Gravitational Waves and the Early Universe: Accelerated Expansion, Dynamical Inhomogeneity, and Beyond

Maya Perez "Phase transitions of a noncommutative Reissner-Nordstrom Black Hole"

13 Mar 2026, 17:20

20m

ES635 (Kobayashi-Maskawa Institute for the Origin of Particles and the Universe (KMI), Nagoya University)

Description

The thermodynamic properties of a noncommutative Reissner–Nordström black hole (NCRN BH) are presented. The analysis is carried out using a Lorentzian source and the framework of Geometrothermodynamics (GTD), which provides a Legendre-invariant geometric description of thermodynamics and allows for a quasihomogeneous analysis. Within this formalism, phase transition curves are obtained from singularities of the Ricci scalar.