Energy loss of supermassive magnetic monopoles and dyons in main sequence stars

被引：3
作者：
Ahlen, SP
De Mitri, I
Hong, JT
Tarle, G
机构：
[1] UNIV AQUILA, DIPARTIMENTO FIS, I-67100 LAQUILA, ITALY
[2] IST NAZL FIS NUCL, I-67100 LAQUILA, ITALY
[3] UNIV MICHIGAN, DEPT PHYS, ANN ARBOR, MI 48109 USA
来源：
PHYSICAL REVIEW D | 1997年 / 55卷 / 10期
关键词：
D O I：
10.1103/PhysRevD.55.6584
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We estimate the energy loss rate for a supermassive magnetic monopole or dyon in the interior of a main sequence star. For this purpose, the medium is shown to behave as a nondegenerate classical electron gas, the nuclear contribution to the stopping power being negligible. A linear dependence of the energy loss from the velocity of the particle is obtained. This result would provide a basic input to detailed calculations of the dynamics of monopoles and dyons in our galaxy.
引用
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页码：6584 / 6590
页数：7
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