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gr-qc2026

: Hawking Radiation from Regular Black Holes

Alexandre Arbey, Marco Calzà, Léa Malacher +2

We present , a major update of the public code designed to compute Hawking radiation spectra of black holes. Building upon previous versions, this release…

gr-qc2025

Primordial regular black holes as all the dark matter. III. Covariant canonical quantum gravity models

Marco Calzà, Davide Pedrotti, Guan-Wen Yuan +1

In earlier companion papers, we showed that non-singular primordial black holes (PBHs) could account for all the dark matter (DM) over a significantly wider mass range compared to…

gr-qc2025

Trinity of black hole correspondences: Shadows, quasinormal modes, graybody factors, and cautionary remarks

Davide Pedrotti, Marco Calzà

Correspondences between apparently distant concepts are ubiquitous in theoretical physics. In the context of black holes (BHs), quasinormal modes (QNMs) were shown to be linked to…

gr-qc2024

Primordial regular black holes as all the dark matter. II. Non-time-radial-symmetric and loop quantum gravity-inspired metrics

Marco Calzà, Davide Pedrotti, Sunny Vagnozzi

It is a common belief that a theory of quantum gravity should ultimately cure curvature singularities which are inevitable within General Relativity, and plague for instance the Sc…

gr-qc2024

Primordial regular black holes as all the dark matter. I. Time-radial-symmetric metrics

Marco Calzà, Davide Pedrotti, Sunny Vagnozzi

Primordial black holes (PBHs) are usually assumed to be described by the Schwarzschild or Kerr metrics, which however feature unwelcome singularities. We study the possibility that…

gr-qc2024

Quasinormal modes-shadow correspondence for rotating regular black holes

Davide Pedrotti, Sunny Vagnozzi

Eikonal quasinormal modes (QNMs) of black holes (BHs) and parameters of null geodesics, ultimately tied to the appearance of BHs to external observers, are known to be related, and…