Measurement of the Cosmic Microwave Background Polarization Lensing Power Spectrum with the POLARBEAR Experiment
2014; American Physical Society; Volume: 113; Issue: 2 Linguagem: Inglês
10.1103/physrevlett.113.021301
ISSN1092-0145
AutoresP. A. R. Ade, Y. Akiba, A. E. Anthony, K. Arnold, M. Atlas, Darcy Barron, D. Boettger, J. Borrill, S. Chapman, Y. Chinone, M. Dobbs, T. Elleflot, J. Errard, Giulio Fabbian, Chang Feng, D. Flanigan, A. Gilbert, W. Grainger, N. W. Halverson, M. Hasegawa, K. Hattori, M. Hazumi, W. L. Holzapfel, Y. Hori, J. Howard, P. Hyland, Y. Inoue, G. Jaehnig, A. Jaffe, Brian Keating, Z. Kermish, R. Keskitalo, T. Kisner, M. Le Jeune, A. T. Lee, E. Linder, E. M. Leitch, Marius Lungu, F. Matsuda, T. Matsumura, X. Meng, N. J. Miller, H. Morii, S. Moyerman, Mike Myers, M. Navaroli, H. Nishino, H. Paar, J. Peloton, E. Quealy, Gabriel M. Rebeiz, C. L. Reichardt, P. L. Richards, C. Ross, I. Schanning, D. E. Schenck, B. D. Sherwin, A. Shimizu, L. Shi, M. Shimon, P. Siritanasak, G. Smecher, H. Spieler, N. Stebor, B. Steinbach, R. Stompor, A. Suzuki, S. Takakura, T. Tomaru, B. Wilson, Amit Yadav, O. Zahn,
Tópico(s)Superconducting and THz Device Technology
ResumoDistortion of the cosmic microwave background by matter in the universe, known as gravitational lensing, is observed by the POLARBEAR collaboration. The technique used here would allow for all gravitating matter to be mapped, and provide important corrections for the detection of primordial gravitational waves in the cosmic microwave background.
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