Observing the Evolution of the Universe

How did the universe evolve? The fine angular scale (l>1000) temperature and polarization anisotropies in the CMB are a Rosetta stone for understanding the evolution of the universe. Through detailed measurements one may address everything from the physics of the birth of the universe to the...

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Detaylı Bibliyografya
Asıl Yazarlar: Aguirre, J, Amblard, A, Ashoorioon, A, Baccigalupi, C, Balbi, A, Bartlett, J, Bartolo, N, Benford, D, Birkinshaw, M, Bock, J, Bond, D, Borrill, J, Bouchet, F, Bridges, M, Bunn, E, Calabrese, E, Cantalupo, C, Caramete, A, Carbone, C, Chatterjee, S, Church, S, Chuss, D, Contaldi, C, Cooray, A, Das, S
Materyal Türü: Journal article
Baskı/Yayın Bilgisi: 2009