Results 1 to 10 of about 201,530,701 (335)
Progress in the numerical studies of the type IIB matrix model [PDF]
The European Physical Journal Special Topics, 2022 The type IIB matrix model, also known as the IKKT model, has been proposed as a promising candidate for a non-perturbative formulation of superstring theory.K. Anagnostopoulos, T. Azuma, Kohta Hatakeyama, M. Hirasawa, Yuta Ito, J. Nishimura, S. Papadoudis, Asato Tsuchiya Physics Department, School of Applied Mathematical, P. Sciences, National Observatory of Athens, Institute for Research in Fundamental Sciences, S. University, T. Center, Institute of Particle, Nuclear Studies, High Energy Accelerator Research Organization, Sezione di Milano-Bicocca, Istituto Nazionale Fisica Nucleare, National Institute of Technology, T. College, Department of Particle, N. Physics, School of Materials Science, G. Studies, D. Physics, Shizuoka University +26 moresemanticscholar +1 more sourceOn the relationship between the multi-region relaxed variational principle and resistive inner layer theory [PDF]
, 2022 We show that the variational energy principle of multi-region relaxed magnetohydrodynamic (MRxMHD) model can be used to predict finite-pressure linear tearing instabilities.A.Kumar, J.Loizu, M. J. Hole, Z. Qu, S. R. Hudson, R. Institute, The Australian National University, Canberra, Act, Australia., S. Center, 'Ecole Polytechnique F'ed'erale de Lausanne, C. Lausanne, Switzerland, Australian Nuclear Science, Technology Organisation, Locked Bag, Kirrawee DC Nsw, Princeton Plasma Physics Laboratory, PO-415, New Jersey, United States of America +21 moresemanticscholar +1 more sourceEuclid preparation. XLI. Galaxy power spectrum modelling in real space [PDF]
Astronomy & Astrophysics, 2023 We investigate the accuracy of the perturbative galaxy bias expansion in view of the forthcoming analysis of the spectroscopic galaxy samples. We compare the performance of a Eulerian galaxy bias expansion using state-of-the-art prescriptions from the ...Euclid Collaboration A. Pezzotta, C. Moretti, M. Zennaro, A. M. Dizgah, M. Crocce, E. Sefusatti, I. Ferrero, K. Pardede, A. Eggemeier, A. Barreira, R. E. Angulo, M. Marinucci, B. Quevedo, S. D. L. Torre, D. Alkhanishvili, M. Biagetti, M.-A. Breton, E. Castorina, G. D'Amico, V. Desjacques, M. Guidi, M. Karcher, Andrea Oddo, M. P. Ib'anez, C. Porciani, A. Pugno, J. Salvalaggio, E. Sarpa, A. Veropalumbo, Z. Vlah, A. Amara, S. Andreon, N. Auricchio, M. Baldi, S. Bardelli, R. Bender, C. Bodendorf, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, V. Capobianco, C. Carbone, V. Cardone, J. Carretero, S. Casas, F. Castander, M. Castellano, S. Cavuoti, A. Cimatti, G. Congedo, C. Conselice, L. Conversi, Y. Copin, L. Corcione, F. Courbin, H. Courtois, A. Silva, H. Degaudenzi, A. Giorgio, J. Dinis, X. Dupac, S. Dusini, A. Ealet, M. Farina, S. Farrens, P. Fosalba, M. Frailis, E. Franceschi, S. Galeotta, B. Gillis, C. Giocoli, B. Granett, A. Grazian, F. Grupp, L. Guzzo, S. Haugan, F. Hormuth, A. Hornstrup, K. Jahnke, B. Joachimi, E. Keihanen, S. Kermiche, A. Kiessling, M. Kilbinger, T. Kitching, B. Kubik, M. Kunz, H. Kurki-Suonio, S. Ligori, P. Lilje, V. Lindholm, I. Lloro, E. Maiorano, O. Mansutti, O. Marggraf, K. Markovič, N. Martinet, F. Marulli, R. Massey, E. Medinaceli, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, Michele Moresco, L. Moscardini, E. Munari, S. Niemi, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, W. Percival, V. Pettorino, S. Pires, G. Polenta, J. Pollack, M. Poncet, L. Popa, L. Pozzetti, F. Raison, A. Renzi, J. Rhodes, G. Riccio, E. Romelli, M. Roncarelli, E. Rossetti, R. Saglia, D. Sapone, B. Sartoris, P. Schneider, T. Schrabback, A. Secroun, G. Seidel, M. Seiffert, S. Serrano, C. Sirignano, G. Sirri, L. Stanco, C. Surace, P. Tallada-Crespí, A. Taylor, I. Tereno, R. Toledo-Moreo, F. Torradeflot, I. Tutusaus, E. Valentijn, L. Valenziano, T. Vassallo, Y. Wang, J. Weller, G. Zamorani, J. Zoubian, E. Zucca, A. Biviano, E. Bozzo, C. Burigana, C. Colodro-Conde, D. Ferdinando, G. Mainetti, M. Martinelli, N. Mauri, Z. Sakr, V. Scottez, M. Tenti, M. Viel, M. Wiesmann, Y. Akrami, V. Allevato, S. Anselmi, C. Baccigalupi, M. Ballardini, F. Bernardeau, A. Blanchard, S. Borgani, S. Bruton, R. Cabanac, A. Cappi, C. Carvalho, G. Castignani, T. Castro, G. C. nas-Herrera, K. Chambers, S. Contarini, A. Cooray, J. Coupon, S. Davini, G. Lucia, G. Desprez, S. Domizio, H. Dole, A. Díaz-Sánchez, J. Vigo, S. Escoffier, P. G. Ferreira, F. Finelli, L. Gabarra, K. Ganga, J. García-Bellido, F. Giacomini, G. Gozaliasl, A. Hall, S. Ili'c, S. Joudaki, J. Kajava, Vanshika Kansal, C. Kirkpatrick, L. Legrand, A. Loureiro, J. Macías-Pérez, M. Magliocchetti, F. Mannucci, R. Maoli, C. Martins, S. Matthew, L. Maurin, R. Metcalf, M. Migliaccio, P. Monaco, G. Morgante, S. Nadathur, N. A. Walton, L. Patrizii, V. Popa, D. Potter, A. Pourtsidou, M. Pontinen, I. Risso, P. Rocci, A. Sánchez, M. Sahl'en, A. Schneider, M. Sereno, P. Simon, A. Mancini, J. Steinwagner, G. Testera, R. Teyssier, S. Toft, S. Tosi, A. Troja, M. Tucci, J. Valiviita, D. Vergani, G. Verza, P. Physics, 1. Giessenbachstr., 85748 Garching, Germany., Sissa, International School for Advanced Studies, Via Bonomea 265, TS 34136Trieste, Italy, I. -. C. N. D. R. I. H. P. Computing, Big Data e Quantum Computing, 2. ViaMagnanelli, Bologna, Institute for Astronomy, U. Edinburgh, R. Observatory, B. Hill, Edinburgh EH9 3HJ, Uk, Inaf Trieste, 11 ViaG.B.Tiepolo, 34127 Trieste, Ifpu, Institute for Fundamental Physics of the Universe, 2. viaBeirut, 34127 Trieste, D. O. Physics, Oxford University, Keble Road, O. 3RH, Universit'e de Geneve, D'epartement de Physique Th'eorique, Centre for Astroparticle Physics, 24 quai Ernest-Ansermet, 4. CH-1211Genève, Switzerland, 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, Infn, Sezione di Trieste, 2. ViaValerio, TS 34127Trieste, I. Astrophysics, U. Oslo, P. O. B. 1. Blindern, 0315 Oslo, Norway, International Centre for Theoretical Physics, 11 StradaCostiera, Universitat Bonn, Argelander Institut fur Astronomie, 71 AufdemHugel, 53121 Bonn, Excellence Cluster Origins, 2. Boltzmannstrassee, Ludwig-Maximilians-University, 4. Schellingstrasse, 81679 Munich, Donostia International Physics Center, P. M. Lardizábal, 20018, Donostia-San Sebasti'an, Guipuzkoa, Ikerbasque, Basque Foundation for Science, 48013, Bilbao, Dipartimento di Scienze Matematiche, Fisiche e Informatiche, U. Parma, Viale delle Scienze 7A 43124 Parma, T. I. O. Technology, Israel, I. D. E. D. Catalunya, Carrer Gran Capit'a 2-4, 08193 Barcelona, A. Universit'e, Cnrs, Cnes, Lam, Marseille, France, Area Science Park, 99 LocalitaPadriciano, 34149, Trieste, Laboratoire Univers et Th'eorie, Observatoire de Paris, Universit'e Psl, Universit'e de Paris Cit'e, 92190 Meudon, Dipartimento di FisicaAldo Pontremoli, Universita di Milano, 16 viaCeloria, 20133 Milano, I. Milano, I. Parma, D. O. Mathematics, Physics, Roma Tre University, 84 viadellaVascaNavale, 00133 Rome, I. R. Tre, 00146, Roma, Universit'e de Toulon, Cpt, D. Astronomia, U. Trieste, 11 ViaTiepolo, 34127 Trieste, Inaf Brera, 28 ViaBrera, 20133 Milano, I. Genova, 33 viaDodecaneso, 16146, Genova, D. Physics, Rudjer Bovskovi'c Institute, Zagreb HR-10000, Croatia., K. Cambridge, Madingley Road, Cambridge, CB3 0HA, Damtp, Centre for Mathematical Sciences, Wilberforce Road, Cambridge CB3 0WA, S. O. Mathematics, U. Surrey, Guildford, Surrey, GU2 7XH, I. Bologna, V. G. 933, 40129 Bologna, D. Astronomia, U. Bologna, V. G. 932, I. Bologna, 62 vialeBertiPichat, 40129 Bologna, Universitatssternwarte Munchen, F. Physik, Ludwig-Maximilians-Universitat Munchen, 1. Scheinerstrasse, 8. Munchen, I. A. D. Torino, 20 viaOsservatorio, 1. P. Torinese, D. Fisica, U. Genova, Department of PhysicsE. 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, U. Torino, 1. viaP.Giuria, 10125 Torino, I. Torino, Inafiasf Milano, 12 ViaAlfonsoCorti, I. Roma, 33 viaFrascati, 00078 Monteporzio Catone, I. Roma, P. A. Moro, 2. -. C. D. D. Fisica, Edificio G. Marconi, 00133 Roma, Institut de F'isica d'Altes Energies, The Barcelona Institute of Science, Technology, 08193 Bellaterra, Port d'Informaci'o Cient'ifica, C. Sn, Institute for Particle Physics, Cosmology, Rwth Aachen University, 52056 Aachen, D. Bologna, J. B. C. F. Astrophysics, Astronomy, U. Manchester, Oxford Road, M13 9PL, European Space AgencyESRIN, 1. LargoGalileoGalilei, 00044 Frascati, Esacesa, Camino Bajo de Castillo, Sn., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, U. Lyon, 1. UnivClaudeBernardLyon, CNRSIN2p3, Ipn Lyon, Umr 5822, 69622 Villeurbanne, I. O. Physics, Laboratory of Astrophysics, E. P. F. Lausanne, Observatoire de Sauverny, 1290 Versoix, 1. UCBLyon, Iuf, 4. R. E. Fermi, 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, I. D. A. E. P. Spaziali, V. F. D. Cavaliere, 100, 00133 Roma, INFN-Padova, 8. ViaMarzolo, 35131 Padova, Universit'e Paris-Saclay, Cea, Aim, 91191, Gif-sur-yvette, Istituto Nazionale Fisica Nucleare, Sezione Infn di Bologna, 46 ViaIrnerio +499 moresemanticscholar +1 more sourceProbing the Extent of Vertical Mixing in Brown Dwarf Atmospheres with Disequilibrium Chemistry [PDF]
Astrophysical Journal, 2022 Evidence of disequilibrium chemistry due to vertical mixing in the atmospheres of many T- and Y-dwarfs has been inferred due to enhanced mixing ratios of CO and reduced NH3.S. Mukherjee, J. Fortney, N. Batalha, T. Karalidi, M. Marley, C. Visscher, B. Miles, A. B. D. O. Astronomy, Astrophysics, U. California, Santa Cruz, Ca, Usa, N. R. Center, MS 245-3, M. Field, D. Physics, U. Florida, Orlando, .fl., Lunar, Planetary Laboratory, The University of Arizona, Tucson, Az, D. University, IA SiouxCenter, Space Telescope Science Institute, Boulder, Co. +29 moresemanticscholar +1 more sourceDARWIN – a next-generation liquid xenon observatory for dark matter and neutrino physics [PDF]
International Conference on Rebooting Computing, 2021
The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for weakly ...J. Aalbers, K. Abe, V. Aerne, F. Agostini, S. A. Maouloud, D. Akerib, D. Akimov, J. Akshat, A. Musalhi, F. Alder, S. Alsum, L. Althueser, C. Amarasinghe, F. Amaro, A. Ames, T. Anderson, B. Andrieu, N. Angelides, E. Angelino, J. Angevaare, V. C. Antochi, D. Martin, B. Antunović, E. Aprile, H. Araújo, J. E. Armstrong, F. Arneodo, M. Arthurs, P. Asadi, S. Baek, X. Bai, D. Bajpai, A. Baker, J. Balajthy, S. Balashov, M. Balzer, A. Bandyopadhyay, J. Bang, E. Barberio, J. Bargemann, L. Baudis, D. Bauer, D. Baur, A. Baxter, A. Baxter, M. Bazyk, K. Beattie, J. Behrens, N. Bell, L. Bellagamba, P. Beltrame, M. Benabderrahmane, E. Bernard, G. Bertone, P. Bhattacharjee, A. Bhatti, A. Biekert, T. P. Biesiadzinski, A. Binau, R. Biondi, Y. Biondi, H. Birch, F. Bishara, A. Bismark, C. Blanco, G. Blockinger, E. Bodnia, C. Boehm, A. Bolozdynya, P. Bolton, S. Bottaro, C. Bourgeois, B. Boxer, P. Br'as, A. Breskin, P. Breur, C. Brew, J. Brod, E. Brookes, A. Brown, E. Brown, S. Bruenner, G. Bruno, R. Budnik, T. Bui, S. Burdin, S. Buse, J. Busenitz, D. Buttazzo, M. Buuck, A. Buzulutskov, R. Cabrita, C. Cai, D. Cai, C. Capelli, J. Cardoso, M. Carmona-Benitez, M. Cascella, R. Catena, S. Chakraborty, C. Chan, S. Chang, A. Chauvin, A. Chawla, H. Chen, V. Chepel, N. Chott, D. Cichon, A. Chavez, B. Cimmino, M. Clark, R. Co, A. Colijn, J. Conrad, M. Converse, M. Costa, A. Cottle, G. Cox, O. Creaner, J. Garcia, J. Cussonneau, J. Cutter, C. Dahl, V. D'Andrea, A. David, M. Decowski, J. Dent, F. Deppisch, L. D. Viveiros, P. Gangi, A. Giovanni, S. D. Pede, J. Dierle, S. Diglio, J. Dobson, M. Doerenkamp, D. Douillet, G. Drexlin, E. Druszkiewicz, D. Dunsky, K. Eitel, A. Elykov, T. Emken, R. Engel, S. R. Eriksen, M. Fairbairn, A. Fan, J. J. Fan, S. Farrell, S. Fayer, N. Fearon, A. Ferella, C. Ferrari, A. Fieguth, S. Fiorucci, H. Fischer, H. Flaecher, M. Flierman, T. Florek, R. Foot, P. J. Fox, R. Franceschini, E. Fraser, C. Frenk, S. Fröhlich, T. Fruth, W. Fulgione, C. Fuselli, P. Gaemers, R. Gaior, R. Gaitskell, M. Galloway, F. Gao, I. G. Garcia, J. Genovesi, C. Ghag, S. Ghosh, E. Gibson, W. Gil, D. Giovagnoli, F. Girard, R. Glade-Beucke, F. Gluck, S. Gokhale, A. Gouvea, L. Gráf, L. Grandi, J. Grigat, B. Grinstein, M. D. Grinten, R. Grossle, H. Guan, M. Guida, R. Gumbsheimer, C. Gwilliam, C. Hall, L. Hall, R. Hammann, K. Han, V. Hannen, S. Hansmann-Menzemer, R. Harata, S. Hardin, E. Hardy, C. Hardy, K. Harigaya, R. Harnik, S. Haselschwardt, M. Hernandez, S. Hertel, A. Higuera, C. Hils, S. Hochrein, L. Hoetzsch, M. Hoferichter, N. Hood, D. Hooper, M. Horn, J. Howlett, D. Huang, Y. Huang, D. Hunt, M. Iacovacci, G. Iaquaniello, R. Ide, C. Ignarra, G. Iloglu, Y. Itow, E. Jacquet, O. Jahangir, J. Jakob, R. James, A. Jansen, Wei Ji, X. Ji, F. Joerg, J. Johnson, A. Joy, A. Kaboth, A. Kamaha, K. Kanezaki, K. Kar, M. Kara, N. Kato, P. Kavrigin, S. Kazama, A. Keaveney, J. Kellerer, D. Khaitan, A. Khazov, G. Khundzakishvili, I. Khurana, B. Kilminster, M. Kleifges, P. Ko, M. Kobayashi, D. Kodroff, G. Koltmann, A. Kopec, A. Kopmann, J. Kopp, L. Korley, V. Kornoukhov, E. Korol'kova, H. Kraus, L. Krauss, S. Kravitz, L. Kreczko, V. Kudryavtsev, F. Kuger, J. Kumar, B. Paredes, L. LaCascio, Q. Lainé, H. Landsman, R. Lang, E. Leason, J. Lee, D. Leonard, K. Lesko, L. Levinson, C. Levy, I. Li, S. Li, Tao Li, S. Liang, C. Liebenthal, J. Lin, Q. Lin, S. Lindemann, M. Lindner, A. Lindote, R. Linehan, W. Lippincott, X. Liu, K. Liu, J. Liu, J. Loizeau, F. Lombardi, J. Long, M. Lopes, E. Asamar, W. Lorenzon, C. Lu, S. Luitz, Y. Ma, P. Machado, C. Macolino, T. Maeda, J. Mahlstedt, P. Majewski, A. Manalaysay, A. Mancuso, L. Manenti, A. Manfredini, R. Mannino, N. Marangou, J. March-Russell, F. Marignetti, T. M. Undagoitia, K. Martens, R. Martin, I. Martinez-Soler, J. Masbou, D. Masson, E. Masson, S. Mastroianni, M. Mastronardi, J. Matías-Lopes, M. E. McCarthy, N. McFadden, E. McGinness, D. McKinsey, J. Mclaughlin, K. McMichael, P. Meinhardt, J. Menéndez, Y. Meng, M. Messina, R. Midha, D. Milisavljevic, E. Miller, B. Milosevic, S. Milutinović, S. Mitra, K. Miuchi, E. Mizrachi, K. Mizukoshi, A. Molinario, A. Monte, C. Monteiro, M. Monzani, J. S. Moore, K. Morra, J. Morad, J. D. Mendoza, S. Moriyama, E. Morrison, E. Morteau, Y. Mosbacher, B. Mount, J. Müller, A. Murphy, M. Murra, D. Naim, S. Nakamura, E. Nash, N. Navaieelavasani, A. Naylor, C. Nedlik, H. Nelson, F. Neves, J. Newstead, K. Ni, J. Nikoleyczik, V. Niro, U. Oberlack, M. Obradović, K. Odgers, C. O’Hare, P. Oikonomou, I. Olcina, K. Oliver-Mallory, A. Oranday, J. Orpwood, I. Ostrovskiy, K. Ozaki, B. Paetsch, S. Pal, J. Palacio, K. Palladino, J. Palmer, P. Panci, M. Pandurović, A. Parlati, N. Parveen, S. Patton, V. Pvevc, Q. Pellegrini, B. Penning, G. Pereira, R. Peres, Y. Perez-Gonzalez, E. Perry, T. Pershing, R. Petrossian-Byrne, J. Pienaar, A. Piepke, G. Pieramico, M. Pierre, M. Piotter, V. Pizella, G. Plante, T. Pollmann, D. Porzio, J. Qi, Y. Qie, J. Qin, N. Raj, M. R. Silva, K. Ramanathan, D. Garc'ia, J. Ravanis, L. Redard-Jacot, D. Redigolo, S. Reichard, J. Reichenbacher, C. Rhyne, A. Richards, Q. Riffard, G. Rischbieter, A. Rocchetti, S. Rosenfeld, R. Rosero, N. Rupp, T. Rushton, S. Saha, L. Sanchez, P. Sanchez-Lucas, D. Santone, J. Santos, I. Sarnoff, G. Sartorelli, A. Sazzad, M. Scheibelhut, R. Schnee, M. Schrank, J. Schreiner, P. Schulte, D. Schulte, H. S. Eißing, M. Schumann, T. Schwemberger, A. Schwenk, T. Schwetz, L. Lavina, P. Scovell, H. Sekiya, M. Selvi, E. Semenov, F. Semeria, P. Shagin, S. Shaw, S. Shi, E. Shockley, T. Shutt, R. Si-Ahmed, J. Silk, C. Silva, M. C. Silva, H. Simgen, F. vSimkovic, G. Sinev, R. Singh, W. Skulski, J. Smirnov, R. Smith, M. Solmaz, V. Solovov, P. Sorensen, J. Soria, T. Sparmann, I. Stancu, M. Steidl, A. Stevens, K. Stifter, L. Strigari, D. Subotić, B. Suerfu, A. M. Suliga, T. Sumner, P. Szabó, M. Szydagis, A. Takeda, Y. Takeuchi, P. Tan, C. Taricco, W. Taylor, D. Temples, A. Terliuk +499 moresemanticscholar +1 more sourceA Monadic Formalization of ML5 [PDF]
Electronic Proceedings in Theoretical Computer Science, 2010 ML5 is a programming language for spatially distributed computing, based on a Curry-Howard correspondence with the modal logic S5. Despite being designed by a correspondence with S5 modal logic, the ML5 programming language differs from the logic in ...Daniel R. Licata, Robert Harperdoaj +1 more source
