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On the Mass Function at the Inner Horizon of a Regular Black Hole

  • NUCLEI, PARTICLES, FIELDS, GRAVITATION, AND ASTROPHYSICS
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Abstract

Calculations of the inner mass function of the Hayward regular black hole with fluxes are reviewed and rederived. We present detailed calculations of the inner mass function in two forms of the Ori approach (the ingoing flux is continuous, the outgoing flux is modeled by a thin null shell) and compare them with calculations in Reissner–Nordström black hole. A formal reason of different results is discussed. The energy density of scalar perturbations propagating from the event horizon into the Hayward black hole measured by a free falling observer near the inner horizon is calculated.

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Notes

  1. Note that in the system of units we use, the gravitational constant is included in the parameter m, which in this case has the dimension of length.

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ACKNOWLEDGMENTS

I thank M. Smolyakov and I. Volobuev for discussion and valuable comments. The research was carried out within the framework of the scientific program of the National Center for Physics and Mathematics, the project “Particle Physics and Cosmology.”

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  1. Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, 119991, Moscow, Russia

    M. Z. Iofa

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  1. M. Z. Iofa
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Iofa, M.Z. On the Mass Function at the Inner Horizon of a Regular Black Hole. J. Exp. Theor. Phys. 135, 647–654 (2022). https://doi.org/10.1134/S1063776122110048

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