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...

Полное описание

Библиографические подробности
Главные авторы: 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
Формат: Journal article
Опубликовано: 2009