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| DOI | 10.1007/s10909-015-1425-4 |
| The POLARBEAR-2 and the Simons Array Experiments | |
| Suzuki, A.2; Ade, P.4; Akiba, Y.24; Aleman, C.6; Arnold, K.25; Baccigalupi, C.7; Barch, B.1; Barron, D.1; Bender, A.8; Boettger, D.13; Borrill, J.9; Chapman, S.10; Chinone, Y.1; Cukierman, A.1; Dobbs, M.11; Ducout, A.12; Dunner, R.13; Elleflot, T.6; Errard, J.27; Fabbian, G.7; Feeney, S.12; Feng, C.14; Fujino, T.3; Fuller, G.6; Gilbert, A.11; Goeckner-Wald, N.1; Groh, J.1; Haan, T. De1; Hall, G.1; Halverson, N.15; Hamada, T.5; Hasegawa, M.5; Hattori, K.5; Hazumi, M.24; Hill, C.1; Holzapfel, W.1; Hori, Y.1; Howe, L.6; Inoue, Y.24; Irie, F.3; Jaehnig, G.15; Jaffe, A.12; Jeong, O.1; Katayama, N.3; Kaufman, J.6; Kazemzadeh, K.6; Keating, B.6; Kermish, Z.16; Keskitalo, R.9; Kisner, T.9; Kusaka, A.17; Jeune, M. Le18; Lee, A.1; Leon, D.6; Linder, E.17; Lowry, L.6; Matsuda, F.6; Matsumura, T.19; Miller, N.20; Mizukami, K.3; Montgomery, J.11; Navaroli, M.6; Nishino, H.5; Peloton, J.18; Poletti, D.18; Puglisi, G.7; Rebeiz, G.21; Raum, C.1; Reichardt, C.22; Richards, P.1; Ross, C.10; Rotermund, K.10; Segawa, Y.5; Sherwin, B.17; Shirley, I.1; Siritanasak, P.6; Stebor, N.6; Stompor, R.18; Suzuki, J.5; Tajima, O.5; Takada, S.23; Takakura, S.26; Takatori, S.5; Tikhomirov, A.10; Tomaru, T.5; Westbrook, B.1; Whitehorn, N.1; Yamashita, T.3; Zahn, A.6; Zahn, O.1 | |
| 来源期刊 | JOURNAL OF LOW TEMPERATURE PHYSICS
 |
| ISSN | 0022-2291 |
| EISSN | 1573-7357 |
| 出版年 | 2016 |
| 卷号 | 184期号:3-4页码:805-810 |
| 英文摘要 | We present an overview of the design and status of the Polarbear-2 and the Simons Array experiments. Polarbear-2 is a cosmic microwave background polarimetry experiment which aims to characterize the arc-minute angular scale B-mode signal from weak gravitational lensing and search for the degree angular scale B-mode signal from inflationary gravitational waves. The receiver has a 365 mm diameter focal plane cooled to 270 mK. The focal plane is filled with 7588 dichroic lenslet-antenna-coupled polarization sensitive transition edge sensor (TES) bolometric pixels that are sensitive to 95 and 150 GHz bands simultaneously. The TES bolometers are read-out by SQUIDs with 40 channel frequency domain multiplexing. Refractive optical elements are made with high-purity alumina to achieve high optical throughput. The receiver is designed to achieve noise equivalent temperature of 5.8 K in each frequency band. Polarbear-2 will deploy in 2016 in the Atacama desert in Chile. The Simons Array is a project to further increase sensitivity by deploying three Polarbear-2 type receivers. The Simons Array will cover 95, 150, and 220 GHz frequency bands for foreground control. The Simons Array will be able to constrain tensor-to-scalar ratio and sum of neutrino masses to at and to 40 meV. |
| 英文关键词 | Cosmic microwave background Inflation Gravitational weak lensing Polarization B-mode |
| 类型 | Article |
| 语种 | 英语 |
| 国家 | USA ; Japan ; Wales ; Italy ; Canada ; England ; Chile ; France ; Australia |
| 收录类别 | SCI-E |
| WOS记录号 | WOS:000379022700043 |
| WOS关键词 | B-MODE POLARIZATION ; SCALES |
| WOS类目 | Physics, Applied ; Physics, Condensed Matter |
| WOS研究方向 | Physics |
| 来源机构 | University of California, Berkeley |
| 资源类型 | 期刊论文 |
| 条目标识符 | http://119.78.100.177/qdio/handle/2XILL650/194595 |
| 作者单位 | 1.Univ Calif, Dept Phys, Berkeley, CA 94720 USA; 2.Univ Calif, Radio Astron Lab, Berkeley, CA 94720 USA; 3.Univ Tokyo, Kavli IPMU WPI, UTIAS, Chiba 2778583, Japan; 4.Cardiff Univ, Sch Phys & Astron, Cardiff CF10 3XQ, Wales; 5.High Energy Accelerator Res Org KEK, Tsukuba, Ibaraki 3050801, Japan; 6.Univ Calif, Dept Phys, San Diego, CA 92093 USA; 7.Int Sch Adv Studies SISSA, I-34136 Trieste, Italy; 8.Argonne Natl Lab, Argonne, IL 60439 USA; 9.Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA; 10.Dalhousie Univ, Dept Phys & Atmospher Sci, Halifax, NS B3H 4R2, Canada; 11.McGill Univ, Dept Phys, Montreal, PQ H3A 0G4, Canada; 12.Imperial Coll London, Dept Phys, Blackett Lab, London SW7 2AZ, England; 13.Pontif Univ Catol, Dept Astron, Santiago, Chile; 14.Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA; 15.Univ Colorado, Ctr Astrophys & Space Astron, Boulder, CO 80309 USA; 16.Princeton Univ, Dept Phys, Princeton, NJ 08544 USA; 17.Lawrence Berkeley Natl Lab, Div Phys, Berkeley, CA 94720 USA; 18.Univ Paris Diderot, AstroParticule & Cosmol, CEA Irfu, Obs Paris, Paris, France; 19.Inst Space & Astronaut Studies ISAS, Tokyo, Japan; 20.NASA Goddard Space Flight Ctr, Observat Cosmol Lab, Code 665, Greenbelt, MD 20771 USA; 21.Univ Calif, Dept Elect & Comp Engn, San Diego, CA 92093 USA; 22.Univ Melbourne, Sch Phys, Parkville, Vic 3010, Australia; 23.Natl Inst Fusion Sci, Toki, Gifu, Japan; 24.SOKENDAI Kamiyamaguchi, Hayama, Miura, Kanagawa 2400115, Japan; 25.Univ Wisconsin, Dept Phys, Madison, WI 53706 USA; 26.Osaka Univ, Dept Phys, Osaka, Japan; 27.Inst Lagrange Paris ILP, Univ Sorbonne, F-75014 Paris, France |
| 推荐引用方式 GB/T 7714 | Suzuki, A.,Ade, P.,Akiba, Y.,et al. The POLARBEAR-2 and the Simons Array Experiments[J]. University of California, Berkeley,2016,184(3-4):805-810. |
| APA | Suzuki, A..,Ade, P..,Akiba, Y..,Aleman, C..,Arnold, K..,...&Zahn, O..(2016).The POLARBEAR-2 and the Simons Array Experiments.JOURNAL OF LOW TEMPERATURE PHYSICS,184(3-4),805-810. |
| MLA | Suzuki, A.,et al."The POLARBEAR-2 and the Simons Array Experiments".JOURNAL OF LOW TEMPERATURE PHYSICS 184.3-4(2016):805-810. |
| 条目包含的文件 | 条目无相关文件。 | |||||
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