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Dark Energy: Investigation and Modeling

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Dark Matter and Dark Energy

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 370))

Abstract

Constantly accumulating observational data continue to confirm that about 70% of the energy density today consists of dark energy responsible for the accelerated expansion of the Universe. We present recent observational bounds on dark energy constrained by the type Ia supernovae, cosmic microwave background, and baryon acoustic oscillations.We review a number of theoretical approaches that have been adopted thus far to explain the origin of dark energy. This includes the cosmological constant, modified matter models (such as quintessence, k-essence, coupled dark energy, unified models of dark energy and dark matter), modified gravity models (such as f (R) gravity, scalar-tensor theories, braneworlds), and inhomogeneous models.We also discuss observational and experimental constraints on those models and clarify which models are favored or ruled out in current observations.

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Authors and Affiliations

  1. Department of Physics, Faculty of Science, Tokyo University of Science, 1-3 Kagurazaka, Shinjuku-ku, Tokyo, 162-8601, Japan

    Shinji Tsujikawa

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  1. Dipartimento di Fisica G. Galilei, Università degli Studi di Padova, Via Marzolo 8, 35131, Padova, Italy

    Sabino Matarrese

  2. Dipartimento di Fisica G. Occhialini, Università de Milano Bicocca, Piazza della Scienza 3, 20126, Milano, Italy

    Monica Colpi

  3. Dipartimento di Fisica e Matematica, Università dell’Insubria, Via Valleggio 11, 22100, Como, Italy

    Vittorio Gorini  & Ugo Moschella  & 

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Tsujikawa, S. (2011). Dark Energy: Investigation and Modeling. In: Matarrese, S., Colpi, M., Gorini, V., Moschella, U. (eds) Dark Matter and Dark Energy. Astrophysics and Space Science Library, vol 370. Springer, Dordrecht. https://doi.org/10.1007/978-90-481-8685-3_8

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