ÈÍÔÎÐÌÀÖÈÎÍÍÛÉ ÁÞËËÅÒÅÍÜ "ÑÒÀÒÜÈ" N.13 29.03.04
001 Íàóêà
1. Êðóãëÿêîâ Ý.Ï. ×åì óãðîæàåò îáùåñòâó ëæåíàóêà? //Âåñòí. ÐÀÍ.
- 2004.- ò.74, N.1. - c.8-16.
2. Ðàñöâåò ëæåíàóêè - ñëåäñòâèå êðèçèñà îáùåñòâåííîãî ñîçíàíèÿ.
Îáñóæäåíèå â Ïðåçèäèóìå ÐÀÍ. //Âåñòí. ÐÀÍ. - 2004.- ò.74, N.1. -
ñ.17-27.
28.08 Ýêîëîãèÿ
3. Êàñèìîâ Í.Ñ. è äð. Êîíöåïöèÿ óñòîé÷èâîãî ðàçâèòèÿ:
âîñïðèÿòèå â Ðîññèè. //Âåñòí. ÐÀÍ. - 2004.- ò.74, N.1. - ñ.28-36.
- Áèáëèîãð.:13.
Ñ 1 ÌÀÒÅÌÀÒÈÊÀ
4. Ãëàãîëåâà Å. Ãåëüôàíä è øêîëà. //ÊÂÀÍÒ. - 2004.- N.1.
- ñ.4-7.
5. Òèõîìèðîâ Ò. Èçðàèëü Ìîèñååâè÷ Ãåëüôàíä //ÊÂÀÍÒ. - 2004.-
N.1. - ñ.2-3.
Ñ 133.2à ÍÅËÈÍÅÉÍÛÅ ÓÐÀÂÍÅÍÈß ÌÀÒÅÌÀÒÈ×ÅÑÊÎÉ ÔÈÇÈÊÈ,
ÑÎËÈÒÎÍÛ.
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Ñ 138 ÃÅÎÌÅÒÐÈß. ÐÈÌÀÍÎÂÀ ÃÅÎÌÅÒÐÈß. ÃÅÎÌÅÒÐÈß
ËÎÁÀ×ÅÂÑÊÎÃÎ
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Ñ 17 ÂÛ×ÈÑËÈÒÅËÜÍÀß ÌÀÒÅÌÀÒÈÊÀ.
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Ñ 3 ÔÈÇÈÊÀ
22. Òðàíêîâñêèé Ñ. Íîáåëåâñêèå ïðåìèè 2003 ãîäà:
Ñâåðõïðîâîäèìîñòü è ñâåðõòåêó÷åñòü. [Â.Ë.Ãèíçáóðã, À.À.Àáðèêîñîâ,
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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
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26. Cohen A.E. Force-Extension Curve of a Polymer in a
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Ñ 322.1 ÎÁÙÀß ÒÅÎÐÈß ÎÒÍÎÑÈÒÅËÜÍÎÑÒÈ È ÃÐÀÂÈÒÀÖÈß
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32. Arik M. a.o. Einstein Spaces in Warped Geometries in Five
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33. Bezerra V.B. a.o. Gravitational Field Around a Timelike
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34. Blagojevic M., Vasilic M. Asymptotic Dynamics in 3D Gravity
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35. Booth I., Fairhurst S. The First Law for Slowly Evolving
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36. Cox D.P.G. Vaidya's "Kerr-Einstein" Metric Cannot be Matched
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37. Frolov A.V., Pen U.-L. Naked Singularity in the Global
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38. Gergely L.A. Generalized Friedmann Branes. //Phys. Rev.D. -
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39. Kanti P. a.o. Quest for Localized 4D Black Holes in Brane
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Ñ 322.2 ÊÎÑÌÎËÎÃÈß.ÃÐÀÂÈÒÀÖÈÎÍÍÛÅ ÂÎËÍÛ
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50. Bastero-Gil M. a.o. What Can WMAP Tell us About the Very
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62. Kantowski R. Lame Equation for the Distance Redshift in a
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Ñ 323 ÊÂÀÍÒÎÂÀß ÌÅÕÀÍÈÊÀ
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Ñ 323 à ÔÓÍÄÀÌÅÍÒÀËÜÍÛÅ ÂÎÏÐÎÑÛ ÊÂÀÍÒÎÂÎÉ ÌÅÕÀÍÈÊÈ.ÑÊÐÛÒÛÅ
ÏÀÐÀÌÅÒÐÛ.ÏÀÐÀÄÎÊÑÛ.ÒÅÎÐÈß ÈÇÌÅÐÅÍÈÉ
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×ÀÑÒÈÖ.ÀËÃÅÁÐÀ ÒÎÊÎÂ.ÊÈÐÀËÜÍÛÅ ÒÅÎÐÈÈ.ÒÅÎÐÈß ÐÅÄÆÅ
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