arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 2011.13833gr-qcastro-ph.EPastro-ph.HEastro-ph.IMhep-ph
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来自小行星的重力梯度噪声

Gravity Gradient Noise from Asteroids

Michael A. Fedderke, Peter W. Graham, Surjeet Rajendran

摘要:

在引力波(GW)探测器中,附近大质量物体与测试质量的引力耦合不能被屏蔽,从而在探测器中产生“引力梯度噪声”(GGN)。在本文中,我们表明,对于任何GW检测器使用本地测试质量的内太阳系,从$\sim 10^5$内太阳系小行星的运动场的GGN提出了一个不可约的噪声地板GW的检测,在低频率呈指数上升。这严重限制了使用频率为$f_{\text{GW}} \lesssim (\text{few})\times 10^{-7}\,$ Hz的本地测试质量进行GW检测的前景。在更高的频率,我们发现小行星GGN下降足够快,检测可能是可能的;然而,现有的小行星目录的不完整性方面的小天体,使这是一个悬而未决的问题,围绕$f_{\text{GW}}\sim μ$赫兹,进一步的研究是必要的。我们表明,放置在外太阳系的探测器网络不会被这种噪音超过$\sim 10\,$ nHz,并提出意见的替代方法,可以克服本地测试群众GW检测在$\sim 10\,$ nHz- $μ$ Hz波段的限制。

英文摘要:

The gravitational coupling of nearby massive bodies to test masses in a gravitational wave (GW) detector cannot be shielded, and gives rise to 'gravity gradient noise' (GGN) in the detector. In this paper we show that for any GW detector using local test masses in the Inner Solar System, the GGN from the motion of the field of $\sim 10^5$ Inner Solar System asteroids presents an irreducible noise floor for the detection of GW that rises exponentially at low frequencies. This severely limits prospects for GW detection using local test masses for frequencies $f_{\text{GW}} \lesssim (\text{few})\times 10^{-7}\,$Hz. At higher frequencies, we find that the asteroid GGN falls rapidly enough that detection may be possible; however, the incompleteness of existing asteroid catalogs with regard to small bodies makes this an open question around $f_{\text{GW}}\sim μ$Hz, and further study is warranted. We show that a detector network placed in the Outer Solar System would not be overwhelmed by this noise above $\sim 10\,$nHz, and make comments on alternative approaches that could overcome the limitations of local test masses for GW detection in the $\sim 10\,$nHz-$μ$Hz band.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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