Feasibility of Probing Dark Energy with Strong Gravitational Lensing Systems. Fisher-Matrix Approach.
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- Yamamoto Kazuhiro
- Department of Physical Science, Hiroshima University, Higashi-Hiroshima 739-8526, Japan
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- Kadoya Yasufumi
- Department of Physical Science, Hiroshima University, Higashi-Hiroshima 739-8526, Japan
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- Murata Tsukasa
- Department of Physical Science, Hiroshima University, Higashi-Hiroshima 739-8526, Japan
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- Futamase Toshifumi
- Astronomical Institute, Graduate School of Science, Tohoku University, Sendai 980-8578, Japan
書誌事項
- タイトル別名
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- --- <i>Fisher-Matrix Approach</i> ---
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抄録
We assess the feasibility of probing dark energy with strong gravitational lensing systems. The capability of the method, which depends on the accuracy with which the lensing systems are modeled, is quantitatively investigated using the Fisher-matrix formalism. We show that this method might place useful constraints on the density parameter and the redshift evolution of the dark energy by combining it with a constraint from supernova measurements. For this purpose, the lens potential needs to be precisely reconstructed. We determine the required quality of data. We also briefly discuss the optimal strategy to constrain the cosmological parameters using gravitational lensing systems.
収録刊行物
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- Progress of Theoretical Physics
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Progress of Theoretical Physics 106 (5), 917-928, 2001
一般社団法人 日本物理学会
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詳細情報 詳細情報について
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- CRID
- 1390001204159292160
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- NII論文ID
- 110001200986
- 210000110832
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- NII書誌ID
- AA00791455
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- BIBCODE
- 2001PThPh.106..917Y
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- ISSN
- 13474081
- 0033068X
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- NDL書誌ID
- 5990515
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- 本文言語コード
- en
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- データソース種別
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- JaLC
- NDL
- Crossref
- CiNii Articles
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- 抄録ライセンスフラグ
- 使用不可