Titlebook: Generalized Perturbations in Modified Gravity and Dark Energy; Jonathan Pearson Book 2014 Springer International Publishing Switzerland 20

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CYN

(Re)Presenting Sherlock Holmes,for parameters which have a “l(fā)arge” effect on observables on “small” scales. It is rather unfortunate, however, that it is most natural for dark sector theories to induce modifications on large scales, since it is only at late times when the dark sector dominates when those large scale modes cross the horizon.

Kinetic

EXUDE

Observational Signatures of Generalized Cosmological Perturbations,for parameters which have a “l(fā)arge” effect on observables on “small” scales. It is rather unfortunate, however, that it is most natural for dark sector theories to induce modifications on large scales, since it is only at late times when the dark sector dominates when those large scale modes cross the horizon.

食草

紡織品

紡織品

https://doi.org/10.1007/978-3-319-72523-9urbations. However, the formalism can be applied in much more diverse systems where relativistic field theories play a central role, such as massive gravities, inflation and even effective theories for quantum gravity.

嬰兒

草率男

放逐

The Effective Action Formalism for Cosmological Perturbations,, supernovae, baryon acoustic oscillations, gravitational lensing and structure formation point to the existence of an additional component dubbed “dark energy”, or a modification to gravity, which needs to be introduced to explain the the observed acceleration [1–5].