BRONNIKOV, Kirill A., Roman KONOPLYA and Thomas PAPPAS. General parametrization of wormhole spacetimes and its application to shadows and quasinormal modes. Physical Review D. College Park (USA): American Physical Society, 2021, vol. 103, No 2, p. "124062-1"-"124062-20", 20 pp. ISSN 2470-0010. Available from: https://dx.doi.org/10.1103/PhysRevD.103.124062.
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Basic information
Original name General parametrization of wormhole spacetimes and its application to shadows and quasinormal modes
Authors BRONNIKOV, Kirill A., Roman KONOPLYA (804 Ukraine, belonging to the institution) and Thomas PAPPAS (300 Greece, belonging to the institution).
Edition Physical Review D, College Park (USA), American Physical Society, 2021, 2470-0010.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher United States of America
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19630/21:A0000117
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.1103/PhysRevD.103.124062
UT WoS 000669042800009
Keywords in English black hole; shadow;quasinormal modes;wormhole background
Tags 2022, , GA19-03950S, RIV22
Tags International impact, Reviewed
Links GA19-03950S, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 23/2/2022 14:08.
Abstract
The general parametrization for spacetimes of spherically symmetric Lorentzian, traversable wormholes in an arbitrary metric theory of gravity is presented. The parametrization is similar in spirit to the post-Newtonian parametrized formalism, but with validity that extends beyond the weak field region and covers the whole space. Our method is based on a continued-fraction expansion in terms of a compactified radial coordinate. Calculations of shadows and quasinormal modes for various examples of parametrization of known wormhole metrics that we have performed show that, for most cases, the parametrization provides excellent accuracy already at the first order. Therefore, only a few parameters are dominant and important for finding potentially observable quantities in a wormhole background. We have also extended the analysis to the regime of slow rotation.
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