Planck 2015 results

PAR, Ade,; Aghanim, N.; Arnaud, M.; Arroja, Frederico; Ashdown, M.; Aumont, J.; Baccigalupi, C.; Ballardini, M.; Banday, A. J.; Barreiro, R. B.; Bartolo, N.; Battaner, E.; Benabed, K.; Benoı̂t, A.; Benoit-Lévy, A.; Bernard, J.-P.; Bersanelli, M.; Bielewicz, P.; Bock, J. J.; Bonaldi, A.; Bonavera, L.; Bond, J. R.; Borrill, J.; Bouchet, F. R.; Boulanger, F.; Bucher, M.; Burigana, C.; Butler, R. C.; Calabrese, E.; J-F, Cardoso,; Catalano, A.; Challinor, A.; Chamballu, A.; R-R, Chary,; Chiang, H. C.; Christensen, P. R.; Church, S.; Clements, D. L.; Colombi, S.; Colombo, L. P. L.; Combet, C.; Contreras, D.; Couchot, F.; Coulais, A.; Crill, B. P.; Curto, A.; Cuttaia, F.; Danese, L.; Davies, R. D.; Davis, Roger J.; Bernardis, P. de; Rosa, A. de; Zotti, G. de; J, Delabrouille,; Désert, F.–X.; Diego, J. M.; H, Dole,; Donzelli, S.; Doré, O.; Douspis, M.; Ducout, A.; Dupac, X.; Efstathiou, G.; Elsner, F.; Enßlin, T. A.; Eriksen, H. K.; Fergusson, J.; Finelli⋆, F.; Forni, O.; Frailis, M.; Fraisse, A. A.; Franceschi, E.; Frejsel, A.; A, Frolov,; Galeotta, S.; Galli, S.; Ganga, K.; Gauthier, C.; Giard, M.; Giraud–Héraud, Y.; Gjerløw, E.; González-Nuevo, J.; Górski, K. M.; Golec, Joseph E.; Gregorio, A.; Gruppuso, A.; Gudmundsson, J. E.; Hamann, J.; Handley, Will; Hansen, F. K.; Hanson, D.; Harrison, D. L.; Henrot–Versillé, S.; Hernández-Monteagudo, C.; Herranz, D.; Hildebrandt, S. R.; Hivon, E.; M, Hobson,; Holmes, W. A.; A, Hornstrup,; W, Hovest,; Z, Huang,; KM, Huffenberger,; G, Hurier,; AH, Jaffe,; TR, Jaffe,; WC, 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,; M, Liguori,; PB, Lilje,; M, Linden-Vørnle,; M, López-Caniego,; PM, Lubin,; Y-Z, Ma,; JF, Macías-Pérez,; G, Maggio,; D, Maino,; N, Mandolesi,; A, Mangilli,; M, Maris,; PG, Martin,; E, Martínez-González,; S, Masi,; S, Matarrese,; P, McGehee,; PR, Meinhold,; A, Melchiorri,; L, Mendes,; A, Mennella,; M, Migliaccio,; S, Mitra,; M-A, Miville-Deschênes,; D, Molinari,; A, Moneti,; L, Montier,; G, Morgante,; D, Mortlock,; A, Moss,; M, Münchmeyer,; D, Munshi,; JA, Murphy,; P, Naselsky,; F, Nati,; P, Natoli,; CB, Netterfield,; HU, Nørgaard-Nielsen,; F, Noviello,; D, Novikov,; I, Novikov,; CA, Oxborrow,; F, Paci,; L, Pagano,; F, Pajot,; R, Paladini,; S, Pandolfi,; D, Paoletti,; F, Pasian,; G, Patanchon,; TJ, Pearson,; HV, Peiris,; O, Perdereau,; L, Perotto,; F, Perrotta,; V, Pettorino,; F, Piacentini,; M, Piat,; E, Pierpaoli,; D, Pietrobon,; S, Plaszczynski,; E, Pointecouteau,; G, Polenta,; L, Popa,; GW, Pratt,; G, Prézeau,; S, Prunet,; J-L, Puget,; JP, Rachen,; WT, Reach,; R, Rebolo,; M, Reinecke,; M, Remazeilles,; C, Renault,; A, Renzi,; I, Ristorcelli,; G, Rocha,; C, Rosset,; M, Rossetti,; G, Roudier,; M, Rowan-Robinson,; JA, Rubiño-Martín,; B, Rusholme,; M, Sandri,; D, Santos,; M, Savelainen,; G, Savini,; D, Scott,; MD, Seiffert,; EPS, Shellard,; M, Shiraishi,; LD, Spencer,; V, Stolyarov,; R, Stompor,; R, Sudiwala,; R, Sunyaev,; D, Sutton,; A-S, Suur-Uski,; J-F, Sygnet,; JA, Tauber,; L, Terenzi,; L, Toffolatti,; M, Tomasi,; M, Tristram,; T, Trombetti,; M, Tucci,; J, Tuovinen,; L, Valenziano,; J, Valiviita,; B, Van Tent,; P, Vielva,; F, Villa,; LA, Wade,; BD, Wandelt,; IK, Wehus,; M, White,; D, Yvon,; A, Zacchei,; JP, Zibin,; A, Zonca,

doi:10.17863/cam.52

preprintCaltechAUTHORS (California Institute of Technology)May 27, 2016GREEN OA

Planck 2015 results

APAde, PARNAN. Aghanim MAM. Arnaud FAFrederico Arroja MAM. Ashdown

Indexed indatacite

Abstract

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…

Citation impact

2,006

total citations

FWCI: 206.60
Percentile: 100%
References: 502

Citations per year

Authors

246

Topics & keywords

Topics

Keywords

Planck
Physics
Inflaton
Cosmic microwave background
Spectral index
Bispectrum
Spectral density
Inflation (cosmology)

No related works found for this paper.