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Observational constraints on kinetic gravity braiding from the integrated Sachs-Wolfe effect

Rampei Kimura1, Tsutomu Kobayashi2,3, and Kazuhiro Yamamoto1

  • 1Department of Physical Science, Hiroshima University, Higashi-Hiroshima 739-8526, Japan
  • 2Hakubi Center, Kyoto University, Kyoto 606-8302, Japan
  • 3Department of Physics, Kyoto University, Kyoto 606-8502, Japan

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Phys. Rev. D 85, 123503 – Published 4 June, 2012

DOI: https://doi.org/10.1103/PhysRevD.85.123503

Abstract

The cross correlation between the integrated Sachs-Wolfe (ISW) effect and the large-scale structure is a powerful tool to constrain dark energy and alternative theories of gravity. In this paper, we obtain observational constraints on kinetic gravity braiding from the ISW–large-scale-structure cross correlation. We find that the late-time ISW effect in the kinetic gravity braiding model anticorrelates with large-scale structures in a wide range of parameters, which clearly demonstrates how one can distinguish modified gravity theories from the lambda cold dark matter model using the ISW effect.

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Phys. Rev. D 85, 123503– Published 4 June, 2012
  • Received 20 October 2011

© 2012 American Physical Society

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