HLEDÍK, Stanislav and Zdeněk STUCHLÍK. Excitation of oscillations by a small inhomogeneity on the surface of a neutron star. In Proceedings of RAGtime 6/7: Workshops on black holes and neutron stars. Opava: Excitation of oscillations by a small inhomogeneity on the surface of a neutron star, 2005, p. 189-208, 19 pp. ISBN 80-7248-334-X.
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Basic information
Original name Excitation of oscillations by a small inhomogeneity on the surface of a neutron star
Authors HLEDÍK, Stanislav and Zdeněk STUCHLÍK.
Edition Opava, Proceedings of RAGtime 6/7: Workshops on black holes and neutron stars, p. 189-208, 19 pp. 2005.
Publisher Excitation of oscillations by a small inhomogeneity on the surface of a neutron star
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
Organization unit Faculty of Philosophy and Science in Opava
ISBN 80-7248-334-X
Keywords in English neutron star, oscillations, surface inhomogeneity
Tags , MSM4781305903, RAGtime, sbornik
Tags International impact
Links MSM4781305903, plan (intention).
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 8/12/2020 13:38.
Abstract
Properties of the gravitational perturbation force caused by a small inhomogeneity located on the surface of a neutron star are studied. The oscillating perturbation force in both the accretion disc rotating around the star and in the interior of a differentially rotating star is determined. Both vertical and radial components of the force are given and their relations are discussed. The frequency of the oscillations is given by the difference of the frequency of the rotation of the star surface, and the orbital frequency in the disc (the frequency of rotation of matter in the star interior). Outside the star, in the disc, the vertical and radial forces vary with the same phase. Inside a differentially rotating star, the variations of the forces are inthe opposite phase in an internal part of the star, while they are in the same phase in an external layer of the star. In an intermediate part of the star, an additional oscillatory change appears.
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