In usual statistical analyses,because of diversities of proper parameters of pulsars,some interesting features might be smeared.In order to remove these diversities,we use the mean values for all quantities of pulsars...In usual statistical analyses,because of diversities of proper parameters of pulsars,some interesting features might be smeared.In order to remove these diversities,we use the mean values for all quantities of pulsars,instead of values of individual one to do statistical analyses.Logp/p3-logτand LogL-logτhave been plotted.The most interesting feature is that the radio luminosity of pulsar evidently appears to regrow up after its initial dropping.This feature is difficult to understand in usual models.Two tentatlive interpretations have been given.展开更多
Neutrinos are rather abundant in the universe, nearly as abundant as photons. The non-vanishing of neutrino’s rest mass should certainly induce many interesting astrophysical effects. in this paper, we shall discuss ...Neutrinos are rather abundant in the universe, nearly as abundant as photons. The non-vanishing of neutrino’s rest mass should certainly induce many interesting astrophysical effects. in this paper, we shall discuss mainly the influence of massive neutrinos on the clustering phenomena in the universe.展开更多
文摘In usual statistical analyses,because of diversities of proper parameters of pulsars,some interesting features might be smeared.In order to remove these diversities,we use the mean values for all quantities of pulsars,instead of values of individual one to do statistical analyses.Logp/p3-logτand LogL-logτhave been plotted.The most interesting feature is that the radio luminosity of pulsar evidently appears to regrow up after its initial dropping.This feature is difficult to understand in usual models.Two tentatlive interpretations have been given.
文摘Neutrinos are rather abundant in the universe, nearly as abundant as photons. The non-vanishing of neutrino’s rest mass should certainly induce many interesting astrophysical effects. in this paper, we shall discuss mainly the influence of massive neutrinos on the clustering phenomena in the universe.
