A class of interiors for Vaidya's radiating metric: singularity-free gravitational collapse

Details A class of interiors for Vaidya's radiating metric: singularity-free gravitational collapse A class of interiors for Vaidya's radiating metric: singularity-free gravitational collapse

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cqgra..25q5009f&link_type=abstract

Classical and Quantum Gravity, Volume 25, Issue 17, pp. 175009 (2008).

Physics

7

Scientific paper

In order to study gravitational collapse we introduce a class of stellar models which neither stabilize nor bounce. In these models all the energy conditions are fulfilled, however the collapsing stars radiate away their matter avoiding the formation of singularities. We discuss the viability of such a collapse and its implications in the resolution of the singularity issue. We also examine the possibility of living in a singularity-free locally open or flat FLRW universe satisfying all the energy conditions.

Affiliated with

Also associated with

No associations

Rating

A class of interiors for Vaidya's radiating metric: singularity-free gravitational collapse 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 A class of interiors for Vaidya's radiating metric: singularity-free gravitational collapse, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A class of interiors for Vaidya's radiating metric: singularity-free gravitational collapse will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1435652