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Saul
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The classical black hole is only one possible solution to what happens to massive bodies as they collapse.
Observational evidence does not support the assertion that the classical hairless BH exists. Quasar specialists have found Quasar structures and quasar morphological differences (what change is required to create a radio loud and a radio quiet quasar that require the massive object to have an intrinsic magnetic field that rotations with the massive object. A classical BH cannot have an intrinsic magnetic field.
The MECO's massive magnetic field exists with or with an accretion disks which explains why 10% of quasars are naked quasars. Naked quasars have no lines of absorption from a accretion disk or gas cloud. There are also naked quasars that emit that have no accompanying galaxy or dust cloud. The point is a classical BH requires a accretion disk to radiate. A rotating MECO does not. The massive magnetic field emits via synchronous radiation by electrons and protons that travel along the field lines.
This is a sample of the series of paper that have been published on this subject. I notice that is now a graduate course that now includes MECO's in their section on quasars.
The MECO object appears based on astronomical observations to not be static. Quasar magnitude pulsate with an asymptotically increasing pulse. As an object cannot increase in emission asymptotically forever it appears the increase leads some event which is then repeated.
The massive MECO object collapse is arrested by the magnetic field that is sufficiently strong to cause space to separate into electrons and positrons.
“The Magnetospheric Eternally Collapsing Object (MECO) Model of Galactic Black Hole Candidates and Active Galactic Nuclei”
http://arxiv.org/pdf/astro-ph/0602453
http://journalofcosmology.com/SchildLeiter1.pdf
Black Hole or MECO? Decided by a thin Luminous Ring Structure deep within Quasar Q0857+561
Tale of two Quasars
http://arxiv.org/PS_cache/arxiv/pdf/0708/0708.2422v1.pdf
http://iopscience.iop.org/1538-3881/135/3/947
Observational evidence does not support the assertion that the classical hairless BH exists. Quasar specialists have found Quasar structures and quasar morphological differences (what change is required to create a radio loud and a radio quiet quasar that require the massive object to have an intrinsic magnetic field that rotations with the massive object. A classical BH cannot have an intrinsic magnetic field.
The MECO's massive magnetic field exists with or with an accretion disks which explains why 10% of quasars are naked quasars. Naked quasars have no lines of absorption from a accretion disk or gas cloud. There are also naked quasars that emit that have no accompanying galaxy or dust cloud. The point is a classical BH requires a accretion disk to radiate. A rotating MECO does not. The massive magnetic field emits via synchronous radiation by electrons and protons that travel along the field lines.
This is a sample of the series of paper that have been published on this subject. I notice that is now a graduate course that now includes MECO's in their section on quasars.
The MECO object appears based on astronomical observations to not be static. Quasar magnitude pulsate with an asymptotically increasing pulse. As an object cannot increase in emission asymptotically forever it appears the increase leads some event which is then repeated.
The massive MECO object collapse is arrested by the magnetic field that is sufficiently strong to cause space to separate into electrons and positrons.
“The Magnetospheric Eternally Collapsing Object (MECO) Model of Galactic Black Hole Candidates and Active Galactic Nuclei”
http://arxiv.org/pdf/astro-ph/0602453
Although there are widely studied models for generating magnetic fields in accretion disks, they can produce equipartition fields at best [Livio, Ogilvie & Pringle 1999], and perhaps at the expense of being too luminous [Bisnovatyi-Kogan & Lovelace 2000] in quiescence and in any case, too weak and comoving in accretion disks to drive jets. While tangled magnetic fields in accretion disks are very likely responsible for their large viscosity, [e.g. Hawley, Balbus & Winters 1999] the highly variable mass accretion rates in LMXB make it unlikely that disk dynamos could produce the stability of fields needed to account for either spectral state switches or quiescent spin-down luminosities.
The spectral, timing, and jet formation properties of neutron stars in low mass x-ray binary systems are influenced by the presence of central magnetic moments. Similar features shown by the galactic black hole candidates (GBHC) strongly suggest that their compact cores might be intrinsically magnetic as well. We show that the existence of intrinsically magnetic GBHC is consistent with a new class of solutions of the Einstein field equations of General Relativity. These solutions are based on a strict adherence to the Strong Principle of Equivalence (SPOE) requirement that the world lines of physical matter must remain timelike in all regions of spacetime. The new solutions emerge when the structure and radiation transfer properties of the energy momentum tensor on the right hand side of the Einstein field equations are appropriately chosen to dynamically enforce this SPOE requirement of timelike world line completeness. In this context, we find that the Einstein field equations allow the existence of highly red shifted, Magnetospheric, Eternally Collapsing Objects (MECO). MECO necessarily possesses intrinsic magnetic moments and they do not have trapped surfaces that lead to event horizons and curvature singularities. Their most striking features are equipartition magnetic fields, pair plasma atmospheres and extreme gravitational redshifts.
http://journalofcosmology.com/SchildLeiter1.pdf
Black Hole or MECO? Decided by a thin Luminous Ring Structure deep within Quasar Q0857+561
Tale of two Quasars
http://arxiv.org/PS_cache/arxiv/pdf/0708/0708.2422v1.pdf
http://iopscience.iop.org/1538-3881/135/3/947
We show how direct microlensing-reverberation analysis performed on two well-known Quasars (Q2237 - The Einstein Cross and Q0957 - The Twin) can be used to observe the inner structure of two quasars which are in significantly different spectral states. These observations allow us to measure the detailed internal structure of quasar Q2237 in a radio quiet high-soft state, and compare it to quasar Q0957 in a radio loud low-hard state. We find that the observed differences in the spectral states of these two quasars can be understood as being due to the location of the inner radii of their accretion disks relative to the corotation radii of rotating intrinsically magnetic supermassive compact objects in the centers of these quasars.