## 抄録

Using a multiple lens-plane algorithm, we study light propagation in inhomogeneous universes, for 43 different COBE-normalized cold dark matter models, with various values of the density parameter Ω_{0}, cosmological constant λ_{0}, Rubble constant H_{0}, and rms density fluctuation σ_{8}. This is the largest cosmological parameter survey ever undertaken in this field. We performed a total of 3798 experiments, each experiment consisting of propagating a square beam of angular size 21″.9 × 21″.9 composed of 116,281 light rays from the observer up to redshift z = 3. These experiments provide statistics of the magnification, shear, and multiple imaging of distant sources. The results of these experiments can be compared with observations and eventually help to constrain the possible values of the cosmological parameters. In addition, they provide insight into the gravitational lensing process and its complex relationship with the various cosmological parameters. Our main results are the following: (1) The magnification distribution depends mostly upon λ_{0} and σ_{8}. As σ_{8} increases, the low tail of the magnification distribution shifts toward lower magnifications, while the high tail is hardly affected. The magnification distribution also becomes wider as λ_{0} increases. This effect is particularly large for models with λ_{0} = 0.8. (2) The magnification probability P_{m} is almost independent of σ_{8}, for any combination of Ω_{0}, λ_{0}, and H_{0}, indicating that P_{m} does not depend strongly upon the amount of large-scale structure. (3) The shear distribution, like the magnification distribution, depends mostly upon λ_{0} and σ_{8}. The shear distribution becomes wider with increasing σ_{8} and increasing λ_{0}. The similarities between the properties of the magnification and shear distributions suggest that both phenomena are caused by weak lensing. (4) About 0.3% of sources have multiple images. The double-image probability P_{2} increases strongly with λ_{0} and is independent of Ω_{0}, H_{0}, and σ_{8}. (5) The distribution of image separations depends strongly upon λ_{0} and is independent of σ_{8}. Summarizing these results, we find that (a) The properties of gravitational lensing, both weak and strong, depend much more strongly upon λ_{0} than any other cosmological parameter, and (b) magnification and shear are examples of weak lensing caused primarily by the distribution of background matter, with negligible contribution from galaxies, while multiple images and rings are examples of strong lensing, caused by direct interaction with galaxies, with negligible contribution from the background matter. Observations of weak lensing can be used to determine the cosmological constant and the density structure of the universe, while observations of strong lensing can be used to determine the cosmological constant and the internal structure of galaxies and clusters. Gravitational lensing depends much more weakly upon Ω_{0} and H_{0} than σ_{8} and λ_{0}, making a determination of these parameters from observations more difficult.

本文言語 | English |
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ページ（範囲） | 7-39 |

ページ数 | 33 |

ジャーナル | Astrophysical Journal, Supplement Series |

巻 | 135 |

号 | 1 |

DOI | |

出版ステータス | Published - 2001 7 |

外部発表 | はい |

## ASJC Scopus subject areas

- 天文学と天体物理学
- 宇宙惑星科学