Internal Delensing of Cosmic Microwave Background Polarization B-Modes with the POLARBEAR experiment
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2020Metadata
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Adachi, S.
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Internal Delensing of Cosmic Microwave Background Polarization B-Modes with the POLARBEAR experiment
Author
- Adachi, S.;
- Aguilar Faúndez, M. A. O.;
- Akiba, Y.;
- Ali, A.;
- Arnold, K.;
- Baccigalupi, C.;
- Barron, D.;
- Beck, D.;
- Bianchini, F.;
- Borrill, J.;
- Carron, J.;
- Cheung, K.;
- Chinone, Y.;
- Crowley, K.;
- El Bouhargani, H.;
- Elleflot, T.;
- Errard, J.;
- Fabbian, G.;
- Feng, C.;
- Fujino, T.;
- Goeckner Wald, N.;
- Hasegawa, M.;
- Hazumi, M.;
- Hill, C. A.;
- Howe, L.;
- Katayama, N.;
- Keating, B.;
- Kikuchi, S.;
- Kusaka, A.;
- Lee, A. T.;
- León, D.;
- Linder, E.;
- Lowry, L. N.;
- Matsuda, F.;
- Matsumura, T.;
- Minami, Y.;
- Namikawa, T.;
- Navaroli, M.;
- Nishino, H.;
- Pelotón, J.;
- Pham, A. T. P.;
- Poletti, D.;
- Puglisi, G.;
- Reichardt, C. L.;
- Segawa, Y.;
- Sherwin, B. D.;
- Silva Feaver, M.;
- Siritanasak, P.;
- Stompor, R.;
- Tajima, O.;
- Takatori, S.;
- Tanabe, D.;
- Teply, G. P.;
- Vergès, C.;
Abstract
Using only cosmic microwave background polarization data from the POLARBEAR experiment, we measure B-mode polarization delensing on subdegree scales at more than 5s significance. We achieve a 14% B-mode power variance reduction, the highest to date for internal delensing, and improve this result to 22% by applying for the first time an iterative maximum a posteriori delensing method. Our analysis demonstrates the capability of internal delensing as a means of improving constraints on inflationary models, paving the way for the optimal analysis of next-generation primordial B-mode experiments.
Patrocinador
National Science Foundation (NSF): AST-0618398, AST-1212230.
Comisión Nacional de Investigación Científica y Tecnológica (CONICYT).
European Research Council (ERC): 616170.
Science & Technology Facilities Council (STFC): ST/P000525/1.
STFC Ernest Rutherford Fellowship.
Ministry of Education, Culture, Sports, Science and Technology, Japan (MEXT).
Ministry of Education, Culture, Sports, Science and Technology, Japan (MEXT).
Japan Society for the Promotion of Science.
Grants-in-Aid for Scientific Research (KAKENHI): JP16K21744, JP18H05539, 18K13558, 18H04347, 19H00674, JP26220709, JP15H05891, JP26800125.
University of Melbourne.
Australian Research Council: FT150100074.
Gordon and Betty Moore Foundation: 4633.
Simons Foundation: 034079.
Templeton Foundation: 58724.
Ax Center for Experimental Cosmology at UC San Diego.
CONICYT UC BerkeleyChile Seed Grant (CLAS fund): 77047.
Comisión Nacional de Investigación Científica y Tecnológica (CONICYT), CONICYT FONDECYT: 1130777, 1171811.
DFI postgraduate scholarship program.
DFI Postgraduate Competitive Fund.
Ministry of Education, Culture, Sports, Science and Technology, Japan (MEXT).
Japan Society for the Promotion of Science.
JSPS Leading Initiative for Excellent Young Researchers (LEADER).
United States Department of Energy (DOE): DE-AC02-05CH11231.
United States Department of Energy (DOE): DE-AC02-05CH11231.
ASICOSMOS network.
INDARK INFN Initiative.
Indexation
Artículo de publicación ISI Artículo de publicación SCOPUS
Identifier
URI: https://repositorio.uchile.cl/handle/2250/174877
DOI: 10.1103/PhysRevLett.124.131301
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Physical Review Letters, 124 (13). a131301
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