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Hints of modified gravity in cosmos and in the lab?

2019/01/11 by Leandros Perivolaropoulos, Lavrentios Kazantzidis · 2 citations
Physics and Astronomy · #Astrophysics #Classical mechanics #Context (archaeology) #Cosmological constant #Cosmology #Cosmology and Gravitation Theories #Dark energy #Fifth force #Galaxies: Formation, Evolution, Phenomena #Galaxy #General relativity #Gravitation #Halo mass function #Metric expansion of space #Physics #Redshift #Redshift survey #Redshift-space distortions #Solar and Space Plasma Dynamics #Theoretical physics #astro-ph.CO #gr-qc #hep-ph

paper · pdf · doi:10.1142/s021827181942001x

published as International Journal of Modern Physics D, Vol. 28, No. 05, 1942001 (2019) · 21 pages (two column), 22 figures. Minor modifications, references added. Invited Review for Special Issue on Modified Gravity. Published in International Journal of Modern Physics D, Vol. 28, No. 05, 1942001 (2019)

openalex publication_date 2019/01/11 · arxiv created 2019/07/15 · arxiv updated 2019/07/17 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

General Relativity (GR) is consistent with a wide range of experiments/observations from millimeter scales up to galactic scales and beyond. However, there are reasons to believe that GR may need to be modified because it includes singularities (it is an incomplete theory) and also it requires fine-tuning to explain the accelerating expansion of the universe through the cosmological constant. Therefore, it is important to check various experiments and observations beyond the above range of scales for possible hints of deviations from the predictions of GR. If such hints are found it is important to understand which classes of modified gravity theories are consistent with them. The goal of this review is to summarize recent progress on these issues. On sub-millimeter scales, we show an analysis of the data of the Washington experiment [D. J. Kapner, T. S. Cook, E. G. Adelberger, J. H. Gundlach, B. R. Heckel, C. D. Hoyle and H. E. Swanson, Phys. Rev. Lett. 98 (2007) 021101, arXiv:hep-ph/0611184 [hep-ph]] searching for modifications of Newton’s Law on sub-millimeter scales and demonstrate that a spatially oscillating signal is hidden in this dataset. We demonstrate that even though this signal cannot be explained in the context of standard modified theories (viable scalar tensor and [Formula: see text] theories), it is a rather generic prediction of nonlocal gravity theories. On cosmological scales we review recent analyses of Redshift Space Distortion (RSD) data which measure the growth rate of cosmological perturbations at various redshifts and show that these data are in some tension with the [Formula: see text]CDM parameter values indicated by Planck/2015 CMB data at about [Formula: see text] level. This tension can be reduced by allowing for an evolution of the effective Newton constant that determines the growth rate of cosmological perturbations. We conclude that even though this tension between the data and the predictions of GR could be due to systematic/statistical uncertainties of the data, it could also constitute early hints pointing towards a new gravitational theory.

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