Planck 2015 results. XIII. Cosmological parameters

We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. These data are consistent with the six-parameter inflationary LCDM cosmology. From the Planck temperature and lensing data, for this cosmology we find a Hubble constant, H0= (67.8 +/...

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Detalles Bibliográficos
Autores principales: Ade, P.A.R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A.J., Barreiro, R.B., Bartlett, J.G., Bartolo, N., Battaner, E., Battye, R., Benabed, K., Benoit, A., Benoit-Levy, A., Bernard, J.P., Bersanelli, M., Bielewicz, P., Bonaldi, A., Bonavera, L., Bond, J.R., Borrill, J., Bouchet, F.R., Boulanger, F., Bucher, M., Burigana, C., Butler, R.C., Calabrese, E., Cardoso, J.F., Catalano, A., Challinor, A., Chamballu, A., Chary, R.R., Chiang, H.C., Chluba, J., Christensen, P.R., Church, S., Clements, D.L., Colombi, S., Colombo, L.P.L., Combet, C., Coulais, A., Crill, B.P., Curto, A., Cuttaia, F., Danese, L., Davies, R.D., Davis, R.J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Desert, F.X., Di Valentino, E., Dickinson, C., Diego, J.M., Dolag, K., Dole, H., Donzelli, S., Dore, O., Douspis, M., Ducout, A., Dunkley, J., Dupac, X., Efstathiou, G., Elsner, F., Ensslin, T.A., Eriksen, H.K., Farhang, M., Fergusson, J., Finelli, F., Forni, O., Frailis, M., Fraisse, A.A., Franceschi, E., Frejsel, A., Galeotta, S., Galli, S., Ganga, K., Gauthier, C., Gerbino, M., Ghosh, T., Giard, M., Giraud-Heraud, Y., Giusarma, E., Gjerlow, E., Gonzalez-Nuevo, J., Gorski, K.M., Gratton, S., Gregorio, A., Gruppuso, A., Gudmundsson, J.E., Hamann, J., Hansen, F.K., Hanson, D., Harrison, D.L., Helou, G., Henrot-Versille, S., Hernandez-Monteagudo, C., Herranz, D., Hildebrandt, S.R., Hivon, E., Hobson, M., Holmes, W.A., Hornstrup, A., Hovest, W., Huang, Z., Huffenberger, K.M., Hurier, G., Jaffe, A.H., Jaffe, T.R., Jones, W.C., Juvela, M., Keihanen, E., Keskitalo, R., Kisner, T.S., Kneissl, R., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lahteenmaki, A., Lamarre, J.M., Lasenby, A., Lattanzi, M., Lawrence, C.R., Leahy, J.P., Leonardi, R., Lesgourgues, J., Levrier, F., Lewis, A., Liguori, M., Lilje, P.B., Linden-Vornle, M., Lopez-Caniego, M., Lubin, P.M., Macias-Perez, J.F., Maggio, G., Mandolesi, N., Mangilli, A., Marchini, A., Martin, P.G., Martinelli, M., Martinez-Gonzalez, E., Masi, S., Matarrese, S., Mazzotta, P., McGehee, P., Meinhold, P.R., Melchiorri, A., Melin, J.B., Mendes, L., Mennella, A., Migliaccio, M., Millea, M., Mitra, S., Miville-Deschenes, M.A., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Murphy, J.A., Naselsky, P., Nati, F., Natoli, P., Netterfield, C.B., Norgaard-Nielsen, H.U., Noviello, F., Novikov, D., Novikov, I., Oxborrow, C.A., Paci, F., Pagano, L., Pajot, F., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, T.J., Perdereau, O., Perotto, L., Perrotta, F., Pettorino, V., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Popa, L., Pratt, G.W., Prezeau, G., Prunet, S., Puget, J.L., Rachen, J.P., Reach, W.T., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Ristorcelli, I., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., d'Orfeuil, B.Rouille, Rowan-Robinson, M., Rubino-Martin, J.A., Rusholme, B., Said, N., Salvatelli, V., Salvati, L., Sandri, M., Santos, D., Savelainen, M., Savini, G., Scott, D., Seiffert, M.D., Serra, P., Shellard, E.P.S., Spencer, L.D., Spinelli, M., Stolyarov, V., Stompor, R., Sudiwala, R., Sunyaev, R., Sutton, D., Suur-Uski, A.S., Sygnet, J.F., Tauber, J.A., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Trombetti, T., Tucci, M., Tuovinen, J., Turler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L.A., Wandelt, B.D., Wehus, I.K., White, M., White, S.D.M., Wilkinson, A., Yvon, D., Zacchei, A., Zonca, A.
Lenguaje:eng
Publicado: 2015
Materias:
Astrophysics and Astronomy
Acceso en línea:https://dx.doi.org/10.1051/0004-6361/201525830
http://cds.cern.ch/record/1987166
_version_ 1780945481356017664
author Ade, P.A.R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A.J.
Barreiro, R.B.
Bartlett, J.G.
Bartolo, N.
Battaner, E.
Battye, R.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J.P.
Bersanelli, M.
Bielewicz, P.
Bonaldi, A.
Bonavera, L.
Bond, J.R.
Borrill, J.
Bouchet, F.R.
Boulanger, F.
Bucher, M.
Burigana, C.
Butler, R.C.
Calabrese, E.
Cardoso, J.F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chary, R.R.
Chiang, H.C.
Chluba, J.
Christensen, P.R.
Church, S.
Clements, D.L.
Colombi, S.
Colombo, L.P.L.
Combet, C.
Coulais, A.
Crill, B.P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R.D.
Davis, R.J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F.X.
Di Valentino, E.
Dickinson, C.
Diego, J.M.
Dolag, K.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dunkley, J.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T.A.
Eriksen, H.K.
Farhang, M.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A.A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Gauthier, C.
Gerbino, M.
Ghosh, T.
Giard, M.
Giraud-Heraud, Y.
Giusarma, E.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K.M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J.E.
Hamann, J.
Hansen, F.K.
Hanson, D.
Harrison, D.L.
Helou, G.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S.R.
Hivon, E.
Hobson, M.
Holmes, W.A.
Hornstrup, A.
Hovest, W.
Huang, Z.
Huffenberger, K.M.
Hurier, G.
Jaffe, A.H.
Jaffe, T.R.
Jones, W.C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T.S.
Kneissl, R.
Knoche, J.
Knox, L.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J.M.
Lasenby, A.
Lattanzi, M.
Lawrence, C.R.
Leahy, J.P.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Lewis, A.
Liguori, M.
Lilje, P.B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P.M.
Macias-Perez, J.F.
Maggio, G.
Mandolesi, N.
Mangilli, A.
Marchini, A.
Martin, P.G.
Martinelli, M.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
Mazzotta, P.
McGehee, P.
Meinhold, P.R.
Melchiorri, A.
Melin, J.B.
Mendes, L.
Mennella, A.
Migliaccio, M.
Millea, M.
Mitra, S.
Miville-Deschenes, M.A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J.A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C.B.
Norgaard-Nielsen, H.U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C.A.
Paci, F.
Pagano, L.
Pajot, F.
Paladini, R.
Paoletti, D.
Partridge, B.
Pasian, F.
Patanchon, G.
Pearson, T.J.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Popa, L.
Pratt, G.W.
Prezeau, G.
Prunet, S.
Puget, J.L.
Rachen, J.P.
Reach, W.T.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
d'Orfeuil, B.Rouille
Rowan-Robinson, M.
Rubino-Martin, J.A.
Rusholme, B.
Said, N.
Salvatelli, V.
Salvati, L.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M.D.
Serra, P.
Shellard, E.P.S.
Spencer, L.D.
Spinelli, M.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A.S.
Sygnet, J.F.
Tauber, J.A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Trombetti, T.
Tucci, M.
Tuovinen, J.
Turler, M.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L.A.
Wandelt, B.D.
Wehus, I.K.
White, M.
White, S.D.M.
Wilkinson, A.
Yvon, D.
Zacchei, A.
Zonca, A.
author_facet Ade, P.A.R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A.J.
Barreiro, R.B.
Bartlett, J.G.
Bartolo, N.
Battaner, E.
Battye, R.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J.P.
Bersanelli, M.
Bielewicz, P.
Bonaldi, A.
Bonavera, L.
Bond, J.R.
Borrill, J.
Bouchet, F.R.
Boulanger, F.
Bucher, M.
Burigana, C.
Butler, R.C.
Calabrese, E.
Cardoso, J.F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chary, R.R.
Chiang, H.C.
Chluba, J.
Christensen, P.R.
Church, S.
Clements, D.L.
Colombi, S.
Colombo, L.P.L.
Combet, C.
Coulais, A.
Crill, B.P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R.D.
Davis, R.J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F.X.
Di Valentino, E.
Dickinson, C.
Diego, J.M.
Dolag, K.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dunkley, J.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T.A.
Eriksen, H.K.
Farhang, M.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A.A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Gauthier, C.
Gerbino, M.
Ghosh, T.
Giard, M.
Giraud-Heraud, Y.
Giusarma, E.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K.M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J.E.
Hamann, J.
Hansen, F.K.
Hanson, D.
Harrison, D.L.
Helou, G.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S.R.
Hivon, E.
Hobson, M.
Holmes, W.A.
Hornstrup, A.
Hovest, W.
Huang, Z.
Huffenberger, K.M.
Hurier, G.
Jaffe, A.H.
Jaffe, T.R.
Jones, W.C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T.S.
Kneissl, R.
Knoche, J.
Knox, L.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J.M.
Lasenby, A.
Lattanzi, M.
Lawrence, C.R.
Leahy, J.P.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Lewis, A.
Liguori, M.
Lilje, P.B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P.M.
Macias-Perez, J.F.
Maggio, G.
Mandolesi, N.
Mangilli, A.
Marchini, A.
Martin, P.G.
Martinelli, M.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
Mazzotta, P.
McGehee, P.
Meinhold, P.R.
Melchiorri, A.
Melin, J.B.
Mendes, L.
Mennella, A.
Migliaccio, M.
Millea, M.
Mitra, S.
Miville-Deschenes, M.A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J.A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C.B.
Norgaard-Nielsen, H.U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C.A.
Paci, F.
Pagano, L.
Pajot, F.
Paladini, R.
Paoletti, D.
Partridge, B.
Pasian, F.
Patanchon, G.
Pearson, T.J.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Popa, L.
Pratt, G.W.
Prezeau, G.
Prunet, S.
Puget, J.L.
Rachen, J.P.
Reach, W.T.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
d'Orfeuil, B.Rouille
Rowan-Robinson, M.
Rubino-Martin, J.A.
Rusholme, B.
Said, N.
Salvatelli, V.
Salvati, L.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M.D.
Serra, P.
Shellard, E.P.S.
Spencer, L.D.
Spinelli, M.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A.S.
Sygnet, J.F.
Tauber, J.A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Trombetti, T.
Tucci, M.
Tuovinen, J.
Turler, M.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L.A.
Wandelt, B.D.
Wehus, I.K.
White, M.
White, S.D.M.
Wilkinson, A.
Yvon, D.
Zacchei, A.
Zonca, A.
author_sort Ade, P.A.R.
collection CERN
description We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. These data are consistent with the six-parameter inflationary LCDM cosmology. From the Planck temperature and lensing data, for this cosmology we find a Hubble constant, H0= (67.8 +/- 0.9) km/s/Mpc, a matter density parameter Omega_m = 0.308 +/- 0.012 and a scalar spectral index with n_s = 0.968 +/- 0.006. (We quote 68% errors on measured parameters and 95% limits on other parameters.) Combined with Planck temperature and lensing data, Planck LFI polarization measurements lead to a reionization optical depth of tau = 0.066 +/- 0.016. Combining Planck with other astrophysical data we find N_ eff = 3.15 +/- 0.23 for the effective number of relativistic degrees of freedom and the sum of neutrino masses is constrained to < 0.23 eV. Spatial curvature is found to be |Omega_K| < 0.005. For LCDM we find a limit on the tensor-to-scalar ratio of r <0.11 consistent with the B-mode constraints from an analysis of BICEP2, Keck Array, and Planck (BKP) data. Adding the BKP data leads to a tighter constraint of r < 0.09. We find no evidence for isocurvature perturbations or cosmic defects. The equation of state of dark energy is constrained to w = -1.006 +/- 0.045. Standard big bang nucleosynthesis predictions for the Planck LCDM cosmology are in excellent agreement with observations. We investigate annihilating dark matter and deviations from standard recombination, finding no evidence for new physics. The Planck results for base LCDM are in agreement with BAO data and with the JLA SNe sample. However the amplitude of the fluctuations is found to be higher than inferred from rich cluster counts and weak gravitational lensing. Apart from these tensions, the base LCDM cosmology provides an excellent description of the Planck CMB observations and many other astrophysical data sets.
id cern-1987166
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2015
record_format invenio
spelling cern-19871662023-10-26T05:06:35Zdoi:10.1051/0004-6361/201525830http://cds.cern.ch/record/1987166engAde, P.A.R.Aghanim, N.Arnaud, M.Ashdown, M.Aumont, J.Baccigalupi, C.Banday, A.J.Barreiro, R.B.Bartlett, J.G.Bartolo, N.Battaner, E.Battye, R.Benabed, K.Benoit, A.Benoit-Levy, A.Bernard, J.P.Bersanelli, M.Bielewicz, P.Bonaldi, A.Bonavera, L.Bond, J.R.Borrill, J.Bouchet, F.R.Boulanger, F.Bucher, M.Burigana, C.Butler, R.C.Calabrese, E.Cardoso, J.F.Catalano, A.Challinor, A.Chamballu, A.Chary, R.R.Chiang, H.C.Chluba, J.Christensen, P.R.Church, S.Clements, D.L.Colombi, S.Colombo, L.P.L.Combet, C.Coulais, A.Crill, B.P.Curto, A.Cuttaia, F.Danese, L.Davies, R.D.Davis, R.J.de Bernardis, P.de Rosa, A.de Zotti, G.Delabrouille, J.Desert, F.X.Di Valentino, E.Dickinson, C.Diego, J.M.Dolag, K.Dole, H.Donzelli, S.Dore, O.Douspis, M.Ducout, A.Dunkley, J.Dupac, X.Efstathiou, G.Elsner, F.Ensslin, T.A.Eriksen, H.K.Farhang, M.Fergusson, J.Finelli, F.Forni, O.Frailis, M.Fraisse, A.A.Franceschi, E.Frejsel, A.Galeotta, S.Galli, S.Ganga, K.Gauthier, C.Gerbino, M.Ghosh, T.Giard, M.Giraud-Heraud, Y.Giusarma, E.Gjerlow, E.Gonzalez-Nuevo, J.Gorski, K.M.Gratton, S.Gregorio, A.Gruppuso, A.Gudmundsson, J.E.Hamann, J.Hansen, F.K.Hanson, D.Harrison, D.L.Helou, G.Henrot-Versille, S.Hernandez-Monteagudo, C.Herranz, D.Hildebrandt, S.R.Hivon, E.Hobson, M.Holmes, W.A.Hornstrup, A.Hovest, W.Huang, Z.Huffenberger, K.M.Hurier, G.Jaffe, A.H.Jaffe, T.R.Jones, W.C.Juvela, M.Keihanen, E.Keskitalo, R.Kisner, T.S.Kneissl, R.Knoche, J.Knox, L.Kunz, M.Kurki-Suonio, H.Lagache, G.Lahteenmaki, A.Lamarre, J.M.Lasenby, A.Lattanzi, M.Lawrence, C.R.Leahy, J.P.Leonardi, R.Lesgourgues, J.Levrier, F.Lewis, A.Liguori, M.Lilje, P.B.Linden-Vornle, M.Lopez-Caniego, M.Lubin, P.M.Macias-Perez, J.F.Maggio, G.Mandolesi, N.Mangilli, A.Marchini, A.Martin, P.G.Martinelli, M.Martinez-Gonzalez, E.Masi, S.Matarrese, S.Mazzotta, P.McGehee, P.Meinhold, P.R.Melchiorri, A.Melin, J.B.Mendes, L.Mennella, A.Migliaccio, M.Millea, M.Mitra, S.Miville-Deschenes, M.A.Moneti, A.Montier, L.Morgante, G.Mortlock, D.Moss, A.Munshi, D.Murphy, J.A.Naselsky, P.Nati, F.Natoli, P.Netterfield, C.B.Norgaard-Nielsen, H.U.Noviello, F.Novikov, D.Novikov, I.Oxborrow, C.A.Paci, F.Pagano, L.Pajot, F.Paladini, R.Paoletti, D.Partridge, B.Pasian, F.Patanchon, G.Pearson, T.J.Perdereau, O.Perotto, L.Perrotta, F.Pettorino, V.Piacentini, F.Piat, M.Pierpaoli, E.Pietrobon, D.Plaszczynski, S.Pointecouteau, E.Polenta, G.Popa, L.Pratt, G.W.Prezeau, G.Prunet, S.Puget, J.L.Rachen, J.P.Reach, W.T.Rebolo, R.Reinecke, M.Remazeilles, M.Renault, C.Renzi, A.Ristorcelli, I.Rocha, G.Rosset, C.Rossetti, M.Roudier, G.d'Orfeuil, B.RouilleRowan-Robinson, M.Rubino-Martin, J.A.Rusholme, B.Said, N.Salvatelli, V.Salvati, L.Sandri, M.Santos, D.Savelainen, M.Savini, G.Scott, D.Seiffert, M.D.Serra, P.Shellard, E.P.S.Spencer, L.D.Spinelli, M.Stolyarov, V.Stompor, R.Sudiwala, R.Sunyaev, R.Sutton, D.Suur-Uski, A.S.Sygnet, J.F.Tauber, J.A.Terenzi, L.Toffolatti, L.Tomasi, M.Tristram, M.Trombetti, T.Tucci, M.Tuovinen, J.Turler, M.Umana, G.Valenziano, L.Valiviita, J.Van Tent, B.Vielva, P.Villa, F.Wade, L.A.Wandelt, B.D.Wehus, I.K.White, M.White, S.D.M.Wilkinson, A.Yvon, D.Zacchei, A.Zonca, A.Planck 2015 results. XIII. Cosmological parametersAstrophysics and AstronomyWe present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. These data are consistent with the six-parameter inflationary LCDM cosmology. From the Planck temperature and lensing data, for this cosmology we find a Hubble constant, H0= (67.8 +/- 0.9) km/s/Mpc, a matter density parameter Omega_m = 0.308 +/- 0.012 and a scalar spectral index with n_s = 0.968 +/- 0.006. (We quote 68% errors on measured parameters and 95% limits on other parameters.) Combined with Planck temperature and lensing data, Planck LFI polarization measurements lead to a reionization optical depth of tau = 0.066 +/- 0.016. Combining Planck with other astrophysical data we find N_ eff = 3.15 +/- 0.23 for the effective number of relativistic degrees of freedom and the sum of neutrino masses is constrained to < 0.23 eV. Spatial curvature is found to be |Omega_K| < 0.005. For LCDM we find a limit on the tensor-to-scalar ratio of r <0.11 consistent with the B-mode constraints from an analysis of BICEP2, Keck Array, and Planck (BKP) data. Adding the BKP data leads to a tighter constraint of r < 0.09. We find no evidence for isocurvature perturbations or cosmic defects. The equation of state of dark energy is constrained to w = -1.006 +/- 0.045. Standard big bang nucleosynthesis predictions for the Planck LCDM cosmology are in excellent agreement with observations. We investigate annihilating dark matter and deviations from standard recombination, finding no evidence for new physics. The Planck results for base LCDM are in agreement with BAO data and with the JLA SNe sample. However the amplitude of the fluctuations is found to be higher than inferred from rich cluster counts and weak gravitational lensing. Apart from these tensions, the base LCDM cosmology provides an excellent description of the Planck CMB observations and many other astrophysical data sets.This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. Our results are in very good agreement with the 2013 analysis of the Planck nominal-mission temperature data, but with increased precision. The temperature and polarization power spectra are consistent with the standard spatially-flat 6-parameter LambdaCDM cosmology with a power-law spectrum of adiabatic scalar perturbations (denoted 'base LambdaCDM' in this paper). From the Planck temperature data combined with Planck lensing, for this cosmology we find a Hubble constant, H_0 = (67.8 +- 0.9) km s^-1Mpc^-1, a matter density parameter Omega_m = 0.308 +- 0.012, and a tilted scalar spectral index with n_s = 0.968 +- 0.006, consistent with the 2013 analysis. Note that in this abstract we quote 68% confidence limits on measured parameters and 95% upper limits on other parameters. We present the first results of polarization measurements with the Low Frequency Instrument at large angular scales. Combined with the Planck temperature and lensing data, these measurements give a reionization optical depth of tau = 0.066 +- 0.016, corresponding to a reionization redshift of [??] . These results are consistent with those from WMAP polarization measurements cleaned for dust emission using 353-GHz polarization maps from the High Frequency Instrument. We find no evidence for any departure from base LambdaCDM in the neutrino sector of the theory; for example, combining Planck observations with other astrophysical data we find N_eff = 3.15 +- 0.23 for the effective number of relativistic degrees of freedom, consistent with the value N_eff = 3.046 of the Standard Model of particle physics. The sum of neutrino masses is constrained to Sigma m_nu . The spatial curvature of our Universe is found to be very close to zero, with | Omega_K | . Adding a tensor component as a single-parameter extension to base LambdaCDM we find an upper limit on the tensor-to-scalar ratio of r_0.002, consistent with the Planck 2013 results and consistent with the B-mode polarization constraints from a joint analysis of BICEP2, Keck Array, and Planck (BKP) data. Adding the BKP B-mode data to our analysis leads to a tighter constraint of r_0.002 and disfavours inflationarymodels with a V(phi) ∝ phi^2 potential. The addition of Planck polarization data leads to strong constraints on deviations from a purely adiabatic spectrum of fluctuations. We find no evidence for any contribution from isocurvature perturbations or from cosmic defects. Combining Planck data with other astrophysical data, including Type Ia supernovae, the equation of state of dark energy is constrained to w = -1.006 +- 0.045, consistent with the expected value for a cosmological constant. The standard big bang nucleosynthesis predictions for the helium and deuterium abundances for the best-fit Planck base LambdaCDM cosmology are in excellent agreement with observations. We also constraints on annihilating dark matter and on possible deviations from the standard recombination history. In neither case do we find no evidence for new physics. The Planck results for base LambdaCDM are in good agreement with baryon acoustic oscillation data and with the JLA sample of Type Ia supernovae. However, as in the 2013 analysis, the amplitude of the fluctuation spectrum is found to be higher than inferred from some analyses of rich cluster counts and weak gravitational lensing. We show that these tensions cannot easily be resolved with simple modifications of the base LambdaCDM cosmology. Apart from these tensions, the base LambdaCDM cosmology provides an excellent description of the Planck CMB observations and many other astrophysical data sets.We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. These data are consistent with the six-parameter inflationary LCDM cosmology. From the Planck temperature and lensing data, for this cosmology we find a Hubble constant, H0= (67.8 +/- 0.9) km/s/Mpc, a matter density parameter Omega_m = 0.308 +/- 0.012 and a scalar spectral index with n_s = 0.968 +/- 0.006. (We quote 68% errors on measured parameters and 95% limits on other parameters.) Combined with Planck temperature and lensing data, Planck LFI polarization measurements lead to a reionization optical depth of tau = 0.066 +/- 0.016. Combining Planck with other astrophysical data we find N_ eff = 3.15 +/- 0.23 for the effective number of relativistic degrees of freedom and the sum of neutrino masses is constrained to < 0.23 eV. Spatial curvature is found to be |Omega_K| < 0.005. For LCDM we find a limit on the tensor-to-scalar ratio of r <0.11 consistent with the B-mode constraints from an analysis of BICEP2, Keck Array, and Planck (BKP) data. Adding the BKP data leads to a tighter constraint of r < 0.09. We find no evidence for isocurvature perturbations or cosmic defects. The equation of state of dark energy is constrained to w = -1.006 +/- 0.045. Standard big bang nucleosynthesis predictions for the Planck LCDM cosmology are in excellent agreement with observations. We investigate annihilating dark matter and deviations from standard recombination, finding no evidence for new physics. The Planck results for base LCDM are in agreement with BAO data and with the JLA SNe sample. However the amplitude of the fluctuations is found to be higher than inferred from rich cluster counts and weak gravitational lensing. Apart from these tensions, the base LCDM cosmology provides an excellent description of the Planck CMB observations and many other astrophysical data sets.arXiv:1502.01589oai:cds.cern.ch:19871662015-02-05
spellingShingle Astrophysics and Astronomy
Ade, P.A.R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A.J.
Barreiro, R.B.
Bartlett, J.G.
Bartolo, N.
Battaner, E.
Battye, R.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J.P.
Bersanelli, M.
Bielewicz, P.
Bonaldi, A.
Bonavera, L.
Bond, J.R.
Borrill, J.
Bouchet, F.R.
Boulanger, F.
Bucher, M.
Burigana, C.
Butler, R.C.
Calabrese, E.
Cardoso, J.F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chary, R.R.
Chiang, H.C.
Chluba, J.
Christensen, P.R.
Church, S.
Clements, D.L.
Colombi, S.
Colombo, L.P.L.
Combet, C.
Coulais, A.
Crill, B.P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R.D.
Davis, R.J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F.X.
Di Valentino, E.
Dickinson, C.
Diego, J.M.
Dolag, K.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dunkley, J.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T.A.
Eriksen, H.K.
Farhang, M.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A.A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Gauthier, C.
Gerbino, M.
Ghosh, T.
Giard, M.
Giraud-Heraud, Y.
Giusarma, E.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K.M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J.E.
Hamann, J.
Hansen, F.K.
Hanson, D.
Harrison, D.L.
Helou, G.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S.R.
Hivon, E.
Hobson, M.
Holmes, W.A.
Hornstrup, A.
Hovest, W.
Huang, Z.
Huffenberger, K.M.
Hurier, G.
Jaffe, A.H.
Jaffe, T.R.
Jones, W.C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T.S.
Kneissl, R.
Knoche, J.
Knox, L.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J.M.
Lasenby, A.
Lattanzi, M.
Lawrence, C.R.
Leahy, J.P.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Lewis, A.
Liguori, M.
Lilje, P.B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P.M.
Macias-Perez, J.F.
Maggio, G.
Mandolesi, N.
Mangilli, A.
Marchini, A.
Martin, P.G.
Martinelli, M.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
Mazzotta, P.
McGehee, P.
Meinhold, P.R.
Melchiorri, A.
Melin, J.B.
Mendes, L.
Mennella, A.
Migliaccio, M.
Millea, M.
Mitra, S.
Miville-Deschenes, M.A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J.A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C.B.
Norgaard-Nielsen, H.U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C.A.
Paci, F.
Pagano, L.
Pajot, F.
Paladini, R.
Paoletti, D.
Partridge, B.
Pasian, F.
Patanchon, G.
Pearson, T.J.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Popa, L.
Pratt, G.W.
Prezeau, G.
Prunet, S.
Puget, J.L.
Rachen, J.P.
Reach, W.T.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
d'Orfeuil, B.Rouille
Rowan-Robinson, M.
Rubino-Martin, J.A.
Rusholme, B.
Said, N.
Salvatelli, V.
Salvati, L.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M.D.
Serra, P.
Shellard, E.P.S.
Spencer, L.D.
Spinelli, M.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A.S.
Sygnet, J.F.
Tauber, J.A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Trombetti, T.
Tucci, M.
Tuovinen, J.
Turler, M.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L.A.
Wandelt, B.D.
Wehus, I.K.
White, M.
White, S.D.M.
Wilkinson, A.
Yvon, D.
Zacchei, A.
Zonca, A.
Planck 2015 results. XIII. Cosmological parameters
title Planck 2015 results. XIII. Cosmological parameters
title_full Planck 2015 results. XIII. Cosmological parameters
title_fullStr Planck 2015 results. XIII. Cosmological parameters
title_full_unstemmed Planck 2015 results. XIII. Cosmological parameters
title_short Planck 2015 results. XIII. Cosmological parameters
title_sort planck 2015 results. xiii. cosmological parameters
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1051/0004-6361/201525830
http://cds.cern.ch/record/1987166
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