Black holes in a Chaplygin-like dark fluid have an upper charge bound for horizons of Q ≈ 0.556 M and a critical fluid parameter bound B_c Q_c^4 = 4/3^9 for multi-horizon solutions, with stronger curvature than RNdS.
Chandrasekhar,The Mathematical Theory of Black Holes
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
gr-qc 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Constructs Kruskal-Szekeres and Carter-Penrose diagrams for the Schwarzschild-like spacetime in Lorentz gauge theory, showing identical causal topology to Schwarzschild but with A0-controlled horizon radius, surface gravity, and geometry.
citing papers explorer
-
Causal structure of black holes immersed in a Chaplygin-like dark fluid environment: Horizons and singularities
Black holes in a Chaplygin-like dark fluid have an upper charge bound for horizons of Q ≈ 0.556 M and a critical fluid parameter bound B_c Q_c^4 = 4/3^9 for multi-horizon solutions, with stronger curvature than RNdS.
-
Maximal extension of Schwarzschild-like spacetimes in Lorentz gauge theory
Constructs Kruskal-Szekeres and Carter-Penrose diagrams for the Schwarzschild-like spacetime in Lorentz gauge theory, showing identical causal topology to Schwarzschild but with A0-controlled horizon radius, surface gravity, and geometry.