LEADER 04029nam  22006735  450 
001 9910300378203321
005 20200702104743.0
010   $a3-319-07746-5
024 7 $a10.1007/978-3-319-07746-8
035   $a(CKB)3710000000129275
035   $a(EBL)1783852
035   $a(SSID)ssj0001276369
035   $a(PQKBManifestationID)11709665
035   $a(PQKBTitleCode)TC0001276369
035   $a(PQKBWorkID)11239731
035   $a(PQKB)10116128
035   $a(MiAaPQ)EBC1783852
035   $a(DE-He213)978-3-319-07746-8
035   $a(PPN)179768220
035   $a(EXLCZ)993710000000129275
100   $a20140613d2014      u|             0
101 0 $aeng
135   $aur|n|---|||||
181   $ctxt
182   $cc
183   $acr
200 14$aThe Large Scale Structures$b[electronic resource] $eA Window on the Dark Components of the Universe /$fby Stéphane Ili?
205   $a1st ed. 2014.
210  1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2014.
215   $a1 online resource (154 p.)
225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053
300   $a"Doctoral Thesis accepted by the University of Paris-Sud, Orsay Cedex, France"--T.p.
311   $a1-322-13691-2 
311   $a3-319-07745-7 
320   $aIncludes bibliographical references.
327   $aIntroduction: The Ingredients of a Good Cosmological Probe -- Unravelling the iSW Effect Through the Matter Distribution -- The Impact of Identified Superstructures in the CMB -- Towards a Full Modelling of the iSW effect -- Studying Dark Matter Through the Lens of Reionization -- Conclusions & Perspectives.
330   $aDark Energy and Dark Matter are among the greatest mysteries in modern cosmology. The present work explores in depth how large cosmic structures can help us unveil the nature of these components of the Universe. One the one hand, it focuses on a signature that Dark Energy imprints on the Cosmic Microwave Background through its impact on the time-evolution of gravitational potentials: the integrated Sachs-Wolfe (iSW) effect. Another cosmological background, the Cosmic Infrared Background, is considered for the first time in the study of the iSW effect and demonstrated to be a highly efficient and promising tracer. Changing the perspective on the problem, the use of superstructures for iSW detection is then extensively reviewed: using precise solutions to Einstein?s general relativity equations, the full iSW effect is computed, especially due to the cosmic voids predicted by the theory. Using measurements from the most recent data, it is subsequently shown how the iSW probes the solidity of the cosmological standard model. On the topic of Dark Matter, an original study is presented, showing that temperature measurements of the intergalactic medium shed light on the nature of Dark Matter particles, providing the tightest constraints on their decay properties.
410  0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053
606   $aCosmology
606   $aGravitation
606   $aNuclear physics
606   $aCosmology$3https://scigraph.springernature.com/ontologies/product-market-codes/P22049
606   $aClassical and Quantum Gravitation, Relativity Theory$3https://scigraph.springernature.com/ontologies/product-market-codes/P19070
606   $aParticle and Nuclear Physics$3https://scigraph.springernature.com/ontologies/product-market-codes/P23002
615  0$aCosmology.
615  0$aGravitation.
615  0$aNuclear physics.
615 14$aCosmology.
615 24$aClassical and Quantum Gravitation, Relativity Theory.
615 24$aParticle and Nuclear Physics.
676   $a523.1126
700   $aIli?$b Stéphane$4aut$4http://id.loc.gov/vocabulary/relators/aut$0791865
801  0$bMiAaPQ
801  1$bMiAaPQ
801  2$bMiAaPQ
906   $aBOOK
912   $a9910300378203321
996   $aThe Large Scale Structures$92530444
997   $aUNINA