... Earlier still lies the remaining frontier, where the first stars, galaxies and massive black holes formed. ... Building on this general framework, and relying on the development of efficient new computational tools, the fragmentation properties of primordial gas inside such minihaloes were investigated with numerical simulations, leading to the result that the first stars, so-called population III, were predominantly very massive4,8 (see Box 1 for the terminology used here). ... Astrophys. ... III. ...

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• http://ocean.phys.msu.ru/courses/stathyd/2005%20Smyth%20et%20al.%2C%20Differential%20diffusion%20in%20breaking%20Kelvin-Helmholtz%20billows.pdf
• http://ocean.phys.msu.ru/courses/geo/lectures-addons/12/2004%20Kanamori%2C%20%20Brodsky%20The%20Physics%20of%20Earthquakes.pdf
• http://ocean.phys.msu.ru/courses/geo/lectures-addons/02/2006%20Wood%20et%20al.%2C%20Accretion%20of%20the%20Earth%20and%20segregation%20of%20its%20core.pdf

... Biological Faculty . Moscow State Lomonosov University . ... EDUCATION : B.S. Lomonosov Moscow State University, 1971 Physics . M.S. Lomonosov Moscow State University, 1972 Biophysics . Ph.D. Lomonosov Moscow State University, 1978 Biophysics . ... Lomonosov Moscow State University, 1990 Biophysics . ... 1972-1978 Research assistant Lomonosov State University, Moscow . ... Mathematical modelling in biology, . ... Lecturer at Biological Faculty, Lomonosov State University, Moscow . ...

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Head of sector, acting head of the Computational Geophysics Division of the M.V. Keldysh Institute for Applied Mathematics, RAS. ... Finished the Electrodynamics and Quantum Theory Department of Faculty of Physics, MSU in 1962. ... Ill-posed problems, stochastic processes, theory of approximation. Mechanics and physics of multi-phase media, phenomena in porous media, difference schemes for some classes of mathematical physics problems (filtration, elasticity theory). ...

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... Physics 1792-1843 F rr = 2m[v в ] ­ () , () : : = : = = ( p, T, ...) = ( p, T, e) = ( p, T, s) p= mR Vµ T= R µ T R a T 8.31 R Ra = µ 0.029 287 p = R a T = p R aT .. p = 101325 T = 273.16 K 1.29 / 3 p a = a R a T = a + w = p a e = w R w T e = p-e RaT + e R wT e p R aT + R wT e R p p 1 - a 1- = RT RaT p R w a e ~ 10 3 1 - 0.38 e p 1 q q q ­ , q eS = A exp ( t ) A = 611 Pa = ... T2 - T1 ~ 10 -1 o o T2 - T1 ~ 100 C 2 a= (/2): , George Hadley, 1735 ( 100 /) «» 2- , r = C rr V V, 0.0025 1995 . ...

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INTERNATIONAL CONFERENCE HYDRODYNAMIC INSTABILITY AND TURBULENCE February 26 - March 05, Moscow, Russia ORGANIZED by Moscow State University, Institute of Mechanics of MSU and Faculty of Mechanics and Mathematics. ... SPONSORED by Russian Foundation for Basic Research, Moscow State University, Institute of Mechanics of MSU. ... Prospective participants must send abstracts in Word to the Organizing Committee (gertsens@imec.msu.ru) not later than 15 January 2006. ... Phone, E-mail and Fax number. ...

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• Moscow 2006
• Nonlinear Problems of Gydrodynamic Stability Theory
• Untitled

... Is it correct ? ... V-gauge ansatz LS-equation V-SFA (first Born, Bauer) V-gauge ansatz The corresponding L-gauge ansatz gives the same V-SFA. Formula (10) generates the gauge-invariant family. L-gauge ansatz LS-equation L-SFA (first Born, Keldysh) L-gauge ansatz The ansatz (11) generates now another gaugeinvariant family. ... Conclusions Correct gauge transformation of the chosen ansatz gives the gauge invariant Born series, which can be called as the gauge invariant family. ...

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• Laboratory of Mathematical Models of Quantum Scattering Processes / MSU