Precision CMB polarization from Dome-c: The brain experiment

S. Masi; P. De Bernardis; C. Giordano; F. Nati; F. Piacentini; G. Polenta; M. Veneziani; M. Gervasi; G. Sironi; A. Tartari; M. Zannoni; S. Peterzen; J. Bartlett; Y. Giraud-Heraud; M. Piat; C. Rosset; M. Giard; R. Pons; B. Maffei; P. Ade; W. Gear; P. Mauskopf; L. Piccirillo; G. Pisano; G. Savini

doi:10.1051/eas:2005014

Precision CMB polarization from Dome-c: The brain experiment

S. Masi, P. De Bernardis, C. Giordano, F. Nati, F. Piacentini, G. Polenta, M. Veneziani, M. Gervasi, G. Sironi, A. Tartari, M. Zannoni, S. Peterzen, J. Bartlett, Y. Giraud-Heraud, M. Piat, C. Rosset, M. Giard, R. Pons, B. Maffei, P. AdeW. Gear, P. Mauskopf, L. Piccirillo, G. Pisano, G. Savini

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

9 Scopus citations

Abstract

In the current cosmological scenario, part of the linearly polarized emission of the CMB is expected to be rotational (B-modes). This component is due to tensor perturbations of the metric produced by primordial gravitational waves, which are generated a split-second after the Big Bang. The signal expected is of the order of ≳0.1 μK, well below the non-rotational component of the polarization signal (E-modes), and beyond the sensitivity of present generation instruments. New, more sensitive instruments are developed in several labs, with the goal to measure the B-modes. Control of systematics and foregrounds will be the key to make the results of these experiments believable. In this paper we shortly outline BRAIN, a bolometric interferometer devoted to B-modes research, and its pathfinder experiment, devoted to test the Dome-C site.

Original language	English (US)
Title of host publication	Proceedings - CIS Workshops 2007, 2007 International Conference on Computational Intelligence and Security Workshops, CISW 2007
Pages	87-92
Number of pages	6
DOIs	https://doi.org/10.1051/eas:2005014
State	Published - 2005
Externally published	Yes
Event	Dome C Astronomy and Astrophysics Meeting - Toulouse, France Duration: Jun 28 2004 → Jun 30 2004

Publication series

Name	EAS Publications Series
Volume	14
ISSN (Print)	1633-4760
ISSN (Electronic)	1638-1963

Other

Other	Dome C Astronomy and Astrophysics Meeting
Country/Territory	France
City	Toulouse
Period	6/28/04 → 6/30/04

ASJC Scopus subject areas

Astronomy and Astrophysics
Engineering(all)
Space and Planetary Science

Access to Document

10.1051/eas:2005014

Cite this

Masi, S., De Bernardis, P., Giordano, C., Nati, F., Piacentini, F., Polenta, G., Veneziani, M., Gervasi, M., Sironi, G., Tartari, A., Zannoni, M., Peterzen, S., Bartlett, J., Giraud-Heraud, Y., Piat, M., Rosset, C., Giard, M., Pons, R., Maffei, B., ... Savini, G. (2005). Precision CMB polarization from Dome-c: The brain experiment. In Proceedings - CIS Workshops 2007, 2007 International Conference on Computational Intelligence and Security Workshops, CISW 2007 (pp. 87-92). (EAS Publications Series; Vol. 14). https://doi.org/10.1051/eas:2005014

Precision CMB polarization from Dome-c : The brain experiment. / Masi, S.; De Bernardis, P.; Giordano, C. et al.

Proceedings - CIS Workshops 2007, 2007 International Conference on Computational Intelligence and Security Workshops, CISW 2007. 2005. p. 87-92 (EAS Publications Series; Vol. 14).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Masi, S, De Bernardis, P, Giordano, C, Nati, F, Piacentini, F, Polenta, G, Veneziani, M, Gervasi, M, Sironi, G, Tartari, A, Zannoni, M, Peterzen, S, Bartlett, J, Giraud-Heraud, Y, Piat, M, Rosset, C, Giard, M, Pons, R, Maffei, B, Ade, P, Gear, W, Mauskopf, P, Piccirillo, L, Pisano, G & Savini, G 2005, Precision CMB polarization from Dome-c: The brain experiment. in Proceedings - CIS Workshops 2007, 2007 International Conference on Computational Intelligence and Security Workshops, CISW 2007. EAS Publications Series, vol. 14, pp. 87-92, Dome C Astronomy and Astrophysics Meeting, Toulouse, France, 6/28/04. https://doi.org/10.1051/eas:2005014

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abstract = "In the current cosmological scenario, part of the linearly polarized emission of the CMB is expected to be rotational (B-modes). This component is due to tensor perturbations of the metric produced by primordial gravitational waves, which are generated a split-second after the Big Bang. The signal expected is of the order of ≳0.1 μK, well below the non-rotational component of the polarization signal (E-modes), and beyond the sensitivity of present generation instruments. New, more sensitive instruments are developed in several labs, with the goal to measure the B-modes. Control of systematics and foregrounds will be the key to make the results of these experiments believable. In this paper we shortly outline BRAIN, a bolometric interferometer devoted to B-modes research, and its pathfinder experiment, devoted to test the Dome-C site.",

author = "S. Masi and {De Bernardis}, P. and C. Giordano and F. Nati and F. Piacentini and G. Polenta and M. Veneziani and M. Gervasi and G. Sironi and A. Tartari and M. Zannoni and S. Peterzen and J. Bartlett and Y. Giraud-Heraud and M. Piat and C. Rosset and M. Giard and R. Pons and B. Maffei and P. Ade and W. Gear and P. Mauskopf and L. Piccirillo and G. Pisano and G. Savini",

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AU - Nati, F.

AU - Piacentini, F.

AU - Polenta, G.

AU - Veneziani, M.

AU - Gervasi, M.

AU - Sironi, G.

AU - Tartari, A.

AU - Zannoni, M.

AU - Peterzen, S.

AU - Bartlett, J.

AU - Giraud-Heraud, Y.

AU - Piat, M.

AU - Rosset, C.

AU - Giard, M.

AU - Pons, R.

AU - Maffei, B.

AU - Ade, P.

AU - Gear, W.

AU - Mauskopf, P.

AU - Piccirillo, L.

AU - Pisano, G.

AU - Savini, G.

PY - 2005

Y1 - 2005

N2 - In the current cosmological scenario, part of the linearly polarized emission of the CMB is expected to be rotational (B-modes). This component is due to tensor perturbations of the metric produced by primordial gravitational waves, which are generated a split-second after the Big Bang. The signal expected is of the order of ≳0.1 μK, well below the non-rotational component of the polarization signal (E-modes), and beyond the sensitivity of present generation instruments. New, more sensitive instruments are developed in several labs, with the goal to measure the B-modes. Control of systematics and foregrounds will be the key to make the results of these experiments believable. In this paper we shortly outline BRAIN, a bolometric interferometer devoted to B-modes research, and its pathfinder experiment, devoted to test the Dome-C site.

AB - In the current cosmological scenario, part of the linearly polarized emission of the CMB is expected to be rotational (B-modes). This component is due to tensor perturbations of the metric produced by primordial gravitational waves, which are generated a split-second after the Big Bang. The signal expected is of the order of ≳0.1 μK, well below the non-rotational component of the polarization signal (E-modes), and beyond the sensitivity of present generation instruments. New, more sensitive instruments are developed in several labs, with the goal to measure the B-modes. Control of systematics and foregrounds will be the key to make the results of these experiments believable. In this paper we shortly outline BRAIN, a bolometric interferometer devoted to B-modes research, and its pathfinder experiment, devoted to test the Dome-C site.

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Precision CMB polarization from Dome-c: The brain experiment

Abstract

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ASJC Scopus subject areas

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