ÈÍÔÎÐÌÀÖÈÎÍÍÛÉ ÁÞËËÅÒÅÍÜ "ÑÒÀÒÜÈ" N 36/37 13.09.04;20.09.04
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Ñ 133 ÄÈÔÔÅÐÅÍÖÈÀËÜÍÛÅ È ÈÍÒÅÃÐÀËÜÍÛÅ ÓÐÀÂÍÅÍÈß
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Ñ 133.2à ÍÅËÈÍÅÉÍÛÅ ÓÐÀÂÍÅÍÈß ÌÀÒÅÌÀÒÈ×ÅÑÊÎÉ ÔÈÇÈÊÈ,
ÑÎËÈÒÎÍÛ.
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25. Xia T. a.o. A Lax Integrable Hierarchy, Bi-Hamiltonian
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Ñ 15 ÒÅÎÐÈß ÂÅÐÎßÒÍÎÑÒÅÉ È ÌÀÒÅÌÀÒÈ×ÅÑÊÀß ÑÒÀÒÈÑÒÈÊÀ
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Ñ 17 ÂÛ×ÈÑËÈÒÅËÜÍÀß ÌÀÒÅÌÀÒÈÊÀ.
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Ñ 17 ê ÐÀÑ×ÅÒÛ ÏÎ ÌÎËÅÊÓËßÐÍÎÉ ÄÈÍÀÌÈÊÅ.×ÈÑËÅÍÍÎÅ
ÌÎÄÅËÈÐÎÂÀÍÈÅ ÔÈÇÈ×ÅÑÊÈÕ ÇÀÄÀ×
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31. Demkowicz M.J., Argon A.S. High-Density Liquidlike Component
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32. Dundas D. Accurate and Efficient Non-Adiabatic Quantum
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33. Egorov S.A. Ion Solvation Dynamics in Supercritical Fluids.
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35. Jagannathan K., Yethiraj A. Molecular Dynamics Simulations
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36. Lee G.W. a.o. Difference in Icosahedral Short-Range Order
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Ñ 3 ÔÈÇÈÊÀ
39. Òðîïèí Â.È. Ðåêòîð Ìîñêîâñêîãî óíèâåðñèòåòà àêàäåìèê Ðåì
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Ñ 31 ÑÈÑÒÅÌÛ ÅÄÈÍÈÖ. ÔÓÍÄÀÌÅÍÒÀËÜÍÛÅ ÔÈÇÈ×ÅÑÊÈÅ
ÊÎÍÑÒÀÍÒÛ
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Ñ 321 ÊËÀÑÑÈ×ÅÑÊÀß ÌÅÕÀÍÈÊÀ
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Ñ 322 ÒÅÎÐÈß ÎÒÍÎÑÈÒÅËÜÍÎÑÒÈ
43. Ïåòðîâ À.Í. Ñîõðàíÿþùèåñÿ òîêè â D-ìåðíîé ãðàâèòàöèè è
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44. Babichev E. a.o. Black Hole Mass Decreasing due to Phantom
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45. Chun E.J. Late Leptogenesis from Radiative Soft Terms.
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46. Dettmann C.P. a.o. Stochastic Stabilization of
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47. Malykh A.A. a.o. Partner Symmetries and Non-Invariant
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48. Muller T. Visual Appearance of a Morris-Thorne-Wormhole.
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Ñ 322.3 ÑÏÅÖÈÀËÜÍÀß ÒÅÎÐÈß ÎÒÍÎÑÈÒÅËÜÍÎÑÒÈ È ÊËÀÑÑÈ×ÅÑÊÀß
ÝËÅÊÒÐÎÄÈÍÀÌÈÊÀ
50. Áîãîëþáîâ À.Í. è äð. Ëîâóøå÷íûå ìîäû â ýëåêòðîìàãíèòíîì
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Ñ 323 à ÔÓÍÄÀÌÅÍÒÀËÜÍÛÅ ÂÎÏÐÎÑÛ ÊÂÀÍÒÎÂÎÉ ÌÅÕÀÍÈÊÈ.ÑÊÐÛÒÛÅ
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Ñ 323.1 ÐÅËßÒÈÂÈÑÒÑÊÈÅ ÂÎËÍÎÂÛÅ ÓÐÀÂÍÅÍÈß. ÓÐÀÂÍÅÍÈß ÒÈÏÀ
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ÏÎËßÐÈÇÀÖÈÎÍÍÛÅ ÝÔÔÅÊÒÛ. ÈÍÂÀÐÈÀÍÒÍÎÅ ÐÀÇËÎÆÅÍÈÅ ÀÌÏËÈÒÓÄ
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Ñ 346.6å ÍÎÂÛÅ ×ÀÑÒÈÖÛ
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Ñ 349 ÄÎÇÈÌÅÒÐÈß È ÔÈÇÈÊÀ ÇÀÙÈÒÛ
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ïðè äåéñòâèè ïó÷êà ýëåêòðîíîâ è èìïóëüñíîãî ýëåêòðè÷åñêîãî ïîëÿ.
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1. Âåñòíèê Ìîñêîâñêîãî óíèâåðñèòåòà.ñåð.3: Ôèçèêà.Àñòðîíîìèÿ.,
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