Authors
PAR Ade, N Aghanim, M Arnaud, F Arroja, Mark Ashdown, J Aumont, Carlo Baccigalupi, Mario Ballardini, AJ Banday, RB Barreiro, Nicola Bartolo, E Battaner, K Benabed, A Benoit, A Benoit-Lévy, J-P Bernard, Matteo Bersanelli, P Bielewicz, JJ Bock, A Bonaldi, L Bonavera, JR Bond, J Borrill, FR Bouchet, F Boulanger, M Bucher, C Burigana, RC Butler, Erminia Calabrese, J-F Cardoso, A Catalano, A Challinor, A Chamballu, R-R Chary, HC Chiang, PR Christensen, S Church, DL Clements, S Colombi, LPL Colombo, C Combet, D Contreras, F Couchot, A Coulais, BP Crill, A Curto, Francesco Cuttaia, L Danese, RD Davies, RJ Davis, Paolo de Bernardis, A De Rosa, Giulia De Zotti, J Delabrouille, F-X Desert, JM Diego, H Dole, SIMONA Donzelli, O Doré, M Douspis, A Ducout, X Dupac, G Efstathiou, F Elsner, TA Enßlin, HK Eriksen, J Fergusson, F Finelli, O Forni, M Frailis, AA Fraisse, E Franceschi, A Frejsel, A Frolov, S Galeotta, S Galli, K Ganga, C Gauthier, M Giard, Y Giraud-Héraud, Eirik Gjerløw, J Gonzalez-Nuevo, KM Gorski, S Gratton, Anna Gregorio, A Gruppuso, Jón E Gudmundsson, J Hamann, W Handley, Frode Kristian Hansen, D Hanson, DL Harrison, S Henrot-Versille, C Hernandez-Monteagudo, D Herranz, SR Hildebrandt, E Hivon, M Hobson, WA Holmes, Allan Hornstrup, W Hovest, Z Huang, KM Huffenberger, G Hurier, AH Jaffe, TR Jaffe, William C Jones, M Juvela, E Keihänen, R Keskitalo, J Kim, TS Kisner, R Kneissl, J Knoche, M Kunz, H Kurki-Suonio, G Lagache, A Lähteenmäki, J-M Lamarre, A Lasenby, M Lattanzi, CR Lawrence, R Leonardi, J Lesgourgues, F Levrier, A Lewis, Michele Liguori, Per Barth Lilje, Michael Linden-Vørnle, M Lopez-Caniego, PM Lubin, Y-Z Ma, JF Macias-Perez, G Maggio, D Maino, N Mandolesi, A Mangilli, M Maris, PG Martin, E Martinez-Gonzalez, Silvia Masi, Sabino Matarrese, P McGehee, PR Meinhold, Alessandro Melchiorri, L Mendes, A Mennella, M Migliaccio, Susanta Mitra, M-A Miville-Deschenes
Publication date
2016/10/1
Journal
Astronomy & Astrophysics
Volume
594
Pages
A20
Publisher
EDP sciences
Description
We present the implications for cosmic inflation of the Planck measurements of the cosmic microwave background (CMB) anisotropies in both temperature and polarization based on the full Planck survey, which includes more than twice the integration time of the nominal survey used for the 2013 release papers. The Planck full mission temperature data and a first release of polarization data on large angular scales measure the spectral index of curvature perturbations to be ns = 0.968 ± 0.006 and tightly constrain its scale dependence to dns/ dlnk = −0.003 ± 0.007 when combined with the Planck lensing likelihood. When the Planck high-ℓ polarization data are included, the results are consistent and uncertainties are further reduced. The upper bound on the tensor-to-scalar ratio is r0.002< 0.11 (95% CL). This upper limit is consistent with the B-mode polarization constraint r< 0.12 (95% CL) obtained from a joint analysis …
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