中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Rotation in gravitational lenses

文献类型:期刊论文

作者Pen, UL; Mao, SD
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2006-04-21
卷号367期号:4页码:1543-1550
关键词gravitational lensing galaxies : evolution galaxies : structure cosmology : theory dark matter
英文摘要Gravitational lensing deflects light. A single lens deflector can only shear images, but cannot induce rotations. Multiple lens planes can induce rotations. Such rotations can be observed in quadruply imaged sources, and can be used to distinguish between two proposed solutions of the flux anomaly problem: substructures in lensing galaxies versus large-scale structure. We predict the expected amount of rotation due to large-scale structure in strong lensing systems, and show how this effect can be measured using similar to mas very long baseline interferometry astrometry of quadruple lenses with extended source structures. The magnitude of rotation is around 1 degrees. The biggest theoretical uncertainty is the power spectrum of dark matter on very small scales. This procedure can potentially be turned around to measure the dark matter power spectrum on very small scales. We list the predicted rms rotation angles for several quadruple lenses with known lens and source redshifts.
收录类别SCI
语种英语
WOS记录号WOS:000236606400017
源URL[http://ir.bao.ac.cn/handle/114a11/7143]  
专题国家天文台_星系宇宙学研究部
作者单位1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada
3.Univ Manchester, Jodrell Bank Observ, Macclesfield SK11 9DL, Cheshire, England
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GB/T 7714
Pen, UL,Mao, SD. Rotation in gravitational lenses[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2006,367(4):1543-1550.
APA Pen, UL,&Mao, SD.(2006).Rotation in gravitational lenses.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,367(4),1543-1550.
MLA Pen, UL,et al."Rotation in gravitational lenses".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 367.4(2006):1543-1550.

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来源:国家天文台

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