In d-dimensional spacetime, strange quark stars gain stability with increasing dimension for ranges of central density, with the mass maximum marking the onset of radial instability, and Newtonian stability holds for adiabatic index at or above 2(d-2)/(d-1).
On naked singularities in higher dimensional Vaidya space-times
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
abstract
We investigate the end state of gravitational collapse of null fluid in higher dimensional space-times. Both naked singularities and black holes are shown to be developing as final outcome of the collapse. The naked singularity spectrum in collapsing Vaidya region (4D) gets covered with increase in dimensions and hence higher dimensions favor black hole in comparison to naked singularity. The Cosmic Censorship Conjecture will be fully respected for a space of infinite dimension.
fields
gr-qc 1years
2019 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Extra dimensions' influence on the equilibrium and radial stability of strange quark stars
In d-dimensional spacetime, strange quark stars gain stability with increasing dimension for ranges of central density, with the mass maximum marking the onset of radial instability, and Newtonian stability holds for adiabatic index at or above 2(d-2)/(d-1).