Results 41 to 50 of about 165,969,103 (172)
THE SL2S GALAXY-SCALE LENS SAMPLE. IV. THE DEPENDENCE OF THE TOTAL MASS DENSITY PROFILE OF EARLY-TYPE GALAXIES ON REDSHIFT, STELLAR MASS, AND SIZE [PDF]
, 2013 We present optical and near-infrared spectroscopy obtained at Keck, Very Large Telescope, and Gemini for a sample of 36 secure strong gravitational lens systems and 17 candidates identified as part of the Strong Lensing Legacy Survey.A. Sonnenfeld, T. Treu, R. Gavazzi, S. Suyu, P. Marshall, M. Auger, C. L. U. O. California, Santa Barbara, Institut d'astrophysique de Paris, I. O. Astronomy, Astrophysics, Academia Sinica, Kavli Institute for Astrophysics, Cosmology, U. Cambridge, University of Bologna +15 moresemanticscholar +1 more sourceLepton Magnetic Moments: What They Tell Us [PDF]
Acta Physica Polonica B, Proceedings SupplementRecently, the exciting new Fermilab (FNAL) Muon \(g-2\) measurement impressively confirmed the final Brookhaven (BNL) result from 2004 and, with a result four times more precise, has launched a new serious attack on the Standard Model (SM).F. Jegerlehnersemanticscholar +1 more sourceCosmological Perturbations in Double Field Theory
Journal of High Energy Physics, 2023 We explore perturbative double field theory about time-dependent (cosmological) backgrounds to cubic order. To this order the theory is consistent in a weakly constrained sense, so that for a toroidal geometry it encodes both momentum and genuine winding Olaf Hohm, Allison F. Pintodoaj +1 more sourceEuclid preparation. Simulations and non-linearities beyond Lambda cold dark matter. I. Numerical methods and validation [PDF]
Astronomy & AstrophysicsTo constrain cosmological models beyond Lambda CDM, the development of the analysis pipeline requires simulations that capture the non-linear phenomenology of such models.Euclid Collaboration J. Adamek, B. Fiorini, M. Baldi, G. Brando, M.-A. Breton, F. Hassani, K. Koyama, A. Brun, G. R'acz, H. Winther, A. Casalino, C. Hern'andez-Aguayo, B. Li, D. Potter, E. Altamura, C. Carbone, C. Giocoli, D. F. Mota, A. Pourtsidou, Z. Sakr, F. Vernizzi, A. Amara, S. Andreon, N. Auricchio, C. Baccigalupi, S. Bardelli, P. Battaglia, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, A. Caillat, S. Camera, V. Capobianco, V. Cardone, J. Carretero, S. Casas, F. Castander, M. Castellano, G. Castignani, S. Cavuoti, A. Cimatti, C. Colodro-Conde, G. Congedo, C. Conselice, L. Conversi, Y. Copin, F. Courbin, H. Courtois, A. Silva, H. Degaudenzi, G. Lucia, M. Douspis, F. Dubath, X. Dupac, S. Dusini, M. Farina, S. Farrens, S. Ferriol, P. Fosalba, M. Frailis, E. Franceschi, M. Fumana, S. Galeotta, B. Gillis, P. Gómez-Alvarez, A. Grazian, F. Grupp, L. Guzzo, S. Haugan, W. Holmes, F. Hormuth, A. Hornstrup, S. Ili'c, K. Jahnke, M. Jhabvala, B. Joachimi, E. Keihanen, S. Kermiche, A. Kiessling, M. Kilbinger, B. Kubik, M. Kummel, M. Kunz, H. Kurki-Suonio, S. Ligori, P. Lilje, V. Lindholm, I. Lloro, G. Mainetti, E. Maiorano, O. Mansutti, O. Marggraf, K. Markovič, M. Martinelli, N. Martinet, F. Marulli, R. Massey, E. Medinaceli, S. Mei, M. Melchior, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, Michele Moresco, L. Moscardini, C. Neißner, S. Niemi, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, W. Percival, V. Pettorino, S. Pires, G. Polenta, M. Poncet, L. Popa, L. Pozzetti, F. Raison, A. Renzi, J. Rhodes, G. Riccio, E. Romelli, M. Roncarelli, R. Saglia, A. Sánchez, D. Sapone, B. Sartoris, M. Schirmer, T. Schrabback, A. Secroun, G. Seidel, S. Serrano, C. Sirignano, G. Sirri, L. Stanco, J. Steinwagner, P. Tallada-Crespí, D. Tavagnacco, I. Tereno, R. Toledo-Moreo, F. Torradeflot, I. Tutusaus, E. Valentijn, L. Valenziano, T. Vassallo, G. Kleijn, A. Veropalumbo, Y. Wang, J. Weller, G. Zamorani, E. Zucca, A. Biviano, C. Burigana, M. Calabrese, D. Ferdinando, J. Vigo, G. Fabbian, F. Finelli, J. Graciá-Carpio, S. Matthew, N. Mauri, A. Pezzotta, M. Pontinen, V. Scottez, M. Tenti, M. Viel, M. Wiesmann, Y. Akrami, V. Allevato, S. Anselmi, M. Archidiacono, F. Atrio-Barandela, A. Balaguera-Antolínez, M. Ballardini, A. Blanchard, L. Blot, H. Böhringer, S. Borgani, S. Bruton, R. Cabanac, A. Calabró, B. Quevedo, G. Cañas-Herrera, A. Cappi, F. Caro, C. Carvalho, T. Castro, K. Chambers, S. Contarini, A. Cooray, G. Desprez, A. Díaz-Sánchez, J. Diaz, S. Domizio, H. Dole, S. Escoffier, A. Ferrari, P. G. Ferreira, I. Ferrero, A. Finoguenov, F. Fornari, L. Gabarra, K. Ganga, J. García-Bellido, T. Gasparetto, V. Gautard, E. Gaztañaga, F. Giacomini, F. Gianotti, G. Gozaliasl, C. M. Gutiérrez, A. Hall, H. Hildebrandt, J. Hjorth, A. Muñoz, S. Joudaki, J. Kajava, Vanshika Kansal, D. Karagiannis, C. Kirkpatrick, S. Kruk, J. L. Graet, L. Legrand, J. Lesgourgues, T. Liaudat, A. Loureiro, G. Maggio, M. Magliocchetti, F. Mannucci, R. Maoli, C. Martins, L. Maurin, R. B. Metcalf, M. Migliaccio, M. Miluzio, P. Monaco, A. Montoro, A. Mora, C. Moretti, G. Morgante, S. Nadathur, L. Patrizii, V. Popa, P. Reimberg, I. Risso, P. Rocci, M. Sahl'en, E. Sarpa, A. Schneider, M. Sereno, A. Silvestri, A. Mancini, K. Tanidis, C. Tao, N. Tessore, G. Testera, R. Teyssier, S. Toft, S. Tosi, A. Troja, M. Tucci, C. Valieri, J. Valiviita, D. Vergani, G. Verza, P. Vielzeuf, N. Astrophysics, U. Zurich, Winterthurerstrasse 190, 8093 Zurich, Switzerland, Institute of Cosmology, Gravitation, University of Portsmouth, PO1 3FX, Uk, D. Astronomia, U. Bologna, V. G. 932, 40129 Bologna, Italy, I. Bologna, V. G. 933, I. Bologna, 62 vialeBertiPichat, 40129 Bologna, M. V. I. O. Physics, 1. AmMuhlenberg, D-14476 Potsdam-Golm, Germany., Institute of Space Sciences, Campus Uab, Carrer de Can Magrans, Sn., 08193 Barcelona, Spain, Institut de Ciències de l'Espai, sn Cerdanyola del Vall'es, Laboratoire Univers et Th'eorie, Observatoire de Paris, Universit'e Psl, Universit'e de Paris Cit'e, Cnrs, 92190 Meudon, France, I. Astrophysics, U. Oslo, P. O. B. 1. Blindern, 0315 Oslo, Norway, Jet Propulsion Laboratory, California institute of Technology, 4800 Oak Grove Drive, Pasadena, Ca, 91109, Usa, Max-Planck-Institut fuer Astrophysik, Karl-Schwarzschild-Str.1, 85748 Garching, D. Physics, Institute for Computational Cosmology, D. University, S. Road, DH1 3LE, J. B. C. F. Astrophysics, Astronomy, U. Manchester, Oxford Road, M13 9PL, Inafiasf Milano, 12 ViaAlfonsoCorti, 20133 Milano, Istituto Nazionale Fisica Nucleare, Sezione Infn di Bologna, 46 ViaIrnerio, 40129 Bologna, Institute for Astronomy, U. Edinburgh, R. Observatory, B. Hill, Edinburgh EH9 3HJ, H. C. F. T. Physics, S. O. Physics, T. D. O. Edinburgh, Edinburgh EH9 3FD, I. Physik, U. Heidelberg, 16 Philosophenweg, 69117 Heidelberg, Institut de Recherche en Astrophysique et Plan'etologie, U. Toulouse, Ups, Cnes, 18 avenue Edouard Belin, 31400 Toulouse, Universit'e St Joseph, Faculty of Nuclear Sciences, Beirut, Lebanon, Institut de Physique Th'eorique, Cea, Universit'e Paris-Saclay 91191 Gif-sur-Yvette Cedex, S. O. Mathematics, Physics, U. Surrey, Guildford, Surrey, GU2 7XH, Inaf Brera, 28 ViaBrera, 20133 Milano, Ifpu, Institute for Fundamental Physics of the Universe, 2. viaBeirut, 34127 Trieste, Inaf Trieste, 11 ViaG.B.Tiepolo, 34127 Trieste, Infn, Sezione di Trieste, 2. ViaValerio, TS 34127Trieste, Sissa, International School for Advanced Studies, Via Bonomea 265, TS 34136Trieste, I. A. D. Torino, 20 viaOsservatorio, 1. P. Torinese, D. Fisica, U. Genova, 33 viaDodecaneso, 16146, Genova, I. Genova, D. O. P. Pancini, University Federico, 6. ViaCinthia, 80126, Napoli, I. A. D. Capodimonte, 16 ViaMoiariello, 80131 Napoli, I. Naples, I. D. A. E. C. D. Espacco, U. Porto, Caup, Rua das Estrelas, PT4150-762 Porto, Portugal, Faculdade de Ciências da Universidade do Porto, Rua do Campo Alegre, 4169-007 Porto, A. Universit'e, Lam, Marseille, U. Torino, 1. viaP.Giuria, 10125 Torino, I. Torino, I. Roma, 33 viaFrascati, 00078 Monteporzio Catone, I. Roma, P. A. Moro, 2. -. C. D. D. Fisica, Edificio G. Marconi, 00133 Roma, Centro de Investigaciones Energ'eticas, Medioambientales Y. Tecnol'ogicas, 40 AvenidaComplutense, 28014 Madrid, Port d'Informaci'o Cient'ifica, C. Sn, 08193 Bellaterra, Institute for Particle Physics, Cosmology, Rwth Aachen University, 52056 Aachen, I. D. E. D. Catalunya, Edifici Rdit, C. Upc, 08860 Castelldefels, Barcelona, D. Bologna, Instituto de Astrofı́sica de Canarias, C. V. L. sn, 38204, San Crist'obal de La Laguna, Tenerife, European Space AgencyESRIN, 1. LargoGalileoGalilei, 00044 Frascati, Roma, Esacesa, Camino Bajo de Castillo, Sn., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, 1. Universit'eClaudeBernardLyon, CNRSIN2p3, Ipn Lyon, Umr 5822, Villeurbanne, F-69100, I. O. Physics, Laboratory of Astrophysics, E. P. F. Lausanne, Observatoire de Sauverny, 1290 Versoix, Institut de Ciències del Cosmos, U. Barcelona, 1. Mart'iiFranques, 08193 Barcelona, I. C. D. R. I. E. Avanccats, 23 PasseigdeLluı́sCompanys, 08193 Barcelona, 1. UCBLyon, Iuf, 4. R. E. Fermi, 69622 Villeurbanne, Departament de F'isica, F. Ciencias, Universidade T'ecnica de Lisboa, C. Edif'icio, C. Grande, P. Lisboa, 1049-001 Lisboa, D. O. Astronomy, U. Geneva, 16 ch.d'Ecogia, Universit'e Paris-Saclay, Institut d'Astrophysique Spatiale, 91405, Orsay +499 moresemanticscholar +1 more sourceSymmergent Gravity, Seesawic New Physics, and Their Experimental Signatures
Advances in High Energy Physics, Volume 2019, Issue 1, 2019., 2019 The standard model of elementary particles (SM) suffers from various problems, such as power‐law ultraviolet (UV) sensitivity, exclusion of general relativity (GR), and absence of a dark matter candidate. The LHC experiments, according to which the TeV domain appears to be empty of new particles, started sidelining TeV‐scale SUSY and other known cures ...Durmuş Demir, Michele Arzanowiley +1 more source