A new death line for radio pulsars is presented in this paper within the framework of vacuum gap and inverse Compton scattering (ICS) induced pair production process. The 8.5s period pulsar PSR J2144-3933 is located above the death line without any additional assumptions. An "appearance line" instead of the so-called "Hubble line", is also presented in this paper. Both of those two lines fit observations well.
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Aix Marseille Univ, CNRS, UMR 6242, FST St Jerome,IM2NP, F-13397 Marseille, FranceAix Marseille Univ, CNRS, UMR 6242, FST St Jerome,IM2NP, F-13397 Marseille, France
Berche, Alexandre
Benigni, Pierre
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Aix Marseille Univ, CNRS, UMR 6242, FST St Jerome,IM2NP, F-13397 Marseille, FranceAix Marseille Univ, CNRS, UMR 6242, FST St Jerome,IM2NP, F-13397 Marseille, France
Benigni, Pierre
Rogez, Jacques
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Aix Marseille Univ, CNRS, UMR 6242, FST St Jerome,IM2NP, F-13397 Marseille, FranceAix Marseille Univ, CNRS, UMR 6242, FST St Jerome,IM2NP, F-13397 Marseille, France
Rogez, Jacques
Record, Marie-Christine
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Aix Marseille Univ, CNRS, UMR 6242, FST St Jerome,IM2NP, F-13397 Marseille, FranceAix Marseille Univ, CNRS, UMR 6242, FST St Jerome,IM2NP, F-13397 Marseille, France