The BRAIN CMB polarization experiment

In the standard cosmological scenario tensor perturbations of the metric produce a rotational component in the Cosmic Microwave Background polarization, called B-modes. The expected signal is of the order of similar to 0.1 mu K, well beyond the sensitivity of current experiments. In this paper, we i...

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Bibliographic Details
Published in:New Astronomy Reviews
Main Authors: POLENTA, GIANLUCA, P. A. R. Ade, J. Bartlett, E. Breelle, CONVERSI, Luca, DE BERNARDIS, Paolo, C. Dufour, M. Gervasi, M. Giard, GIORDANO, CLAUDIA, Y. Giraud Heraud, B. Maffei, MASI, Silvia, NATI, FEDERICO, A. Orlando, S. Peterzen, PIACENTINI, Francesco, M. Piat, L. Piccirillo, PISANO, Giampaolo, R. Pons, C. Rosset, SAVINI, Giorgio, G. Sironi, A. Tartari, VENEZIANI, MARCELLA, M. Zannoni
Other Authors: Polenta, Gianluca, P. A. R., Ade, J., Bartlett, E., Breelle, Conversi, Luca, C., Dufour, M., Gervasi, M., Giard, Giordano, Claudia, Y., Giraud Heraud, B., Maffei, Masi, Silvia, Nati, Federico, A., Orlando, S., Peterzen, Piacentini, Francesco, M., Piat, L., Piccirillo, Pisano, Giampaolo, R., Pon, C., Rosset, Savini, Giorgio, G., Sironi, A., Tartari, Veneziani, Marcella, M., Zannoni
Format: Conference Object
Language:English
Published: ELSEVIER SCI LTD 2007
Subjects:
background radiation
cosmology
interferometry
polarimetry
Austral
Concordia Station
Antarc*
Antarctica
Online Access:http://hdl.handle.net/11573/358365
https://doi.org/10.1016/j.newar.2006.11.065
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