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Site / Abstract
Page modified on March 16, 2016, at 05:13 PM
- Status of art on observational evidences.
- Cosmic acceleration and large scale structure motivates bot MOG and DS.
- How can we discriminate between Dark Side and MOG?
- There exists some observation/experiment capable of being addressed just in one way (MOG or DS)?
- Non-linear relativistic effects in structure formation needs to be understood: they may be relevant when extremely large scales scales are considered in simulations, in view of next generation surveys
- Primordial GR effects on very large scales can be studied with non-linear perturbative methods and are relevant for measuring non-Gaussianity and affect bias.
- Fully-non linear scales can be studied with post-Newtonian methods, and the goal is to implement these in simulations
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