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...
Main Authors: | 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 |
---|---|
Format: | Journal article |
Published: |
2009
|
Similar Items
-
The Origin of the Universe as Revealed Through the Polarization of the
Cosmic Microwave Background
by: Dodelson, S, et al.
Published: (2009) -
Prospects for polarized foreground removal
by: Dunkley, J, et al.
Published: (2009) -
Planck Intermediate Results. IV. The XMM-Newton validation programme for
new Planck galaxy clusters
by: Collaboration, P, et al.
Published: (2012) -
Planck intermediate results. XIII. Constraints on peculiar velocities
by: Collaboration, P, et al.
Published: (2013) -
Planck intermediate results. VI: The dynamical structure of
PLCKG214.6+37.0, a Planck discovered triple system of galaxy clusters
by: Collaboration, P, et al.
Published: (2012)