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  1. 5281
    por Renzini, Alvio, Bender, Ralf
    Publicado 2005
    “…Theoretical models of galaxy formation and cosmological evolution now face a serious challenge to match the plethora of observational data. …”
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    Multiwavelength Mapping of Galaxy Formation and Evolution
  2. 5282
    por Lesgourgues, Julien, Tram, Thomas
    Publicado 2011
    “…When adding one massive neutrino to the minimal cosmological model, CLASS becomes just 1.5 times slower, instead of about 5 times in other codes (for fixed accuracy requirements). …”
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    The Cosmic Linear Anisotropy Solving System (CLASS) IV: efficient implementation of non-cold relics
  3. 5283
    por Beringer, J, Arguin, J F, Barnett, R M, Copic, K, Dahl, O, Groom, D E, Lin, C J, Lys, J, Murayama, H, Wohl, C G, Yao, W M, Zyla, P A, Amsler, C, Antonelli, M, Asner, D M, Baer, H, Band, H R, Basaglia, T, Bauer, C W, Beatty, J J, Belousov, V I, Bergren, E, Bernardi, G, Bertl, W, Bethke, S, Bichsel, H, Biebel, O, Blucher, E, Blusk, S, Brooijmans, G, Buchmueller, O, Cahn, R N, Carena, M, Ceccucci, A, Chakraborty, D, Chen, M C, Chivukula, R S, Cowan, G, D'Ambrosio, G, Damour, T, de Florian, D, de Gouvea, A, DeGrand, T, de Jong, P, Dissertori, G, Dobrescu, B, Doser, M, Drees, M, Edwards, D A, Eidelman, S, Erler, J, Ezhela, V V, Fetscher, W, Fields, B D, Foster, B, Gaisser, T K, Garren, L, Gerber, H J, Gerbier, G, Gherghetta, T, Golwala, S, Goodman, M, Grab, C, Gritsan, A V, Grivaz, J F, Grunewald, M, Gurtu, A, Gutsche, T, Haber, H E, Hagiwara, K, Hagmann, C, Hanhart, C, Hashimoto, S, Hayes, K G, Heffner, M, Heltsley, B, Hernandez-Rey, J J, Hikasa, K, Hocker, A, Holder, J, Holtkamp, A, Huston, J, Jackson, J D, Johnson, K F, Junk, T, Karlen, D, Kirkby, D, Klein, S R, Klempt, E, Kowalewski, R V, Krauss, F, Kreps, M, Krusche, B, Kuyanov, Yu.V, Kwon, Y, Lahav, O, Laiho, J, Langacker, P, Liddle, A, Ligeti, Z, Liss, T M, Littenberg, L, Lugovsky, K S, Lugovsky, S B, Mannel, T, Manohar, A V, Marciano, W J, Martin, A D, Masoni, A, Matthews, J, Milstead, D, Miquel, R, Monig, K, Moortgat, F, Nakamura, K, Narain, M, Nason, P, Navas, S, Neubert, M, Nevski, P, Nir, Y, Olive, K A, Pape, L, Parsons, J, Patrignani, C, Peacock, J A, Petcov, S T, Piepke, A, Pomarol, A, Punzi, G, Quadt, A, Raby, S, Raffelt, G, Ratcliff, B N, Richardson, P, Roesler, S, Rolli, S, Romaniouk, A, Rosenberg, L J, Rosner, J L, Sachrajda, C T, Sakai, Y, Salam, G P, Sarkar, S, Sauli, F, Schneider, O, Scholberg, K, Scott, D, Seligman, W G, Shaevitz, M H, Sharpe, S R, Silari, M, Sjostrand, T, Skands, P, Smith, J G, Smoot, G F, Spanier, S, Spieler, H, Stahl, A, Stanev, T, Stone, S L, Sumiyoshi, T, Syphers, M J, Takahashi, F, Tanabashi, M, Terning, J, Titov, M, Tkachenko, N P, Tornqvist, N A, Tovey, D, Valencia, G, van Bibber, K, Venanzoni, G, Vincter, M G, Vogel, P, Vogt, A, Walkowiak, W, Walter, C W, Ward, D R, Watari, T, Weiglein, G, Weinberg, E J, Wiencke, L R, Wolfenstein, L, Womersley, J, Woody, C L, Workman, R L, Yamamoto, A, Zeller, G P, Zenin, O V, Zhang, J, Zhu, R Y, Harper, G, Lugovsky, V S, Schaffner, P
    Publicado 2012
    “…Among the 112 reviews are many that are new or heavily revised including those on Heavy-Quark and Soft-Collinear Effective Theory, Neutrino Cross Section Measurements, Monte Carlo Event Generators, Lattice QCD, Heavy Quarkonium Spectroscopy, Top Quark, Dark Matter, Vcb & Vub, Quantum Chromodynamics, High-Energy Collider Parameters, Astrophysical Constants, Cosmological Parameters, and Dark Matter.…”
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    Review of Particle Physics, 2012-2013
  4. 5284
    por Aghanim, N, Armitage-Caplan, C, Arnaud, M, Ashdown, M, Atrio-Barandela, F, Aumont, J, Baccigalupi, C, Banday, A J, Barreiro, R B, Battaner, E, Benabed, K, Benoît, A, Benoit-Lévy, A, Bernard, J -P, Bersanelli, M, Bielewicz, P, Bobin, J, Bock, J J, Bonaldi, A, Bonavera, L, Bond, J R, Borrill, J, Bouchet, F R, Bridges, M, Bucher, M, Burigana, C, Butler, R C, Cardoso, J -F, Catalano, A, Chamballu, A, Chiang, L -Y, Christensen, P R, Church, S, Colombi, S, Colombo, L P L, Crill, B P, Cruz, M, Curto, A, Cuttaia, F, Danese, L, Davies, R D, Davis, R J, de Bernardis, P, de Rosa, A, de Zotti, G, Delabrouille, J, Dick, J, Dickinson, C, Diego, J M, Dole, H, Donzelli, S, Doré, O, Douspis, M, Dupac, X, Efstathiou, G, Enßlin, T A, Eriksen, H K, Finelli, F, Forni, O, Frailis, M, Franceschi, E, Gaier, T C, Galeotta, S, Ganga, K, Giard, M, Giraud-Héraud, Y, Gjerløw, E, González-Nuevo, J, Górski, K M, Gratton, S, Gregorio, A, Gruppuso, A, Hansen, F K, Hanson, D, Harrison, D, Henrot-Versillé, S, Hernández-Monteagudo, C, Herranz, D, Hildebrandt, S R, Hivon, E, Hobson, M, Holmes, W A, Hornstrup, A, Hovest, W, Huffenberger, K M, Jaffe, T R, Jaffe, A H, Jewell, J, Jones, W C, Juvela, M, Kangaslahti, P, Keihänen, E, Keskitalo, R, Kiiveri, K, Kisner, T S, Knoche, J, Knox, L, Kunz, M, Kurki-Suonio, H, Lagache, G, Lähteenmäki, A, Lamarre, J -M, Lasenby, A, Laureijs, R J, Lawrence, C R, Leahy, J P, Leonardi, R, Lesgourgues, J, Liguori, M, Lilje, P B, Lindholm, V, Linden-Vørnle, M, López-Caniego, M, Lubin, P M, Macías-Pérez, J F, Maino, D, Mandolesi, N, Maris, M, Marshall, D J, Martin, P G, Martínez-González, E, Masi, S, Matarrese, S, Matthai, F, Mazzotta, P, Meinhold, P R, Melchiorri, A, Mendes, L, Mennella, A, Migliaccio, M, Mitra, S, Moneti, A, Montier, L, Morgante, G, Mortlock, D, Moss, A, Munshi, D, Naselsky, P, Natoli, P, Netterfield, C B, Nørgaard-Nielsen, H U, Novikov, D, Novikov, I, O'Dwyer, I J, Osborne, S, Paci, F, Pagano, L, Paladini, R, Paoletti, D, Partridge, B, Pasian, F, Patanchon, G, Pearson, D, Peel, M, Perdereau, O, Perotto, L, Perrotta, F, Pierpaoli, E, Pietrobon, D, Plaszczynski, S, Platania, P, Pointecouteau, E, Polenta, G, Ponthieu, N, Popa, L, Poutanen, T, Pratt, G W, Prézeau, G, Prunet, S, Puget, J -L, Rachen, J P, Rebolo, R, Reinecke, M, Remazeilles, M, Ricciardi, S, Riller, T, Rocha, G, Rosset, C, Rossetti, M, Roudier, G, Rubiño-Martín, J A, Rusholme, B, Sandri, M, Santos, D, Scott, D, Seiffert, M D, Shellard, E P S, Spencer, L D, Starck, J -L, Stolyarov, V, Stompor, R, Sureau, F, Sutton, D, Suur-Uski, A -S, Sygnet, J -F, Tauber, J A, Tavagnacco, D, Terenzi, L, Toffolatti, L, Tomasi, M, Tristram, M, Tucci, M, Tuovinen, J, Türler, M, Umana, G, Valenziano, L, Valiviita, J, Van Tent, B, Varis, J, Vielva, P, Villa, F, Vittorio, N, Wade, L A, Wandelt, B D, Watson, R, Wilkinson, A, Yvon, D, Zacchei, A, Zonca, A
    Publicado 2013
    “…We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the first release of the Planck cosmological results. We give an overview of the main effects and of the tools and methods applied to assess residuals in maps and power spectra. …”
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    Planck 2013 results. III. LFI systematic uncertainties
  5. 5285
    por Bussey, Peter
    Publicado 2016
    “…Written in clear, accessible prose, Bussey provides a primer on topics such as the laws of nature, quantum physics, fine-tuning, and current cosmological models. He shows that despite the remarkable achievements of science, the latest research in these fields does not lead to simple physicalism in which physical processes are able to explain everything that exists. …”
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    Signposts to God: how modern physics and astronomy point the way to belief
  6. 5286
    por Suchek, Stanislav, Brandt, Oleg
    Publicado 2018
    “…Dark Matter comprises a significant part of the visible Universe. Despite a solid cosmological evidence, its particle nature and properties is still to be unraveled. …”
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    Search for Dark Matter produced in association with a $W$ or $Z$ boson with the ATLAS Experiment at 13 TeV
  7. 5287
    por Kanas, Nick
    Publicado 2019
    “…Also covered in this book are more contemporary cosmological ideas, constellation representations, and cartographic advances. …”
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    Star maps: history, artistry, and cartography
  8. 5288
    “…Nevertheless, there is continuously growing astrophysical and cosmological evidence for its existence. To address present and future developments in the field, novel ideas, theories, and approaches are called for. …”
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    Illuminating Dark Matter : Proceedings of a Simons Symposium
  9. 5289
    “…Cosmological and astrophysical observation point to the existence of an exotic type of matter known as Dark Matter (DM) that accounts for about 27% of the total mass-energy of the Universe. …”
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    Search for new phenomena in mono-X final states using pp collision data collected in Run-2 by the ATLAS experiment at the LHC
  10. 5290
    “…They discuss the difference between the massive and the massless case, highlighting how the two phenomena arise from the same vector portal between the dark and the visible sector. A review of the cosmological and astrophysical observations is provided, together with the connection to dark matter physics. …”
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    The physics of the dark photon: a primer
  11. 5291
    por Lopez Solis, Alvaro
    Publicado 2022
    “…--HTML--><p><span>Astrophysical and cosmological measurements consistently find a presence of dark matter in the universe with an abundance significantly exceeding that of the visible baryonic matter. …”
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    Peeking into the dark with the ATLAS detector
  12. 5292
    por Jones, Dominic
    Publicado 2023
    “…Models of Supersymmetry with Staus masses in this range are of particular interest as they can yield a dark-matter relic density consistent with cosmological observations. This poster will detail a new ATLAS Stau search which utilises multiple Boosted Decision Trees to improve the sensitivity compared to the first wave search, particularly for these low Stau Mass scenarios. …”
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    ATLAS Full Run 2 Search for Direct Stau Production using Machine Learning
  13. 5293
    por Joyce, Michael
    Publicado 1996
    “…A period where the energy in the universe is dominated by such a mode, which I term {\it kination}, can occur as a scalar field rolls down an exponential potential well motivated in many extensions of standard model physics. A cosmological ``constant'' at the present epoch may also result.…”
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    Electroweak Baryogenesis and the Expansion Rate of the Universe
  14. 5294
    “…The number of black holes with $M \sim 100M_{\odot}$ and above is comparable with the number of galaxies within the modern cosmological horizon. The primordial fractal structure of galaxies can find natural grounds in the framework of model we developed . …”
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    Strong Primordial Inhomogeneities and Galaxy Formation
  15. 5295
    por Kirilova, Daniela
    Publicado 2002
    “…It was found that in the resonant case it plays a considerable role even for very big delta N_s ~ 0.8. We discuss cosmological constraints on neutrino mixing for small delta N_s.…”
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    Neutrino Spectrum Distortion Due to Oscillations and its BBN Effect
  16. 5296
    “…We study the parameter space of the constrained Minimal Supersymmetric Standard Model (cMSSM) in a global fit, taking into account the non- observation of supersymmetry at the LHC, Higgs mass and rate measurements, as well as several cosmological and low energy observables. Before the start of the LHC, global fits of the cMSSM showed a favourable goodness-of-fit and indicated a strong preference for the existence of light SUSY particles. …”
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    Killing the cMSSM softly
  17. 5297
    por Lakić, Biljana
    Publicado 2020
    “…IAXO will probe a substantial unexplored region of the axion and ALP parameter space which is theoretically and cosmologically motivated, and thus will have significant discovery potential. …”
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    International Axion Observatory (IAXO) status and prospects
  18. 5298
    por Trout, Aaron D.
    Publicado 2013
    “…Our model predicts a time-varying non-zero cosmological constant with a current value, [Image: see text] in natural units, in agreement with observation. …”
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    Online Artículo Texto
    Dark Energy from Discrete Spacetime
  19. 5299
    “…Fluid dynamics in intrinsically curved geometries is encountered in many physical systems in nature, ranging from microscopic bio-membranes all the way up to general relativity at cosmological scales. Despite the diversity of applications, all of these systems share a common feature: the free motion of particles is affected by inertial forces originating from the curvature of the embedding space. …”
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    Online Artículo Texto
    Energy dissipation in flows through curved spaces
  20. 5300
    “…The cosmic optical background is an important observable that constrains energy production in stars and more exotic physical processes in the universe, and provides a crucial cosmological benchmark against which to judge theories of structure formation. …”
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    Online Artículo Texto
    Measurement of the cosmic optical background using the long range reconnaissance imager on New Horizons
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