Issue |
A&A
Volume 594, October 2016
Planck 2015 results
|
|
---|---|---|
Article Number | A17 | |
Number of page(s) | 66 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/201525836 | |
Published online | 20 September 2016 |
Planck 2015 results
XVII. Constraints on primordial non-Gaussianity
1 APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, 10 rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
2 Aalto University Metsähovi Radio Observatory and Dept of Radio Science and Engineering, PO Box 13000, 00076 Aalto, Finland
3 African Institute for Mathematical Sciences, 6-8 Melrose Road, Muizenberg 7945, Cape Town, South Africa
4 Agenzia Spaziale Italiana Science Data Center, via del Politecnico snc, 00133 Roma, Italy
5 Aix-Marseille Université, CNRS, LAM (Laboratoire d’Astrophysique de Marseille) UMR 7326, 13388 Marseille, France
6 Astrophysics Group, Cavendish Laboratory, University of Cambridge, J J Thomson Avenue, Cambridge CB3 0HE, UK
7 Astrophysics & Cosmology Research Unit, School of Mathematics, Statistics & Computer Science, University of KwaZulu-Natal, Westville Campus, Private Bag X54001, Durban 4000, South Africa
8 CGEE, SCS Qd 9, Lote C, Torre C, 4° andar, Ed. Parque Cidade Corporate, 70308-200 Brasília, DF, Brazil
9 CITA,University of Toronto, 60 St. George St., Toronto, ON M5S 3H8, Canada
10 CNRS, IRAP, 9 Av. colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France
11 CRANN, Trinity College, Dublin, Ireland
12 California Institute of Technology, Pasadena, CA 91125, USA
13 Centre for Theoretical Cosmology, DAMTP, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK
14 Centro de Estudios de Física del Cosmos de Aragón (CEFCA), Plaza San Juan, 1, planta 2, 44001 Teruel, Spain
15 Computational Cosmology Center, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA
16 Consejo Superior de Investigaciones Científicas (CSIC), 28006 Madrid, Spain
17 DSM/Irfu/SPP, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
18 DTU Space, National Space Institute, Technical University of Denmark, Elektrovej 327, 2800 Kgs. Lyngby, Denmark
19 Département de Physique Théorique, Université de Genève, 24 quai E. Ansermet, 1211 Genève 4, Switzerland
20 Departamento de Astrofísica, Universidad de La Laguna (ULL), 38206 La Laguna, Tenerife, Spain
21 Departamento de Física, Universidad de Oviedo, Avda. Calvo Sotelo s/n, 33007 Oviedo, Spain
22 Department of Astronomy and Astrophysics, University of Toronto, 50 Saint George Street, Toronto, Ontario, Canada
23 Department of Astrophysics/IMAPP, Radboud University Nijmegen, PO Box 9010, 6500 GL Nijmegen, The Netherlands
24 Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia, Canada
25 Department of Physics and Astronomy, Dana and David Dornsife College of Letter, Arts and Sciences, University of Southern California, Los Angeles, CA 90089, USA
26 Department of Physics and Astronomy, University College London, London WC1E 6BT, UK
27 Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, UK
28 Department of Physics, Florida State University, Keen Physics Building, 77 Chieftan Way, Tallahassee, Florida, USA
29 Department of Physics, Gustaf Hällströmin katu 2a, University of Helsinki, 00014 Helsinki, Finland
30 Department of Physics, Princeton University, Princeton, NJ 08544, USA
31 Department of Physics, University of California, Santa Barbara, CA 93106, USA
32 Department of Physics, University of Illinois at Urbana-Champaign, 1110 West Green Street, Urbana, Illinois, USA
33 Dipartimento di Fisica e Astronomia G. Galilei, Università degli Studi di Padova, via Marzolo 8, 35131 Padova, Italy
34 Dipartimento di Fisica e Astronomia, Alma Mater Studiorum, Università degli Studi di Bologna, viale Berti Pichat 6/2, 40127 Bologna, Italy
35 Dipartimento di Fisica e Scienze della Terra, Università di Ferrara, via Saragat 1, 44122 Ferrara, Italy
36 Dipartimento di Fisica, Università La Sapienza, P.le A. Moro 2, 00185 Roma, Italy
37 Dipartimento di Fisica, Università degli Studi di Milano, via Celoria 16, 20133 Milano, Italy
38 Dipartimento di Fisica, Università degli Studi di Trieste, via A. Valerio 2, 34127 Trieste, Italy
39 Dipartimento di Matematica, Università di Roma Tor Vergata, via della Ricerca Scientifica 1, 00133 Roma, Italy
40 Discovery Center, Niels Bohr Institute, Blegdamsvej 17, 2100 Copenhagen, Denmark
41 Discovery Center, Niels Bohr Institute, Copenhagen University, Blegdamsvej 17, 2100 Copenhagen, Denmark
42 European Space Agency, ESAC, Planck Science Office, Camino bajo del Castillo, s/n, Urbanización Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain
43 European Space Agency, ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
44 Gran Sasso Science Institute, INFN, viale F. Crispi 7, 67100 L’ Aquila, Italy
45 HGSFP and University of Heidelberg, Theoretical Physics Department, Philosophenweg 16, 69120 Heidelberg, Germany
46 Helsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, 00014 Helsinki, Finland
47 ICTP South American Institute for Fundamental Research, Instituto de Física Teórica, Universidade Estadual Paulista, 01140-070 São Paulo, Brazil
48 INAF–Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, 35122 Padova, Italy
49 INAF–Osservatorio Astronomico di Roma, via di Frascati 33, 00040 Monte Porzio Catone, Italy
50 INAF–Osservatorio Astronomico di Trieste, via G.B. Tiepolo 11, 40127 Trieste, Italy
51 INAF/IASF Bologna, via Gobetti 101, 40129 Bologna, Italy
52 INAF/IASF Milano, via E. Bassini 15, 20133 Milano, Italy
53 INFN, Sezione di Bologna, via Irnerio 46, 40126 Bologna, Italy
54 INFN, Sezione di Roma 1, Università di Roma Sapienza, P.le Aldo Moro 2, 00185 Roma, Italy
55 INFN, Sezione di Roma 2, Università di RomaTor Vergata, via della Ricerca Scientifica 1, 00185 Roma, Italy
56 INFN/National Institute for Nuclear Physics, via Valerio 2, 34127 Trieste, Italy
57 IPAG: Institut de Planétologie et d’Astrophysique de Grenoble, Université Grenoble Alpes, IPAG, CNRS, IPAG, 38000 Grenoble, France
58 IUCAA, Post Bag 4, Ganeshkhind, Pune University Campus, 411 007 Pune, India
59 Imperial College London, Astrophysics group, Blackett Laboratory, Prince Consort Road, London, SW7 2AZ, UK
60 Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA
61 Institut Néel, CNRS, Université Joseph Fourier Grenoble I, 25 rue des Martyrs, Grenoble, France
62 Institut Universitaire de France, 103 bd Saint-Michel, 75005 Paris, France
63 Institut d’Astrophysique Spatiale, CNRS, Univ. Paris-Sud, Université Paris-Saclay, Bât. 121, 91405 Orsay Cedex, France
64 Institut d’Astrophysique de Paris, CNRS (UMR 7095), 98bis boulevard Arago, 75014 Paris, France
65 Institut für Theoretische Teilchenphysik und Kosmologie, RWTH Aachen University, 52056 Aachen, Germany
66 Institute for Space Sciences, 077125 Bucharest-Magurale, Romania
67 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
68 Institute of Theoretical Astrophysics, University of Oslo, Blindern, 0371 Oslo, Norway
69 Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, La Laguna, 38205 Tenerife, Spain
70 Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avda. de los Castros s/n, 39005 Santander, Spain
71 Istituto Nazionale di Fisica Nucleare, Sezione di Padova, via Marzolo 8, 35131 Padova, Italy
72 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 31109, USA
73 Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, UK
74 Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA
75 Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
76 Kazan Federal University, 18 Kremlyovskaya St., 420008 Kazan, Russia
77 LAL, Université Paris-Sud, CNRS/IN2P3, 91898 Orsay, France
78 LERMA, CNRS, Observatoire de Paris, 61 avenue de l’Observatoire, 75014 Paris, France
79 Laboratoire AIM, IRFU/Service d’Astrophysique – CEA/DSM – CNRS – Université Paris Diderot, Bât. 709, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
80 Laboratoire Traitement et Communication de l’Information, CNRS (UMR 5141) and Télécom ParisTech, 46 rue Barrault, 75634 Paris Cedex 13, France
81 Laboratoire de Physique Subatomique et Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3, 53 rue des Martyrs, 38026 Grenoble Cedex, France
82 Laboratoire de Physique Théorique, Université Paris-Sud 11 & CNRS, Bâtiment 210, 91405 Orsay, France
83 Lawrence Berkeley National Laboratory, Berkeley, California, USA
84 Lebedev Physical Institute of the Russian Academy of Sciences, Astro Space Centre, 84/32 Profsoyuznaya st., GSP-7, 117997 Moscow, Russia
85 Leung Center for Cosmology and Particle Astrophysics, National Taiwan University, Taipei 10617, Taiwan
86 Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching, Germany
87 McGill Physics, Ernest Rutherford Physics Building, McGill University, 3600 rue University, Montréal, QC, H3A 2T8, Canada
88 National University of Ireland, Department of Experimental Physics, Maynooth, Co. Kildare, Ireland
89 Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw, Poland
90 Niels Bohr Institute, Blegdamsvej 17, 2100 Copenhagen, Denmark
91 Niels Bohr Institute, Copenhagen University, Blegdamsvej 17, 2100 Copenhagen, Denmark
92 Nordita (Nordic Institute for Theoretical Physics), Roslagstullsbacken 23, 106 91 Stockholm, Sweden
93 Optical Science Laboratory, University College London, Gower Street, WC1E 6 BT London, UK
94 Perimeter Institute for Theoretical Physics, Waterloo ON N2L 2Y5, Canada
95 SISSA, Astrophysics Sector, via Bonomea 265, 34136 Trieste, Italy
96 SMARTEST Research Centre, Università degli Studi e-Campus, via Isimbardi 10, 22060 Novedrate (CO), Italy
97 School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, UK
98 School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, UK
99 Sorbonne Université-UPMC, UMR 7095, Institut d’Astrophysique de Paris, 98bis boulevard Arago, 75014 Paris, France
100 Space Research Institute (IKI), Russian Academy of Sciences, Profsoyuznaya Str, 84/32, 117997 Moscow, Russia
101 Space Sciences Laboratory, University ofCalifornia, Berkeley, CA 94720, USA
102 Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnij Arkhyz, Zelenchukskiy region, 369167 Karachai-Cherkessian Republic, Russia
103 Stanford University, Dept of Physics, Varian Physics Bldg, 382 via Pueblo Mall, Stanford, California, CA 94305-4060, USA
104 Sub-Department of Astrophysics, University of Oxford, Keble Road, Oxford OX1 3RH, UK
105 Sydney Institute for Astronomy, School of Physics A28, University of Sydney, NSW 2006, Australia
106 The Oskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, AlbaNova, 106 91 Stockholm, Sweden
107 Theory Division, PH-TH, CERN, 1211 Geneva 23, Switzerland
108 UPMC Univ. Paris 06, UMR 7095, 98bis boulevard Arago, 75014 Paris, France
109 Université de Toulouse, UPS-OMP, IRAP, 31028 Toulouse Cedex 4, France
110 University of Granada, Departamento de Física Teórica y del Cosmos, Facultad de Ciencias, 18071 Granada, Spain
111 University of Granada, Instituto Carlos I de Física Teórica y Computacional, 18071 Granada, Spain
112 Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478 Warszawa, Poland
⋆
Corresponding author: Nicola Bartolo, e-mail: bartolo@pd.infn.it
Received: 6 February 2015
Accepted: 27 January 2016
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 ƒlocalNL = 2.5 ± 5.7, ƒequilNL= -16 ± 70, , and ƒorthoNL = -34 ± 32 (68% CL, statistical). Combining temperature and polarization data we obtain ƒlocalNL = 0.8 ± 5.0, ƒequilNL= -4 ± 43, and ƒorthoNL = -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 𝓰localNL = (-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.
Key words: cosmic background radiation / cosmology: observations / cosmology: theory / early Universe / inflation / methods: data analysis
© ESO, 2016
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