A Model for Period Clustering of Long-Period Pulsars(Astrophysics and Relativity)

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概要

• 論文の詳細を見る

• We explore the possibility that the P - P^^・ distribution of observed pulsars can be understood in terms of a model of a rotating neutron star that possesses two types of magnetic fields, a fossil magnetic field of O(10^<10-13>) G at the stellar surface, and the field due to the ferromagnetic core of a neutron star, which is assumed to be of O(10^<14-15>) G. This model, when combined with the assumption of an appropriate mass distribution, together with the observational selection effect on an assumed magnetic dipole pulse luminosity proportional to P^<-4>, is shown to be consistent with the 'period clustering' of the observed SGRs and AXPs.

• 理論物理学刊行会の論文
• 2003-07-25

著者

• TAKAHASHI Keitaro

  Department of Physics, School of Science, University of Tokyo

• Takahashi Keitaro

  Department Of Physics University Of Tokyo

• Takahashi K

  Department Of Energy & Safety Engineering Yokohama National University

• Takahashi Koichi

  Department Of Biology Faculty Of Science Shinshu University

• Takahashi Koichi

  Department Of Liberal Arts Tohoku Gakuin University

• TAKAHASHI Koichi

  Department of Liberal Arts, Tohoku Gakuin University

• TAKAHASHI Koichi

  Physics Department, Faculty of Science Tohoku University

• TAKAHASHI Koichi

  College of Liberal Arts, Tohoku Gakuin University

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