TAPIR Seminar

An Experiment to Demonstrate an alpha-omega Dynamo in the Accretion Disk leading to Galaxy and MBH formation

Stirling Colgate, Los Alamos National Lab,

The largest concentrations of free energy in the universe are the radio lobes associated with the central galactic black hole formation, ~10e62 ergs of B2/8¿, ~ 10% of MBH c2.
How do we get to a 108 Msolar BH and a Flat Rotation curve galaxy with a MBH at its exact, 10-3 of rotation radius, center, and the free energy in magnetic fields. This may mean that 10e5 Msolar of low energy (~few mev) neutrinos are emitted in the process. Could we detect them with Gadzooks? How do Baryons do this in a dark matter potential? (Turbulence inhibits a dynamo, which must have coherence and phase information (Cattaneo and Tobias) in Baryon-dominated hydrodynamics. The proof is in an experiment.

Event Sponsors:

Theoretical AstroPhysics Including Relativity and Cosmology (TAPIR) - More events from this Sponsor

For more information, please contact JoAnn Boyd by phone at 4280 or by email at [email protected].