SGRs and AXPs as white dwarf pulsars

被引：3

作者：

Coelho, J. G. ^{[1
]}

Malheiro, M. ^{[1
]}

机构：

[1] ITA, Dept Fis, BR-12228900 Sao Jose Dos Campos, SP, Brazil

来源：

XII HADRON PHYSICS | 2013年 / 1520卷

关键词：

SGRs/AXPs; white dwarf; neutron stars; MAGNETIZED NEUTRON-STARS; X-RAY; REPEATERS;

D O I：

10.1063/1.4795967

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

Recently, a new view of SGRs/AXPs expressed in terms of massive highly magnetized rotating white dwarfs (WDs) in total analogy with the case of pulsars originating their energy from the rotational energy of the neutron stars has been presented. Furthermore, we present the recent discoveries of two SGRs with low magnetic field sharing some properties with the recent detected fast WD pulsar AE Aquarii, to support the description of SGRs/AXPs as white dwarf pulsar. In order to test this new view, we present several properties of these SGRs/AXPs as WD pulsar, in particular the X-ray luminosity and surface dipole magnetic field.

引用

页码：258 / 263

页数：6

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