A Measurement of the Cosmic Microwave Background B-mode Polarization Power Spectrum at Subdegree Scales from Two Years of POLARBEAR Data
- Cardiff Univ., (UK). School of Physics
- Univ. de Chile, Santiago (Chile). Dept. de Fisica
- SOKENDAI, Kanagawa (Japan); High Energy Accelerator Research Organization (KEK), Tsukuba (Japan)
- Univ. of California, San Diego, CA (United States). Dept. of Physics
- The International School for Advanced Studies SISSA, Triste (Italy); The National Inst. for Nuclear Physics INFN, Triste (Italy)
- Univ. of California, Berkeley, CA (United States). Space Sciences Lab.
- Univ. Paris Diderot, Sorbonne Paris Cite (France). AstroParticule et Cosmologie
- Univ. of Melbourne (Australia). School of Physics
- Pontificia Univ. Catolica de Chile, Santiago (Chile). Centro de Astro-Ingenieria
- Univ. of California, Berkeley, CA (United States). Space Sciences Lab.; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Computational Cosmology Center
- Dalhousie Univ., Halifax, NS (Canada). Dept. of Physics and Atmospheric Science
- Univ. of California, Berkeley, CA (United States). Dept. of Physics; Univ. of Tokyo (Japan). Kavli IPMU
- Univ. of California, Berkeley, CA (United States). Dept. of Physics
- McGill Univ., Montreal, QC (Canada). Dept of Physics
- Univ. of Tokyo (Japan). Kavli IPMU
- Univ. Paris-Sud, Orsay (France). Inst. d'Astrophysique Spatiale
- Flatiron Inst., New York, NY (United States). Center for Computational Astrophysics; Imperial College, London (United Kingdom). Blackett Lab., Dept. of Physics
- Univ. of California, Irvine, CA (United States). Dept. of Physics and Astronomy
- Yokohama National Univ. (Japan)
- Harvard Univ., Cambridge, MA (United States). Harvard-Smithsonian Center for Astrophysics
- Univ. of Colorado, Boulder, CO (United States). Dept. of Astrophysical and Planetary Sciences; Univ. of Colorado, Boulder, CO (United States). Dept. of Physics; Univ. of Colorado, Boulder, CO (United States). Dept. of Astrophysical and Planetary Sciences
- High Energy Accelerator Research Organization (KEK), Tsukuba (Japan); Tohoku Univ., Sendai (Japan). Astronomical Inst., Graduate School of Science
- SOKENDAI (Japan); High Energy Accelerator Research Organization (KEK), Tsukuba (Japan)
- High Energy Accelerator Research Organization (KEK), Tsukuba (Japan); SOKENDAI (Japan); Univ. of Tokyo (Japan). Kavli IMPU; Japan Aerospace Exploration Agency, Tsukuba (Japan). Inst. of Space and Astronautical Science
- Univ. of California, Berkeley, CA (United States). Dept. of Physics; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Physics Dept.
- High Energy Accelerator Research Organization (KEK), Tsukuba (Japan); Academia Sinica, Taipei (Taiwan). Inst. of Physics
- Univ. of Colorado, Boulder, CO (United States) Center for Astrophysics and Space Astronomy; Univ. of Colorado, Boulder, CO (United States). Dept. of Physics
- Imperial College, London (United Kingdom). Blackett Lab., Dept. of Physics
- The International School for Advanced Studies SISSA, Triste (Italy)
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Physics Division; Univ. of Tokyo (Japan). Dept. of Physics
- Univ. of California, Berkeley, CA (United States). Dept. of Physics; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). Physics Division; Univ. of California, Berkeley, CA (United States). Radio Astronomy Lab.
- Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); Univ. of Chicago, IL (United States). Dept. of Astronomy and Astrophysics. et al.
We report an improved measurement of the cosmic microwave background B-mode polarization power spectrum with the Polarbear experiment at 150 GHz. By adding new data collected during the second season of observations (2013-2014) to re-analyzed data from the first season (2012-2013), we have reduced twofold the band-power uncertainties. The band powers are reported over angular multipoles 500 ≤ ℓ ≤ 2100, where the dominant B-mode signal is expected to be due to the gravitational lensing of E-modes. We reject the null hypothesis of no B-mode polarization at a confidence of 3.1σ including both statistical and systematic uncertainties. We test the consistency of the measured B-modes with the Λ Cold Dark Matter (ΛCDM) framework by fitting for a single lensing amplitude parameter A L = 0.60 +0.26-0.24(stat)+0.00-0.04 (inst) ± 0.14(foreground) ± 0.04(multi), where A L = 1 relative to the Planck 2015 best-fit model prediction. We obtain ±0.14(foreground) ±0.04(multi), where is the fiducial ΛCDM value.
- Research Organization:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
- Sponsoring Organization:
- USDOE Office of Science (SC)
- Contributing Organization:
- The POLARBEAR Collaboration
- Grant/Contract Number:
- AC02-05CH11231
- OSTI ID:
- 1524240
- Alternate ID(s):
- OSTI ID: 1525246
- Journal Information:
- The Astrophysical Journal (Online), Vol. 848, Issue 2; ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Web of Science
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