ÈÍÔÎÐÌÀÖÈÎÍÍÛÉ ÁÞËËÅÒÅÍÜ "ÑÒÀÒÜÈ" N.34 25.08.03
Ñ 131 ÂÛÑØÀß ÀËÃÅÁÐÀ.ËÈÍÅÉÍÀß ÀËÃÅÁÐÀ.ÒÅÎÐÈß ÌÀÒÐÈÖ
1. Ìîõîâ Î.È. Êâàçèôðîáåíèóñîâû àëãåáðû è èõ èíòåãðèðóåìûå
N-ïàðàìåòðè÷åñêèå äåôîðìàöèè, çàäàâàåìûå ñîãëàñîâàííûìè (N x
N)-ìåòðèêàìè ïîñòîÿííîé ðèìàíîâîé êðèâèçíû. //Òåîð. è ìàòåì. ôèç. -
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Ñ 133.2à ÍÅËÈÍÅÉÍÛÅ ÓÐÀÂÍÅÍÈß ÌÀÒÅÌÀÒÈ×ÅÑÊÎÉ ÔÈÇÈÊÈ,
ÑÎËÈÒÎÍÛ.
3. Ïàêóëÿê Ñ.Ý., Ñåðãååâ Ñ.Ì. Ñïåêòðàëüíûå êðèâûå è
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Ñ 135 ÔÓÍÊÖÈÎÍÀËÜÍÛÉ ÀÍÀËÈÇ
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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 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. Krasnikov S. Quantum Inequalities do not Forbid Spacetime
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27. Lambiase G. MSW Effect in Loop Quantum Gravity and
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Ñ 322.1 ÎÁÙÀß ÒÅÎÐÈß ÎÒÍÎÑÈÒÅËÜÍÎÑÒÈ È ÃÐÀÂÈÒÀÖÈß
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29. Alvi K. Note on Ingoing Coordinates for Binary Black Holes.
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30. Bhadra A. Gravitational Lensing by a Charged Black Hole of
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31. Bona C. a.o. General-Covariant Evolution Formalism for
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33. Charmousis C. a.o. Gravitation Lensing by Dark Matter
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36. Dubvosky S.L., Rubakov V.A. Brane-Induced Gravity in More
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42. Lake K. All Static Spherically Symmetric Perfect-Fluid
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Ñ 322.2 ÊÎÑÌÎËÎÃÈß.ÃÐÀÂÈÒÀÖÈÎÍÍÛÅ ÂÎËÍÛ
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55. Buonanno A. a.o. Detecting Gravitational Waves from
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58. Chassande-Mottin E. Learning Approach to the Detection of
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59. Chung D.J.H., Freese K. Lensed Density Perturbations in
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60. Collins H., Holman R. Invisible Axion in a Randall-Sundrum
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62. D'Ambrosio E. Nonspherical Mirrors to Reduce Thermoelastic
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65. Fairbairn M. a.o. Radion Assisted Gauge Inflation. //Phys.
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66. Garcia-Bellido J. a.o. Symmetry Breaking and False Vacuum
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67. Goheer N., Dunsby P.K.S. Exponential Potentials on the
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68. Hartl M.D. Survey of Spinning Test Particle Orbits in Kerr
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69. Jhingan S., Tanaka T. Improvement on the Metric
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72. Lemoine M. a.o. Trans-Planckian Dark Energy? //Phys.
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75. Majumdar D. Direct Detection Rates for Kaluza-Klein Dark
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76. Maor I., Brustein R. Distinguishing Among Scalar Field
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Ñ 323 ÊÂÀÍÒÎÂÀß ÌÅÕÀÍÈÊÀ
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