Consistency test of general relativity from large scale structure
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We propose a consistency test of general relativity on cosmological scales. This test enables us to distinguish between two possibilities to explain the late time accelerated expansion of the universe, that is, dark energy models based on general relativity and modified gravity models without dark energy. We propose a way to perform this test using future observations.
This talk is part of the DAMTP Friday GR Seminar series.
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