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Toward a 10,000-element B-Mode Experiment

Published online by Cambridge University Press:  30 January 2013

Chao-Lin Kuo  and
for the BICEP3 and POLAR1 Collaborations
Chao-Lin Kuo
Affiliation:
Dept. of Physics, Stanford University, Kavli Institute for Particle Astrophysics and Cosmology, 385 Via Pueblo Mall, Stanford, CA94305, USA email: [email protected]
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Abstract

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In this paper, we introduce two compact, large-throughput CMB polarimeter designs (POLAR1 and BICEP3). These pathfinder experiments will pave the way for a comprehensive multi-frequency South Pole B-mode survey that, when jointly analyzed with arcminute-scale polarization data, can conclusively answer the question whether there is an appreciable fraction (>1%) of the primordial perturbations in the form of tensor modes (gravitational waves).

Keywords

Cosmology: cosmic microwave backgroundinstrumentation: polarimeters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S288: Astrophysics from Antarctica , August 2012 , pp. 80 - 83
Copyright
Copyright © International Astronomical Union 2013

References

Bischoff, C.et al. 2012, These Proceedings.Google Scholar
Pryke, C.et al. 2012, These Proceedings.Google Scholar
Benson, B.et al. 2012, These Proceedings.Google Scholar