Publications

BibTex format

@article{Aghanim:2020:0004-6361/201833910,
author = {Aghanim, N and Akrami, Y and Ashdown, M and Aumont, J and Baccigalupi, C and Ballardini, M and Banday, AJ and Barreiro, RB and Bartolo, N and Basak, S and Battye, R and Benabed, K and Bernard, J-P and Bersanelli, M and Bielewicz, P and Bock, JJ and Bond, JR and Borrill, J and Bouchet, FR and Boulanger, F and Bucher, M and Burigana, C and Butler, RC and Calabrese, E and Cardoso, J-F and Carron, J and Challinor, A and Chiang, HC and Chluba, J and Colombo, LPL and Combet, C and Contreras, D and Crill, BP and Cuttaia, F and de, Bernardis P and de, Zotti G and Delabrouille, J and Delouis, J-M and Di, Valentino E and Diego, JM and Doré, O and Douspis, M and Ducout, A and Dupac, X and Dusini, S and Efstathiou, G and Elsner, F and Enßlin, TA and Eriksen, HK and Fantaye, Y and Farhang, M and Fergusson, J and Fernandez-Cobos, R and Finelli, F and Forastieri, F and Frailis, M and Fraisse, AA and Franceschi, E and Frolov, A and Galeotta, S and Galli, S and Ganga, K and Génova-Santos, RT and Gerbin},
doi = {0004-6361/201833910},
journal = {Astronomy & Astrophysics},
pages = {A6--A6},
title = {Planck 2018 results: cosmological parameters},
url = {http://dx.doi.org/10.1051/0004-6361/201833910},
volume = {641},
year = {2020}
}

Download

RIS format (EndNote, RefMan)

TY  - JOUR
AB  - We present cosmological parameter results from the final full-mission Planck measurements of the cosmic microwave background (CMB) anisotropies, combining information from the temperature and polarization maps and the lensing reconstruction. Compared to the 2015 results, improved measurements of large-scale polarization allow the reionization optical depth to be measured with higher precision, leading to significant gains in the precision of other correlated parameters. Improved modelling of the small-scale polarization leads to more robust constraints on many parameters, with residual modelling uncertainties estimated to affect them only at the 0.5σ level. We find good consistency with the standard spatially-flat 6-parameter ΛCDM cosmology having a power-law spectrum of adiabatic scalar perturbations (denoted “base ΛCDM” in this paper), from polarization, temperature, and lensing, separately and in combination. A combined analysis gives dark matter density Ωch2=0.120±0.001, baryon density Ωbh2=0.0224±0.0001, scalar spectral index ns=0.965±0.004, and optical depth τ=0.054±0.007 (in this abstract we quote 68% confidence regions on measured parameters and 95% on upper limits). The angular acoustic scale is measured to 0.03% precision, with 100θ=1.0411±0.0003. These results are only weakly dependent on the cosmological model and remain stable, with somewhat increased errors, in many commonly considered extensions. Assuming the base-ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H0=(67.4±0.5)kms−1Mpc−1; matter density parameter Ωm=0.315±0.007; and matter fluctuation amplitude σ8=0.811±0.006. We find no compelling evidence for extensions to the base-ΛCDM model. Combining with baryon acoustic oscillation (BAO) measurements (and considering singl
AU  - Aghanim,N
AU  - Akrami,Y
AU  - Ashdown,M
AU  - Aumont,J
AU  - Baccigalupi,C
AU  - Ballardini,M
AU  - Banday,AJ
AU  - Barreiro,RB
AU  - Bartolo,N
AU  - Basak,S
AU  - Battye,R
AU  - Benabed,K
AU  - Bernard,J-P
AU  - Bersanelli,M
AU  - Bielewicz,P
AU  - Bock,JJ
AU  - Bond,JR
AU  - Borrill,J
AU  - Bouchet,FR
AU  - Boulanger,F
AU  - Bucher,M
AU  - Burigana,C
AU  - Butler,RC
AU  - Calabrese,E
AU  - Cardoso,J-F
AU  - Carron,J
AU  - Challinor,A
AU  - Chiang,HC
AU  - Chluba,J
AU  - Colombo,LPL
AU  - Combet,C
AU  - Contreras,D
AU  - Crill,BP
AU  - Cuttaia,F
AU  - de,Bernardis P
AU  - de,Zotti G
AU  - Delabrouille,J
AU  - Delouis,J-M
AU  - Di,Valentino E
AU  - Diego,JM
AU  - Doré,O
AU  - Douspis,M
AU  - Ducout,A
AU  - Dupac,X
AU  - Dusini,S
AU  - Efstathiou,G
AU  - Elsner,F
AU  - Enßlin,TA
AU  - Eriksen,HK
AU  - Fantaye,Y
AU  - Farhang,M
AU  - Fergusson,J
AU  - Fernandez-Cobos,R
AU  - Finelli,F
AU  - Forastieri,F
AU  - Frailis,M
AU  - Fraisse,AA
AU  - Franceschi,E
AU  - Frolov,A
AU  - Galeotta,S
AU  - Galli,S
AU  - Ganga,K
AU  - Génova-Santos,RT
AU  - Gerbino,M
AU  - Ghosh,T
AU  - González-Nuevo,J
AU  - Górski,KM
AU  - Gratton,S
AU  - Gruppuso,A
AU  - Gudmundsson,JE
AU  - Hamann,J
AU  - Handley,W
AU  - Hansen,FK
AU  - Herranz,D
AU  - Hildebrandt,SR
AU  - Hivon,E
AU  - Huang,Z
AU  - Jaffe,AH
AU  - Jones,WC
AU  - Karakci,A
AU  - Keihänen,E
AU  - Keskitalo,R
AU  - Kiiveri,K
AU  - Kim,J
AU  - Kisner,TS
AU  - Knox,L
AU  - Krachmalnicoff,N
AU  - Kunz,M
AU  - Kurki-Suonio,H
AU  - Lagache,G
AU  - Lamarre,J-M
AU  - Lasenby,A
AU  - Lattanzi,M
AU  - Lawrence,CR
AU  - Le,Jeune M
AU  - Lemos,P
AU  - Lesgourgues,J
AU  - Levrier,F
AU  - Lewis,A
AU  - Liguori,M
AU  - Lilje,PB
AU  - Lilley,M
AU  - Lindholm,V
AU  - López-Caniego,M
AU  - Lubin,PM
AU  - Ma,Y-Z
AU  - Macías-Pérez,JF
AU  - Maggio,G
AU  - Maino,D
AU  - Mandolesi,N
AU  - Mangilli,A
AU  - Marcos-Caballero,A
AU  - Maris,M
AU  - Martin,PG
AU  - Martinelli,M
AU  - Martínez-González,E
AU  - Matarrese,S
AU  - Mauri,N
AU  - McEwen,JD
AU  - Meinhold,PR
AU  - Melchiorri,A
AU  - Mennella,A
AU  - Migliaccio,M
AU  - Millea,M
AU  - Mitra,S
AU  - Miville-Deschênes,M-A
AU  - Molinari,D
AU  - Montier,L
AU  - Morgante,G
AU  - Moss,A
AU  - Natoli,P
AU  - Nørgaard-Nielsen,HU
AU  - Pagano,L
AU  - Paoletti,D
AU  - Partridge,B
AU  - Patanchon,G
AU  - Peiris,HV
AU  - Perrotta,F
AU  - Pettorino,V
AU  - Piacentini,F
AU  - Polastri,L
AU  - Polenta,G
AU  - Puget,J-L
AU  - Rachen,JP
AU  - Reinecke,M
AU  - Remazeilles,M
AU  - Renzi,A
AU  - Rocha,G
AU  - Rosset,C
AU  - Roudier,G
AU  - Rubiño-Martín,JA
AU  - Ruiz-Granados,B
AU  - Salvati,L
AU  - Sandri,M
AU  - Savelainen,M
AU  - Scott,D
AU  - Shellard,EPS
AU  - Sirignano,C
AU  - Sirri,G
AU  - Spencer,LD
AU  - Sunyaev,R
AU  - Suur-Uski,A-S
AU  - Tauber,JA
AU  - Tavagnacco,D
AU  - Tenti,M
AU  - Toffolatti,L
AU  - Tomasi,M
AU  - Trombe
DO  - 0004-6361/201833910
EP  - 6
PY  - 2020///
SN  - 0004-6361
SP  - 6
TI  - Planck 2018 results: cosmological parameters
T2  - Astronomy & Astrophysics
UR  - http://dx.doi.org/10.1051/0004-6361/201833910
UR  - https://www.aanda.org/articles/aa/abs/2020/09/aa33910-18/aa33910-18.html
UR  - http://hdl.handle.net/10044/1/82575
VL  - 641
ER  -

Download

Professor Andrew H Jaffe

Contact

Assistant

Location

Summary

Citation

BibTex format

RIS format (EndNote, RefMan)