Issue |
A&A
Volume 571, November 2014
Planck 2013 results
|
|
---|---|---|
Article Number | A16 | |
Number of page(s) | 66 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/201321591 | |
Published online | 29 October 2014 |
Planck 2013 results. XVI. Cosmological parameters
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,
Metsähovintie 114, 02540
Kylmälä,
Finland
3
African Institute for Mathematical Sciences,
6-8 Melrose Road, Muizenberg,
7950
Cape Town, South
Africa
4
Agenzia Spaziale Italiana Science Data Center, via del Politecnico
snc, 00133
Roma,
Italy
5
Agenzia Spaziale Italiana, Viale Liegi 26,
00198
Roma,
Italy
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, 4000
Durban, South
Africa
8
Atacama Large Millimeter/submillimeter Array, ALMA Santiago
Central Offices, Alonso de Cordova 3107, Vitacura, Casilla 763 0355 ,
Santiago,
Chile
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
California Institute of Technology, Pasadena, California, USA
12
Centre for Theoretical Cosmology, DAMTP, University of
Cambridge, Wilberforce
Road, Cambridge
CB3 0WA,
UK
13
Centro de Estudios de Física del Cosmos de Aragón (CEFCA), Plaza
San Juan 1, planta 2, 44001
Teruel,
Spain
14
Computational Cosmology Center, Lawrence Berkeley National
Laboratory, Berkeley,
California,
USA
15
Consejo Superior de Investigaciones Científicas
(CSIC), 28006
Madrid,
Spain
16
DSM/Irfu/SPP, CEA-Saclay, 91191
Gif-sur-Yvette Cedex,
France
17
DTU Space, National Space Institute, Technical University of
Denmark, Elektrovej
327, 2800
Kgs. Lyngby,
Denmark
18
Département de Physique Théorique, Université de
Genève, 24 Quai E.
Ansermet, 1211
Genève 4,
Switzerland
19
Departamento de Física Fundamental, Facultad de Ciencias,
Universidad de Salamanca, 37008
Salamanca,
Spain
20
Departamento de Física, Universidad de Oviedo,
Avda. Calvo Sotelo s/n,
33007
Oviedo,
Spain
21
Department of Astronomy and Astrophysics, University of
Toronto, 50 Saint George Street,
Toronto, Ontario,
Canada
22
Department of Astrophysics/IMAPP, Radboud University
Nijmegen, PO Box
9010, 6500 GL
Nijmegen, The
Netherlands
23
Department of Electrical Engineering and Computer Sciences,
University of California, Berkeley, California, USA
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, New Jersey, USA
31
Department of Physics, University of California,
Berkeley, California, USA
32
Department of Physics, University of California,
One Shields Avenue,
Davis, California, USA
33
Department of Physics, University of California,
Santa Barbara, California, USA
34
Department of Physics, University of Illinois at
Urbana-Champaign, 1110 West Green
Street, Urbana,
Illinois,
USA
35
Dipartimento di Fisica e Astronomia G. Galilei, Università degli
Studi di Padova, via Marzolo
8, 35131
Padova,
Italy
36
Dipartimentodi Fisica e Scienze della Terra, Università di
Ferrara, via Saragat
1, 44122
Ferrara,
Italy
37
Dipartimento di Fisica, Università La Sapienza,
P.le A. Moro 2, 00185
Roma,
Italy
38
Dipartimento di Fisica, Università degli Studi di
Milano, via Celoria,
16, 20133
Milano,
Italy
39
Dipartimento di Fisica, Università degli Studi di
Trieste, via A. Valerio
2, 34127
Trieste,
Italy
40
Dipartimento di Fisica, Università di Roma Tor
Vergata, via della Ricerca
Scientifica, 1, 00133
Roma,
Italy
41
Discovery Center, Niels Bohr Institute,
Blegdamsvej 17, 2100
Copenhagen,
Denmark
42
Dpto. Astrofísica, Universidad de La Laguna (ULL),
38206, La Laguna, Tenerife, Spain
43
European Southern Observatory, ESO Vitacura, Alonso de Cordova 3107, Vitacura, Casilla
19001
Santiago,
Chile
44
European Space Agency, ESAC, Planck Science Office, Camino bajo
del Castillo, s/n, Urbanización Villafranca del Castillo, Villanueva de la
Cañada, 28691
Madrid,
Spain
45
European Space Agency, ESTEC, Keplerlaan 1,
2201 AZ
Noordwijk, The
Netherlands
46
Finnish Centre for Astronomy with ESO (FINCA), University of
Turku, Väisäläntie
20, 21500
Piikkiö,
Finland
47
Haverford College Astronomy Department,
370 Lancaster Avenue,
Haverford, Pennsylvania, USA
48
Helsinki Institute of Physics, Gustaf Hällströmin katu 2,
University of Helsinki, 00014
Helsinki,
Finland
49
INAF – Osservatorio Astrofisico di Catania, via S. Sofia
78, 95123
Catania,
Italy
50
INAF – Osservatorio Astronomico di Padova, Vicolo
dell’Osservatorio 5, 35122
Padova,
Italy
51
INAF – Osservatorio Astronomico di Roma, via di Frascati
33, 00040
Monte Porzio Catone,
Italy
52
INAF – Osservatorio Astronomico di Trieste, via G.B. Tiepolo
11, Trieste,
Italy
53
INAF Istituto di Radioastronomia, via P. Gobetti
101, 40129
Bologna,
Italy
54
INAF/IASF Bologna, via Gobetti 101, 40129
Bologna,
Italy
55
INAF/IASF Milano, via E. Bassini 15, 20133
Milano,
Italy
56
INFN, Sezione di Bologna, via Irnerio 46,
40126
Bologna,
Italy
57
INFN, Sezione di Roma 1, Università di Roma
Sapienza, Piazzale Aldo Moro
2, 00185
Roma,
Italy
58
IPAG: Institut de Planétologie et d’Astrophysique de Grenoble,
Université Joseph Fourier, Grenoble 1/CNRS-INSU, UMR 5274,
38041
Grenoble,
France
59
ISDC Data Centre for Astrophysics, University of
Geneva, ch. d’Ecogia
16, 1290
Versoix,
Switzerland
60
IUCAA, Post Bag 4, Ganeshkhind, Pune University
Campus, 411 007
Pune,
India
61
Imperial College London, Astrophysics group, Blackett
Laboratory, Prince Consort
Road, London,
SW7 2AZ,
UK
62
Infrared Processing and Analysis Center, California Institute of
Technology, Pasadena
CA
91125,
USA
63
Institut Néel, CNRS, Université Joseph Fourier Grenoble
I, 25 rue des
Martyrs, 38042
Grenoble,
France
64
Institut Universitaire de France, 103 bd Saint-Michel, 75005
Paris,
France
65
Institut d’Astrophysique Spatiale, CNRS UMR8617, Université
Paris-Sud 11, Bâtiment
121, 91405
Orsay,
France
66
Institut d’Astrophysique de Paris, CNRS UMR7095,
98bis Bd Arago, 75014
Paris,
France
67
Institute for Space Sciences, 077125
Bucharest-Magurale,
Romania
68
Institute of Astronomy and Astrophysics, Academia
Sinica, 106
Taipei,
Taiwan
69
Institute of Astronomy, University of Cambridge,
Madingley Road, Cambridge
CB3 0HA,
UK
70
Institute of Theoretical Astrophysics, University of
Oslo, Blindern,
0315
Oslo,
Norway
71
Instituto de Astrofísica de Canarias, C/vía Láctea s/n, 38200,
La Laguna, Tenerife,
Spain
72
Instituto de Física de Cantabria (CSIC-Universidad de
Cantabria), Avda. de los Castros
s/n, 39005
Santander,
Spain
73
Istituto di Fisica del Plasma, CNR-ENEA-EURATOM Association, via
R. Cozzi 53, 20125
Milano,
Italy
74
Jet Propulsion Laboratory, California Institute of
Technology, 4800 Oak Grove
Drive, Pasadena,
California,
USA
75
Jodrell Bank Centre for Astrophysics, Alan Turing Building, School
of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester
M13 9PL,
UK
76
Kavli Institute for Cosmology Cambridge,
Madingley Road, Cambridge
CB3 0HA,
UK
77
LAL, Université Paris-Sud, CNRS/IN2P3,
91405
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 de Cosmologie, Université
Joseph Fourier Grenoble I, CNRS/IN2P3, Institut National Polytechnique de
Grenoble, 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
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741
Garching,
Germany
85
McGill Physics, Ernest Rutherford Physics Building, McGill
University, 3600 rue University, Montréal, QC
H3A 2T8,
Canada
86
MilliLab, VTT Technical Research Centre of Finland, Tietotie
3, 02044
Espoo,
Finland
87
National University of Ireland, Department of Experimental
Physics, Maynooth,
Co. Kildare,
Ireland
88
Niels Bohr Institute, Blegdamsvej 17, 2100
Copenhagen,
Denmark
89
Observational Cosmology, Mail Stop 367-17, California Institute of
Technology, Pasadena
CA
91125,
USA
90
Optical Science Laboratory, University College
London, Gower
Street, London,
UK
91
SB-ITP-LPPC, EPFL, 1015, Lausanne,
Switzerland
92
SISSA, Astrophysics Sector, via Bonomea 265,
34136
Trieste,
Italy
93
School of Physics and Astronomy, Cardiff University,
Queens Buildings, The Parade,
Cardiff
CF24 3AA,
UK
94
School of Physics and Astronomy, University of
Nottingham, Nottingham
NG7 2RD,
UK
95
Space Research Institute (IKI), Russian Academy of
Sciences, Profsoyuznaya Str,
84/32, 117997
Moscow,
Russia
96
Space Sciences Laboratory, University of California,
Berkeley, California, USA
97
Special Astrophysical Observatory, Russian Academy of
Sciences, Nizhnij Arkhyz,
Zelenchukskiy region, 369167
Karachai-Cherkessian Republic,
Russia
98
Stanford University, Dept of Physics, Varian Physics Bldg, 382 via Pueblo
Mall, Stanford,
California,
USA
99
Sub-Department of Astrophysics, University of
Oxford, Keble Road,
Oxford
OX1 3RH,
UK
100
Theory Division, PH-TH, CERN, 1211, Geneva 23, Switzerland
101
UPMC Univ Paris 06, UMR7095, 98bis Boulevard Arago, 75014
Paris,
France
102
Université de Toulouse, UPS-OMP, IRAP, 31028
Toulouse Cedex 4,
France
103
Universities Space Research Association, Stratospheric Observatory
for Infrared Astronomy, MS
232-11, Moffett
Field
CA
94035,
USA
104
University Observatory, Ludwig Maximilian University of
Munich, Scheinerstrasse
1, 81679
Munich,
Germany
105
University of Granada, Departamento de Física Teórica y del
Cosmos, Facultad de Ciencias, 18071
Granada,
Spain
106
Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478
Warszawa,
Poland
Received: 28 March 2013
Accepted: 24 February 2014
This paper presents the first cosmological results based on Planck measurements of the cosmic microwave background (CMB) temperature and lensing-potential power spectra. We find that the Planck spectra at high multipoles (ℓ ≳ 40) are extremely well described by the standard spatially-flat six-parameter ΛCDM cosmology with a power-law spectrum of adiabatic scalar perturbations. Within the context of this cosmology, the Planck data determine the cosmological parameters to high precision: the angular size of the sound horizon at recombination, the physical densities of baryons and cold dark matter, and the scalar spectral index are estimated to be θ∗ = (1.04147 ± 0.00062) × 10-2, Ωbh2 = 0.02205 ± 0.00028, Ωch2 = 0.1199 ± 0.0027, and ns = 0.9603 ± 0.0073, respectively(note that in this abstract we quote 68% errors on measured parameters and 95% upper limits on other parameters). For this cosmology, we find a low value of the Hubble constant, H0 = (67.3 ± 1.2) km s-1 Mpc-1, and a high value of the matter density parameter, Ωm = 0.315 ± 0.017. These values are in tension with recent direct measurements of H0 and the magnitude-redshift relation for Type Ia supernovae, but are in excellent agreement with geometrical constraints from baryon acoustic oscillation (BAO) surveys. Including curvature, we find that the Universe is consistent with spatial flatness to percent level precision using Planck CMB data alone. We use high-resolution CMB data together with Planck to provide greater control on extragalactic foreground components in an investigation of extensions to the six-parameter ΛCDM model. We present selected results from a large grid of cosmological models, using a range of additional astrophysical data sets in addition to Planck and high-resolution CMB data. None of these models are favoured over the standard six-parameter ΛCDM cosmology. The deviation of the scalar spectral index from unity isinsensitive to the addition of tensor modes and to changes in the matter content of the Universe. We find an upper limit of r0.002< 0.11 on the tensor-to-scalar ratio. There is no evidence for additional neutrino-like relativistic particles beyond the three families of neutrinos in the standard model. Using BAO and CMB data, we find Neff = 3.30 ± 0.27 for the effective number of relativistic degrees of freedom, and an upper limit of 0.23 eV for the sum of neutrino masses. Our results are in excellent agreement with big bang nucleosynthesis and the standard value of Neff = 3.046. We find no evidence for dynamical dark energy; using BAO and CMB data, the dark energy equation of state parameter is constrained to be w = -1.13-0.10+0.13. We also use the Planck data to set limits on a possible variation of the fine-structure constant, dark matter annihilation and primordial magnetic fields. Despite the success of the six-parameter ΛCDM model in describing the Planck data at high multipoles, we note that this cosmology does not provide a good fit to the temperature power spectrum at low multipoles. The unusual shape of the spectrum in the multipole range 20 ≲ ℓ ≲ 40 was seen previously in the WMAP data and is a real feature of the primordial CMB anisotropies. The poor fit to the spectrum at low multipoles is not of decisive significance, but is an “anomaly” in an otherwise self-consistent analysis of the Planck temperature data.
Key words: cosmic background radiation / cosmological parameters / early Universe / inflation / primordial nucleosynthesis
© ESO, 2014
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