Stochastic gravitational background from inflationary phase transitions

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

12 pages, 3 figures. Phys.Rev.D in press

Scientific paper

10.1103/PhysRevD.56.4610

We consider true vacuum bubbles generated in a first order phase transition occurring during the slow rolling era of a two field inflation: it is known that gravitational waves are produced by the collision of such bubbles. We find that the epoch of the phase transition strongly affects the characteristic peak frequency of the gravitational waves, causing an observationally interesting redshift in addition to the post-inflationary expansion. In particular it is found that a phase transition occurring typically 10$\div$20 $e-$foldings before the reheating at $kT\simeq 10^{15}$ GeV may be detected by the next Ligo gravity waves interferometers. Moreover, for recently proposed models capable of generating the observed large scale voids as remnants of the primordial bubbles (for which the characteristic wave lengths are several tens of Mpc), it is found that the level of anisotropy of the cosmic microwave background provides a deep insight upon the physical parameters of the effective Lagrangian.

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

Stochastic gravitational background from inflationary phase transitions 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 Stochastic gravitational background from inflationary phase transitions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stochastic gravitational background from inflationary phase transitions will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-379328

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