<!DOCTYPE html PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN"> <html> <head> <div align="Left"><a href="EPot2008.html"> RAN Programm "Physics of elementary particles and fundamental Nuclear Physics 2008" "</a> <br> <br> <meta http-equiv="content-type" content="text/html; charset=KOI8-R"> <title>0A?>@B @>5:B0 @>3@0<<K $   $878:0 M;5<5=B0@=KE G0AB8F 8 DC=40<5=B0;L=0O O45@=0O D878:0 </title> </head> <body text="#000000" bgcolor="#ffffff" link="#0000ee" vlink="#cc33cc" alink="#0000ee"> <div align="Center"><font size="+3"> @>3@0<<0 $  </font><br> <br> <font size="+2"><b> $878:0 M;5<5=B0@=KE G0AB8F 8 <br>DC=40<5=B0;L=0O O45@=0O D878:0 </font></div></b> <br> <div align="Left"><font size="+2"><b><u> </u></b></font> <hr width="100%" size="2" align="Left"><br> <br> <div align="Left"><font size="+2"><b><u> 1. 0720=85 @>5:B0. </u></b></font> <br> "5>@8O AB@C=, :>=D>@<=0O B5>@8O ?>;O 8 B5>@8O 3@028B0F88. <br> <br> <br> <div align="Left"><font size="+2"><b><u> 2. #G0AB=8:8 @>5:B0 (8=AB8BCBK, >@30=870F88, ?>4@0745;5=8O), :>;8G5AB2> =0CG=KE A>B@C4=8:>2, G8A;> <>;>4KE A>B@C4=8:>2 4> 35 ;5B, @C:>2>48B5;L ?@>5:B0. </u></b></font> <br> =AB8BCB B5>@5B8G5A:>9 D878:8 8<. . . 0=40C . <br> >;8G5AB2> =0CG=KE A>B@C4=8:>2: 16. <br> >;8G5AB2> <>;>4KE A>B@C4=8:>2 (4> 35 ;5B): 3. <br> C:>2>48B5;8 ?@>5:B0:G;5=-:>@@.  . . !B0@>18=A:89 8 ?@>D. . . 5;028=. <br> <div align="Left"><font size="+2"><b><u> 3. 5@8>4 2K?>;=5=8O ?@>5:B0 8 53> MB0?>2. </u></b></font> <br> 2003-2006 3. <br> <br> <div align="Left"><font size="+2"><b><u> 4. @0B:0O D>@<C;8@>2:0 F5;59 @>5:B0 8 53> >A=>2=KE MB0?>2. </u></b></font> <br> AA;54>20=85 @07;8G=KE :>=D>@<=KE B5>@89 ?>;O 8 1>;55 >1I8E 8=B53@8@C5<KE <0AA82=KE B5>@89 ?>;O :0: <0B5<0B8G5A:>3> 0??0@0B0 4;O 2KG8A;5=8O :>@@5;OF8>==KE DC=:F89 2 B5>@88 AB@C=. 7CG5=85 4C0;L=>9 M:2820;5=B=>AB8 <564C :>=D>@<=K<8 B5>@8O<8 ?>;O 8 B5>@859 3@028B0F88. 07@01>B:0 AB@C==KE <>45;59 B5>@88 :20=B>2>9 3@028B0F88 8 8AA;54>20=85 8E =01;N40B5;L=KE 0AB@>D878G5A:8E 8 :>A<>;>38G5A:8E ?>A;54AB289. <br> <br> <div align="Left"><font size="+2"><b><u> 5. 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AA;54>20=> 2;8O=85 B@5EG0AB8G=>3> 2708<>459AB28O <564C 8=D;0B>=>< 8 ?>;O<8 <0B5@88 =0 @07>3@52 ?>A;5 AB0488 AB>E0AB8G5A:>9 8=D;OF88 2 @0==59 A5;5==>9. >AB@>5=0 0=0;8B8G5A:0O B5>@8O @07>3@520 2 @568<5 B0E8>==>3> @57>=0=A0. (.~. >4>;LA:89) [27]. <br> <br> <br> <div align="Left"><font size="+2"><b><u> 6. C1;8:0F88: </u></b></font> <br> - @5D5@8@C5<K5 6C@=0;K (2:;NG0O @01>BK, ?@8=OBK5 : ?5G0B8), <br> - 4>:;04K =0 :>=D5@5=F8OE 8 H:>;0E, <br> - 70I8B0 48AA5@B0F89, <br> - ?>43>B>2:0 48?;><=KE (10:0;02@A:8E, <038AB5@A:8E) @01>B, <br> - ?C1;8:0F88 2 A@54AB20E <0AA>2>9 8=D>@<0F88 8 4@. <br> C1;8:0F88. <br> <br> [1] A. Belavin,Al. Zamolodchikov. Moduli Integrals,Ground Ring and Four-point function, "$, 147,v.3,339 (2006) <br> [2] A.Belavin,Al.Zamolodchikov. Higher Equations of Motion in N=1 SUSY Liouville Field Theory, JETP Letters 84,issue 8,496-502(2006), hep-th/0610316 <br> [3] V. Fateev, V. Postnikov and Y. Pugai. On scaling fields in $Z_N$ Ising models, JETP Lett. 83 (2006) 172-178. <br> [4] S.E. Parkhomenko. Free-Field representation of Permutation Branes in Gepner Models. JETP, T.129, V.6, pp. 1026-1042 (2006) <br> [5] A. Losev, I. Polyubin, Quantum Field Theory and Moduli Spaces, to be published in AMS Transl (Advances in the Mathematical Sciences) pp1-18 <br> [6] N.N. Nikolaev, W. Schaefer, B.G. Zakharov, V.R. Zoller. Unitarity constraints for DIS off nuclei: predictions for electron-ion colliders. arXiv:hep-ph/0610319. =0?@02;5=0 v Phys. Rev. D <br> [7] N.N. Nikolaev, W. Schaefer, B.G. Zakharov, V.R. Zoller. Glue in the pomeron from nonlinear $k_{T}$-factorization. arXiv:hep-ph/0602070; JETP Lett. 83, pp.192-197 (2006). <br> [8] D. Schildknecht, B.G. Zakharov. Transition radiation in the quantum regime as a diffractive phenomenon. Phys. Lett., A355, pp. 289-292 (2006). <br> [9] B. Feigin, E. Feigin. Two dimensional current algebras and affine fusion product. math.QA/0607091 <br> [10] B.L. Feigin, A.M. Gainutdinov, A.M. Semikhatov, I.Yu. Tipunin. Kazhdan--Lusztig-dual quantum group for logarithmic extensions of Virasoro minimal models math.QA/0606506 <br> [11] B.L. Feigin, A.M. Gainutdinov, A.M. Semikhatov, I.Yu. Tipunin. Logarithmic extensions of minimal models: characters and modular transformations Nucl.Phys. B757 (2006) 303-343 <br> [12] B. Feigin, E. Feigin, M. Jimbo, T. Miwa, Y. Takeyama A $\phi_{1,3}$-filtration of the Virasoro minimal series M(p,p') with 1<p'/p< 2. math.QA/0603070 <br> [13] B. Feigin, B. Shoikhet. On $[A,A]/[A,[A,A]]$ and on a $W_n$-action on the consecutive commutators of free associative algebra math.QA/0610410 <br> [14] A.O. Barvinsky, A.Yu. Kamenshchik. Cosmological Landscape From Nothing: Some Like It Hot, JCAP 0609, 014 (2006). <br> [15] A.O. Barvinsky, A.Yu. Kamenshchik. Thermodynamics via Creation from Nothing: Limiting the Cosmological Constant Landscape, Preprint hep-th/0611206 (2006). <br> [16] G. Esposito, G. Fucci, A. Yu. Kamenshchik, K. Kirsten. New Developments in the Spectral Asymptotics of Quantum Gravity, J.Phys. A39, 6317-6322 (2006). <br> [17] R. Casadio, F. Finelli, A.Yu. Kamenshchik, M. Luzzi, G. Venturi. Method of comparison equations for cosmological perturbations, JCAP 0604, 011 (2006). <br> [18] S.N. Vergeles, One more variant of discrete gravity having "naive" continual limit, Nucl. Phys. B 375, 172-191 (2006). <br> [19] S.N. Vergeles, Discrete quantum gravity: continuum limit and the problem of state counting, hep-th/0606102 (2006). <br> [20] R. Gannouji, D. Polarski, A. Ranquet, A.A. Starobinsky. Scalar-tensor models of normal and phantom dark energy', JCAP {\bf 0609}, 016 (2006). <br> [21] V. Sahni, A.A. Starobinsky. Reconstructing dark energy, Int. J. Mod. Phys. D {\bf 15}, in press, 2006; arXiv:astro-ph/0610026. <br> [22] A. Shafieloo, U. Alam, V. Sahni, A.A. Starobinsky. Smoothing supernova data to reconstruct the expansion of the Universe and its age, MNRAS {\bf 366}, 1081-1095 (2006). <br> [23] K.A. Bronnikov, A.A. Starobinsky, No static wormholes for scalar-tensor phantom dark energy without ghosts, 8AL<0 2 -"$, {\bf 84}, 2006 (2 ?5G0B8). <br> [24] J.F. Macias-Perez, G. Lagache, B. Maffei et al. (Archeops collaboration including A. A. Starobinsky). Archeops in-flight performance, data processing and map making'', Astron. Astroph., 2006, in press; astro-ph/0603665. <br> [25] C. Kiefer, I. Lohmar, D. Polarsky, A.A. Starobinsky. Pointer states for primordial fluctuations in inflationary cosmology. Class. Quant. Grav., in press, 2007; astro-ph/0610700. <br> [26] G.E. Volovik. Emergent physics on vacuum energy and cosmological constant, AIP Conference Proceedings, {\bf 850}, 26 (2006); arXiv:cond-mat/0507454. <br> [27] G.~E. Volovik. Vacuum Energy: Myths and Reality, to be published in special issue of Int. J. Mod. Phys. devoted to dark energy and dark matter; gr-qc/0604062. <br> [28] J.F.Dufaux, G.Felder, L.Kofman, M.Peloso and D.Podolsky. Preheating with trilinear interactions: tachyonic resonance'', JCAP {\bf 0607}, 006 (2006). <br> <br> <div align="Left"><font size="+2"><b><u> >:;04K =0 :>=D5@5=F8OE 8 H:>;0E. </u></b></font> <br> <br> [1] . 5;028=. "Kvarki 2006", !. 5B5@1C@3, 09 2006 On new results in the Minimal Liouvill gravity. <br> [2] . 5;028=. 4-E B>G5G=K5 :>@@5;OF8>==K5 DC=:F89 2 <8=8<0;L=>9 ;8C28;;52A:>9 3@028B0F88. Integrable Models (45:01@L 2006, 8>B>, RIMS, /?>=8O). <br> [3] .. !B0@>18=A:89. 564C=0@>4=0O :>=D5@5=F8O ?> 3@028B0F88, :>A<>;>388, 0AB@>D878:5 8 =5AB0F8>=0@=>9 307>48=0<8:5, ?>A2OI5==0O 90-;5B8N A> 4=O @>645=8O ?@>D. .. !B0=N:>28G0. >A:20, 01--05.03.2006. !>-?@54A540B5;L >@3:><8B5B0. ;5=0@=K9 4>:;04 ""5<=0O M=5@38O 2 A:0;O@=>-B5=7>@=>9 B5>@88 3@028B0F88". <br> [4] .. !B0@>18=A:89. 3-5 <564C=0@>4=>5 A>25I0=85 ?> :>A<8G5A:8< ;CG0< A25@E2KA>:>9 M=5@388 8 8E 8AB>G=8:0< "GZK-40: forty years of the GZK problem". >A:20, 16--18.05.2006. >:;04 "Trans-Planckian particle creation and UHECR". <br> [5] .. !B0@>18=A:89. 14-K9 <564C=0@>4=K9 A5<8=0@ ?> D878:5 2KA>:8E M=5@389 QUARKS'2006. !.-5B5@1C@3, 19--25.05.2006. ;5=0@=K9 4>:;04 "Dark energy models in scalar-tensor and f(R) gravity". <br> [6] .. !B0@>18=A:89. 2-5 <564C=0@>4=>5 A>25I0=85 ?> 3@028B0F88 8 :>A<>;>388 "Santa Clara 2006". !0=B0-;0@0, C10, 29.05--01.06.2006. ;5=0@=K9 4>:;04 "Scalar-tensor models of dark energy". <br> [7] .. !B0@>18=A:89. 22->9 :>;;>:28C< 0@86A:>3> =AB8BCB0 0AB@>D878:8 "Inflation + 25. The first 25 years of inflationary cosmology". 0@86, $@0=F8O, 26--30.06.2006. ;5=0@=K9 4>:;04 "Stochastic inflation and perturbations". <br> [8] .. !B0@>18=A:89. 2-0O <564C=0@>4=0O :>=D5@5=F8O ?> :20=B>2K< B5>@8O< 8 @5=>@<0;870F8>==>9 3@C??5 2 3@028B0F88 8 :>A<>;>388 IRGAC2006. 0@A5;>=0, A?0=8O, 10--15.07.2006. ';5= <564C=0@>4=>3> @30=870F8>==>3> :><8B5B0. ;5=0@=K9 4>:;04 "Stochastic inflation and perturbations". <br> [9]. 11-0O <564C=0@>4=0O :>=D5@5=F8O ?> >1I59 B5>@88 >B=>A8B5;L=>AB8 8<. 0@A5;O @>AA<0=0. 5@;8=, 5@<0=8O, 23--29.07.2006. ';5= <564C=0@>4=>3> >>@48=0F8>==>3> :><8B5B0, ?@54A540B5;L A5:F88. 0??>@B5@A:89 4>:;04 =0 A5:F88 "Dark energy in the Universe". <br> [10] 6-0O <564C=0@>4=0O :>=D5@5=F8O "Recontre du Vietnam. Challenges in particle astrophysics". %0=>9, L5B=0<, 07--12.08.2006. ;5=0@=K9 4>:;04 "Dark energy in the Universe". <br> [11] .. !B0@>18=A:89. 1-0O 5<1@846 - 8BG5;; - "5E0AA:0O :>=D5@5=F8O ?> :>A<>;>388. 5<1@846, 5;8:>1@8B0=8O, 21--26.08.2006. ;5=0@=K9 4>:;04 "The Gibbons-Hawking temperature and the correlation radius in the de Sitter and inflationary space-times". <br> [12] .. !B0@>18=A:89. 4-0O <564C=0@>4=0O ;5B=OO 2KAH0O H:>;0 ?> A>2@5<5==>9 <0B5<0B8G5A:>9 D878:5. /, C1=0, 03--12.09.2006. \\ 3 ;5:F88 =0 B5<C: "Dark energy: observational status and theoretical models". <br> [13] .. !B0@>18=A:89. >=D5@5=F8O ?> :>A<><8:@>D878:5 8 :>A<>;>388. $;>@5=F8O, B0;8O, 28.08--11.11.2006. 2 4>:;040: "Phantom without ghosts: scalar-tensor models of dark energy","Exact solutions in the theory of generation of primordial scalar perturbations". <br> [14] .. !B0@>18=A:89. 0CG=0O ?@>3@0<<0 "General relativity trimester. Gravitational waves, relativistic astrophysics and cosmology". 0@86, $@0=F8O, 18.09--15.12.2006. 8 ;5:F88 =0 B5<C "Dark energy in the Universe". <br> [15] .. !B0@>18=A:89. International workshop "Cosmology and Astroparticles". Montpellier, Frantsiya, 23--24.11.2006. So-predsedatel' Orgkomiteta. 1 plenarnyi doklad "Geometrical dark energy". <br> [16] .. !B0@>18=A:89. !5<8=0@ ?> ?@>1;5<0< 87<5@8<>AB8 2 :20=B>2>9 3@028B0F88 8 B5<=>9 <0B5@88 2> A5;5==>9. !.-5B5@1C@3, 30.11--02.12.2006. @54A540B5;L @30=870F8>==>3> :><8B5B0. 1 ;5=0@=K9 4>:;04 ""5<=0O M=5@38O 2> A5;5==>9". <br> [17] .. !B0@>18=A:89. International conference "High Energy, Cosmology and Strings", Parij, Frantsiya, 11--15.12.2006. 1 plenarnyi doklad "Dark energy in scalar-tensor and f(R) gravity". <br> [18] Possiskaya konferentsiya HEA-2006 "Astrofizika vysokih energii segodnya i zavtra". Moskva, 25--27.12.2006. 1 plenarnyi doklad "Skopleniya galaktik i temnaya energiya". <br> [19] . . $5938=, <564C=0@>4=>5 A>25I0=85 "Infinite dimensional algebras and integrable models I". >A:20, 7-14 <0@B0 2006. @30=870B>@. <br> [20] . . $5938=, <564C=0@>4=>5 A>25I0=85 "Infinite dimensional algebras and integrable models II". >A:20, 23-20 A5=BO1@O 2006. @30=870B>@. <br> [21] ... 0<5=I8:. International Workshop on Pseudo-Hermitian Hamiltonians in Quantum Physics (July 3-5, 2006), Bologna, Italy, Priglashennyj doklad `` Complex Lagrangians and phantom cosmology". <br> [22] ... 0<5=I8:. 2nd International Conference on Quantum Theories and Renormalization Group in Gravity and Cosmology, Barcelona, July 11-15 2006, Spain, ``Cosmological landscape and Euclidean quantum gravity" <br> [23] ... 0<5=I8:. Eleventh Marcel Grossmann Meeting on General Relativity , July 23 - 29, 2006, Berlin, Germany, ``Cosmological landscape and Euclidean quantum gravity", ``Chaplygin gas and tachyons as dark energy models", ``Smooth crossing of the phantom divide line in cosmology". <br> [24] ... 0<5=I8:. Dynamical Systems: Classical, Quantum and Stochastic Rome, October 2-5, 2006, Italy Priglashennyj doklad ``Chaplygin gas and tachyons in modern cosmology?. <br> [25] ... 0<5=I8:. Cosmology Workshop Montpellier06, Motpellier, 23-24 November 2006, France. Priglashennyj doklad ``Tachyons in cosmology". <br> <br> <div align="Left"><font size="+2"><b><u> 0I8B0 48AA5@B0F89 </u></b></font> <br> [1] . 8B28=>2, 48AA5@B0F8O =0 AB5?5=L :.D.-<.=, ">@@5;OF8>==K5 DC=:F88 2 8=B53@8@C5<KE <>45;OE B5>@88 ?>;O", 2006. 0I8B0 =07=0G5=0 =0 29.12.2006 3. <br> C1;8:0F88 2 A@54AB20E <0AA>2>9 8=D>@<0F88. <br> 5B. <br> <br> <div align="Left"><font size="+2"><b><u> 7. >445@6:0 @01>BK 70 AG5B 3@0=B>2 $$, 3>A:>=B@0:B>2, 2=51N465B=KE 8 ?@>G8E A@54AB2. </u></b></font> <br> 1. $$ 05-02-17450 "AA;54>20=85 B5<=>9 M=5@388 8 B5<=>9 <0B5@88 2> A5;5==>9", @C:>2>48B5;L .. !B0@>18=A:89, 2005-2007. <br> 2. @>3@0<<0 ?>445@6:8 254CI8E =0CG=KE H:>; (-1157.2006.2, 2006-2007, A>@C:>2>48B5;8 .. %0;0B=8:>2 8 .. !B0@>18=A:89, 2005-2007. <br> 3. $$ 04-02-16027 "">G=> @5H05<K5 <>45;8 :20=B>2>9 B5>@88 ?@>AB@0=AB2 A>AB>O=89 :20=B>2KE 8=B53@8@C5<KE <>45;59", @C:>2>48B5;L ..5;028=, 2004-2006. <br> 4. $$ 05-01-01007  @54AB02;5=8O 15A:>=5G=><5@=KE 0;351@, 25@H8==K5 >?5@0B>@K, 1>7>=870F8O 8 :>@@5;OF8>==K5 DC=:F88 2 :20=B>2KE 8=B53@8@C5<KE <>45;OE , @C:>2>48B5;L ..$5938=, 2005-2007. <br> 5.@>3@0<<0 ?>445@6:8 254CI8E =0CG=KE H:>; (-2044.2003.2, @C:>2>48B5;L ..5;028=, 2005-2007. <br> 6. INTAS 03-51-3350 "Correlation functions in integrable models of quantum field theory and their applications to phase transitions in low-dimensional systems". <br> <br> <div align="Left"><font size="+2"><b><u> 8. $>@<C;8@>2:0 >A=>2=KE 7040G ?> @>5:BC =0 2007 3>4. </u></b></font> <br> > B5<5 I: <br> 1. @>4>;68BL 8AA;54>20=85 8=8<0;L=>9 B5>@88 AB@C= - 42C<5@=>9 3@028B0F88 8C28;;O.  G0AB=>AB8 =09B8 0<?;8BC4K 5=5F80=> (:>@@5;OF8>==K5 DC=:F88) 4;O n>4, 0 B0:65 4;O A;CG0O 2K@>645==KE D878G5A:8E 25@H8==KE >?5@0B>@>2. <br> 2. >AB@>8BL A2>1>4=>-?>;52>5 ?@54AB02;5=85 4;O 3@0=8G=KE A>AB>O=89 2 <>45;OE 5?=5@0, A2O70==K5 A 3@C??>9 ?5@5AB0=>2>:. 7CG8BL 35><5B@8N 3@0=8G=KE A>AB>O=89 A2O70==KE A 3@C??0<8 ?5@5AB0=>2>: 2 <>45;OE 5?=5@0. 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AA;54>20BL ?@>AB@0=AB2> ;>:0;L=KE >?5@0B>@>2 8 =09B8 0;351@08G5A:89 ?>4E>4 : D>@< D0:B>@0< 2 2>7<CI5==KE :>=D>@<=KE B5>@8OE ?>;O. <br> > B5<5 II: <br> 1. @>4>;65=85 8AA;54>20=8O =5A8=3C;O@=KE :>A<>;>38G5A:8E <>45;59, 2>7=8:0NI8E 2 AB@C==>9 :>A<>;>388 8 8E =01;N40B5;L=KE A;54AB289, 2 B.G. @0AG5B A?5:B@>2 <>I=>AB8 A:0;O@=KE (048010B8G5A:8E 8 87>:@8287=>2KE) 2>7<CI5=89 8 3@028B0F8>==KE 2>;=. <br> 2. >AB@>5=85 8 8AA;54>20=85 :20=B>2KE :>A<>;>38G5A:8E <>45;59 A A> <=>38<8 20:CC<=K<8 A>AB>O=8O<8 2 >1;0AB8 =87:8E M=5@389. <br> 3. @>4>;65=85 8AA;54>20=8O @50;870F88 MDD5:B0 3@028B0F8>==>3> B@0=A-?;0=:>2A:>3> @>645=8O G0AB8F 2 @0AH8@ONI59AO A5;5==>9 =0 >A=>25 AB@C==KE <>45;59 <0B5@88, 254CI8E : =5AB0=40@B=>9 A2O78 <564C 8<?C;LA>< 8 M=5@3859 M;5<5=B0@=KE G0AB8F ?@8 A25@E2KA>:8E M=5@38OE. <br> 4. 0;L=59H89 0=0;87 4C0;L=>9 M:2820;5=B=>AB8 <564C :>=D>@<=K<8 B5>@8O<8 ?>;O 8 B5>@859 3@028B0F88 =0 ?@8<5@5 :>A<>;>38G5A:8E 2>7<CI5=89, 35=5@8@C5<KE 87 20:CC<=KE :20=B>2KE D;C:BC0F89 =0 8=D;OF8>==>9 AB0488 2 @0==59 A5;5==>9. <br> <br> <div align="Left"><font size="+2"><b><u> 9.1J5< D8=0=A8@>20=8O @01>B ?> @>5:BC 2 2006 3>4C 8 70O2:0 =0 2007 3. </u></b></font> <br> 0 AG5B @>3@0<<K 2 2006 3. - 600 BKA. C1. <br> 0O2:0 =0 2007 3. - 600 BKA. @C1. <br> <br> <div align="Left"><font size="+2"><b><u> C:>2>48B5;8 ?@>5:B0: </u></b></font> <br><br> <b> G;5=-:>@@.  .. !B0@>18=A:89 <br><br> ?@>D. 4.D-<.=. .. 5;028=</b> <br>