研究了红移简并和粘性介质的阻尼效应对引力波信号信息提取的影响

Shou-Li Ning, Lixin Xu
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引用次数: 0

摘要

考虑到宇宙学红移$z_c$,从GW信号中提取的GW源质量为其本征值的$1+z_c$的1倍,将探测器与GW源之间的距离作为光度距离。然而,在对GW数据的分析中,除了宇宙学红移之外,还有其他类型的红移需要考虑,但实际上被忽略了,如多普勒红移和引力红移,因此从GW中提取的参数可能会偏离其固有值。影响GW的另一个因素是GW传播路径中的粘性介质,其阻尼率为$16{\pi}G{\eta}$。一些研究表明暗物质可能相互作用,因此暗物质可能是宇宙介质粘度的起源。然后,GW可能会被由暗物质构成的粘性介质迅速阻尼,例如暗物质在中等质量黑洞周围的“小尖峰”。本文主要讨论了多普勒和引力红移以及粘性介质的阻尼效应如何影响从GW信号中提取的GW源质量和红移等信息。
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The effect of redshift degeneracy and the damping effect of viscous medium on the information extracted from gravitational wave signals
Considering the cosmological redshift $z_c$ , the mass of GW source extracted from GW signal is $1+z_c$ times larger than its intrinsic value, and distance between detector and GW source should be regarded as luminosity distance. However, besides cosmological redshift, there are other kinds of redshifts should be considered, which is actually ignored, in the analysis of GW data, such as Doppler redshift and gravitational redshift, so the parameters extracted from GW may deviate from their intrinsic values. Another factor that may affect GW is the viscous medium in propagation path of GW, which may damp the GW with a damping rate of $16{\pi}G{\eta}$. Some studies indicate dark matter may interact with each other, thus dark matter may be the origin of viscosity of cosmic medium. Then the GW may be rapidly damped by the viscous medium that is made of dark matter, such as dark matter "mini-spike" around intermediate mass black hole. In this article, we mainly discuss how Doppler and gravitational redshift, together with the damping effect of viscous medium, affect the informations, such as the mass and redshift of GW source, extracted from GW signals.
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