VRBA, Jaroslav, Martin URBANEC and Zdeněk STUCHLÍK. Escape cones of null-geodesics from the interior of rotating compact stars. In Z. Stuchlík, G. Török a V. Karas. Proceedings of RAGtime 17–19: Workshops on black holes and neutron stars, 17–19/23–26 Oct., 1–5 Nov. 2015/2016/2017, Opava, Czech Republic. 1st ed. Opava (Česká republika): Slezská univerzita v Opavě, Filozoficko–přírodovědecká fakulta v Opavě, Ústav fyziky, 2017, p. 223-235. ISBN 978-80-7510-256-0.
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Basic information
Original name Escape cones of null-geodesics from the interior of rotating compact stars
Authors VRBA, Jaroslav (203 Czech Republic, guarantor, belonging to the institution), Martin URBANEC (203 Czech Republic, belonging to the institution) and Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution).
Edition 1. vyd. Opava (Česká republika), Proceedings of RAGtime 17–19: Workshops on black holes and neutron stars, 17–19/23–26 Oct., 1–5 Nov. 2015/2016/2017, Opava, Czech Republic, p. 223-235, 13 pp. 2017.
Publisher Slezská univerzita v Opavě, Filozoficko–přírodovědecká fakulta v Opavě, Ústav fyziky
Other information
Original language English
Type of outcome Proceedings paper
Field of Study 10308 Astronomy
Country of publisher Czech Republic
Confidentiality degree is not subject to a state or trade secret
Publication form printed version "print"
WWW RAGtime 17-19
RIV identification code RIV/47813059:19240/17:A0000036
Organization Filozoficko-přírodovědecká fakulta – Slezská univerzita v Opavě – Repository
ISBN 978-80-7510-256-0
ISSN 2336-5668
Keywords in English compact object; axially symmetric spacetime; trapped null-geodesic; effective potential; escape cone
Tags ASTROCOMP, CTP, GA17-16287S, GB14-37086G, RAGtime 17-19, SGS-15-2016, ÚF
Tags International impact, Reviewed
Links GA17-16287S, research and development project. GB14-37086G, research and development project.
Changed by Changed by: Jan Hladík, učo 1305. Changed: 6/4/2018 08:55.
Abstract
In this work we present investigation of the escape cones of null-geodesics from the interior of rotating homogeneous compact stars in the model, where only terms linear in the star’s rotational frequency are assumed. We focus on the single model of the star with particular radius R = 2.8M (using units in which c = G = 1) rotating with different values of angular momentum J. We vary the position of the isotropically radiating source both in radial and latitudinal direction and we show the impact of the position and the rotational rate on the shape of the escape cone of null-geodesics. We find that even for small rotational rate corresponding to j = J/M^2 = 0.1 the impact on the escape cones is rather strong. The escape cones are no longer symmetrical around radial direction, and it is clearly seen that the radiation in the direction of the rotation can easily reach the infinity. On the other hand, the radiation in the direction opposite to the rotation will be trapped in the interior of the star. We discuss possible astrophysical relevance of our results.
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