The Structure of Cosmic String Wakes (Proceedings)

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Proceedings for 18th Texas Symposium on Relativistic Astrophysics, Latex, 3 pages

Scientific paper

We present results of a cosmological hydrodynamical study of gravitational accretion in cosmic string wakes and filaments. Cosmic string wakes are formed by fast moving (v ~ c) strings. A conical deficit angle in the string spacetime induces a velocity perturbation in the background matter and a two-dimensional wake accretes in the path of the string. Filaments are formed by slow moving strings with a large amount of small scale structure. The major gravitational perturbation from slow moving strings is due to the Newtonian field induced by the effective mass of the wiggles. In cosmic string wakes, cool streams of baryons collide and are trapped at the center of the wake causing an enhancement of baryons versus dark matter by a factor of 2.4. In filaments, a high pressure is induced at the filament core and baryonic matter is expelled leading to a baryon deficit in the center of the filament.

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 Structure of Cosmic String Wakes (Proceedings) 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 Structure of Cosmic String Wakes (Proceedings), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Structure of Cosmic String Wakes (Proceedings) will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-489750

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