Algebraic equations from Hamiltonian constraints on vacuum spherically symmetric metrics describe non-homogeneous dust collapse and bounce, applied to quantum-inspired models to recover or find new bounce results.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
gr-qc 2verdicts
UNVERDICTED 2representative citing papers
Analysis of trapping horizons shows McVittie and Glass-Mashhoon spacetimes lack suitable future outer trapping horizons for cosmological black holes, while Culetu and Sultana-Dyer can describe them in the matter-dominated era if energy conditions hold.
citing papers explorer
-
Dust collapse and bounce in spherically symmetric quantum-inspired gravity models
Algebraic equations from Hamiltonian constraints on vacuum spherically symmetric metrics describe non-homogeneous dust collapse and bounce, applied to quantum-inspired models to recover or find new bounce results.
-
Cosmological Black hole Candidates: A Detailed Analysis of McVittie, Culetu, Sultana-Dyer, and Glass-Mashhoon Spacetimes
Analysis of trapping horizons shows McVittie and Glass-Mashhoon spacetimes lack suitable future outer trapping horizons for cosmological black holes, while Culetu and Sultana-Dyer can describe them in the matter-dominated era if energy conditions hold.