Chapter 2 Exploring the Components of the Universe Through Higher-Order Weak Lensing Statistics Higher-Order Weak Lensing Statistics
Our current cosmological model, backed by a large body of evidence from a variety of different cosmological probes (for example, see [1, 2]), describes a Universe comprised of around 5% normal baryonic matter, 22% cold dark matter and 73% dark energy. While many cosmologists accept this so-called...
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| Ētahi atu kaituhi: | , , , |
| Hōputu: | Tāhiko Wāhanga pukapuka |
| Reo: | Ingarihi |
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InTechOpen
2012
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| Ngā marau: | |
| Urunga tuihono: | OAPEN Library: download the publication OAPEN Library: description of the publication |
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OAPEN Library: download the publicationOAPEN Library: description of the publication
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| Tau karanga: |
A1234.567 |
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| Tārua 1 | Wātea |