KOLOŠ, Martin and Zdeněk STUCHLÍK. Test of the string loop oscillation model using kHz quasiperiodic oscillations in a neutron star binary. General Relativity and Gravitation. US - Spojené státy americké, 2015, vol. 47, No 3, p. "27-1"-"27-23", 23 pp. ISSN 0001-7701. Available from: https://dx.doi.org/10.1007/s10714-015-1863-y.
Other formats:   BibTeX LaTeX RIS
Basic information
Original name Test of the string loop oscillation model using kHz quasiperiodic oscillations in a neutron star binary
Authors KOLOŠ, Martin and Zdeněk STUCHLÍK.
Edition General Relativity and Gravitation, US - Spojené státy americké, 2015, 0001-7701.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Confidentiality degree is not subject to a state or trade secret
WWW www
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1007/s10714-015-1863-y
UT WoS 000350690000011
Keywords in English XTE J1701-407; QPOs; string loop
Tags UF
Tags International impact, Reviewed
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 26/1/2021 17:37.
Abstract
The model of current-carrying string loop oscillations is tested to explain the special set of frequencies related to the high-frequency quasiperiodic oscillations (HF QPOs) observed recently in the low-mass X-ray binary XTE J1701-407 containing a neutron star. The external geometry of the neutron star is approximated by the Kerr geometry, introducing errors not exceeding 10% for slowly rotating massive neutron stars. The frequencies of the radial and vertical string loop oscillations are then governedby the mass M and dimensionless spin a of the neutron star, and by the dimensionless parameter omega describing combined effects of the string loop tension and its angular momentum. It is explicitly demonstrated that the string-loop oscillation model canexplain the observed kHz frequencies for the neutron star parameters restricted to the intervals 0.2 < a < 0.4 and 2.1 < M/M_{circle dot} < 2.5. However, the stringy parameter omega cannot be the same for all the three HF QPO observation
PrintDisplayed: 4/5/2024 04:29