Journal
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Volume -, Issue 6, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2018/06/017
Keywords
dark energy theory; modified gravity; weak gravitational lensing
Funding
- Council of Scientific & Industrial Research (CSIR), Govt. of India through Senior Research Fellowship (SRF) [09/466(0157)/2012-EMR-I]
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The cubic Galileon model containing the lowest non-trivial order action of the full Galileon action can produce the stable late-time cosmic acceleration. This model can have a significant role in the growth of structures. The signatures of the cubic Galileon model in the structure formation can be probed by the weak lensing statistics. Weak lensing convergence statistics is one of the strongest probes to the structure formation and hence it can probe the dark energy or modified theories of gravity models. In this work, we investigate the detectability of the cubic Galileon model from the ACDM model or from the canonical quintessence model through the convergence power spectrum and bi-spectrum.
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