Planck 2015 results. XIII. Cosmological parameters
Peter A. R. Ade,Nabila Aghanim,Monique Arnaud,M. Ashdown,J. Aumont,Carlo Baccigalupi,A. J. Banday,R. B. Barreiro,James G. Bartlett,N. Bartolo,E. Battaner,Richard A. Battye,K. Benabed,Alain Benoit,A. Benoit-Lévy,J.-P. Bernard,Marco Bersanelli,P. Bielewicz,J. J. Bock,Anna Bonaldi,Laura Bonavera,J. R. Bond,Julian Borrill,François R. Bouchet,F. Boulanger,M. Bucher,Carlo Burigana,R. C. Butler,Erminia Calabrese,Jean-François Cardoso,A. Catalano,Anthony Challinor,A. Chamballu,Ranga-Ram Chary,H. C. Chiang,Jens Chluba,P. R. Christensen,Sarah E. Church,David L. Clements,S. Colombi,L. P. L. Colombo,C. Combet,A. Coulais,B. P. Crill,A. Curto,F. Cuttaia,Luigi Danese,R. D. Davies,R. J. Davis,P. de Bernardis,A. de Rosa,G. de Zotti,Jacques Delabrouille,F.-X. Désert,E. Di Valentino,Clive Dickinson,Jose M. Diego,Klaus Dolag,H. Dole,S. Donzelli,Olivier Doré,Marian Douspis,A. Ducout,Jo Dunkley,X. Dupac,George Efstathiou,F. Elsner,Torsten A. Ensslin,H. K. Eriksen,Marzieh Farhang,James R. Fergusson,Fabio Finelli,Olivier Forni,M. Frailis,A. A. Fraisse,E. Franceschi,A. Frejsel,S. Galeotta,S. Galli,K. Ganga,C. Gauthier,Martina Gerbino,Tuhin Ghosh,M. Giard,Y. Giraud-Héraud,Elena Giusarma,E. Gjerløw,J. González-Nuevo,Krzysztof M. Gorski,Serge Gratton,A. Gregorio,Alessandro Gruppuso,Jon E. Gudmundsson,Jan Hamann,F. K. Hansen,Duncan Hanson,D. L. Harrison,George Helou,Sophie Henrot-Versille,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,W. A. Holmes,Allan Hornstrup,W. Hovest,Zhiqi Huang,Kevin M. Huffenberger,G. Hurier,Andrew H. Jaffe,T. R. Jaffe,W. C. Jones,Mika Juvela,E. Keihänen,Reijo Keskitalo,Theodore Kisner,R. Kneissl,J. Knoche,Lloyd Knox,Martin Kunz,Hannu Kurki-Suonio,Guilaine Lagache,Anne Lähteenmäki,J.-M. Lamarre,Anthony Lasenby,Massimiliano Lattanzi,Charles R. Lawrence,J. P. Leahy,R. Leonardi,Julien Lesgourgues,François Levrier,Antony Lewis,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,G. Maggio,Davide Maino,N. Mandolesi,A. Mangilli,A. Marchini,Peter G. Martin,M. Martinelli,E. Martínez-González,Silvia Masi,Sabino Matarrese,Pasquale Mazzotta,P. McGehee,Peter Meinhold,Alessandro Melchiorri,J.-B. Melin,L. Mendes,A. Mennella,M. Migliaccio,M. Millea,S. Mitra,M.-A. Miville-Deschênes,A. Moneti,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Adam Moss,Dipak Munshi,J. A. Murphy,Pavel Naselsky,Federico Nati,Paolo Natoli,Calvin B. Netterfield,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,C. A. Oxborrow,F. Paci,L. Pagano,F. Pajot,R. Paladini,Daniela Paoletti,Bruce Partridge,F. Pasian,G. Patanchon,T. J. Pearson,O. Perdereau,L. Perotto,Francesca Perrotta,Valeria Pettorino,F. Piacentini,M. Piat,E. Pierpaoli,Davide Pietrobon,Stéphane Plaszczynski,Etienne Pointecouteau,G. Polenta,L. Popa,G. W. Pratt,G. Prézeau,Simon Prunet,J.-L. Puget,Jörg P. Rachen,William T. Reach,Rafael Rebolo,M. Reinecke,Mathieu Remazeilles,C. Renault,A. Renzi,I. Ristorcelli,Graca Rocha,C. Rosset,M. Rossetti,G. Roudier,B. Rouillé d'Orfeuil,Michael Rowan-Robinson,Jose Alberto Rubino-Martin,Ben Rusholme,Najla Said,Valentina Salvatelli,L. Salvati,M. Sandri,D. Santos,M. Savelainen,Giorgio Savini,Douglas Scott,Michael Seiffert,Paolo Serra,E. P. S. Shellard,Locke D. Spencer,M. Spinelli,V. Stolyarov,R. Stompor,R. Sudiwala,R. A. Sunyaev,D. Sutton,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,M. Tomasi,M. Tristram,T. Trombetti,M. Tucci,J. Tuovinen,M. Turler,G. Umana,Luca Valenziano,Jussi-Pekka Väliviita,B. Van Tent,P. Vielva,Fabrizio Villa,L. A. Wade,Benjamin D. Wandelt,Ingunn Kathrine Wehus,Martin White,Simon D. M. White,Althea Wilkinson,D. Yvon,Andrea Zacchei,Andrea Zonca +260 more
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In this paper, the authors present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB, which are consistent with the six-parameter inflationary LCDM cosmology.Abstract:
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.read more
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The Atacama Cosmology Telescope: Two-season ACTPol spectra and parameters
Thibaut Louis,Thibaut Louis,E. Grace,Matthew Hasselfield,Marius Lungu,Loïc Maurin,Graeme E. Addison,Peter A. R. Ade,Simone Aiola,Simone Aiola,R. Allison,Mandana Amiri,Elio Angile,Nicholas Battaglia,James A. Beall,Francesco De Bernardis,J. Richard Bond,Joseph W. Britton,Erminia Calabrese,Erminia Calabrese,Hsiao-Mei Cho,Steve K. Choi,Kevin Coughlin,Devin Crichton,Kevin T. Crowley,Rahul Datta,Mark J. Devlin,Simon Dicker,Joanna Dunkley,Joanna Dunkley,Rolando Dünner,Simone Ferraro,Anna E. Fox,Patricio A. Gallardo,Patricio A. Gallardo,Megan Gralla,Mark Halpern,Shawn W. Henderson,J. Colin Hill,Gene C. Hilton,Matt Hilton,Adam D. Hincks,Adam D. Hincks,Renée Hlozek,S. P. Patty Ho,Zhiqi Huang,Johannes Hubmayr,Kevin M. Huffenberger,John P. Hughes,Leopoldo Infante,Kent D. Irwin,Simon Muya Kasanda,Jeff Klein,Brian J. Koopman,Arthur Kosowsky,Dale Li,Mathew S. Madhavacheril,Tobias A. Marriage,Jeff McMahon,Felipe Menanteau,Kavilan Moodley,Charles Munson,Sigurd Naess,Federico Nati,Laura Newburgh,John P. Nibarger,Michael D. Niemack,Michael R. Nolta,Carolina Núñez,Carolina Núñez,Carolina Núñez,Lyman A. Page,Christine G. Pappas,Bruce Partridge,Felipe Rojas,Emmanuel Schaan,Benjamin L. Schmitt,Neelima Sehgal,Blake D. Sherwin,Jon Sievers,Sara M. Simon,David N. Spergel,Suzanne T. Staggs,Eric R. Switzer,Eric R. Switzer,Robert Thornton,Robert Thornton,Hy Trac,Jesse Treu,Carole Tucker,Alexander van Engelen,Jonathan T. Ward,Edward J. Wollack +92 more
TL;DR: In this paper, the Atacama Cosmology Telescope Polarimeter (ACTPol) was used to estimate cosmological parameters from the temperature, polarization, and temperature-polarization cross-correlations.
Journal ArticleDOI
Measurements of the temperature and E-mode polarization of the CMB from 500 square degrees of SPTpol data
Jason W. Henning,J. T. Sayre,Christian L. Reichardt,Peter A. R. Ade,Adam Anderson,Jason E. Austermann,James A. Beall,Amy N. Bender,Amy N. Bender,Bradford Benson,Bradford Benson,Lindsey Bleem,Lindsey Bleem,John E. Carlstrom,C. L. Chang,C. L. Chang,H. C. Chiang,H-M. Cho,Robert I. Citron,C. Corbett Moran,T. M. Crawford,A. T. Crites,A. T. Crites,T. de Haan,Matt Dobbs,Matt Dobbs,W. B. Everett,Jason Gallicchio,Jason Gallicchio,Elizabeth George,Elizabeth George,A. J. Gilbert,N. W. Halverson,N. L. Harrington,Gene C. Hilton,Gilbert Holder,Gilbert Holder,W. L. Holzapfel,S. Hoover,Zhen Hou,J. D. Hrubes,N. Huang,Johannes Hubmayr,Kent D. Irwin,Ryan Keisler,Lloyd Knox,Adrian T. Lee,Adrian T. Lee,E. M. Leitch,Dale Li,Dale Li,A. E. Lowitz,A. Manzotti,Jeff McMahon,S. S. Meyer,L. M. Mocanu,Joshua Montgomery,Joshua Montgomery,Andrew Nadolski,T. Natoli,John P. Nibarger,V. Novosad,Stephen Padin,Stephen Padin,C. Pryke,J. E. Ruhl,Benjamin Saliwanchik,K. K. Schaffer,K. K. Schaffer,C. Sievers,Graeme Smecher,Antony A. Stark,K. T. Story,Carole Tucker,K. Vanderlinde,T. Veach,Joaquin Vieira,Gensheng Wang,Nathan Whitehorn,Nathan Whitehorn,W. L. K. Wu,Volodymyr Yefremenko +81 more
TL;DR: Henning et al. as discussed by the authors measured the E-mode polarization angular power spectrum (EE) and temperature-E-mode cross-power spectrum (TE) of the cosmic microwave background (CMB) using 150 GHz data from three seasons of SPTpol observations.
Journal ArticleDOI
Anatomy of the inert two-Higgs-doublet model in the light of the LHC and non-LHC dark matter searches
Alexander Belyaev,Alexander Belyaev,Giacomo Cacciapaglia,Igor P. Ivanov,Felipe Rojas-Abatte,Felipe Rojas-Abatte,Marc Thomas,Marc Thomas +7 more
TL;DR: The inert two-Higgs-doublet model (i2HDM) is a theoretically well-motivated example of a minimal consistent dark matter (DM) model which provides monojet, mono-Z, mono Higgs, and vector-boson-fusion+ETmiss signatures at the LHC, complemented by signals in direct and indirect DM search experiments as mentioned in this paper.
Journal ArticleDOI
$H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method
Adrià Gómez-Valent,Luca Amendola +1 more
TL;DR: In this article, the authors presented new constraints on the Hubble parameter $H_0$ using the available data on $H(z)$ obtained from cosmic chronometers (CCH); the Hubble rate data points extracted from the supernovae of Type Ia (SnIa) of the Pantheon compilation and the Hubble Space Telescope (HST) CANDELS and CLASH Multy-Cycle Treasury (MCT) programs.
Journal ArticleDOI
Low-mass dark matter search with CDMSlite
R. Agnese,Adam Anderson,T. Aralis,Tsuguo Aramaki,I. J. Arnquist,W. Baker,D. Balakishiyeva,D. Barker,R. Basu Thakur,D. A. Bauer,T. Binder,M. A. Bowles,P. L. Brink,R. Bunker,Blas Cabrera,David O. Caldwell,R. Calkins,C. Cartaro,David G. Cerdeño,Yu Kai Chang,H. Chagani,Yi Chen,Jodi Cooley,B. Cornell,P. Cushman,Miguel Daal,P. Di Stefano,T. Doughty,L. Esteban,E. Fascione,Enectali Figueroa-Feliciano,Matthew Fritts,G. Gerbier,M. Ghaith,G.L. Godfrey,Sunil Golwala,J. Hall,H. R. Harris,Ziqing Hong,Eric W. Hoppe,L. Hsu,Martin E. Huber,V. Iyer,D. Jardin,A. Jastram,Chitrasen Jena,M. H. Kelsey,A. Kennedy,A. Kubik,Noah Kurinsky,A. Leder,B. Loer,E. Lopez Asamar,P. Lukens,D. MacDonell,R. Mahapatra,Vuk Mandic,N. Mast,E. H. Miller,N. Mirabolfathi,Robert A. Moffatt,Bedangadas Mohanty,J. D. Morales Mendoza,J. K. Nelson,John L. Orrell,S. M. Oser,K. L. Page,W. A. Page,R. Partridge,M. Pepin,M. Peñalver Martinez,A. Phipps,S. S. Poudel,Matt Pyle,H. Qiu,W. Rau,P. Redl,A. Reisetter,T. Reynolds,Amy Roberts,A. E. Robinson,H. E. Rogers,Tarek Saab,Bernard Sadoulet,J. Sander,K. Schneck,R. W. Schnee,S. Scorza,Kartik Senapati,B. Serfass,Danielle Speller,M. Stein,J. Street,Hiromasa Tanaka,D. Toback,R. Underwood,A. N. Villano,B. von Krosigk,B. Welliver,John Wilson,M. J. Wilson,D. H. Wright,S. J. Yellin,J. J. Yen,Betty A. Young,X. Zhang,Xingbo Zhao +106 more
TL;DR: The SuperCDMS experiment at the Soudan Underground Laboratory was designed to directly detect weakly interacting massive particles (WIMPs) that may constitute the dark matter in our Galaxy as discussed by the authors.
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TL;DR: In this paper, the authors present the first results based on Planck measurements of the CMB temperature and lensing-potential power spectra, which are extremely well described by the standard spatially-flat six-parameter LCDM cosmology.
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Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
Eiichiro Komatsu,Jo Dunkley,M. R. Nolta,Charles L. Bennett,B. Gold,Gary Hinshaw,Norman Jarosik,David L. Larson,Michele Limon,L. Page,David N. Spergel,Mark Halpern,Robert S. Hill,A. Kogut,S. S. Meyer,G. S. Tucker,Janet Weiland,Edward J. Wollack,Edward L. Wright +18 more
TL;DR: In this paper, the authors show that the tensor-to-scalar ratio r 1 is disfavored regardless of r. They provide a set of "WMAP distance priors, to test a variety of dark energy models.
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Big-Bang Nucleosynthesis
TL;DR: In this article, a critical review of the current status of cosmological nucleosynthesis is given, where the baryon-to-photon ratio of deuterium and helium-4 is consistent with the independent determination of $\eta$ from observations of anisotropies in the cosmic microwave background.
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HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
Krzysztof M. Gorski,E. Hivon,A. J. Banday,Benjamin D. Wandelt,F. K. Hansen,Martin Reinecke,M. Bartelman +6 more
TL;DR: The Hierarchical Equal Area iso-Latitude Pixelization (HEALPix) as discussed by the authors is a data structure with an associated library of computational algorithms and visualization software that supports fast scientific applications executable directly on very large volumes of astronomical data and large area surveys in the form of discretized spherical maps.
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Planck 2013 results. XVI. Cosmological parameters
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