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@article{29864,
author = {Kološ, Martin and Tursunov, Arman and Stuchlík, Zdeněk},
article_number = {12},
doi = {http://dx.doi.org/10.1140/epjc/s10052-017-5431-3},
keywords = {X-ray binaries; black-hole binaries; Lens-Thirring precession; high-frequency QPOs; GRO J1655-40; naked singularities; charged-particles; large-scale; mass; model},
language = {eng},
issn = {1434-6044},
journal = {European Physical Journal C},
title = {Possible signature of the magnetic fields related to quasi-periodic oscillations observed in microquasars},
url = {https://link.springer.com/article/10.1140%2Fepjc%2Fs10052-017-5431-3},
volume = {77},
year = {2017}
}
TY - JOUR
ID - 29864
AU - Kološ, Martin - Tursunov, Arman - Stuchlík, Zdeněk
PY - 2017
TI - Possible signature of the magnetic fields related to quasi-periodic oscillations observed in microquasars
JF - European Physical Journal C
VL - 77
IS - 12
SP - „860-1“-„860-17“
EP - „860-1“-„860-17“
SN - 14346044
KW - X-ray binaries
KW - black-hole binaries
KW - Lens-Thirring precession
KW - high-frequency QPOs
KW - GRO J1655-40
KW - naked singularities
KW - charged-particles
KW - large-scale
KW - mass
KW - model
UR - https://link.springer.com/article/10.1140%2Fepjc%2Fs10052-017-5431-3
L2 - https://link.springer.com/article/10.1140%2Fepjc%2Fs10052-017-5431-3
N2 - The study of quasi-periodic oscillations (QPOs) of X-ray flux observed in the stellar-mass black hole binaries can provide a powerful tool for testing of the phenomena occurring in the strong gravity regime. Magnetized versions of the standard geodesic models of QPOs can explain the observationally fixed data from the three microquasars. We perform a successful fitting of the HF QPOs observed for three microquasars, GRS 1915+105, XTE 1550-564 and GRO 1655-40, containing black holes, for magnetized versions of both epicyclic resonance and relativistic precession models and discuss the corresponding constraints of parameters of the model, which are the mass and spin of the black hole and the parameter related to the external magnetic field. The estimated magnetic field intensity strongly depends on the type of objects giving the observed HF QPOs. It can be as small as 10^(-5) G if electron oscillatory motion is relevant, but it can be by many orders higher for protons or ions (0.02-1 G), or even higher for charged dust or such exotic objects as lighting balls, etc. On the other hand, if we know by any means the magnetic field intensity, our model implies strong limit on the character of the oscillating matter, namely its specific charge.
ER -
KOLOŠ, Martin, Arman TURSUNOV and Zdeněk STUCHLÍK. Possible signature of the magnetic fields related to quasi-periodic oscillations observed in microquasars. \textit{European Physical Journal C}. 2017, vol.~77, No~12, p.~„860-1“-„860-17“, 17 pp. ISSN~1434-6044. Available from: https://dx.doi.org/10.1140/epjc/s10052-017-5431-3.
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