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gr-qc2025

Complexity hierarchies in Euclidean stars

L. Herrera, A. Di Prisco, J. Ospino

We establish a hierarchy of Euclidean stars according to their degree of complexity, as measured by the complexity factor and the complexity of the pattern of evolution. We conside…

gr-qc2025

The hyperbolically symmetric black hole

L. Herrera, L. Witten

We describe some properties of the hyperbolically symmetric black hole (hereafter referred to as the ) proposed a few years ago. We start by explaining the main motivation be…

gr-qc2025

Axially symmetric ghost stars

L. Herrera, J. L. Hernandez-Pastora, J. Ospino +1

We present static axially symmetric fluid distributions not producing gravitational field outside their boundaries (i.e. fluid sources which match smoothly on the boundary surface…

gr-qc2025

The birth of a ghost star

L. Herrera, A. Di Prisco, J. Ospino

We present a model of an evolving spherically symmetric dissipative self-gravitating fluid distribution which tends asymptotically to a ghost star, meaning that the end state of su…

gr-qc2024

Modified Landauer principle according to Tsallis entropy

L. Herrera

The Landauer principle establishes a lower bound in the amount of energy that should be dissipated in the erasure of one bit of information. The specific value of this dissipated e…

gr-qc2024

Evolution of self-gravitating fluid spheres involving ghost stars

L. Herrera, A. Di Prisco, J. Ospino

Exact solutions are presented which describe, either the evolution of fluid distributions corresponding to a ghost star (vanishing total mass), or describing the evolution of fluid…