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Title: Planck 2015 results: XIII. Cosmological parameters

Abstract

Here, 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 ΛCDM cosmology with a power-law spectrum of adiabatic scalar perturbations (denoted “base ΛCDM” in this paper). From the Planck temperature data combined with Planck lensing, for this cosmology we find a Hubble constant, H0 = (67.8 ± 0.9) km s-1Mpc-1, a matter density parameter Ωm = 0.308 ± 0.012, and a tilted scalar spectral index with ns = 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 τ = 0.066 ± 0.016, corresponding to a reionization redshift of zre= 8.8$$+1.7\atop{-1.4}$$. 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 ΛCDM in the neutrino sector of the theory; for example, combining Planck observations with other astrophysical data we find Neff = 3.15 ± 0.23 for the effective number of relativistic degrees of freedom, consistent with the value Neff = 3.046 of the Standard Model of particle physics. The sum of neutrino masses is constrained to Σ mν < 0.23 eV. The spatial curvature of our Universe is found to be very close to zero, with | ΩK | < 0.005. Adding a tensor component as a single-parameter extension to base ΛCDM we find an upper limit on the tensor-to-scalar ratio of r0.002< 0.11, 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 r0.002 < 0.09 and disfavours inflationarymodels with a V(φ) ∝ φ2 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 ΛCDM 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 ΛCDM 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 ΛCDM cosmology. Finally, apart from these tensions, the base ΛCDM cosmology provides an excellent description of the Planck CMB observations and many other astrophysical data sets.

Authors:
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Publication Date:
Research Org.:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
Contributing Org.:
Planck Collaboration
OSTI Identifier:
1398426
Grant/Contract Number:  
AC02-05CH11231
Resource Type:
Accepted Manuscript
Journal Name:
Astronomy and Astrophysics
Additional Journal Information:
Journal Volume: 594; Journal ID: ISSN 0004-6361
Publisher:
EDP Sciences
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; cosmology: observations; cosmology: thoery; cosmic background radiation; cosmological parameters

Citation Formats

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., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bock, J. J., 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., Désert, F. -X., Di Valentino, E., Dickinson, C., Diego, J. M., Dolag, K., Dole, H., Donzelli, S., Doré, 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-Héraud, Y., Giusarma, E., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Gudmundsson, J. E., Hamann, J., Hansen, F. K., Hanson, D., Harrison, D. L., Helou, G., Henrot-Versillé, S., Hernández-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., Keihänen, E., Keskitalo, R., Kisner, T. S., Kneissl, R., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, 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-Vørnle, M., López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Marchini, A., Maris, M., Martin, P. G., Martinelli, M., Martínez-González, E., Masi, S., Matarrese, S., McGehee, P., Meinhold, P. R., Melchiorri, A., Melin, J. -B., Mendes, L., Mennella, A., Migliaccio, M., Millea, M., Mitra, S., Miville-Deschênes, 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., Nørgaard-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., Prézeau, 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., Rouillé d’Orfeuil, B., Rowan-Robinson, M., Rubiño-Martín, 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., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, F., 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., and Zonca, A. Planck 2015 results: XIII. Cosmological parameters. United States: N. p., 2016. Web. doi:10.1051/0004-6361/201525830.
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., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bock, J. J., 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., Désert, F. -X., Di Valentino, E., Dickinson, C., Diego, J. M., Dolag, K., Dole, H., Donzelli, S., Doré, 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-Héraud, Y., Giusarma, E., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Gudmundsson, J. E., Hamann, J., Hansen, F. K., Hanson, D., Harrison, D. L., Helou, G., Henrot-Versillé, S., Hernández-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., Keihänen, E., Keskitalo, R., Kisner, T. S., Kneissl, R., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, 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-Vørnle, M., López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Marchini, A., Maris, M., Martin, P. G., Martinelli, M., Martínez-González, E., Masi, S., Matarrese, S., McGehee, P., Meinhold, P. R., Melchiorri, A., Melin, J. -B., Mendes, L., Mennella, A., Migliaccio, M., Millea, M., Mitra, S., Miville-Deschênes, 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., Nørgaard-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., Prézeau, 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., Rouillé d’Orfeuil, B., Rowan-Robinson, M., Rubiño-Martín, 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., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, F., 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. United States. doi:10.1051/0004-6361/201525830.
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., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bock, J. J., 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., Désert, F. -X., Di Valentino, E., Dickinson, C., Diego, J. M., Dolag, K., Dole, H., Donzelli, S., Doré, 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-Héraud, Y., Giusarma, E., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Gudmundsson, J. E., Hamann, J., Hansen, F. K., Hanson, D., Harrison, D. L., Helou, G., Henrot-Versillé, S., Hernández-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., Keihänen, E., Keskitalo, R., Kisner, T. S., Kneissl, R., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lähteenmäki, 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-Vørnle, M., López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Marchini, A., Maris, M., Martin, P. G., Martinelli, M., Martínez-González, E., Masi, S., Matarrese, S., McGehee, P., Meinhold, P. R., Melchiorri, A., Melin, J. -B., Mendes, L., Mennella, A., Migliaccio, M., Millea, M., Mitra, S., Miville-Deschênes, 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., Nørgaard-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., Prézeau, 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., Rouillé d’Orfeuil, B., Rowan-Robinson, M., Rubiño-Martín, 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., Türler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, F., 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., and Zonca, A. Tue . "Planck 2015 results: XIII. Cosmological parameters". United States. doi:10.1051/0004-6361/201525830. https://www.osti.gov/servlets/purl/1398426.
@article{osti_1398426,
title = {Planck 2015 results: XIII. Cosmological parameters},
author = {Ade, P. A. R. and Aghanim, N. and Arnaud, M. and Ashdown, M. and Aumont, J. and Baccigalupi, C. and Banday, A. J. and Barreiro, R. B. and Bartlett, J. G. and Bartolo, N. and Battaner, E. and Battye, R. and Benabed, K. and Benoît, A. and Benoit-Lévy, A. and Bernard, J. -P. and Bersanelli, M. and Bielewicz, P. and Bock, J. J. and Bonaldi, A. and Bonavera, L. and Bond, J. R. and Borrill, J. and Bouchet, F. R. and Boulanger, F. and Bucher, M. and Burigana, C. and Butler, R. C. and Calabrese, E. and Cardoso, J. -F. and Catalano, A. and Challinor, A. and Chamballu, A. and Chary, R. -R. and Chiang, H. C. and Chluba, J. and Christensen, P. R. and Church, S. and Clements, D. L. and Colombi, S. and Colombo, L. P. L. and Combet, C. and Coulais, A. and Crill, B. P. and Curto, A. and Cuttaia, F. and Danese, L. and Davies, R. D. and Davis, R. J. and de Bernardis, P. and de Rosa, A. and de Zotti, G. and Delabrouille, J. and Désert, F. -X. and Di Valentino, E. and Dickinson, C. and Diego, J. M. and Dolag, K. and Dole, H. and Donzelli, S. and Doré, O. and Douspis, M. and Ducout, A. and Dunkley, J. and Dupac, X. and Efstathiou, G. and Elsner, F. and Enßlin, T. A. and Eriksen, H. K. and Farhang, M. and Fergusson, J. and Finelli, F. and Forni, O. and Frailis, M. and Fraisse, A. A. and Franceschi, E. and Frejsel, A. and Galeotta, S. and Galli, S. and Ganga, K. and Gauthier, C. and Gerbino, M. and Ghosh, T. and Giard, M. and Giraud-Héraud, Y. and Giusarma, E. and Gjerløw, E. and González-Nuevo, J. and Górski, K. M. and Gratton, S. and Gregorio, A. and Gruppuso, A. and Gudmundsson, J. E. and Hamann, J. and Hansen, F. K. and Hanson, D. and Harrison, D. L. and Helou, G. and Henrot-Versillé, S. and Hernández-Monteagudo, C. and Herranz, D. and Hildebrandt, S. R. and Hivon, E. and Hobson, M. and Holmes, W. A. and Hornstrup, A. and Hovest, W. and Huang, Z. and Huffenberger, K. M. and Hurier, G. and Jaffe, A. H. and Jaffe, T. R. and Jones, W. C. and Juvela, M. and Keihänen, E. and Keskitalo, R. and Kisner, T. S. and Kneissl, R. and Knoche, J. and Knox, L. and Kunz, M. and Kurki-Suonio, H. and Lagache, G. and Lähteenmäki, A. and Lamarre, J. -M. and Lasenby, A. and Lattanzi, M. and Lawrence, C. R. and Leahy, J. P. and Leonardi, R. and Lesgourgues, J. and Levrier, F. and Lewis, A. and Liguori, M. and Lilje, P. B. and Linden-Vørnle, M. and López-Caniego, M. and Lubin, P. M. and Macías-Pérez, J. F. and Maggio, G. and Maino, D. and Mandolesi, N. and Mangilli, A. and Marchini, A. and Maris, M. and Martin, P. G. and Martinelli, M. and Martínez-González, E. and Masi, S. and Matarrese, S. and McGehee, P. and Meinhold, P. R. and Melchiorri, A. and Melin, J. -B. and Mendes, L. and Mennella, A. and Migliaccio, M. and Millea, M. and Mitra, S. and Miville-Deschênes, M. -A. and Moneti, A. and Montier, L. and Morgante, G. and Mortlock, D. and Moss, A. and Munshi, D. and Murphy, J. A. and Naselsky, P. and Nati, F. and Natoli, P. and Netterfield, C. B. and Nørgaard-Nielsen, H. U. and Noviello, F. and Novikov, D. and Novikov, I. and Oxborrow, C. A. and Paci, F. and Pagano, L. and Pajot, F. and Paladini, R. and Paoletti, D. and Partridge, B. and Pasian, F. and Patanchon, G. and Pearson, T. J. and Perdereau, O. and Perotto, L. and Perrotta, F. and Pettorino, V. and Piacentini, F. and Piat, M. and Pierpaoli, E. and Pietrobon, D. and Plaszczynski, S. and Pointecouteau, E. and Polenta, G. and Popa, L. and Pratt, G. W. and Prézeau, G. and Prunet, S. and Puget, J. -L. and Rachen, J. P. and Reach, W. T. and Rebolo, R. and Reinecke, M. and Remazeilles, M. and Renault, C. and Renzi, A. and Ristorcelli, I. and Rocha, G. and Rosset, C. and Rossetti, M. and Roudier, G. and Rouillé d’Orfeuil, B. and Rowan-Robinson, M. and Rubiño-Martín, J. A. and Rusholme, B. and Said, N. and Salvatelli, V. and Salvati, L. and Sandri, M. and Santos, D. and Savelainen, M. and Savini, G. and Scott, D. and Seiffert, M. D. and Serra, P. and Shellard, E. P. S. and Spencer, L. D. and Spinelli, M. and Stolyarov, V. and Stompor, R. and Sudiwala, R. and Sunyaev, R. and Sutton, D. and Suur-Uski, A. -S. and Sygnet, J. -F. and Tauber, J. A. and Terenzi, L. and Toffolatti, L. and Tomasi, M. and Tristram, M. and Trombetti, T. and Tucci, M. and Tuovinen, J. and Türler, M. and Umana, G. and Valenziano, L. and Valiviita, J. and Van Tent, F. and Vielva, P. and Villa, F. and Wade, L. A. and Wandelt, B. D. and Wehus, I. K. and White, M. and White, S. D. M. and Wilkinson, A. and Yvon, D. and Zacchei, A. and Zonca, A.},
abstractNote = {Here, 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 ΛCDM cosmology with a power-law spectrum of adiabatic scalar perturbations (denoted “base ΛCDM” in this paper). From the Planck temperature data combined with Planck lensing, for this cosmology we find a Hubble constant, H0 = (67.8 ± 0.9) km s-1Mpc-1, a matter density parameter Ωm = 0.308 ± 0.012, and a tilted scalar spectral index with ns = 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 τ = 0.066 ± 0.016, corresponding to a reionization redshift of zre= 8.8$+1.7\atop{-1.4}$. 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 ΛCDM in the neutrino sector of the theory; for example, combining Planck observations with other astrophysical data we find Neff = 3.15 ± 0.23 for the effective number of relativistic degrees of freedom, consistent with the value Neff = 3.046 of the Standard Model of particle physics. The sum of neutrino masses is constrained to Σ mν < 0.23 eV. The spatial curvature of our Universe is found to be very close to zero, with | ΩK | < 0.005. Adding a tensor component as a single-parameter extension to base ΛCDM we find an upper limit on the tensor-to-scalar ratio of r0.002< 0.11, 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 r0.002 < 0.09 and disfavours inflationarymodels with a V(φ) ∝ φ2 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 ΛCDM 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 ΛCDM 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 ΛCDM cosmology. Finally, apart from these tensions, the base ΛCDM cosmology provides an excellent description of the Planck CMB observations and many other astrophysical data sets.},
doi = {10.1051/0004-6361/201525830},
journal = {Astronomy and Astrophysics},
number = ,
volume = 594,
place = {United States},
year = {2016},
month = {9}
}

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    • Piccirilli, María Pía; León, Gabriel; Landau, Susana J.
    • International Journal of Modern Physics D, Vol. 28, Issue 02
    • DOI: 10.1142/s021827181950041x

    Perspectives for tests of neutrino mass generation at the GeV scale: Experimental reach versus theoretical predictions
    journal, October 2016


    Connecting early and late epochs by f ( z )CDM cosmography
    journal, December 2019


    Halo concentration, galaxy red fraction, and gas properties of optically defined merging clusters†
    journal, July 2019

    • Okabe, Nobuhiro; Oguri, Masamune; Akamatsu, Hiroki
    • Publications of the Astronomical Society of Japan, Vol. 71, Issue 4
    • DOI: 10.1093/pasj/psz059

    Measurement of d + Be 7 Cross Sections for Big-Bang Nucleosynthesis
    journal, May 2019


    The PAU Survey: early demonstration of photometric redshift performance in the COSMOS field
    journal, January 2019

    • Eriksen, M.; Alarcon, A.; Gaztanaga, E.
    • Monthly Notices of the Royal Astronomical Society, Vol. 484, Issue 3
    • DOI: 10.1093/mnras/stz204

    Viscous cosmology for early- and late-time universe
    journal, December 2017

    • Brevik, Iver; Grøn, Øyvind; de Haro, Jaume
    • International Journal of Modern Physics D, Vol. 26, Issue 14
    • DOI: 10.1142/s0218271817300245

    Dark matter is a genuine spin-2 field
    journal, December 2018


    The Distance to NGC 4993: The Host Galaxy of the Gravitational-wave Event GW170817
    journal, October 2017

    • Hjorth, Jens; Levan, Andrew J.; Tanvir, Nial R.
    • The Astrophysical Journal, Vol. 848, Issue 2
    • DOI: 10.3847/2041-8213/aa9110

    FR0 CAT : a FIRST catalog of FR 0 radio galaxies
    journal, December 2017


    MUSE unravels the ionisation and origin of metal-enriched absorbers in the gas halo of a z = 2.92 radio galaxy
    journal, May 2019


    Standard sirens with a running Planck mass
    journal, April 2019


    Subjecting Dark Matter Candidates to the Cluster Test
    journal, November 2019


    Merging groups and clusters of galaxies from the SDSS data: The catalogue of groups and potentially merging systems⋆
    journal, June 2017


    Comparison of hydrostatic and dynamical masses of distant X-ray luminous galaxy clusters
    journal, October 2017


    Latest astronomical constraints on some non-linear parametric dark energy models
    journal, January 2018

    • Yang, Weiqiang; Pan, Supriya; Paliathanasis, Andronikos
    • Monthly Notices of the Royal Astronomical Society, Vol. 475, Issue 2
    • DOI: 10.1093/mnras/sty019

    Kinematics and dynamics of the luminous infrared galaxy pair NGC 5257/58 (Arp 240)
    journal, December 2018


    A comparison of the $$R_{\mathrm{h}}=ct$$ R h = c t and $$\varLambda $$ Λ CDM cosmologies based on the observed halo mass function
    journal, July 2019


    An updated Type II supernova Hubble diagram
    journal, March 2018


    Cosmology via thermodynamics of polytropic gas
    journal, October 2017


    $$H_0$$ H 0 tension: clue to common nature of dark sector?
    journal, July 2019


    Formation pathway of Population III coalescing binary black holes through stable mass transfer
    journal, March 2017

    • Inayoshi, Kohei; Hirai, Ryosuke; Kinugawa, Tomoya
    • Monthly Notices of the Royal Astronomical Society, Vol. 468, Issue 4
    • DOI: 10.1093/mnras/stx757

    Supersymmetric versus SO(10) models of dark matter
    journal, May 2017


    A comparison of the $$R_{\mathrm{h}}=ct$$ R h = c t and $$\varLambda $$ Λ CDM cosmologies based on the observed halo mass function
    journal, July 2019


    Insensitivity of the distance ladder Hubble constant determination to Cepheid calibration modelling choices
    journal, March 2018

    • Follin, B.; Knox, L.
    • Monthly Notices of the Royal Astronomical Society, Vol. 477, Issue 4
    • DOI: 10.1093/mnras/sty720

    Interacting Chaplygin gas revisited
    journal, June 2017

    • Saha, Subhajit; Ghosh, Saumya; Gangopadhyay, Sunandan
    • Modern Physics Letters A, Vol. 32, Issue 22
    • DOI: 10.1142/s0217732317501097

    A topological approach to neutrino masses by using exotic smoothness
    journal, April 2019


    Tantalizing new physics from the cosmic purview
    journal, August 2019


    Decay rate of electroweak vacuum in the standard model and beyond
    journal, June 2018


    Determining thermal dust emission from Planck HFI data using a sparse, parametric technique
    journal, February 2019

    • Irfan, Melis O.; Bobin, Jérôme; Miville-Deschênes, Marc-Antoine
    • Astronomy & Astrophysics, Vol. 623
    • DOI: 10.1051/0004-6361/201834394

    High scale boundary conditions with an additional complex singlet
    journal, June 2018


    Direct measurement of nuclear cross-section of astrophysical interest: Results and perspectives
    journal, March 2018

    • Cavanna, Francesca; Prati, Paolo
    • International Journal of Modern Physics A, Vol. 33, Issue 09
    • DOI: 10.1142/s0217751x18430108

    Schwinger–Keldysh mechanism in extended quasi-single field inflation
    journal, May 2019


    A topological approach to neutrino masses by using exotic smoothness
    journal, April 2019


    Supermassive black holes and their feedback effects in the IllustrisTNG simulation
    journal, June 2018

    • Weinberger, Rainer; Springel, Volker; Pakmor, Rüdiger
    • Monthly Notices of the Royal Astronomical Society, Vol. 479, Issue 3
    • DOI: 10.1093/mnras/sty1733

    Baryogenesis from B meson oscillations
    journal, October 2019


    FRII CAT : A FIRST catalog of FR II radio galaxies
    journal, May 2017


    Inhomogeneous cosmology with numerical relativity
    journal, March 2017


    Dark matter freeze-out during matter domination
    journal, September 2018


    Neutrinoless double beta decay in minimal left–right symmetric model with universal seesaw
    journal, December 2018

    • Borah, Debasish; Dasgupta, Arnab; Patra, Sudhanwa
    • International Journal of Modern Physics A, Vol. 33, Issue 35
    • DOI: 10.1142/s0217751x18501981

    Type Ia supernova Hubble diagram with near-infrared and optical observations
    journal, July 2018


    Cosmological dynamics of mimetic gravity
    journal, February 2018

    • Dutta, Jibitesh; Khyllep, Wompherdeiki; Saridakis, Emmanuel N.
    • Journal of Cosmology and Astroparticle Physics, Vol. 2018, Issue 02
    • DOI: 10.1088/1475-7516/2018/02/041

    Flaring radio lanterns along the ridge line: long-term oscillatory motion in the jet of S5 1803+784
    journal, April 2018

    • Kun, E.; Karouzos, M.; Gabányi, K. É
    • Monthly Notices of the Royal Astronomical Society, Vol. 478, Issue 1
    • DOI: 10.1093/mnras/sty981

    Invisible decay of the Higgs boson in the context of a thermal and nonthermal relic in MSSM
    journal, May 2017

    • Barman, Rahool Kumar; Bélanger, Genevieve; Bhattacherjee, Biplob
    • Physical Review D, Vol. 95, Issue 9
    • DOI: 10.1103/physrevd.95.095018

    Nonminimal dark sector physics and cosmological tensions
    journal, March 2020


    Impact of SZ cluster residuals in CMB maps and CMB–LSS cross-correlations
    journal, June 2018

    • Chen, T.; Remazeilles, M.; Dickinson, C.
    • Monthly Notices of the Royal Astronomical Society, Vol. 479, Issue 3
    • DOI: 10.1093/mnras/sty1730

    Ultra-high-energy cosmic rays from radio galaxies
    journal, February 2018


    The angular momentum-mass relation: a fundamental law from dwarf irregulars to massive spirals
    journal, April 2018


    Lensing covariance on cut sky and SPT P l a n c k lensing tensions
    journal, January 2019


    Pulsational Pair-instability Supernovae in Very Close Binaries
    journal, August 2019

    • Marchant, Pablo; Renzo, Mathieu; Farmer, Robert
    • The Astrophysical Journal, Vol. 882, Issue 1
    • DOI: 10.3847/1538-4357/ab3426

    The impact of baryonic physics and massive neutrinos on weak lensing peak statistics
    journal, July 2019

    • Fong, Matthew; Choi, Miyoung; Catlett, Victoria
    • Monthly Notices of the Royal Astronomical Society, Vol. 488, Issue 3
    • DOI: 10.1093/mnras/stz1882

    A broad-band spectro-polarimetric view of the NVSS rotation measure catalogue – I. Breaking the nπ-ambiguity
    journal, May 2019

    • Ma, Yik Ki; Mao, S. A.; Stil, Jeroen
    • Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 3
    • DOI: 10.1093/mnras/stz1325

    The dawn of FIMP Dark Matter: A review of models and constraints
    journal, September 2017

    • Bernal, Nicolás; Heikinheimo, Matti; Tenkanen, Tommi
    • International Journal of Modern Physics A, Vol. 32, Issue 27
    • DOI: 10.1142/s0217751x1730023x

    Current status and future prospects of the singlet-doublet dark matter model with C P violation
    journal, February 2019


    The $$f(R,T^\phi )$$ f ( R , T ϕ ) gravity models with conservation of energy–momentum tensor
    journal, July 2018


    Merging groups and clusters of galaxies from the SDSS data: The catalogue of groups and potentially merging systems⋆
    journal, June 2017


    Comparison of hydrostatic and dynamical masses of distant X-ray luminous galaxy clusters
    journal, October 2017


    Recent discoveries from the cosmic microwave background: a review of recent progress
    journal, February 2018

    • Staggs, Suzanne; Dunkley, Jo; Page, Lyman
    • Reports on Progress in Physics, Vol. 81, Issue 4
    • DOI: 10.1088/1361-6633/aa94d5

    Impact of the mean pressure profile of galaxy clusters on the cosmological constraints from the Planck tSZ power spectrum
    journal, September 2019

    • Ruppin, F.; Mayet, F.; Macías-Pérez, J. F.
    • Monthly Notices of the Royal Astronomical Society, Vol. 490, Issue 1
    • DOI: 10.1093/mnras/stz2669

    A Hamiltonian formalism for the universe and its implications
    journal, October 2018


    Search for a Narrow Resonance Lighter than 200 GeV Decaying to a Pair of Muons in Proton-Proton Collisions at s = 13 TeV
    journal, April 2020


    Optical validation and characterization of Planck PSZ1 sources at the Canary Islands observatories : I. First year of ITP13 observations
    journal, August 2018


    Statistical properties of polarized CMB foreground maps
    journal, June 2019

    • von Hausegger, Sebastian; Gammelgaard Ravnebjerg, Aske; Liu, Hao
    • Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 4
    • DOI: 10.1093/mnras/stz1582

    Galactic cold cores: IV. Cold submillimetre sources: catalogue and statistical analysis⋆⋆⋆⋆⋆⋆
    journal, November 2015


    The effect of tides on the Sculptor dwarf spheroidal galaxy
    journal, May 2019

    • Iorio, G.; Nipoti, C.; Battaglia, G.
    • Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 4
    • DOI: 10.1093/mnras/stz1342

    Frequency-dependent responses in third generation gravitational-wave detectors
    journal, October 2017


    Dynamical dark energy: Scalar fields and running vacuum
    journal, March 2017

    • Solà, Joan; Gómez-Valent, Adrià; de Cruz Pérez, Javier
    • Modern Physics Letters A, Vol. 32, Issue 09
    • DOI: 10.1142/s0217732317500547

    Fermi-LAT kills dark matter interpretations of AMS-02 data. Or not?
    journal, January 2017

    • Belotsky, Konstantin; Budaev, Ruslan; Kirillov, Alexander
    • Journal of Cosmology and Astroparticle Physics, Vol. 2017, Issue 01
    • DOI: 10.1088/1475-7516/2017/01/021

    Asymmetric tribimaximal texture
    journal, September 2018


    Falsifying cosmological models based on a non-linear electrodynamics
    journal, June 2018


    Evidence for non-axisymmetry in M 31 from wide-field kinematics of stars and gas
    journal, March 2018


    Projected distances to host galaxy reduce SNIa dispersion
    journal, September 2018

    • Hill, Ryley; Shariff, H.; Trotta, R.
    • Monthly Notices of the Royal Astronomical Society, Vol. 481, Issue 2
    • DOI: 10.1093/mnras/sty2510

    A Search for Fast Radio Bursts with the GBNCC Pulsar Survey
    journal, August 2017


    Axially symmetric shear-free fluids in f(R,T) gravity
    journal, September 2017


    Cosmological backgrounds of gravitational waves
    journal, July 2018


    Observational constraints on constant roll inflation
    journal, May 2019

    • Ghersi, José T. Gálvez; Zucca, Alex; Frolov, Andrei V.
    • Journal of Cosmology and Astroparticle Physics, Vol. 2019, Issue 05
    • DOI: 10.1088/1475-7516/2019/05/030

    Effect of turbulent reacceleration on electrons produced by dark matter annihilation in the Coma cluster
    journal, July 2019

    • Marchegiani, P.
    • Monthly Notices of the Royal Astronomical Society, Vol. 488, Issue 1
    • DOI: 10.1093/mnras/stz1798

    Fruitbat: A Python Package for Estimating Redshifts of Fast Radio Bursts
    journal, May 2019


    Implications of hydrodynamical simulations for the interpretation of direct dark matter searches
    journal, July 2017

    • Bozorgnia, Nassim; Bertone, Gianfranco
    • International Journal of Modern Physics A, Vol. 32, Issue 21
    • DOI: 10.1142/s0217751x17300162

    FR0 CAT : a FIRST catalog of FR 0 radio galaxies
    journal, December 2017


    Kinetically coupled dark energy
    journal, March 2019