860 research outputs found
Slowly rotating black holes in the Einstein-Maxwell-scalar theory
We make the research on a slowly rotating black hole solution in a new
Einstein-Maxwell-scalar theory, which is an extension of the
Einstein-Maxwell-dilaton theory. The gyromagnetic ratio of this black hole is
calculated and it increases with the parameter , but decreases with the
parameter . In the Einstein-Maxwell-dilaton theory where the parameter
is in the absence, the gyromagnetic ratio is always less than , the
gyromagnetic ratio for Kerr-Newman black hole. Now we find that the standard
gyromagnetic ratio can also be realized in this Einstein-Maxwell-scalar
theory by increasing and simultaneously. The same value of
angular velocity of locally non-rotating observer as that in Kerr-Newman black
hole can also be obtained in the same way. We also investigated the correction
of period for circular orbits with respect to charge to mass ratio and the
correction of radius of innermost stable circular orbits. We find that the
correction becomes smaller and smaller with the increase of . It is also
shown that the radiative efficiency in the thin accretion disk model, for small
value of and large value of charge to mass ratio, the efficiency
vanishes due to lacking of the enough stress and dynamic friction in the
accretion model. A phantom Maxwell black hole is investigated in this theory as
an example of exact slowly rotating black hole solution. Therefore, formula for
angular velocity of the event horizon is shown. Correction of the radius of
innermost stable circular orbits and of radiative efficiency are investigated
subsequently. It is found that the correction up to first order of the
perturbation parameter can vanish for some value of charge-to-mass ratio. The
total radiative efficiency can also vanish once the effect of rotation is
considered.Comment: 27 figure
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