Development of voids in the thin-wall approximation. I - General characteristics of spherical vacuum voids

Details Development of voids in the thin-wall approximation. I - General characteristics of spherical vacuum voids Development of voids in the thin-wall approximation. I - General characteristics of spherical vacuum voids

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...298..439l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 298, Nov. 15, 1985, p. 439-447. NSERC-supported research.

Computer Science

Numerical Analysis

26

Astronomical Models, Cosmology, Thin Walls, Voids, Numerical Analysis, Relativistic Theory, Star Distribution

Scientific paper

The evolution of spherical vacuum voids in a Robertson-Walker background is studied within the context of the general relativistic thin-wall approximation. The authors extend the work of Maeda and Sato so as to include a background pressure, interior mass, and surface pressure (or tension). They find that these refinements each have important effects on the evolution of voids. Moreover, in comparable situations, the integrations given here differ in significant ways from those presented previously.

Affiliated with

Also associated with

No associations

Rating

Development of voids in the thin-wall approximation. I - General characteristics of spherical vacuum voids 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 Development of voids in the thin-wall approximation. I - General characteristics of spherical vacuum voids, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Development of voids in the thin-wall approximation. I - General characteristics of spherical vacuum voids will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-977910