About: Super-spinning compact objects and models of high-frequency quasi-periodic oscillations observed in Galactic microquasars     Goto   Sponge   NotDistinct   Permalink

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  • We have previously applied several models of high-frequency quasi-periodic oscillations (HF QPOs) to estimate the spin of the central Kerr black hole in the three Galactic microquasars, GRS 1915+105, GRO J1655-40, and XTE J1550-564. Here we explore the alternative possibility that the central compact body is a super-spinning object (or a naked singularity) with the external space-time described by Kerr geometry with a dimensionless spin parameter a \equiv cJ/GM^2 > 1. We calculate the relevant spin intervals for a subset of HF QPO models considered in the previous study. Our analysis indicates that for all but one of the considered models there exists at least one interval of a > 1 that is compatible with constraints given by the ranges of the central compact object mass independently estimated for the three sources. For most of the models, the inferred values of a are several times higher than the extreme Kerr black hole value a = 1. These values may be too high since the spin of superspinars is often assumed to rapidly decrease due to accretion when a \gg 1. In this context, we conclude that only the epicyclic and the Keplerian resonance model provides estimates that are compatible with the expectation of just a small deviation from a = 1.
  • We have previously applied several models of high-frequency quasi-periodic oscillations (HF QPOs) to estimate the spin of the central Kerr black hole in the three Galactic microquasars, GRS 1915+105, GRO J1655-40, and XTE J1550-564. Here we explore the alternative possibility that the central compact body is a super-spinning object (or a naked singularity) with the external space-time described by Kerr geometry with a dimensionless spin parameter a \equiv cJ/GM^2 > 1. We calculate the relevant spin intervals for a subset of HF QPO models considered in the previous study. Our analysis indicates that for all but one of the considered models there exists at least one interval of a > 1 that is compatible with constraints given by the ranges of the central compact object mass independently estimated for the three sources. For most of the models, the inferred values of a are several times higher than the extreme Kerr black hole value a = 1. These values may be too high since the spin of superspinars is often assumed to rapidly decrease due to accretion when a \gg 1. In this context, we conclude that only the epicyclic and the Keplerian resonance model provides estimates that are compatible with the expectation of just a small deviation from a = 1. (en)
Title
  • Super-spinning compact objects and models of high-frequency quasi-periodic oscillations observed in Galactic microquasars
  • Super-spinning compact objects and models of high-frequency quasi-periodic oscillations observed in Galactic microquasars (en)
skos:prefLabel
  • Super-spinning compact objects and models of high-frequency quasi-periodic oscillations observed in Galactic microquasars
  • Super-spinning compact objects and models of high-frequency quasi-periodic oscillations observed in Galactic microquasars (en)
skos:notation
  • RIV/47813059:19240/14:#0005073!RIV15-MSM-19240___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • I, P(GB14-37086G), P(GPP209/12/P740), S
http://linked.open...iv/cisloPeriodika
  • December
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
  • 48570
http://linked.open...ai/riv/idVysledku
  • RIV/47813059:19240/14:#0005073
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • X-rays: binaries; black hole physics; accretion, accretion disks (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • FR - Francouzská republika
http://linked.open...ontrolniKodProRIV
  • [07412F64E0D0]
http://linked.open...i/riv/nazevZdroje
  • Astronomy and Astrophysics
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...v/svazekPeriodika
  • 572
http://linked.open...iv/tvurceVysledku
  • Kotrlová, Andrea
  • Stuchlík, Zdeněk
  • Török, Gabriel
  • Šrámková, Eva
http://linked.open...ain/vavai/riv/wos
  • 000346101700099
issn
  • 0004-6361
number of pages
http://bibframe.org/vocab/doi
  • 10.1051/0004-6361/201424407
http://localhost/t...ganizacniJednotka
  • 19240
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