Results 21 to 30 of about 536,719 (375)
SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: COSMOLOGICAL INTERPRETATION [PDF]
, 2010 The combination of seven-year data from WMAP and improved astrophysical data rigorously tests the standard cosmological model and places new constraints on its basic parameters and extensions.E. Komatsu, K. Smith, J. Dunkley, C. Bennett, B. Gold, G. Hinshaw, N. Jarosik, D. Larson, M. Nolta, L. Page, D. Spergel, M. Halpern, R. Hill, A. Kogut, M. Limon, S. Meyer, N. Odegard, G. Tucker, J. Weiland, Edward J. Wollack, E. L. Wright +20 moresemanticscholar +1 more sourceRASTALL COSMOLOGY [PDF]
International Journal of Modern Physics: Conference Series, 2012 We review the difficulties of the generalized Chaplygin gas model to fit observational data, due to the tension between background and perturbative tests. We argue that such issues may be circumvented by means of a self-interacting scalar field representation of the model.Julio C. Fabris, PIATTELLA O, Davi C. Rodrigues, Carlos E. M. Batista, Mahamadou H. Daouda +4 moreopenaire +3 more sourcesUnveiling the Universe with emerging cosmological probes [PDF]
Living Reviews in Relativity, 2022 The detection of the accelerated expansion of the Universe has been one of the major breakthroughs in modern cosmology. Several cosmological probes (Cosmic Microwave Background, Supernovae Type Ia, Baryon Acoustic Oscillations) have been studied in depth Michele Moresco, L. Amati, L. Amendola, S. Birrer, J. Blakeslee, M. Cantiello, A. Cimatti, J. Darling, M. Valle, M. Fishbach, C. Grillo, N. Hamaus, D. Holz, L. Izzo, R. Jimenez, E. Lusso, M. Meneghetti, E. Piedipalumbo, A. Pisani, A. Pourtsidou, L. Pozzetti, M. Quartin, G. Risaliti, P. Rosati, L. Verde +24 moresemanticscholar +1 more sourceFirst-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters [PDF]
, 2003 WMAP precision data enable accurate testing of cosmological models. We find that the emerging standard model of cosmology, a flat Λ-dominated universe seeded by a nearly scale-invariant adiabatic Gaussian fluctuations, fits the WMAP data.D. Spergel, L. Verde, H. Peiris, E. Komatsu, M. Nolta, C. Bennett, M. Halpern, G. Hinshaw, N. Jarosik, A. Kogut, M. Limon, S. Meyer, L. Page, G. Tucker, J. Weiland, Edward J. Wollack, E. L. W. Princeton, Nasa Gsfc, Ubc, U. Chicaco, Brown, Ssai, Ucla +22 moresemanticscholar +1 more sourceHomogeneous cosmologies with a cosmological constant [PDF]
Physical Review D, 1999 Spatially homogeneous cosmological models with a positive cosmological constant are investigated, using dynamical systems methods. We focus on the future evolution of these models. In particular, we address the question whether there are models within this class that are de Sitter-like in the future, but are tilted.Goliath, Martin, Ellis, George F. R.openaire +2 more sourcesNINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS [PDF]
, 2012 We present cosmological parameter constraints based on the final nine-year Wilkinson Microwave Anisotropy Probe (WMAP) data, in conjunction with a number of additional cosmological data sets.G. Hinshaw, D. Larson, E. Komatsu, D. Spergel, C. Bennett, J. Dunkley, M. Nolta, M. Halpern, R. Hill, N. Odegard, L. Page, K. Smith, J. Weiland, B. Gold, N. Jarosik, A. Kogut, M. Limon, S. Meyer, G. Tucker, Edward J. Wollack, E. Wright +20 moresemanticscholar +1 more sourceIs the observable Universe consistent with the cosmological principle? [PDF]
Classical and quantum gravity, 2022 The cosmological principle (CP)—the notion that the Universe is spatially isotropic and homogeneous on large scales—underlies a century of progress in cosmology.Pavan K. Aluri, P. Cea, P. Chingangbam, M. Chu, R. Clowes, D. Hutsem'ekers, Joby P. Kochappan, Andrzej Krasi'nski, Alexia M. Lopez, Lang Liu, N. C. Martens, C. Martins, K. Migkas, Eoin 'O Colg'ain, Pratyush Pranav, L. Shamir, A. Singal, M. Sheikh-Jabbari, J. Wagner, Shao-Jiang Wang, D. Wiltshire, S. Yeung, Lu Yin, Wen Zhao +23 moresemanticscholar +1 more sourceCompleted SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory [PDF]
Physical Review D, 2020 We present the cosmological implications from final measurements of clustering using galaxies, quasars, and Ly$\alpha$ forests from the completed Sloan Digital Sky Survey (SDSS) lineage of experiments in large-scale structure. These experiments, composed S. Alam, M. Aubert, S. Ávila, C. Balland, J. Bautista, M. Bershady, D. Bizyaev, M. Blanton, A. Bolton, J. Bovy, J. Brinkmann, J. Brownstein, É. Burtin, S. Chabanier, Michael J. Chapman, P. D. Choi, C. Chuang, J. Comparat, M. Cousinou, A. Cuceu, K. Dawson, Sylvain de la Torre, A. de Mattia, Victoria de Sainte Agathe, Hélion du Mas des Bourboux, S. Escoffier, T. Etourneau, J. Farr, A. Font-Ribera, P. Frinchaboy, S. Fromenteau, H. Gil-Marín, J. Le Goff, A. González-Morales, V. Gonzalez-Perez, K. Grabowski, J. Guy, A. Hawken, Jiamin Hou, H. Kong, James Parker, M. Klaene, J. Kneib, Sicheng Lin, D. Long, B. Lyke, A. de la Macorra, P. Martini, K. Masters, F. G. Mohammad, J. Moon, E. Mueller, A. Muñoz-Gutiérrez, A. Myers, S. Nadathur, R. Neveux, J. Newman, P. Noterdaeme, A. Oravetz, D. Oravetz, N. Palanque-Delabrouille, K. Pan, R. Paviot, W. Percival, I. Pérez-Ràfols, P. Petitjean, M. Pieri, A. Prakash, A. Raichoor, C. Ravoux, M. Rezaie, J. Rich, A. Ross, G. Rossi, R. Ruggeri, V. Ruhlmann-Kleider, A. Sánchez, F. Sa'nchez, J. Sánchez-Gallego, Conor Sayres, D. Schneider, H. Seo, A. Shafieloo, A. Slosar, Alex Smith, Julianna Stermer, A. Tamone, J. Tinker, R. Tojeiro, M. Vargas-Magaña, A. Variu, Yuting Wang, B. Weaver, A. Weijmans, C. Yéche, P. Zarrouk, Cheng Zhao, Gong-Bo Zhao, Zheng Zheng +98 moresemanticscholar +1 more sourcePlanck 2013 results. XVI. Cosmological parameters [PDF]
, 2013 This paper presents the first cosmological results based on Planck measurements of the cosmic microwave background (CMB) temperature and lensing-potential power spectra. We find that the Planck spectra at high multipoles (l greater than or similar to 40) P. Ade, N. Aghanim, C. Armitage-Caplan, M. Arnaud, M. Ashdown, F. Atrio-Barandela, J. Aumont, C. Baccigalupi, A. Banday, R. B. Barreiro, J. G. Bartlett, E. Battaner, K. Benabed, A. Benoit, A. Benoit-Lévy, J. Bernard, M. Bersanelli, P. Bielewicz, J. Bobin, J. Bock, A. Bonaldi, J. Bond, J. Borrill, F. Bouchet, M. Bridges, M. Bucher, C. Burigana, R. C. Butler, E. Calabrese, B. Cappellini, J. Cardoso, A. Catalano, A. Challinor, A. Chamballu, R. Chary, Xun Chen, H. Chiang, L. Chiang, P. Christensen, S. Church, D. Clements, S. Colombi, L. Colombo, F. Couchot, A. Coulais, B. Crill, A. Curto, F. Cuttaia, L. Danese, R. Davies, R. Davis, P. Bernardis, A. Rosa, G. Zotti, J. Delabrouille, J. Delouis, F. Désert, C. Dickinson, J. Diego, K. Dolag, H. Dole, S. Donzelli, O. Doré, M. Douspis, J. Dunkley, X. Dupac, G. Efstathiou, F. Elsner, T. Ensslin, H. Eriksen, F. Finelli, O. Forni, M. Frailis, A. Fraisse, E. Franceschi, T. Gaier, S. Galeotta, S. Galli, K. Ganga, M. Giard, G. Giardino, Y. Giraud-Héraud, E. Gjerløw, J. González-Nuevo, K. Górski, S. Gratton, A. Gregorio, A. Gruppuso, J. Gudmundsson, J. Haissinski, J. Hamann, F. Hansen, D. Hanson, D. Harrison, S. Henrot-Versillé, C. Hernández-Monteagudo, D. Herranz, S. Hildebrandt, E. Hivon, M. Hobson, W. Holmes, A. Hornstrup, Z. Hou, W. Hovest, K. Huffenberger, A. Jaffe, T. Jaffe, J. Jewell, W. Jones, M. Juvela, E. Keihänen, R. Keskitalo, T. Kisner, R. Kneissl, J. Knoche, L. Knox, M. Kunz, H. Kurki-Suonio, G. Lagache, A. Lähteenmäki, J. Lamarre, A. Lasenby, M. Lattanzi, R. Laureijs, C. Lawrence, S. Leach, J. Leahy, R. Leonardi, J. León-Tavares, J. Lesgourgues, Antony Lewis, M. Liguori, P. Lilje, M. Linden-Vørnle, M. López-Caniego, P. Lubin, J. Macías-Pérez, B. Maffei, D. Maino, N. Mandolesi, M. Maris, D. Marshall, P. Martin, E. Martinez-Gonzalez, S. Masi, M. Massardi, S. Matarrese, F. Matthai, P. Mazzotta, P. Meinhold, A. Melchiorri, J. Melin, L. Mendes, E. Menegoni, A. Mennella, M. Migliaccio, M. Millea, S. Mitra, M. Miville-Deschênes, A. Moneti, L. Montier, G. Morgante, D. Mortlock, A. Moss, D. Munshi, J. Murphy, P. Naselsky, F. Nati, P. Natoli, C. Netterfield, H. Nørgaard-Nielsen, F. Noviello, D. Novikov, I. Novikov, I. O'Dwyer, S. Osborne, C. A. Oxborrow, F. Paci, L. Pagano, F. Pajot, R. Paladini, D. Paoletti, B. Partridge, F. Pasian, G. Patanchon, D. Pearson, T. Pearson, H. Peiris, O. Perdereau, L. Perotto, F. Perrotta, V. Pettorino, F. Piacentini, M. Piat, E. Pierpaoli, D. Pietrobon, S. Plaszczynski, P. Platania, E. Pointecouteau, G. Polenta, N. Ponthieu, L. Popa, T. Poutanen, G. Pratt, G. Prezeau, S. Prunet, J. Puget, J. Rachen, W. Reach, R. Rebolo, M. Reinecke, M. Remazeilles, C. Renault, S. Ricciardi, T. Riller, I. Ristorcelli, G. Rocha, C. Rosset, G. Roudier, M. Rowan‐Robinson, J. Rubiño-Martín, B. Rusholme, M. Sandri, D. Santos, M. Savelainen, G. Savini, D. Scott, M. Seiffert, E. Shellard, L. Spencer, Jean-Luc Starck, V. Stolyarov, R. Stompor, R. Sudiwala, R. Sunyaev, F. Sureau, D. Sutton, A.-S. Suur-Uski, J. Sygnet, J. Tauber, D. Tavagnacco, L. Terenzi, L. Toffolatti, M. Tomasi, M. Tristram, M. Tucci, J. Tuovinen, M. Türler, G. Umana, L. Valenziano, J. Valiviita, B. Tent, P. Vielva, F. Villa, N. Vittorio, L. Wade, B. Wandelt, I. Wehus, M. White, S. White, A. Wilkinson, D. Yvon, A. Zacchei, A. Zonca +263 moresemanticscholar +1 more source