Motion of test particles in quasi anti-de Sitter regular black holes

Author:

Corona Dario1ORCID,Giambò Roberto123ORCID,Luongo Orlando12456ORCID

Affiliation:

1. School of Science and Technology, University of Camerino, Via Madonna delle Carceri, Camerino 62032, Italy

2. Istituto Nazionale di Fisica Nucleare, INFN, Sezione di Perugia, Perugia 06123, Italy

3. IAPS, INAF — Tor Vergata, Roma 00133, Italy

4. SUNY Polytechnic Institute, Utica 13502, NY, USA

5. INAF — Osservatorio Astronomico di Brera, Milano 20121, Italy

6. Al-Farabi University, Al-Farabi, 71, Almaty 050040, Kazakhstan

Abstract

In this paper, we explore the characteristics of two novel regular spacetimes that exhibit a nonzero vacuum energy term, under the form of a (quasi) anti-de Sitter phase. Specifically, the first metric is spherical, while the second, derived by applying the generalized Newman–Janis algorithm to the first, is axisymmetric. We show that the equations of state of the effective fluids associated with the two metrics asymptotically tend to negative values, resembling quintessence. In addition, we study test particle motions, illustrating the main discrepancies among our models and more conventional metrics exhibiting non-vanishing anti-de Sitter phase.

Funder

Italian National Institute of High Mathematics

Ministry of Education and Science of the Republic of Kazakhstan

Publisher

World Scientific Pub Co Pte Ltd

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