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(116) Rev. Lett. 98, 131302 24) Amendola L., Tsujikawa S., 2007, Phys. Lett. B, submitted 25) Nojiri S., Odintsov S. D., Sasaki M., 2005, Phys. Rev. D 71, 123509 26) Dvali G. R., Gabadadze G., Porrati M., 2000, Phys. Lett. B 485, 208 27) Huterer A., Turner M., 2001, Phys. Rev. D 64, 123527 28) Bassett B. A., Corasaniti P. S., Kunz M., 2004, Astrophys. J. 617, L1 29) Eisenstein D. J., et al., 2005, Astrophys. J. 633, 560. 472. What Is the Origin of Dark Energy ? Shinji TSUJIKAWA Gunma National College of Technology, 580 Toriba, Maebashi, Gunma 371ῌ8530, Japan Abstract : The recent data of Supernova Ia and other observations suggest that the universe has entered the stage of an accelerated expansion after the matter-dominated epoch. The origin of dark energy responsible for this accelerated expansion is a serious mistery. I review recent theoretical attempts to investigate the origin of dark energy such as scalar field models and modified gravity models. I also address the method to determine the evolution of the equation of state of dark energy from observations.. ῍῏ῌῐ. 2007 ῎ 9 ῌ.
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H ernández , Positive and free boundary solutions to singular nonlinear elliptic problems with absorption; An overview and open problems, in: Proceedings of the Variational
The only thing left to observe that (−) ∨ is a functor from the ordinary category of cartesian (respectively, cocartesian) fibrations to the ordinary category of cocartesian
Keywords: Convex order ; Fréchet distribution ; Median ; Mittag-Leffler distribution ; Mittag- Leffler function ; Stable distribution ; Stochastic order.. AMS MSC 2010: Primary 60E05
In Section 3, we show that the clique- width is unbounded in any superfactorial class of graphs, and in Section 4, we prove that the clique-width is bounded in any hereditary