Issue |
A&A
Volume 641, September 2020
Planck 2018 results
|
|
---|---|---|
Article Number | A9 | |
Number of page(s) | 47 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/201935891 | |
Published online | 11 September 2020 |
Planck 2018 results
IX. Constraints on primordial non-Gaussianity
1
AIM, CEA, CNRS, Université Paris-Saclay, Université Paris-Diderot, Sorbonne Paris Cité, 91191 Gif-sur-Yvette, France
2
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
3
African Institute for Mathematical Sciences, 6-8 Melrose Road, Muizenberg, Cape Town, South Africa
4
Astrophysics Group, Cavendish Laboratory, University of Cambridge, J J Thomson Avenue, Cambridge CB3 0HE, UK
5
Astrophysics & Cosmology Research Unit, School of Mathematics, Statistics & Computer Science, University of KwaZulu-Natal, Westville Campus, Private Bag X54001, Durban 4000, South Africa
6
CITA, University of Toronto, 60 St. George St., Toronto, ON M5S 3H8, Canada
7
CNRS, IRAP, 9 Av. colonel Roche, BP 44346, 31028 Toulouse cedex 4, France
8
California Institute of Technology, Pasadena, CA, USA
9
Centre for Theoretical Cosmology, DAMTP, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK
10
Computational Cosmology Center, Lawrence Berkeley National Laboratory, Berkeley, CA, USA
11
Département de Physique Théorique, Université de Genève, 24 quai E. Ansermet, 1211 Genève 4, Switzerland
12
Département de Physique, École normale supérieure, PSL Research University, CNRS, 24 rue Lhomond, 75005 Paris, France
13
Departamento de Astrofísica, Universidad de La Laguna (ULL), 38206 La Laguna, Tenerife, Spain
14
Departamento de Física, Universidad de Oviedo, C/ Federico García Lorca, 18, Oviedo, Spain
15
Department of Astrophysics/IMAPP, Radboud University, PO Box 9010, 6500 GL Nijmegen, The Netherlands
16
Department of General Education, National Institute of Technology, Kagawa College, 355 Chokushi-cho, Takamatsu, Kagawa 761-8058, Japan
17
Department of Mathematics, University of Stellenbosch, Stellenbosch 7602, South Africa
18
Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia, Canada
19
Department of Physics & Astronomy, University of the Western Cape, Cape Town 7535, South Africa
20
Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, UK
21
Department of Physics, Gustaf Hällströmin katu 2a, University of Helsinki, Helsinki, Finland
22
Department of Physics, Princeton University, Princeton, NJ, USA
23
Department of Physics, University of California, Santa Barbara, CA, USA
24
Dipartimento di Fisica e Astronomia G. Galilei, Università degli Studi di Padova, Via Marzolo 8, 35131 Padova, Italy
25
Dipartimento di Fisica e Scienze della Terra, Università di Ferrara, Via Saragat 1, 44122 Ferrara, Italy
26
Dipartimento di Fisica, Università La Sapienza, P.le A. Moro 2, Roma, Italy
27
Dipartimento di Fisica, Università degli Studi di Milano, Via Celoria, 16, Milano, Italy
28
Dipartimento di Fisica, Università degli Studi di Trieste, Via A. Valerio 2, Trieste, Italy
29
Dipartimento di Fisica, Università di Roma Tor Vergata, Via della Ricerca Scientifica, 1, Roma, Italy
30
European Space Agency, ESAC, Planck Science Office, Camino bajo del Castillo, s/n, Urbanización Villafranca del Castillo, Villanueva de la Cañada, Madrid, Spain
31
European Space Agency, ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
32
Gran Sasso Science Institute, INFN, viale F. Crispi 7, 67100 L’Aquila, Italy
33
HEP Division, Argonne National Laboratory, Lemont, IL 60439, USA
34
Haverford College Astronomy Department, 370 Lancaster Avenue, Haverford, PA, USA
35
Helsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland
36
INAF – OAS Bologna, Istituto Nazionale di Astrofisica – Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Area della Ricerca del CNR, Via Gobetti 101, 40129 Bologna, Italy
37
INAF – Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, Padova, Italy
38
INAF – Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, Trieste, Italy
39
INAF, Istituto di Radioastronomia, Via Piero Gobetti 101, 40129 Bologna, Italy
40
INAF/IASF Milano, Via E. Bassini 15, Milano, Italy
41
INFN – CNAF, viale Berti Pichat 6/2, 40127 Bologna, Italy
42
INFN, Sezione di Bologna, viale Berti Pichat 6/2, 40127 Bologna, Italy
43
INFN, Sezione di Ferrara, Via Saragat 1, 44122 Ferrara, Italy
44
INFN, Sezione di Milano, Via Celoria 16, Milano, Italy
45
INFN, Sezione di Roma 1, Università di Roma Sapienza, Piazzale Aldo Moro 2, 00185 Roma, Italy
46
INFN, Sezione di Roma 2, Università di Roma Tor Vergata, Via della Ricerca Scientifica, 1, Roma, Italy
47
Imperial College London, Astrophysics group, Blackett Laboratory, Prince Consort Road, London SW7 2AZ, UK
48
Institut d’Astrophysique Spatiale, CNRS, Univ. Paris-Sud, Université Paris-Saclay, Bât. 121, 91405 Orsay cedex, France
49
Institut d’Astrophysique de Paris, CNRS (UMR7095), 98bis boulevard Arago, 75014 Paris, France
50
Institute Lorentz, Leiden University, PO Box 9506, 2300 RA Leiden, The Netherlands
51
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
52
Institute of Theoretical Astrophysics, University of Oslo, Blindern, Oslo, Norway
53
Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, La Laguna, Tenerife, Spain
54
Instituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências da Universidade de Lisboa, Campo Grande, 1749-016 Lisboa, Portugal
55
Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avda. de los Castros s/n, Santander, Spain
56
Istituto Nazionale di Fisica Nucleare, Sezione di Padova, Via Marzolo 8, 35131 Padova, Italy
57
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, USA
58
Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester M13 9PL, UK
59
Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge CB3 0HA, UK
60
Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI), UTIAS, The University of Tokyo, Chiba 277- 8583, Japan
61
Laboratoire d’Océanographie Physique et Spatiale (LOPS), Univ. Brest, CNRS, Ifremer, IRD, Brest, France
62
Laboratoire de Physique Subatomique et Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3, 53 rue des Martyrs, 38026 Grenoble Cedex, France
63
Laboratoire de Physique Théorique, Université Paris-Sud 11 & CNRS, Bâtiment 210, 91405 Orsay, France
64
Low Temperature Laboratory, Department of Applied Physics, Aalto University, Espoo 00076, Finland
65
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching, Germany
66
Mullard Space Science Laboratory, University College London, Surrey RH5 6NT, UK
67
NAOC-UKZN Computational Astrophysics Centre (NUCAC), University of KwaZulu-Natal, Durban 4000, South Africa
68
National Centre for Nuclear Research, ul. L. Pasteura 7, 02-093 Warsaw, Poland
69
Perimeter Institute for Theoretical Physics, Waterloo, ON N2L 2Y5, Canada
70
Purple Mountain Observatory, No. 8 Yuan Hua Road, 210034 Nanjing, PR China
71
SISSA, Astrophysics Sector, Via Bonomea 265, 34136 Trieste, Italy
72
San Diego Supercomputer Center, University of California, San Diego, 9500 Gilman Drive, La Jolla CA, 92093, USA
73
School of Chemistry and Physics, University of KwaZulu-Natal, Westville Campus, Private Bag X54001, Durban 4000, South Africa
74
School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff CF24 3AA, UK
75
School of Physics and Astronomy, Sun Yat-sen University, 2 Daxue Rd, Tangjia, Zhuhai, PR China
76
School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, UK
77
School of Physics, Indian Institute of Science Education and Research Thiruvananthapuram, Maruthamala PO, Vithura, Thiruvananthapuram, 695551 Kerala, India
78
School of Physics, The University of New South Wales, Sydney, NSW 2052, Australia
79
Simon Fraser University, Department of Physics, 8888 University Drive, Burnaby, BC, Canada
80
Sorbonne Université, Observatoire de Paris, Université PSL, École normale supérieure, CNRS, LERMA, 75005 Paris, France
81
Sorbonne Université, UMR7095, Institut d’Astrophysique de Paris, 98bis boulevard Arago, 75014 Paris, France
82
Space Research Institute (IKI), Russian Academy of Sciences, Profsoyuznaya Str, 84/32, Moscow 117997, Russia
83
Space Science Data Center – Agenzia Spaziale Italiana, Via del Politecnico snc, 00133 Roma, Italy
84
Space Sciences Laboratory, University of California, Berkeley, CA, USA
85
The Oskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, AlbaNova, 106 91 Stockholm, Sweden
86
Université de Toulouse, UPS-OMP, IRAP, 31028 Toulouse Cedex 4, France
87
Van Swinderen Institute for Particle Physics and Gravity, University of Groningen, Nijenborgh 4, 9747 AG Groningen, The Netherlands
88
Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478 Warszawa, Poland
Received:
15
May
2019
Accepted:
5
November
2019
We analyse the Planck full-mission cosmic microwave background (CMB) temperature and E-mode polarization maps to obtain constraints on primordial non-Gaussianity (NG). We compare estimates obtained from separable template-fitting, binned, and optimal modal bispectrum estimators, finding consistent values for the local, equilateral, and orthogonal bispectrum amplitudes. Our combined temperature and polarization analysis produces the following final results: fNLlocal = −0.9 ± 5.1; fNLequil = −26 ± 47; and fNLortho = −38 ± 24 (68% CL, statistical). These results include low-multipole (4 ≤ ℓ < 40) polarization data that are not included in our previous analysis. The results also pass an extensive battery of tests (with additional tests regarding foreground residuals compared to 2015), and they are stable with respect to our 2015 measurements (with small fluctuations, at the level of a fraction of a standard deviation, which is consistent with changes in data processing). Polarization-only bispectra display a significant improvement in robustness; they can now be used independently to set primordial NG constraints with a sensitivity comparable to WMAP temperature-based results and they give excellent agreement. In addition to the analysis of the standard local, equilateral, and orthogonal bispectrum shapes, we consider a large number of additional cases, such as scale-dependent feature and resonance bispectra, isocurvature primordial NG, and parity-breaking models, where we also place tight constraints but do not detect any signal. The non-primordial lensing bispectrum is, however, detected with an improved significance compared to 2015, excluding the null hypothesis at 3.5σ. Beyond estimates of individual shape amplitudes, we also present model-independent reconstructions and analyses of the Planck CMB bispectrum. Our final constraint on the local primordial trispectrum shape is gNLlocal = (−5.8 ± 6.5) × 104 (68% CL, statistical), while constraints for other trispectrum shapes are also determined. Exploiting the tight limits on various bispectrum and trispectrum shapes, we constrain the parameter space of different early-Universe scenarios that generate primordial NG, including general single-field models of inflation, multi-field models (e.g. curvaton models), models of inflation with axion fields producing parity-violation bispectra in the tensor sector, and inflationary models involving vector-like fields with directionally-dependent bispectra. Our results provide a high-precision test for structure-formation scenarios, showing complete agreement with the basic picture of the ΛCDM cosmology regarding the statistics of the initial conditions, with cosmic structures arising from adiabatic, passive, Gaussian, and primordial seed perturbations.
Key words: cosmic background radiation / cosmology: observations / cosmology: theory / early Universe / inflation / methods: data analysis
© ESO 2020
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