Do Black Hole Candidates Exhibit Magnetic Moments Instead of Event Horizons?

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Observational evidence supports the existence of intrinsically magnetized central objects in galactic black hole candidates (GBHC) [Robertson and Leiter, ApJ, v565, pg 447, (2002)]. This has been shown to be consistent with a new class of solutions of the Einstein field equations of General Relativity [Leiter and Robertson, Found. Phys. Lett. v16 , No.2 , pg 143, (2003)], [Robertson and Leiter, ApJ, v596, L203, (2003)] which describe highly red shifted, magnetospheric, eternally collapsing objects (MECO) that do not have trapped surfaces leading to event horizons. The MECO solutions emerge from the requirement that the physical structure and radiation transfer properties of the energy-momentum tensor on the right hand side of the Einstein field equations be dynamically chosen so as to always satisfy the Strong Principle of Equivalence requirement of timelike worldline completeness. Since the highly redshifted (MECO) have lifetimes many orders of magnitude greater than a Hubble time they can be shown (see the following talk by Stanley Robertson in this session) to represent an elegant and unified framework which can describe the broad range of observations associated with GBHC and active galactic nuclei AGN .

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