Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
2003-08-06
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
4 pages, Letter, Revised version,clarity improved
Scientific paper
We investigate here how the shearing effects present within a collapsing matter cloud influence the outcome of gravitational collapse in terms of formation of either a black hole or a naked singularity as the final end state. For collapse of practically all physically reasonable matter fields, we prove that it would always end up in a black hole if it is either shear-free or has homogeneous density. Thus it follows that whenever a naked singularity forms as end product, the collapsing cloud must necessarily be shearing with inhomogeneous density. Our consideration brings out the physical forces at work which could cause a naked singularity to result as collapse end state, rather than a black hole.
Dadhich Naresh
Goswami Rituparno
Joshi Pankaj S.
No associations
LandOfFree
The critical role of shear in 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 The critical role of shear in gravitational collapse, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The critical role of shear in gravitational collapse will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-685738