伽马射线照明量被认为超过了其无线电亮度，但基于以下假设，即伽马射线脉冲脉冲距离衰减的假设像无线电脉冲的通量一样，遵守反平方向。但是，测试通过efron-petrosian统计数据测试仪表脉冲的独立性和距离脉冲脉冲的距离的结果，这意味着第二个{\ it fermi}目录中的观察数据与依赖性$ s \ s \ 3/2/3/3/2/3/3/3/3/3/3/3/3/fl fl fl fl fl fl fl fl fl flly pul s of s $ s y y fl fl fl fl fllas y s $ s in与依赖关系$ s \ propto d^{-2} $相比，其意义水平。这与能源保护的要求不兼容，因为Ardavan中描述的辐射过程[{\ it Mon。不是。 R. Astron。 soc。}，{\ bf 507}，4530--4563（2021）]，通过它，在中子恒星的磁层中，超值移动的电流表被证明可以产生观察到的伽玛 - 射线脉冲，这是固有的瞬时的脉冲：与这些螺态的范围内的范围内的跨度在跨越的范围内，这是跨度的范围，这些螺态均在范围内均匀地构成了跨度的范围，这是在这些范围内的范围，而在这些范围内，均在跨越的范围内，均在范围内均衡。球。一旦纠正了其值的过度估计，γ-射线脉冲星的亮度与无线电脉冲星的亮度相同的值范围。
Pulsars' gamma-ray luminosities are thought to exceed their radio luminosities by several orders of magnitude: a notion that is based on the assumption that the decay with distance of the flux of gamma-ray pulses obeys the inverse-square law as does that of the flux of radio pulses. However, results of testing the hypothesis of independence of luminosities and distances of gamma-ray pulsars by means of the Efron--Petrosian statistic imply that the observational data in the second {\it FERMI} catalogue are consistent with the dependence $S\propto D^{-3/2}$ of the flux densities $S$ of these pulsars on their distances $D$ at substantially higher levels of significance than they are with the dependence $S\propto D^{-2}$. This is not incompatible with the requirements of the conservation of energy because the radiation process described in Ardavan [{\it Mon. Not. R. Astron. Soc.}, {\bf 507}, 4530--4563 (2021)], by which the superluminally moving current sheet in the magnetosphere of a neutron star is shown to generate the observed gamma-ray pulses, is intrinsically transient: the difference in the fluxes of power across any two spheres centred on the star is balanced by the change with time of the energy contained inside the shell bounded by those spheres. Once the over-estimation of their values is rectified, the luminosities of gamma-ray pulsars turn out to have the same range of values as do the luminosities of radio pulsars.
