Planar Carrollian statistical physics is well-defined thanks to central extensions and rotation, yielding logarithmic entropy scaling with disc area and two-dimensional ideal-gas pressure.
Embedding Galilean and Carrollian geometries I. Gravitational waves
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
years
2026 3verdicts
UNVERDICTED 3representative citing papers
Rotating black holes are constructed in magnetic Carroll gravity, including an intrinsically Carrollian dressed solution and a Kerroll black hole from an odd-power c-expansion of GR, with conserved charges computed.
Difference-angle geometry reconstructs parabolas via a focal function, derives a pseudo-inner product and Stewart theorem analog from it, defines associated trigonometric functions, and recovers the difference angle as the parabolic degeneration of the Cayley-Klein cross-ratio angle.
citing papers explorer
-
Statistical Physics of Planar Carroll Systems
Planar Carrollian statistical physics is well-defined thanks to central extensions and rotation, yielding logarithmic entropy scaling with disc area and two-dimensional ideal-gas pressure.
-
Kerroll black holes
Rotating black holes are constructed in magnetic Carroll gravity, including an intrinsically Carrollian dressed solution and a Kerroll black hole from an odd-power c-expansion of GR, with conserved charges computed.
-
The Fourth Geometry II: From Angle Axioms to Metric Foundations
Difference-angle geometry reconstructs parabolas via a focal function, derives a pseudo-inner product and Stewart theorem analog from it, defines associated trigonometric functions, and recovers the difference angle as the parabolic degeneration of the Cayley-Klein cross-ratio angle.