The evolution of cosmological gravitational waves in f(R) gravity

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

19 pages, 4 figures; v2: corrected to match version accepted for publication in PRD

Scientific paper

10.1103/PhysRevD.77.024033

We give a rigorous and mathematically clear presentation of the Covariant and Gauge Invariant theory of gravitational waves in a perturbed Friedmann-Lemaitre-Robertson-Walker universe for Fourth Order Gravity, where the matter is described by a perfect fluid with a barotropic equation of state. As an example of a consistent analysis of tensor perturbations in Fourth Order Gravity, we apply the formalism to a simple background solution of R^n gravity. We obtain the exact solutions of the perturbation equations for scales much bigger than and smaller than the Hubble radius. It is shown that the evolution of tensor modes is highly sensitive to the choice of n and an interesting new feature arises. During the radiation dominated era, their exist a growing tensor perturbation for nearly all choices of n. This occurs even when the background model is undergoing accelerated expansion as opposed to the case of General Relativity. Consequently, cosmological gravitational wave modes can in principle provide a strong constraint on the theory of gravity independent of other cosmological data sets.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

The evolution of cosmological gravitational waves in f(R) gravity does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The evolution of cosmological gravitational waves in f(R) gravity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The evolution of cosmological gravitational waves in f(R) gravity will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-333053

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.