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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| Aineistotyyppi: | Elektroninen Kirjan osa |
| Kieli: | englanti |
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InTechOpen
2012
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| Linkit: | OAPEN Library: download the publication OAPEN Library: description of the publication |
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Internet
OAPEN Library: download the publicationOAPEN Library: description of the publication
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| Nide 1 | Saatavissa |