Pulsar radio emission mechanism: Why no consensus?

被引:11
|
作者
Melrose, D. B. [1 ]
Rafat, M. Z. [1 ]
机构
[1] Univ Sydney, Sch Phys, SIfA, Sydney, NSW 2006, Australia
来源
INTERNATIONAL CONFERENCE PHYSICS OF NEUTRON STARS: 50 YEARS AFTER, 2017 | 2017年 / 932卷
关键词
POLAR-CAP CASCADE; LARGE-AMPLITUDE; PAIR PLASMA; MAGNETOSPHERES; INSTABILITY; DISPERSION; CONVERSION; RADIATION;
D O I
10.1088/1742-6596/932/1/012011
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Pulsar radio emission involves a coherent emission mechanism involving relativistic particles, but there is no consensus on what the specific emission mechanism is. There are arguments for and against several suggested mechanisms of long-standing, including two, relativistic plasma emission and anomalous Doppler emission, that depend explicitly on the dispersive properties of waves in a pulsar plasma. Models that do not include dispersion due to the relativistic spread in energy of the plasma particles can be misleading, and including the effects of this spread on the wave dispersion leads to severe constraints on these two suggested mechanisms. It is argued that all suggested mechanisms are implausible. A variant of relativistic plasma emission involving large-amplitude oscillations needs to be explored as a possible alternative.
引用
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页数:7
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