2018
On the charge of the Galactic centre black hole
ZAJAČEK, Michal, Arman TURSUNOV, Andreas ECKART and Silke BRITZENBasic information
Original name
On the charge of the Galactic centre black hole
Authors
ZAJAČEK, Michal (703 Slovakia), Arman TURSUNOV (860 Uzbekistan, guarantor, belonging to the institution), Andreas ECKART (276 Germany) and Silke BRITZEN (276 Germany)
Edition
Monthly Notices of the Royal Astronomical Society, 2018, 0035-8711
Other information
Language
English
Type of outcome
Article in a journal
Field of Study
10308 Astronomy
Country of publisher
United Kingdom of Great Britain and Northern Ireland
Confidentiality degree
is not subject to a state or trade secret
References:
Impact factor
Impact factor: 5.231
RIV identification code
RIV/47813059:19240/18:A0000244
Organization unit
Faculty of Philosophy and Science in Opava
UT WoS
000449617100011
Keywords in English
Galaxy: centre; black hole physics; radiation mechanisms: general
Tags
International impact, Reviewed
Links
GJ16-03564Y, research and development project.
Changed: 23/4/2020 14:07, RNDr. Arman Tursunov, Ph.D.
Abstract
V originále
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 SMBII charge and put realistic limits on its value, time-scales of charging and discharging, and observable consequences of the potential, small charge associated with the Galactic centre black hole. The electric charge due to classical arguments based on the mass difference between protons and electrons is less than or similar to 10^9 C and is of a transient nature on the viscous time-scale. However, the rotation of a black hole in magnetic field generates electric field due to the twisting of magnetic field lines. This electric field can be associated with induced charge, for which we estimate an upper limit of less than or similar to 10^{15} C. Moreover, this charge is most likely positive due to an expected alignment between the magnetic field and the black hole spin. Even a small charge of this order significantly shifts the position of the innermost stable circular orbit (ISCO) of charged particles. In addition, we propose a novel observational test based on the presence of the bremsstrahlung surface brightness decrease, which is more sensitive for smaller unshielded electric charges than the black hole shadow size. Based on this test, the current upper observational limit on the charge of Sgr A* is less than or similar to 3 x 10^8 C.