Cosmic structure sizes in generic dark energy models
Abstract The maximum allowable size of a spherical cosmic structure as a function of its mass is determined by the maximum turn around radius $$R_\mathrm{TA,max}$$ R TA , max , the distance from its center where the attraction on a radial test particle due to the spherical mass is balanced with the...
| Những tác giả chính: | , |
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| Định dạng: | Bài viết |
| Ngôn ngữ: | English |
| Được phát hành: |
SpringerOpen
2017-08-01
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| Loạt: | European Physical Journal C: Particles and Fields |
| Truy cập trực tuyến: | http://link.springer.com/article/10.1140/epjc/s10052-017-5102-4 |