TY  - CHAP
AU  - Dupé, François-Xavier
AU  - Pires, Sandrine
AU  - Starck, Jean-Luc
AU  - Leonard, Adrienne
AU  - Leonard, Adrienne
AU  - Starck, Jean-Luc
AU  - Pires, Sandrine
AU  - Dupé, Franois-Xavier
AB  - 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.
DO  - 10.5772/51871
ID  - OAPEN ID: 612591
ID  - OAPEN ID: OCN: 1030818880
KW  - statistics
KW  - exploring
KW  - universe
KW  - statistics
KW  - exploring
KW  - universe
KW  - Algorithm
KW  - Cross-correlation matrix
KW  - Discrete wavelet transform
KW  - Higher-order statistics
KW  - Physical cosmology
KW  - Redshift
KW  - Wavelet
KW  - Weak gravitational lensing
L1  - https://library.oapen.org/bitstream/id/086eede9-d255-435e-8002-c6ad11421ffb/612591.pdf
LA  - English
LK  - http://library.oapen.org/handle/20.500.12657/32344
PB  - InTechOpen
PY  - 2012
TI  - Chapter 2 Exploring the Components of the Universe Through Higher-Order Weak Lensing Statistics  Higher-Order Weak Lensing Statisticsnull
ER  - 
