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Paper: The Physical Properties of the Cosmic Acceleration
Volume: 424, Proceedings of the 9th International Conference of the Hellenic Astronomical Society
Page: 334
Authors: Basilakos, S.
Abstract: The observed late-time acceleration of the cosmic expansion constitutes a fundamental problem in modern theoretical physics and cosmology. In an attempt to weight the validity of a large number of dark energy models, I use the recent measurements of the expansion rate of the Universe, the clustering of galaxies the CMB fluctuations as well as the large scale structure formation, to put tight constraints on the different models.
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