VRBA, Jaroslav, Martin URBANEC, Zdeněk STUCHLÍK and John MILLER. Trapping of null geodesics in slowly rotating spacetimes. European Physical Journal C. 2020, vol. 80, No 11, p. "1065-1"-"1065-20", 20 pp. ISSN 1434-6044. Available from: https://dx.doi.org/10.1140/epjc/s10052-020-08642-z.
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Basic information
Original name Trapping of null geodesics in slowly rotating spacetimes
Authors VRBA, Jaroslav (203 Czech Republic, belonging to the institution), Martin URBANEC (203 Czech Republic, belonging to the institution), Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution) and John MILLER (826 United Kingdom of Great Britain and Northern Ireland).
Edition European Physical Journal C, 2020, 1434-6044.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10303 Particles and field physics
Country of publisher United States of America
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19630/20:A0000058
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.1140/epjc/s10052-020-08642-z
UT WoS 000595358600007
Keywords in English NEUTRON-STARS; DENSITY
Tags , FÚ2020, LTC18058, RIV21
Tags International impact, Reviewed
Links LTC18058, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 23/3/2021 22:12.
Abstract
Extremely compact objects containing a region of trapped null geodesics could be of astrophysical relevance due to trapping of neutrinos with consequent impact on cooling processes or trapping of gravitational waves. These objects have previously been studied under the assumption of spherical symmetry. In the present paper, we consider a simple generalization by studying trapping of null geodesics in the framework of the Hartle-Thorne slow-rotation approximation taken to first order in the angular velocity, and considering a uniform-density object with uniform emissivity for the null geodesics. We calculate effective potentials and escape cones for the null geodesics and how they depend on the parameters of the spacetimes, and also calculate the "local" and "global" coefficients of efficiency for the trapping. We demonstrate that due to the rotation the trapping efficiency is different for co-rotating and retrograde null geodesics, and that trapping can occur even for R>3GM/c2, contrary to what happens in the absence of rotation.
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