Compact dark matter objects, asteroseismology, and gravitational waves radiated by sun

被引：0
|
作者：
Yu. E. Pokrovsky
机构：
[1] National Research Center Kurchatov Institute,
来源：
Physics of Atomic Nuclei | 2015年 / 78卷
关键词：
dark matter; gravitational waves; solar structure; asteroseismology;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
The solar surface oscillations observed by Crimean Astrophysical Observatory and Solar Helioseismic Observatory are considered to be excited by a small fraction of Dark Matter in form of Compact Dark Matter Objects (CDMO) in the solar structure. Gravitational Waves (GW) radiated by these CDMO are predicted to be the strongest at the Earth and are easily detectable by European Laser Interferometer Space Antenna or by Gravitational-Wave Observatory “Dulkyn” which can solve two the most challenging tasks in the modern physics: direct detection of GW and DM.
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页码：1523 / 1527
页数：4
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