Title: | Planck 2015 results |
Author(s): | Ade, P. A R ; Aghanim, N. ; Arnaud, M. ; Arroja, F. ; Ashdown, M. ; Aumont, J. ; Baccigalupi, C. ; Ballardini, M. ; Banday, A. J. ; Barreiro, R. B. ; Bartolo, N. ; Basak, S. ; Battaner, E. ; Benabed, K. ; Benoît, 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. ; Cardoso, J. F. ; Catalano, A. ; Challinor, A. ; Chamballu, A. ; Chiang, H. C. ; Christensen, P. R. ; Church, S. ; Clements, D. L. ; Colombi, S. ; Colombo, L. P L ; Combet, C. ; Couchot, F. ; Coulais, A. ; Crill, B. P. ; Curto, A. ; Cuttaia, F. ; Danese, L. ; Davies, R. D. ; Davis, R. J. ; De Bernardis, P. ; De Rosa, A. ; De Zotti, G. ; Delabrouille, J. ; Désert, F. X. ; Diego, J. M. ; Dole, H. ; 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. ; Galeotta, S. ; Galli, S. ; Ganga, K. ; Gauthier, C. ; Ghosh, T. ; Giard, M. ; Giraud-Héraud, Y. ; Gjerløw, E. ; González-Nuevo, J. ; Górski, K. M. ; Gratton, S. ; Gregorio, A. ; Gruppuso, A. ; Gudmundsson, J. E. ; Hamann, J. ; Hansen, F. K. ; Hanson, D. ; Harrison, D. L. ; Heavens, A. ; Helou, G. ; Henrot-Versillé, S. ; Hernández-Monteagudo, C. ; Herranz, D. ; Hildebrandt, S. R. ; Hivon, E. ; Hobson, M. ; Holmes, W. A. ; Hornstrup, A. ; Hovest, W. ; Huang, Z. ; Huffenberger, K. M. ; Hurier, G. ; Jaffe, A. H. ; Jaffe, T. R. ; Jones, W. C. ; Juvela, M. ; Keihänen, E. ; Keskitalo, R. ; Kim, Jaiseung ; Kisner, T. S. ; Knoche, J. ; Kunz, M. ; Kurki-Suonio, H. ; Lacasa, F. ; Lagache, G. ; Lähteenmäki, A. ; Lamarre, J. M. ; Lasenby, A. ; Lattanzi, M. ; Lawrence, C. R. ; Leonardi, R. ; Lesgourgues, J. ; Levrier, F. ; Lewis, A. ; Liguori, M. ; Lilje, P. B. ; Linden-Vørnle, M. ; López-Caniego, M. ; Lubin, P. M. ; Maciás-Pérez, J. F. ; Maggio, G. ; Maino, D. ; Mandolesi, N. ; Mangilli, A. ; Marinucci, D. ; Maris, M. ; Martin, P. G. ; Martínez-González, E. ; Masi, S. ; Matarrese, S. ; Mcgehee, P. ; Meinhold, P. R. ; Melchiorri, A. ; Mendes, L. ; Mennella, A. ; Migliaccio, M. ; Mitra, S. ; Miville-Deschênes, M. A. ; Moneti, A. ; Montier, L. ; Morgante, G. ; Mortlock, D. ; Moss, A. ; Münchmeyer, M. ; Munshi, D. ; Murphy, J. A. ; Naselsky, P. ; Nati, F. ; Natoli, P. ; Netterfield, C. B. ; Nørgaard-Nielsen, H. U. ; Noviello, F. ; Novikov, D. ; Novikov, I. ; Oxborrow, C. A. ; Paci, F. ; Pagano, L. ; Pajot, F. ; Paoletti, D. ; Pasian, F. ; Patanchon, G. ; Peiris, H. V. ; Perdereau, O. ; Perotto, L. ; Perrotta, F. ; Pettorino, V. ; Piacentini, F. ; Piat, M. ; Pierpaoli, E. ; Pietrobon, D. ; Plaszczynski, S. ; Pointecouteau, E. ; Polenta, G. ; Popa, L. ; Pratt, G. W. ; Prézeau, G. ; Prunet, S. ; Puget, J. L. ; Rachen, J. P. ; Racine, B. ; Rebolo, R. ; Reinecke, M. ; Remazeilles, M. ; Renault, C. ; Renzi, A. ; Ristorcelli, I. ; Rocha, G. ; Rosset, C. ; Rossetti, M. ; Roudier, G. ; Rubinõ-Martín, J. A. ; Rusholme, B. ; Sandri, M. ; Santos, D. ; Savelainen, M. ; Savini, G. ; Scott, D. ; Seiffert, M. D. ; Shellard, E. P S ; Shiraishi, M. ; Smith, K. ; Spencer, L. D. ; Stolyarov, V. ; Stompor, R. ; Sudiwala, R. ; Sunyaev, R. ; Sutter, P. ; Sutton, D. ; Suur-Uski, A. S. ; Sygnet, J. F. ; Tauber, J. A. ; Terenzi, L. ; Toffolatti, L. ; Tomasi, M. ; Tristram, M. ; Troja, A. ; Tucci, M. ; Tuovinen, J. ; Valenziano, L. ; Väliviita, J. ; Van Tent, B. ; Vielva, P. ; Villa, F. ; Wade, L. A. ; Wandelt, B. D. ; Wehus, I. K. ; Yvon, D. ; Zacchei, A. ; Zonca, A. |
Date: | 2016-10-01 |
Language: | en |
Pages: | 66 |
Department: | Cardiff University Université Paris-Saclay Centre National de la Recherche Scientifique (CNRS) National Taiwan University Kavli Institute for Cosmology Cambridge International School for Advanced Studies INAF/IASF Bologna IRAP Universidad de Cantabria University of Padova University of Granada UMR7095 Universite Joseph Fourier INAF/IASF Milano California Institute of Technology University of Manchester University of Toronto University of California Berkeley Institut d 'Astrophysique de Paris Astroparticle and Cosmology Laboratory University of Oxford Telecom ParisTech Institut national de physique nucléaire et de physique des particules Princeton University Niels Bohr Institute Stanford University Imperial College London University of Southern California LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres Università La Sapienza INAF, Osservatorio Astronomico di Padova Université Grenoble Alpes European Space Agency - ESA University of Cambridge Max-Planck-Institut für Astrophysik University of Oslo INAF - Osservatorio Astronomico di Trieste University of Chicago University of Warsaw Università Degli Studi di Trieste Stockholm University CERN McGill University Technical University of Denmark Florida State University University of Helsinki Lawrence Berkeley National Laboratory Department of Radio Science and Engineering University of Ferrara Centro de Gestão e Estudos Estratégicos University of Sussex University of California Santa Barbara Università di Roma Tor Vergata European Space Astronomy Centre University of Nottingham National University of Ireland, Galway University of Copenhagen RAS - P.N. Lebedev Physics Institute University College London Heidelberg University INAF, Osservatorio Astronomico di Roma Institute for Space Sciences CEA Saclay Instituto de Astrofísica de Canarias University of British Columbia Perimeter Institute for Theoretical Physics Special Astrophysical Observatory of the Russian Academy of Sciences Space Research Institute of the Russian Academy of Sciences European Space Research and Technology Centre Università degli Studi eCampus Università degli Studi di Milano University of Geneva Trinity College Dublin |
Series: | Astronomy and Astrophysics, Volume 594 |
ISSN: | 0004-6361 1432-0746 |
DOI-number: | 10.1051/0004-6361/201525836 |
Keywords: | Cosmic background radiation, Cosmology: observations, Cosmology: theory, Early Universe, Inflation, Methods: data analysis |
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Ade , P A R , Aghanim , N , Arnaud , M , Arroja , F , Ashdown , M , Aumont , J , Baccigalupi , C , Ballardini , M , Banday , A J , Barreiro , R B , Bartolo , N , Basak , S , Battaner , E , Benabed , K , Benoît , 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 , Cardoso , J F , Catalano , A , Challinor , A , Chamballu , A , Chiang , H C , Christensen , P R , Church , S , Clements , D L , Colombi , S , Colombo , L P L , Combet , C , Couchot , F , Coulais , A , Crill , B P , Curto , A , Cuttaia , F , Danese , L , Davies , R D , Davis , R J , De Bernardis , P , De Rosa , A , De Zotti , G , Delabrouille , J , Désert , F X , Diego , J M , Dole , H , 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 , Galeotta , S , Galli , S , Ganga , K , Gauthier , C , Ghosh , T , Giard , M , Giraud-Héraud , Y , Gjerløw , E , González-Nuevo , J , Górski , K M , Gratton , S , Gregorio , A , Gruppuso , A , Gudmundsson , J E , Hamann , J , Hansen , F K , Hanson , D , Harrison , D L , Heavens , A , Helou , G , Henrot-Versillé , S , Hernández-Monteagudo , C , Herranz , D , Hildebrandt , S R , Hivon , E , Hobson , M , Holmes , W A , Hornstrup , A , Hovest , W , Huang , Z , Huffenberger , K M , Hurier , G , Jaffe , A H , Jaffe , T R , Jones , W C , Juvela , M , Keihänen , E , Keskitalo , R , Kim , J , Kisner , T S , Knoche , J , Kunz , M , Kurki-Suonio , H , Lacasa , F , Lagache , G , Lähteenmäki , A , Lamarre , J M , Lasenby , A , Lattanzi , M , Lawrence , C R , Leonardi , R , Lesgourgues , J , Levrier , F , Lewis , A , Liguori , M , Lilje , P B , Linden-Vørnle , M , López-Caniego , M , Lubin , P M , Maciás-Pérez , J F , Maggio , G , Maino , D , Mandolesi , N , Mangilli , A , Marinucci , D, Maris , M , Martin , P G , Martínez-González , E , Masi , S , Matarrese , S , Mcgehee , P , Meinhold , P R , Melchiorri , A , Mendes , L , Mennella , A , Migliaccio , M , Mitra , S , Miville-Deschênes , M A , Moneti , A , Montier , L , Morgante , G , Mortlock , D , Moss , A , Münchmeyer , M , Munshi , D , Murphy , J A , Naselsky , P , Nati , F , Natoli , P , Netterfield , C B , Nørgaard-Nielsen , H U , Noviello , F , Novikov , D , Novikov , I , Oxborrow , C A , Paci , F , Pagano , L , Pajot , F , Paoletti , D , Pasian , F , Patanchon , G , Peiris , H V , Perdereau , O , Perotto , L , Perrotta , F , Pettorino , V , Piacentini , F , Piat , M , Pierpaoli , E , Pietrobon , D , Plaszczynski , S , Pointecouteau , E , Polenta , G , Popa , L , Pratt , G W , Prézeau , G , Prunet , S , Puget , J L , Rachen , J P , Racine , B , Rebolo , R , Reinecke , M , Remazeilles , M , Renault , C , Renzi , A , Ristorcelli , I , Rocha , G , Rosset , C , Rossetti , M , Roudier , G , Rubinõ-Martín , J A , Rusholme , B , Sandri , M , Santos , D , Savelainen , M , Savini , G , Scott , D , Seiffert , M D , Shellard , E P S , Shiraishi , M , Smith , K , Spencer , L D , Stolyarov , V , Stompor , R , Sudiwala , R , Sunyaev , R , Sutter , P , Sutton , D , Suur-Uski , A S , Sygnet , J F , Tauber , J A , Terenzi , L , Toffolatti , L , Tomasi , M , Tristram , M , Troja , A , Tucci , M , Tuovinen , J , Valenziano , L , Väliviita , J , Van Tent , B , Vielva , P , Villa , F , Wade , L A , Wandelt , B D , Wehus , I K , Yvon , D , Zacchei , A & Zonca , A 2016 , ' Planck 2015 results : XVII. Constraints on primordial non-Gaussianity ' , Astronomy and Astrophysics , vol. 594 , A17 . https://doi.org/10.1051/0004-6361/201525836 |
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Abstract:The Planck full mission cosmic microwave background (CMB) temperature and E-mode polarization maps are analysed to obtain constraints on primordial non-Gaussianity (NG). Using three classes of optimal bispectrum estimators-separable template-fitting (KSW), binned, and modal-we obtain consistent values for the primordial local, equilateral, and orthogonal bispectrum amplitudes, quoting as our final result from temperature alone local NL = 2.5 ± 5.7, equil NL=-16 ± 70, fNLlocal=2.5±5.7, fNLequil=-16±70, and ortho NL =-34 ± 32fNLortho=-34±33 (68% CL, statistical). Combining temperature and polarization data we obtain fNLlocal=0.8±5.0, fNLequil=-4±43, and fNLortho=-26±21local NL = 0.8 ± 5.0, equil NL=-4 ± 43, and ortho NL =-26 ± 21 (68% CL, statistical). The results are based on comprehensive cross-validation of these estimators on Gaussian and non-Gaussian simulations, are stable across component separation techniques, pass an extensive suite of tests, and are consistent with estimators based on measuring the Minkowski functionals of the CMB. The effect of time-domain de-glitching systematics on the bispectrum is negligible. In spite of these test outcomes we conservatively label the results including polarization data as preliminary, owing to a known mismatch of the noise model in simulations and the data. Beyond estimates of individual shape amplitudes, we present model-independent, three-dimensional reconstructions of the Planck CMB bispectrum and derive constraints on early universe scenarios that generate primordial NG, including general single-field models of inflation, axion inflation, initial state modifications, models producing parity-violating tensor bispectra, and directionally dependent vector models. We present a wide survey of scale-dependent feature and resonance models, accounting for the "look elsewhere" effect in estimating the statistical significance of features. We also look for isocurvature NG, and find no signal, but we obtain constraints that improve significantly with the inclusion of polarization. The primordial trispectrum amplitude in the local model is constrained to be glocal NL = (-0.9 ± 7.7) X 104(68% CL statistical), and we perform an analysis of trispectrum shapes beyond the local case. The global picture that emerges is one of consistency with the premises of the ΛCDM cosmology, namely that the structure we observe today was sourced by adiabatic, passive, Gaussian, and primordial seed perturbations.
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