The WiggleZ Dark Energy Survey: constraining the evolution of Newton's constant using the growth rate of structure
Savvas Nesseris, Chris Blake, Tamara Davis, David Parkinson

TL;DR
This paper uses large-scale structure data from the WiggleZ survey to test the evolution of Newton's constant, providing model-independent constraints that are consistent with General Relativity and aligning with cosmic microwave background measurements.
Contribution
It introduces two novel, model-independent methods to constrain the evolution of Newton's constant using growth rate data without relying on the Universe's expansion history.
Findings
Constraints on the second derivative of Newton's constant are consistent with zero.
Measured $\sigma_8$ values agree with cosmic microwave background results.
The methods do not require assumptions about the expansion history of the Universe.
Abstract
We constrain the evolution of Newton's constant using the growth rate of large-scale structure measured by the WiggleZ Dark Energy Survey in the redshift range . We use this data in two ways. Firstly we constrain the matter density of the Universe, (assuming General Relativity), and use this to construct a diagnostic to detect the presence of an evolving Newton's constant. Secondly we directly measure the evolution of Newton's constant, , that appears in Modified Gravity theories, without assuming General Relativity to be true. The novelty of these approaches are that, contrary to other methods, they do not require knowledge of the expansion history of the Universe, , making them model independent tests. Our constraints for the second derivative of Newton's constant at the present day, assuming it is slowly evolving as suggested by Big Bang…
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