612591.pdf

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-cal...

Πλήρης περιγραφή

Λεπτομέρειες βιβλιογραφικής εγγραφής
Γλώσσα:English
Έκδοση: InTechOpen 2019
id oapen-20.500.12657-32344
record_format dspace
spelling oapen-20.500.12657-323442021-11-12T16:21:42Z Chapter 2 Exploring the Components of the Universe Through Higher-Order Weak Lensing Statistics Higher-Order Weak Lensing Statistics Dupé, François-Xavier Pires, Sandrine Starck, Jean-Luc Leonard, Adrienne Leonard, Adrienne Starck, Jean-Luc Pires, Sandrine Dupé, Franois-Xavier statistics exploring universe statistics exploring universe Algorithm Cross-correlation matrix Discrete wavelet transform Higher-order statistics Physical cosmology Redshift Wavelet Weak gravitational lensing bic Book Industry Communication::P Mathematics & science::PD Science: general issues 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 concordance cosmology – the ΛCDM cosmological model – as accurate, very little is known about the nature and properties of these dark components of the Universe. Studies of the cosmic microwave background (CMB), combined with other observational evidence of big bang nucleosynthesis indicate that dark matter is non-baryonic. This supports measurements on galaxy and cluster scales, which found evidence of a large proportion of dark matter. This dark matter appears to be cold and collisionless, apparent only through its gravitational effects. 2019-10-04 14:29:00 2020-04-01T14:06:58Z 2016-08-01 23:55 2019-10-04 14:29:00 2020-04-01T14:06:58Z 2016-12-31 23:55:55 2019-10-04 14:29:00 2020-04-01T14:06:58Z 2020-04-01T14:06:58Z 2012 chapter 612591 OCN: 1030818880 http://library.oapen.org/handle/20.500.12657/32344 eng application/pdf n/a 612591.pdf InTechOpen Open Questions in Cosmology 10.5772/51871 10.5772/51871 09f6769d-48ed-467d-b150-4cf2680656a1 5d588364-6507-4874-ae75-99773e51d619 7292b17b-f01a-4016-94d3-d7fb5ef9fb79 European Research Council (ERC) 1 228261 FP7 FP7 Ideas: European Research Council FP7-IDEAS-ERC - Specific Programme: "Ideas" Implementing the Seventh Framework Programme of the European Community for Research, Technological Development and Demonstration Activities (2007 to 2013) open access
institution OAPEN
collection DSpace
language English
description 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 concordance cosmology – the ΛCDM cosmological model – as accurate, very little is known about the nature and properties of these dark components of the Universe. Studies of the cosmic microwave background (CMB), combined with other observational evidence of big bang nucleosynthesis indicate that dark matter is non-baryonic. This supports measurements on galaxy and cluster scales, which found evidence of a large proportion of dark matter. This dark matter appears to be cold and collisionless, apparent only through its gravitational effects.
title 612591.pdf
spellingShingle 612591.pdf
title_short 612591.pdf
title_full 612591.pdf
title_fullStr 612591.pdf
title_full_unstemmed 612591.pdf
title_sort 612591.pdf
publisher InTechOpen
publishDate 2019
_version_ 1771297586719752192