Results 91 to 100 of about 3,390,969 (202)
An analytical model of radial dust trapping in protoplanetary disks
, 2019 We study dust concentration in axisymmetric gas rings in protoplanetary
disks. Given the gas surface density, we derived an analytical total dust
surface density by taking into account the differential concentration of all
the grain sizes.Carrasco-González, Carlos, Flock, Mario, Lizano, Susana, Macías, Enrique, Osorio, Mayra, Sierra, Anibal +5 morecore +1 more sourceThe Hubbard model within the equations of motion approach
, 2004 The Hubbard model has a special role in Condensed Matter Theory as it is
considered as the simplest Hamiltonian model one can write in order to describe
anomalous physical properties of some class of real materials.Abrikosov A, Abrikosov AA, Aksenov V, Alexandrov A, Allega AM, Alvarez J, Alvarez J, Anderson P, Anderson P, Andrei EY, Anlage S, Annett J, Ashcroft N, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Avella A, Bak M, Bak M, Bala J, Barnes SE, Barrett S, Becca F, Becker KW, Beenen J, Belkhir L, Bickers N, Bickers N, Bickers N, Birgenau R, Boer JD, Boer JD, Bogoliubov N, Bogoliubov N, Bogolubov N, Bonca J, Bonner J, Bosse J, Brenig W, Brewer DF, Brinkman WF, Brodale GE, Bruus H, Bulla R, Bulut N, Bulut N, Bulut N, Buzatu FD, Bénard P, Bénard P, Calandra M, Callen H, Canali C, Cannon J, Carmelo J, Carter SA, Carter SA, Carter SA, Chao KA, Chatterji T, Chattopadhyay B, Chen CH, Chen H, Chen YC, Cheong SW, Chitra R, Chow DS, Coldea R, Coleman P, Cooper S, Dagotto E, Dagotto E, Dagotto E, Dagotto E, Dai P, Dai P, Damascelli A, Dancoff SM, Deguchi T, Dessau D, Dessau DS, Dho J, Di Matteo T, DI Matteo T, DI Matteo T, Dongen PV, Dongen PV, Dorneich A, Dover RV, Duffy D, Duffy D, Duffy D, Duffy D, Emery V, Eskes H, Fano G, Fazekas P, Fazekas P, Fazekas P, Fedro AJ, Feiner LF, Feng S, Fernandez J, Ferrer J, Fetter A, Fiorentino V, Fischer J, Fleck M, Fong H, Friedel J, Fujimori A, Fulde P, Fulde P, Furukawa N, Furukawa N, Furukawa N, Gebhard F, Gebhard F, Geipel G, Georges A, Georges A, Georges A, Germann A, Gofron K, Gonzalez J, Gooding R, Gradshteyn IS, Grewe N, Greywall DS, Grilli M, Gutzwiller M, Halboth C, Hardy W, Harlingen DV, Hashimoto K, Heeger AJ, Hellberg C, Herrmann T, Herrmann T, Hewson AC, Hirsch J, Hirsch JE, Hirsch JE, Hirsch JE, Hirsch JE, Hirsch JE, Hoang A, Horbach M, Horbach M, Howell RH, Huang Z, Hubbard J, Hubbard J, Hubbard J, Huber DL, Imada M, Imada M, Imada M, Imada M, Ino A, Ino A, Ino A, Ino A, Ioffe L, Irkhin V, Ishihara S, Izyumov Y, Izyumov Y, Izyumov Y, Jaklič J, Janner A, Japaridze G, Jarrell M, Jarrell M, Jeckelmann E, Jelitto R, Johnston D, Jüttner G, K. J., Kalashnikov OK, Kalashnikov OK, Kampf A, Kampf A, Kampf AP, Kanamori J, Kawakami N, Kellen SB, Kim C, King DM, Kohn W, Kotliar G, Kotliar G, Kotliar G, Krüger P, Kubo K, Kubo R, Kumagai K, Kuramoto Y, Kwork P, Langer W, Lee PA, Lenck S, Leplae L, Liang W, Lieb E, Lieb E, Lieb EH, Lieb EH, Lilly L, Lin H, Littlewood P, Littlewood P, Lonke A, Loram J, Loram J, Loram J, Loram JW, Loram JW, Luttinger JM, MacDonald A, MacDonald A, Maier T, Maier T, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Mancini F, Manske D, Mao J, Markiewicz R, Markiewicz R, Markiewicz RS, Martindale J, Martindale J, Mason T, Mason TE, Matsuda M, Matsumoto H, Matsumoto H, Matsumoto H, Matsumoto H, Matsumoto H, Matsumoto H, Matsumoto H, Mattis D, Mattis D, McKenzie RH, McWhan DB, McWhan DB, Mehlig B, Merino J, Metzner W, Metzner W, Metzner W, Micnas R, Millis A, Millis AJ, Mills R, Monien H, Monthoux P, Monthoux P, Monthoux P, Monthoux P, Monthoux P, Monthoux P, Monthoux P, Moreo A, Moreo A, Moreo A, Moreo A, Moreo A, Mori H, Mori H, Morita T, Moriya T, Mott N, Mott NF, Münzner R, Nagaoka Y, Nakamura M, Newns D, Newns D, Newns DM, Nolting W, Nolting W, Nozières P, Nozières P, Nélisse H, Ochiai A, Ogata M, Ohama T, Okajima Y, Okamoto T, Oleś A, Onoda S, Onoda S, Onoda S, Ovchinnikov A, Pao C-H, Pao C-H, Park SK, Peres N, Peters C, Phillips NE, Pietig R, Pines D, Plakida N, Plakida N, Plakida N, Plakida N, Plakida N, Plakida N, Plakida NM, Plekhanov E, Potthoff M, Pruschke T, Pruschke T, Pruschke T, Putikka WO, Qin S, Raimondi R, Randeria M, Randeria M, Randeria M, Randeria M, Robaszkiewicz S, Roger M, Roth LM, Rowe DJ, Rozenberg MJ, Rozenberg MJ, Rozenberg MJ, Rønnow H, Salamon M, Sato M, Scalapino D, Scalapino DJ, Schlager HG, Schneider T, Schulte J, Sengupta P, Seo H, Shafer M, Shastry B, Shen S-Q, Shen Z, Shen Z, Shen Z-X, Shiba H, Shiba H, Shimahara H, Shirane G, Shirane G, Si Q, Sigrist M, Simón M, Singh R, Sonier J, Sorella S, Sorella S, Spałek J, Spałek J, Spałek J, Spałek J, Stanescu T, Stanescu T, Stanescu T, Steglich F, Stephan W, Stephan W, Stevens K, Strack R, Suzuki M, Syljuåsen O, Sánchez-Lopez M, Sánchez-Lopez M, Sánchez-Lopez M, Takahashi M, Takahashi M, Takahashi M, Takahashi Y, Takigawa M, Tamasaku K, Tanamoto T, Tasaki H, Tasaki H, Tasaki H, Tasaki H, Tasaki H, Thomas GA, Thurston T, Thurston T, Tian G, Tohyama T, Tokura Y, Tomioka Y, Torrance J, Torrance J, Tranquada J, Trapper U, Trapper U, Tserkovnikov YA, Tserkovnikov YA, Tsuchiizu M, Tsuei C, Tutuc E, Tyablikov S, Uchida S, Ueda K, Ueda Y, Usuki T, Vaks V, van den Brink J, van den Brink J, Varma C, Varma C, Varma C, Vilk YM, Villani D, Visser AD, Vojta M, Vollhardt D, Vollhardt D, Vollhardt D, Von Der Linden W, Wada N, Ward J, Wells B, Wermbter S, Westerholt K, White SR, Wigner E, Xu JH, Xu JH, Yamada K, Yamada K, Yamaji K, Yang CN, Yokohama H, Yoon J, Yu R, Yushankhai V, Yushankhai V, Zaitsev R, Zhang F, Zhang W, Zhang W, Zhang XY, Zhang XY, Zhou Y, Zubarev D, Zubarev DN +492 morecore +1 more sourceAnalytic pulsar models
, 1974 An analytic and fully general relativistic solution to Einstein's field equations is given. This analytic model of a slowly rotating neutron star can describe differentially as well as uniformly rotating stars. (auth)Adams, R.C., Cohen, J.M., Adler, R.J., Sheffield, C. +3 moreopenaire +3 more sourcesReview of current knee biomechanical modeling techniques [PDF]
, 2011 In this paper we are going to present an essential modification of an existing analytical model. The model creation normally starts with a simplified, less complex analytical model, where the phenomena can be easily interpreted, checked and controlled ...Abdel Wahab, Magd, Csizmadia, Béla, De Baets, Patrick, Fekete, Gusztáv +3 morecore +1 more sourceAn analytical model of lateral condylar plate working length. [PDF]
Clin Biomech (Bristol), 2023 Roytman GR, Beitler B, LaMonica J, Spero M, Toy K, Ramji AF, Yoo B, Leslie MP, Baumgaertner M, Tommasini SM, Wiznia DH. +10 moreeuropepmc +1 more source
