Comment on “Can accretion disk properties observationally distinguish black holes from naked singularities?”

Bertrand Chauvineau
Phys. Rev. D 98, 088501 – Published 16 October 2018

Abstract

One points out that a metric used as a General Relativity filled by a massless scalar φ solution in several studies, and that would have been a generalization of the Janis-Newman-Winicour spherical solution to the rotating case, does not solve the corresponding Einstein equation Rab=aφbφ. As a consequence, the (conformally related) Krori-Bhattacharjee spacetime is not a vacuum Brans-Dicke solution.

  • Received 7 May 2018

DOI:https://doi.org/10.1103/PhysRevD.98.088501

© 2018 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Bertrand Chauvineau*

  • Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange, 06 304 Nice, France

  • *Bertrand.Chauvineau@oca.eu

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Vol. 98, Iss. 8 — 15 October 2018

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