An exact relativistic fluid model is constructed whose asymptotic endpoint is a static ghost star with vanishing total mass and regions of negative energy density.
Evolution of Self-Gravitatin g Fluid Spheres Involving Ghost Stars
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
gr-qc 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
The birth of a ghost star
An exact relativistic fluid model is constructed whose asymptotic endpoint is a static ghost star with vanishing total mass and regions of negative energy density.