About: String loop oscillation model applied to the twin HF QPOs in the atoll source 4U 1636-53     Goto   Sponge   NotDistinct   Permalink

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  • 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 a neutron 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 magnetic field of the neutron star.
  • 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 a neutron 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 magnetic field of the neutron star. (en)
Title
  • String loop oscillation model applied to the twin HF QPOs in the atoll source 4U 1636-53
  • String loop oscillation model applied to the twin HF QPOs in the atoll source 4U 1636-53 (en)
skos:prefLabel
  • String loop oscillation model applied to the twin HF QPOs in the atoll source 4U 1636-53
  • String loop oscillation model applied to the twin HF QPOs in the atoll source 4U 1636-53 (en)
skos:notation
  • RIV/47813059:19240/14:#0005103!RIV15-MSM-19240___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • I, P(EE2.3.20.0071), P(GB14-37086G), S
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 47765
http://linked.open...ai/riv/idVysledku
  • RIV/47813059:19240/14:#0005103
http://linked.open...riv/jazykVysledku
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  • string loop oscillations; X-ray variability; HF QPO observations (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...ontrolniKodProRIV
  • [64FD753B4A23]
http://linked.open...v/mistoKonaniAkce
  • Opava, Czech Republic
http://linked.open...i/riv/mistoVydani
  • Opava
http://linked.open...i/riv/nazevZdroje
  • Proceedings of RAGtime 10-13: Workshops on black holes and neutron stars
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...iv/tvurceVysledku
  • Stuchlík, Zdeněk
  • Kološ, Martin
http://linked.open...vavai/riv/typAkce
http://linked.open.../riv/zahajeniAkce
issn
  • 2336-5668
number of pages
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  • Slezská univerzita v Opavě
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  • 978-80-7510-124-2
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  • 19240
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