Black hole equations are quasi-homogeneous, enabling Legendre-invariant metrics in geometrothermodynamics whose curvature singularities correspond directly to phase transitions identified by heat capacity divergences.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
gr-qc 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Quasi-homogeneous black hole geometrothermodynamics in Einstein-Maxwell theory
Black hole equations are quasi-homogeneous, enabling Legendre-invariant metrics in geometrothermodynamics whose curvature singularities correspond directly to phase transitions identified by heat capacity divergences.