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TI Planck 2018 results: VI. Cosmological parameters
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AF AGHANIM, N.
   AKRAMI, Y.
   ASHDOWN, M.
   AUMONT, J.
   BACCIGALUPI, C.
   BALLARDINI, M.
   BANDAY, A. J.
   BARREIRO, R. B.
   BARTOLO, N.
   BASAK, S.
   BATTYE, R.
   BENABED, K.
   BERNARD, J. -P.
   BERSANELLI, M.
   BIELEWICZ, P.
   BOCK, J. J.
   BOND, J. R.
   BORRILL, J.
   BOUCHET, F. R.
   BOULANGER, F.
   BUCHER, M.
   BURIGANA, C.
   BUTLER, R. C.
   CALABRESE, E.
   CARDOSO, J. -F.
   CARRON, J.
   CHALLINOR, A.
   CHIANG, H. C.
   CHLUBA, J.
   COLOMBO, L. P. L.
   COMBET, C.
   CONTRERAS, D.
   CRILL, B. P.
   CUTTAIA, F.
   DE BERNARDIS, P.
   DE ZOTTI, G.
   DELABROUILLE, J.
   DELOUIS, Jean Marc
   DI VALENTINO, E.
   DIEGO, J. M.
   DORE, O.
   DOUSPIS, M.
   DUCOUT, A.
   DUPAC, X.
   DUSINI, S.
   EFSTATHIOU, G.
   ELSNER, F.
   ENSSLIN, T. A.
   ERIKSEN, H. K.
   FANTAYE, Y.
   FARHANG, M.
   FERGUSSON, J.
   FERNANDEZ-COBOS, R.
   FINELLI, F.
   FORASTIERI, F.
   FRAILIS, M.
   FRAISSE, A. A.
   FRANCESCHI, E.
   FROLOV, A.
   GALEOTTA, S.
   GALLI, S.
   GANGA, K.
   GENOVA-SANTOS, R. T.
   GERBINO, M.
   GHOSH, T.
   GONZALEZ-NUEVO, J.
   GORSKI, K. M.
   GRATTON, S.
   GRUPPUSO, A.
   GUDMUNDSSON, J. E.
   HAMANN, J.
   HANDLEY, W.
   HANSEN, F. K.
   HERRANZ, D.
   HILDEBRANDT, S. R.
   HIVON, E.
   HUANG, Z.
   JAFFE, A. H.
   JONES, W. C.
   KARAKCI, A.
   KEIHANEN, E.
   KESKITALO, R.
   KIIVERI, K.
   KIM, J.
   KISNER, T. S.
   KNOX, L.
   KRACHMALNICO, N.
   KUNZ, M.
   KURKI-SUONIO, H.
   LAGACHE, G.
   LAMARRE, J. -M.
   LASENBY, A.
   LATTANZI, M.
   LAWRENCE, C. R.
   LE JEUNE, M.
   LEMOS, P.
   LESGOURGUES, J.
   LEVRIER, F.
   LEWIS, A.
   LIGUORI, M.
   LILJE, P. B.
   LILLEY, M.
   LINDHOLM, V.
   LOPEZ-CANIEGO, M.
   LUBIN, PM
   MA, Y. -Z.
   MACIAS-PEREZ, J. F.
   MAGGIO, G.
   MAINO, D.
   MANDOLESI, N.
   MANGILLI, A.
   MARCOS-CABALLERO, A.
   MARIS, M.
   MARTIN, PG
   MARTINELLI, M.
   MARTINEZ-GONZALEZ, E.
   MATARRESE, S.
   MAURI, N.
   MCEWEN, J. D.
   MEINHOLD, P. R.
   MELCHIORRI, A.
   MENNELLA, A.
   MIGLIACCIO, M.
   MILLEA, M.
   MITRA, S.
   MIVILLE-DESCHENES, M. -A.
   MOLINARI, D.
   MONTIER, L.
   MORGANTE, G.
   MOSS, A.
   NATOLI, P.
   NORGAARD-NIELSEN, H. U.
   PAGANO, L.
   PAOLETTI, D.
   PARTRIDGE, B.
   PATANCHON, G.
   PEIRIS, H. V.
   PERROTTA, F.
   PETTORINO, V.
   PIACENTINI, F.
   POLASTRI, L.
   POLENTA, G.
   PUGET, J. -L.
   RACHEN, J. P.
   REINECKE, M.
   REMAZEILLES, M.
   RENZI, A.
   ROCHA, G.
   ROSSET, C.
   ROUDIER, G.
   RUBINO-MARTIN, J. A.
   RUIZ-GRANADOS, B.
   SALVATI, L.
   SANDRI, M.
   SAVELAINEN, M.
   SCOTT, D.
   SHELLARD, E. P. S.
   SIRIGNANO, C.
   SIRRI, G.
   SPENCER, L. D.
   SUNYAEV, R.
   SUUR-USKI, A. -S.
   TAUBER, J. A.
   TAVAGNACCO, D.
   TENTI, M.
   TOFFOLATTI, L.
   TOMASI, M.
   TROMBETTI, T.
   VALENZIANO, L.
   VALIVIITA, J.
   VAN TENT, B.
   VIBERT, L.
   VIELVA, P.
   VILLA, F.
   VITTORIO, N.
   WANDELT, B. D.
   WEHUS, I. K.
   WHITE, M.
   WHITE, S. D. M.
   ZACCHEI, A.
   ZONCA, A.
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UM LOPS
IN WOS Cotutelle UMR
   copubli-france
   copubli-europe
   copubli-univ-france
   copubli-int-hors-europe
   copubli-sud
IF 5.802
TC 1762
UR https://archimer.ifremer.fr/doc/00654/76633/77785.pdf
   https://archimer.ifremer.fr/doc/00654/76633/88063.pdf
LA English
DT Article
DE ;cosmic background radiation;cosmological parameters
AB CDM at over 2 sigma, which pulls some parameters that affect the lensing amplitude away from the Lambda CDM model; however, this is not supported by the lensing reconstruction or (in models that also change the background geometry) BAO data. The joint constraint with BAO measurements on spatial curvature is consistent with a flat universe, Omega (K)=0.001 +/- 0.002. Also combining with Type Ia supernovae (SNe), the dark-energy equation of state parameter is measured to be w(0)=-1.03 +/- 0.03, consistent with a cosmological constant. We find no evidence for deviations from a purely power-law primordial spectrum, and combining with data from BAO, BICEP2, and Keck Array data, we place a limit on the tensor-to-scalar ratio r(0.002)< 0.06. Standard big-bang nucleosynthesis predictions for the helium and deuterium abundances for the base-CDM cosmology are in excellent agreement with observations. The Planck base-Lambda CDM results are in good agreement with BAO, SNe, and some galaxy lensing observations, but in slight tension with the Dark Energy Survey's combined-probe results including galaxy clustering (which prefers lower fluctuation amplitudes or matter density parameters), and in significant, 3.6 sigma, tension with local measurements of the Hubble constant (which prefer a higher value). Simple model extensions that can partially resolve these tensions are not favoured by the Planck data. 
PY 2020
PD SEP
SO Astronomy & Astrophysics
SN 0004-6361
PU Edp Sciences S A
VL 641
IS A6
UT 000571763700006
DI 10.1051/0004-6361/201833910
ID 76633
ER

EF