A possible influence on standard model of quasars and active galactic nuclei in strong magnetic field
Qiu-He Peng, Jing-Jing Liu, and Chih-Kang Chou

TL;DR
This paper challenges the standard black hole model for the Galactic Center by proposing a super-massive stellar object with magnetic monopoles, explaining strong magnetic fields and radiation observations.
Contribution
It introduces a model replacing the black hole with a super-massive stellar object containing magnetic monopoles, addressing magnetic field and radiation anomalies.
Findings
Observed magnetic field strength exceeds dynamo mechanism predictions.
Radiation near Galactic Center cannot originate from accretion disk gas.
Model predicts magnetic monopoles as a natural explanation for observations.
Abstract
Recent observational evidence indicates that the center of our Milky Way harbours a super-massive object with ultra-strong radial magnetic field (Eatough et al., 2013). Here we demonstrate that the radiations observed in the vicinity of the Galactic Center (GC) (Falcke and Marko 2013) cannot be emitted by the gas of the accretion disk since the accreting plasma is prevented from approaching to the GC by the abnormally strong radial magnetic field. These fields obstruct the infalling accretion flow from the inner region of the disk and the central massive black hole in the standard model. It is expected that the observed radiations near the Galactic Center cannot be generated by the central black hole. We also demonstrate that the observed ultra-strong radial magnetic field near the Galactic Center ( Eatough et al., 2013) cannot be generated by the - turbulence dynamo mechanism of…
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