Mountains on neutron stars

被引:2
|
作者
Haskell, B. [1 ]
机构
[1] Univ Southampton, Sch Math, Southampton SO17 1BJ, Hants, England
关键词
dense matter; stars neutron; EQUATION; STATE;
D O I
10.1007/s10509-007-9378-y
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The aim of this work is to compare a neutron star with an accreted crust and one with a non-accreted crust, and estimate which one is potentially a better source of gravitational waves (i.e. can sustain a larger "mountain"). To do this we present a new formalism, and find that a non-accreted crust can sustain a slightly larger "mountain". We also discuss the importance of relativistic effects.
引用
收藏
页码:541 / 543
页数:3
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