Martinelli, Matteo, Calabrese, Erminia ![]() |
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Official URL: http://dx.doi.org/10.1103/PhysRevD.83.023012
Abstract
Future proposed satellite missions such as Euclid can offer the opportunity to test general relativity on cosmic scales through mapping of the galaxy weak-lensing signal. In this paper we forecast the ability of these experiments to constrain modified gravity scenarios such as those predicted by scalar-tensor and f(R) theories. We find that Euclid will improve constraints expected from the Planck satellite on these modified theories of gravity by 2 orders of magnitude. We discuss parameter degeneracies and the possible biases introduced by modifications to gravity.
Item Type: | Article |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Publisher: | American Physical Society |
ISSN: | 1550-7998 |
Date of First Compliant Deposit: | 10 October 2017 |
Date of Acceptance: | 21 December 2010 |
Last Modified: | 04 May 2023 02:18 |
URI: | https://orca.cardiff.ac.uk/id/eprint/105354 |
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