Spherically symmetric collapse in quantum gravity

Details Spherically symmetric collapse in quantum gravity Spherically symmetric collapse in quantum gravity

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981phlb..106..307f&link_type=abstract

Physics Letters B, Volume 106, Issue 4, p. 307-313.

Physics

52

Scientific paper

The problem of classical singularities is revised on the basis of the quantum-gravity effective equations. We find a simple rule for establishing the Birkhoff theorem in spherically symmetric problems. All exact solutions of the lagrangian with C2αβγσ are obtained. Spherically symmetric collapse of the thin null shell of mass M is considered in the framework of a local theory describing vacuum polarization effects. The boundary-value problem is set and the asymptotic solution is obtained. It is found that the shell collapses to r = 0 without the rise of a singularity, and begins expanding. The global behaviour of the solution is obtained for small M. For large M it is conjectured that the event horizon does not form, and the apparent horizon is closed. An object forms, possessing the observable properties of a black hole, but living a finite time.

Affiliated with

Also associated with

No associations

Rating

Spherically symmetric collapse in quantum 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 Spherically symmetric collapse in quantum gravity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spherically symmetric collapse in quantum gravity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-744624