Strong gravitational lensing constraints on holographic dark energy
Strong gravitational lensing （SGL） has provided an important tool for probing galaxies and cosmology. In this paper, we use the SGL data to constrain the holographic dark energy model, as well as models that have the same parameter number, such as the wCDM and Ricci dark energy models. We find that...
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| Published in | Science China. Physics, mechanics & astronomy Vol. 58; no. 11; pp. 68 - 74 |
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| Main Authors | , , , |
| Format | Journal Article |
| Language | English |
| Published |
Beijing
Science China Press
01.11.2015
Springer Nature B.V |
| Subjects | |
| Online Access | Get full text |
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| Abstract | Strong gravitational lensing （SGL） has provided an important tool for probing galaxies and cosmology. In this paper, we use the SGL data to constrain the holographic dark energy model, as well as models that have the same parameter number, such as the wCDM and Ricci dark energy models. We find that only using SGL is difficult to effectively constrain the model parameters. However, when the SGL data are combined with CBS （CMB＋BAO＋SN） data, the reasonable estimations can be given and the constraint precision is improved to a certain extent, relative to the case of CBS only. Therefore, SGL is an useful way to tighten constraints on model parameters. |
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| AbstractList | Strong gravitational lensing (SGL) has provided an important tool for probing galaxies and cosmology. In this paper, we use the SGL data to constrain the holographic dark energy model, as well as models that have the same parameter number, such as the wCDM and Ricci dark energy models. We find that only using SGL is difficult to effectively constrain the model parameters. However, when the SGL data are combined with CBS (CMB+BAO+SN) data, the reasonable estimations can be given and the constraint precision is improved to a certain extent, relative to the case of CBS only. Therefore, SGL is an useful way to tighten constraints on model parameters. Strong gravitational lensing (SGL) has provided an important tool for probing galaxies and cosmology. In this paper, we use the SGL data to constrain the holographic dark energy model, as well as models that have the same parameter number, such as the w CDM and Ricci dark energy models. We find that only using SGL is difficult to effectively constrain the model parameters. However, when the SGL data are combined with CBS (CMB+BAO+SN) data, the reasonable estimations can be given and the constraint precision is improved to a certain extent, relative to the case of CBS only. Therefore, SGL is an useful way to tighten constraints on model parameters. Strong gravitational lensing （SGL） has provided an important tool for probing galaxies and cosmology. In this paper, we use the SGL data to constrain the holographic dark energy model, as well as models that have the same parameter number, such as the wCDM and Ricci dark energy models. We find that only using SGL is difficult to effectively constrain the model parameters. However, when the SGL data are combined with CBS （CMB＋BAO＋SN） data, the reasonable estimations can be given and the constraint precision is improved to a certain extent, relative to the case of CBS only. Therefore, SGL is an useful way to tighten constraints on model parameters. |
| ArticleNumber | 110402 |
| Author | CUIJingLei XUYueYao ZHANGJingFei ZHANGXin |
| AuthorAffiliation | DepartmentofPhysics,CollegeofSciences,NortheasternUniversity,Shenyang110819,China CenterforHighEnergyPhysics,PekingUniversity,Beijing100080,China |
| Author_xml | – sequence: 1 givenname: JingLei surname: Cui fullname: Cui, JingLei organization: Department of Physics, College of Sciences, Northeastern University – sequence: 2 givenname: YueYao surname: Xu fullname: Xu, YueYao organization: Department of Physics, College of Sciences, Northeastern University – sequence: 3 givenname: JingFei surname: Zhang fullname: Zhang, JingFei organization: Department of Physics, College of Sciences, Northeastern University – sequence: 4 givenname: Xin surname: Zhang fullname: Zhang, Xin email: zhangxin@mail.neu.edu.cn organization: Department of Physics, College of Sciences, Northeastern University, Center for High Energy Physics, Peking University |
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| Keywords | cosmological constraints strong gravitational lensing holographic dark energy |
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| Notes | Strong gravitational lensing （SGL） has provided an important tool for probing galaxies and cosmology. In this paper, we use the SGL data to constrain the holographic dark energy model, as well as models that have the same parameter number, such as the wCDM and Ricci dark energy models. We find that only using SGL is difficult to effectively constrain the model parameters. However, when the SGL data are combined with CBS （CMB＋BAO＋SN） data, the reasonable estimations can be given and the constraint precision is improved to a certain extent, relative to the case of CBS only. Therefore, SGL is an useful way to tighten constraints on model parameters. cosmological constraints, strong gravitational lensing, holographic dark energy 11-5849/N |
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| Publisher | Science China Press Springer Nature B.V |
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| Snippet | Strong gravitational lensing （SGL） has provided an important tool for probing galaxies and cosmology. In this paper, we use the SGL data to constrain the... Strong gravitational lensing (SGL) has provided an important tool for probing galaxies and cosmology. In this paper, we use the SGL data to constrain the... |
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| SubjectTerms | Astronomy Classical and Continuum Physics Constraint modelling Dark energy Galaxies Gravitational lenses Holography Observations and Techniques Parameters Physics Physics and Astronomy 力学 天文学 物理学 科学学 科学知识 |
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| Title | Strong gravitational lensing constraints on holographic dark energy |
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