Abstract
We study the evolution of a naked singularity surrounded by an accreting disk of matter; we consider two kinds of disk: the standard thin-disk model and the thick barytropic model, for several initial conditions. We show that any Kerr naked singularity slows down in a finite time to a maximal Kerr black hole. We evaluate the final mass, the luminosity and the time of evolution of the singularity.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
