TY - JOUR
T1 - A new simple model for high-frequency quasi-periodic oscillations in black hole candidates
AU - Rezzolla, L.
AU - Yoshida, S'i
AU - Maccarone, T. J.
AU - Zanotti, O.
PY - 2003/9/21
Y1 - 2003/9/21
N2 - Observations of X-ray emissions from binary systems have long since been considered important tools to test general relativity in strong-field regimes. The high-frequency quasi-periodic oscillations (HFQPOs) observed in binaries containing a black hole candidate, in particular, have been proposed as a means to measure more directly the properties of the black hole, such as its mass and spin. Numerous models have been suggested to explain the HFQPOs and the rich phenomenology accompanying them. Many of these models rest on a number of assumptions and are at times in conflict with the most recent observations. We here propose a new, simple model in which the HFQPOs result from basic p-mode oscillations of a small accretion torus orbiting close to the black hole. We show that within this model the key properties of the HFQPOs can be explained simply, given a single reasonable assumption. We also discuss observational tests that can refute the model.
AB - Observations of X-ray emissions from binary systems have long since been considered important tools to test general relativity in strong-field regimes. The high-frequency quasi-periodic oscillations (HFQPOs) observed in binaries containing a black hole candidate, in particular, have been proposed as a means to measure more directly the properties of the black hole, such as its mass and spin. Numerous models have been suggested to explain the HFQPOs and the rich phenomenology accompanying them. Many of these models rest on a number of assumptions and are at times in conflict with the most recent observations. We here propose a new, simple model in which the HFQPOs result from basic p-mode oscillations of a small accretion torus orbiting close to the black hole. We show that within this model the key properties of the HFQPOs can be explained simply, given a single reasonable assumption. We also discuss observational tests that can refute the model.
KW - Accretion, accretion discs
KW - Relativity
KW - Stars: oscillations
KW - X-rays: binaries
UR - http://www.scopus.com/inward/record.url?scp=0142229935&partnerID=8YFLogxK
U2 - 10.1046/j.1365-8711.2003.07018.x
DO - 10.1046/j.1365-8711.2003.07018.x
M3 - Article
AN - SCOPUS:0142229935
VL - 344
SP - L37-L41
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
SN - 0035-8711
IS - 3
ER -