Results 11 to 20 of about 1,370,806 (214)
The chaotic universe [PDF]
Chaos, Solitons & Fractals, 2000 It is shown that the mysterious quantum prescription of microphysics has analogues at the scale of stars, galaxies and superclusters, the common feature in all these cases being Brownian type fractality. These considerations are shown to lead to pleasingly meaningful results in agreement with observed data.Abbott, Agnese, B.G. Sidharth, Borgani, Caldirola, Carneiro, El Naschie, Godel, Hawking, Hoyle, Laskar, Nelson, Ralston, Sidharth, Sidharth, Sidharth, Weinberg +16 morecore +15 more sourcesObjaverse-XL: A Universe of 10M+ 3D Objects [PDF]
Neural Information Processing Systems, 2023 Natural language processing and 2D vision models have attained remarkable proficiency on many tasks primarily by escalating the scale of training data. However, 3D vision tasks have not seen the same progress, in part due to the challenges of acquiring ...Matt Deitke, Ruoshi Liu, Matthew Wallingford, Huong Ngo, Oscar Michel, Aditya Kusupati, Alan Fan, Christian Laforte, Vikram S. Voleti, S. Gadre, Eli VanderBilt, Aniruddha Kembhavi, Carl Vondrick, Georgia Gkioxari, Kiana Ehsani, Ludwig Schmidt, Ali Farhadi +16 moresemanticscholar +1 more sourceObjaverse: A Universe of Annotated 3D Objects [PDF]
Computer Vision and Pattern Recognition, 2022 Massive data corpora like WebText, Wikipedia, Conceptual Captions, WebImageText, and LAION have propelled recent dramatic progress in AI. Large neural models trained on such datasets produce impressive results and top many of today's benchmarks.Matt Deitke, Dustin Schwenk, Jordi Salvador, Luca Weihs, Oscar Michel, Eli VanderBilt, Ludwig Schmidt, Kiana Ehsani, Aniruddha Kembhavi, Ali Farhadi +9 moresemanticscholar +1 more sourceObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant [PDF]
, 1998 We present spectral and photometric observations of 10 Type Ia supernovae (SNe Ia) in the redshift range 0.16 ≤ z ≤ 0.62. The luminosity distances of these objects are determined by methods that employ relations between SN Ia luminosity and light curve ...A. Riess, A. Filippenko, P. Challis, A. Clocchiatti, A. Diercks, P. Garnavich, R. Gilliland, C. Hogan, S. Jha, R. Kirshner, B. Leibundgut, M. Phillips, D. Reiss, B. Schmidt, R. Schommer, R. C. Smith, R. C. Smith, J. Spyromilio, C. Stubbs, N. Suntzeff, J. Tonry +20 moresemanticscholar +2 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 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 sourceDetection of early-universe gravitational-wave signatures and fundamental physics [PDF]
General Relativity and Gravitation, 2022 Detection of a gravitational-wave signal of non-astrophysical origin would be a landmark discovery, potentially providing a significant clue to some of our most basic, big-picture scientific questions about the Universe.R. Caldwell, Yanou Cui, Huai-Ke Guo, V. Mandic, Alberto Mariotti, J. No, M. Ramsey-Musolf, M. Sakellariadou, K. Sinha, Lian-tao Wang, G. White, Yue Zhao, H. An, C. Caprini, S. Clesse, J. Cline, G. Cusin, Ryusuke Jinno, B. Laurent, N. Levi, Kunfeng Lyu, Miguel Ángel Martínez, Andrew L. Miller, D. Redigolo, C. Scarlata, A. Sevrin, Barmak Shams Es Haghi, Jing Shu, X. Siemens, D. Steer, R. Sundrum, C. Tamarit, D. Weir, B. Fornal, Ke-Pan Xie, Fengwei Yang, Siyi Zhou +36 moresemanticscholar +1 more sourceIceCube-Gen2: the window to the extreme Universe [PDF]
Journal of Physics G: Nuclear and Particle Physics, 2020 The observation of electromagnetic radiation from radio to $\gamma$-ray wavelengths has provided a wealth of information about the universe. However, at PeV (10$^{15}$ eV) energies and above, most of the universe is impenetrable to photons.T. I. C. M. G. Aartsen, R. Abbasi, M. Ackermann, J. Adams, J. Aguilar, M. Ahlers, M. Ahrens, C. Alispach, P. Allison, N. M. Amin, K. Andeen, T. Anderson, I. Ansseau, G. Anton, C. Arguelles, T. Arlen, J. Auffenberg, S. Axani, H. Bagherpour, X. Bai, V. A.Balagopal, A. Barbano, I. Bartos, B. Bastian, V. Basu, V. Baum, S. Baur, R. Bay, J. Beatty, K. Becker, J. Tjus, S. Benzvi, D. Berley, E. Bernardini, D. Besson, G. Binder, D. Bindig, E. Blaufuss, S. Blot, C. Bohm, M. Bohmer, S. Boser, O. Botner, J. Bottcher, E. Bourbeau, J. Bourbeau, F. Bradascio, J. Braun, S. Bron, J. Brostean-Kaiser, A. Burgman, R. Burley, J. Buscher, R. Busse, M. Bustamante, M. Campana, E. Carnie-Bronca, T. Carver, C. Chen, P. Chen, E. Cheung, D. Chirkin, S. Choi, B. Clark, K. Clark, L. Classen, A. Coleman, G. Collin, A. Connolly, J. Conrad, P. Coppin, P. Correa, D. Cowen, R. Cross, P. Dave, C. Deaconu, C. Clercq, J. DeLaunay, S. D. Kockere, H. Dembinski, K. Deoskar, S. Ridder, A. Desai, P. Desiati, K. D. Vries, G. Wasseige, M. With, T. DeYoung, S. Dharani, A. Diaz, J. C. D'iaz-V'elez, H. Dujmovic, M. Dunkman, M. DuVernois, E. Dvorak, T. Ehrhardt, P. Eller, R. Engel, J. Evans, P. Evenson, S. Fahey, K. Farrag, A. Fazely, J. Felde, A. Fienberg, K. Filimonov, C. Finley, L. Fischer, D. Fox, A. Franckowiak, E. Friedman, A. Fritz, T. Gaisser, J. Gallagher, E. Ganster, D.Garcia-Fernandez, S. Garrappa, A. Gartner, L. Gerhardt, R. Gernhaeuser, A. Ghadimi, C. Glaser, T. Glauch, T. Glusenkamp, A. Goldschmidt, J. G. Gonzalez, S. Goswami, D. Grant, T. Gr'egoire, Z. Griffith, S. Griswold, M. Gunduz, C. Haack, A. Hallgren, R. Halliday, L. Halve, F. Halzen, J. Hanson, K. Hanson, J. Hardin, J. Haugen, A. Haungs, S. Hauser, D. Hebecker, D. Heinen, P. Heix, K. Helbing, R. Hellauer, F. Henningsen, S. Hickford, J. Hignight, C. Hill, G. Hill, K. Hoffman, B. Hoffmann, R. Hoffmann, T. Hoinka, B. Hokanson-Fasig, K. Holzapfel, K. Hoshina, F. Huang, M. Huber, T. Huber, T. Huege, K. Hughes, K. Hultqvist, Mirco Hünnefeld, R. Hussain, S. In, N. Iovine, A. Ishihara, M. Jansson, G. Japaridze, M. Jeong, B. Jones, F. Jonske, R. Joppe, O. Kalekin, D. Kang, W. Kang, X. Kang, A. Kappes, D. Kappesser, T. Karg, M. Karl, A. Karle, T. Katori, U. Katz, M. Kauer, A. Keivani, M. Kellermann, J. Kelley, A. Kheirandish, J. Kim, K. Kin, T. Kintscher, J. Kiryluk, T. Kittler, M. Kleifges, S. R. Klein, R. Koirala, H. Kolanoski, L. Kopke, C. Kopper, S. Kopper, D. Koskinen, P. Koundal, M. Kovacevich, M. Kowalski, C. Krauss, K. Krings, G. Kruckl, N. Kulacz, N. Kurahashi, C. L. Gualda, R. Lahmann, J. Lanfranchi, M. Larson, U. Latif, F. Lauber, J. Lazar, K. Leonard, A. Leszczy'nska, Y. Li, Q. Liu, E. Lohfink, J. LoSecco, C. J. L. Mariscal, L. Lu, F. Lucarelli, A. Ludwig, J. Lunemann, W. Luszczak, Y. Lyu, W. Ma, J. Madsen, G. Maggi, K. Mahn, Y. Makino, P. Mallik, S. Mancina, S. Mandalia, I. Marics, S. Márka, Z. Márka, R. Maruyama, K. Mase, R. Maunu, F. McNally, K. Meagher, A. Medina, M. Meier, S. Meighen-Berger, J. Merz, Z. Meyers, J. Micallef, D. Mockler, G. Moment'e, T. Montaruli, R. Moore, R. Morse, M. Moulai, P. Muth, R. Naab, R. Nagai, J. Nam, U. Naumann, J. Necker, G. Neer, A. Nelles, L. Nguyen, H. Niederhausen, M. Nisa, S. Nowicki, D. Nygren, E. Oberla, A. Pollmann, M. Oehler, A. Olivas, E. O’Sullivan, Y. Pan, H. Pandya, D. Pankova, L. Papp, N. Park, G. Parker, E. Paudel, P. Peiffer, C. P. D. L. Heros, T. Petersen, S. Philippen, D. Pieloth, S. Pieper, J. Pinfold, A. Pizzuto, I. Plaisier, M. Plum, Y. Popovych, A. Porcelli, M. Rodriguez, P. Price, G. Przybylski, C. Raab, A. Raissi, M. Rameez, L. Rauch, K. Rawlins, I. C. Rea, A. Rehman, R. Reimann, M. Renschler, G. Renzi, E. Resconi, S. Reusch, W. Rhode, M. Richman, B. Riedel, M. Riegel, E. Roberts, S. Robertson, G. Roellinghoff, M. Rongen, C. Rott, T. Ruhe, D. Ryckbosch, D. R. Cantu, I. Safa, S. S. Herrera, A. Sandrock, J. Sandroos, P. Sandstrom, M. Santander, S. Sarkar, K. Satalecka, Maximilian Karl Scharf, M. Schaufel, H. Schieler, P. Schlunder, T. Schmidt, A. Schneider, J. Schneider, F. Schroder, L. Schumacher, S. Sclafani, D. Seckel, S. Seunarine, M. Shaevitz, A. Sharma, S. Shefali, M. Silva, D. Smith, B. Smithers, R. Snihur, J. Soedingrekso, D. Soldin, S. Soldner-Rembold, M. Song, D. Southall, G. Spiczak, C. Spiering, J. Stachurska, M. Stamatikos, T. Stanev, R. Stein, J. Stettner, A. Steuer, T. Stezelberger, R. Stokstad, N. Strotjohann, T. Sturwald, T. Stuttard, G. Sullivan, I. Taboada, A. Taketa, H. Tanaka, F. Tenholt, S. Ter-Antonyan, A. Terliuk, S. Tilav, K. Tollefson, L. Tomankova, C. Tonnis, J. Torres, S. Toscano, D. Tosi, A. Trettin, M. Tselengidou, C. Tung, A. Turcati, R. Turcotte, C. Turley, J. P. Twagirayezu, B. Ty, E. Unger, M. U. Elorrieta, J. Vandenbroucke, D. Eijk, N. Eijndhoven, D. Vannerom, J. Santen, D. Veberič, S. Verpoest, A. Vieregg, M. Vraeghe, C. Walck, T. Watson, C. Weaver, A. Weindl, L. Weinstock, M. Weiss, J. Weldert, C. Welling, C. Wendt, J. Werthebach, N. Whitehorn, K. Wiebe, C. Wiebusch, D. Williams, S. Wissel, M. Wolf, T. R. Wood, K. Woschnagg, G. Wrede, S. Wren, J. Wulff, X. Xu, Y. Xu, J. Yáñez, S. Yoshida, T. Yuan, Z. Zhang, S. Zierke, M. Zocklein +432 moresemanticscholar +1 more source