KOLOŠ, Martin and Zdeněk STUCHLÍK. String loop oscillation model applied to the twin HF QPOs in the atoll source 4U 1636-53. In Proceedings of RAGtime 10-13: Workshops on black holes and neutron stars. Opava: Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky, 2014, p. 197-209. ISBN 978-80-7510-124-2.
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Basic information
Original name String loop oscillation model applied to the twin HF QPOs in the atoll source 4U 1636-53
Authors KOLOŠ, Martin and Zdeněk STUCHLÍK.
Edition Opava, Proceedings of RAGtime 10-13: Workshops on black holes and neutron stars, p. 197-209, 13 pp. 2014.
Publisher Slezská univerzita v Opavě, Filozoficko-přírodovědecká fakulta, Ústav fyziky
Other information
Original language English
Type of outcome Proceedings paper
Field of Study 10308 Astronomy
Confidentiality degree is not subject to a state or trade secret
Organization unit Faculty of Philosophy and Science in Opava
ISBN 978-80-7510-124-2
ISSN 2336-5668
Keywords in English string loop oscillations; X-ray variability; HF QPO observations
Tags RAGtime, UF
Tags International impact, Reviewed
Links EE2.3.20.0071, research and development project. GB14-37086G, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 26/1/2021 14:08.
Abstract
The current-carrying string loops oscillating around a stable equilibrium position in the Kerr background are considered to explain the twin high-frequency quasiperiodic oscillations (HF QPOs) observed in the low-mass X-ray binary 4U 1636-53 containing aneutron star. The frequencies of the radial and vertical string loop oscillations are governed by the mass and spin parameters of the neutron star, and by the string parameter describing combined effects of its tension and angular momentum. The frequencies of the radial and vertical modes of the string loop oscillations can cover the large scatter of the twin HF QPO data observed in the 4U 1636-53 source, but the estimates of the mass M and spin a of the neutron star are rather high, M 2:65 M and a 0:45, while related to the theory of the neutron star structure. Therefore, the string loop oscillation model in the case of the 4U 1636-53 source requires a correction based on an electrically charged string loop interacting with the magnet
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