2018
DOI: 10.1093/mnras/sty2182
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On the charge of the Galactic centre black hole

Abstract: The Galactic centre supermassive black hole (SMBH), in sharp contrast with its complex environment, is characterized by only three classical parameters -mass, spin, and electric charge. Its charge is poorly constrained. It is, however, usually assumed to be zero because of neutralization due to the presence of plasma. We revisit the question of the SMBH charge and put realistic limits on its value, timescales of charging and discharging, and observable consequences of the potential, small charge associated wit… Show more

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Cited by 132 publications
(110 citation statements)
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References 77 publications
(136 reference statements)
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“…Thus, the assumption of the Kerr hypothesis is well founded. However, it would turn out, as we show below, that black hole charge would play crucial role in making energy extraction process ultra-efficient, so much so that efficiency could range over 10 10 . In the next section, we describe the black hole charging mechanisms in astrophysical context and discuss its possible screening by surrounding plasma.…”
Section: Introductionmentioning
confidence: 90%
See 1 more Smart Citation
“…Thus, the assumption of the Kerr hypothesis is well founded. However, it would turn out, as we show below, that black hole charge would play crucial role in making energy extraction process ultra-efficient, so much so that efficiency could range over 10 10 . In the next section, we describe the black hole charging mechanisms in astrophysical context and discuss its possible screening by surrounding plasma.…”
Section: Introductionmentioning
confidence: 90%
“…Maximal theoretical value of the charge of a black hole of mass M is given by Q = 2G 1/2 M, written in Gaussian units. For spinning black hole, it is of order [10]…”
Section: Black Hole Chargementioning
confidence: 99%
“…On the other hand, the characterstic ordered charge oscillations of the plasma (plasma frequency) and cyclotron motions take place on much shorter timescales than the viscous or free-fall timescale. For details, see the analysis presented in [43].…”
Section: Theoretical Constraints On the Charge Of Sgr A*mentioning
confidence: 99%
“…(15), one to an orthonormal vector spanned by ∂/∂r, i.e., the vector defined in Eq. (20), R µ stat , and two normal vectors spanned by ∂/∂ϕ and ∂/∂θ, Φ µ and Θ µ . By suitably choosing an orientation of the coordinate system, a null geodesic is of the form…”
Section: The "Dark Shell" Phenomenonmentioning
confidence: 99%