Zajacek, Michal ORCID: 0000-0001-6450-1187, Tursunov, Arman, Eckart, Andreas and Britzen, Silke (2018). On the charge of the Galactic centre black hole. Mon. Not. Roy. Astron. Soc., 480 (4). S. 4408 - 4424. OXFORD: OXFORD UNIV PRESS. ISSN 1365-2966

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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 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.

Item Type: Journal Article
Creators:
CreatorsEmailORCIDORCID Put Code
Zajacek, MichalUNSPECIFIEDorcid.org/0000-0001-6450-1187UNSPECIFIED
Tursunov, ArmanUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Eckart, AndreasUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Britzen, SilkeUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
URN: urn:nbn:de:hbz:38-167183
DOI: 10.1093/mnras/sty2182
Journal or Publication Title: Mon. Not. Roy. Astron. Soc.
Volume: 480
Number: 4
Page Range: S. 4408 - 4424
Date: 2018
Publisher: OXFORD UNIV PRESS
Place of Publication: OXFORD
ISSN: 1365-2966
Language: English
Faculty: Faculty of Mathematics and Natural Sciences
Divisions: Faculty of Mathematics and Natural Sciences > Department of Physics > Institute of Physics I
Subjects: no entry
Uncontrolled Keywords:
KeywordsLanguage
SGR-A-ASTERISK; STELLAR PROPER MOTIONS; ACCRETION; MODEL; POLARIMETRY; FLARES; FIELD; MILKY; SIZE; MASSMultiple languages
Astronomy & AstrophysicsMultiple languages
Refereed: Yes
URI: http://kups.ub.uni-koeln.de/id/eprint/16718

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