GroundBIRD: an experiment for CMB polarization measurements at a large angular scale from the ground

Odd-parity patterns in the cosmic microwave background (CMB) polarization, B-modes, could provide important cosmological information. Detection of the primordial B-mode power at a large angular scale would be a smoking gun signature of the inflationary universe. In particular, detecting a reionization bump (at a multipole of ≤ 10) should be a clear evidence of it. GroundBIRD is designed to detect the B-mode signal at this large angular scale from the ground. We will use superconducting detector arrays with small telescope that will also be cooled down to 4K. Therefore, the basic design can be extended to a satellite experiment. GroundBIRD employs a high-speed (20 rpm) rotation scan instead of the usual left–right azimuthal scan; this allows us to maintain a high-speed scan without any deceleration, resulting in a significant expansion of the scan range to 60° without any effect of the detector 1/f noise. Our target is measuring the CMB polarization power in a multipole (l) range of 6 ≤ l ≤ 300. We plan to start commissioning the instruments in Japan in early 2014; they will then be moved to the Atacama Desert in Chile for scientific observations.

[1]  A. Barrau,et al.  Observing the Big Bounce with tensor modes in the cosmic microwave background: phenomenology and fundamental loop quantum cosmology parameters , 2010, 1011.1811.

[2]  J. Carlstrom,et al.  Detection of polarization in the cosmic microwave background using DASI , 2002, Nature.

[3]  Paul J Steinhardt,et al.  Inflationary predictions for scalar and tensor fluctuations reconsidered. , 2006, Physical review letters.

[4]  E. Leitch,et al.  IMPROVED MEASUREMENTS OF THE TEMPERATURE AND POLARIZATION OF THE COSMIC MICROWAVE BACKGROUND FROM QUaD , 2009, 0906.1003.

[5]  I. Buder Measurement of the CMB Polarization at 95 GHz from QUIET , 2012, 1209.1277.

[6]  Edward J. Wollack,et al.  FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION , 2008, 0803.0547.

[7]  I. Buder,et al.  Novel Calibration System with Sparse Wires for CMB Polarization Receivers , 2011 .

[8]  P. A. R. Ade,et al.  MEASUREMENT OF COSMIC MICROWAVE BACKGROUND POLARIZATION POWER SPECTRA FROM TWO YEARS OF BICEP DATA , 2009, 0906.1181.

[9]  U. Seljak,et al.  Signature of gravity waves in polarization of the microwave background , 1996, astro-ph/9609169.

[10]  D. Barkats,et al.  New Measurements of Fine-Scale CMB Polarization Power Spectra from CAPMAP at Both 40 and 90 GHz , 2008 .

[11]  I. Buder,et al.  FIRST SEASON QUIET OBSERVATIONS: MEASUREMENTS OF COSMIC MICROWAVE BACKGROUND POLARIZATION POWER SPECTRA AT 43 GHz IN THE MULTIPOLE RANGE 25 ⩽ ⩽ 475 , 2010, 1012.3191.

[12]  M. Akagawa,et al.  Offset dual reflector antenna , 1976 .

[13]  Andrew R. Liddle,et al.  Cosmological Inflation and Large-Scale Structure , 2000 .

[14]  William L. Holzapfel,et al.  LiteBIRD: a small satellite for the study of B-mode polarization and inflation from cosmic background radiation detection , 2012, Other Conferences.

[15]  I. Buder,et al.  FIRST SEASON QUIET OBSERVATIONS : MEASUREMENTS OF CMB POLARIZATION POWER SPECTRA AT 43 GHZ IN THE MULTIPOLE RANGE 25 ≤ l ≤ 475 QUIET Collaboration , 2010 .