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Radiative kinetics of mass-data stacking and magnetic steady-state relativistic stellar size plasmoid torus models as an alternative to the singularity

Radiative kinetics of mass-data stacking and magnetic steady-state relativistic stellar size plasmoid torus models as an alternative to the singularity Scott DeGirolamo
Princeton University Center For Advanced Studies, Astronomical Academy Of Sciences, University of California, Berkeley, Princeton AS 2021, 00-12 Princeton, New Jersey, Berkeley, California
s.degirolamo@cgpcsolutions.com
20 May 2021

ABSTRACT
I present the results of 3D, 2D, and 1D mass-data stacking simulations of relativistic dimensional limitations within a stellar remnant plasmoid torus, including the dynamical influence of the synchrotron of Hawking’s radiation process, the observation of singularity reduction in mass-data stacking and integrating the observable mass-data stacking emission signatures. The simulations are initiated with a single stellar mass space-time layer with a mass-data stack in sub dimensions. We achieve a steady-state connection with unrestricted outflows by means of open boundary conditions those allowing the replacement of singularity equations by space-time lightcurve mass-data stacking. the radiative cooling efficiency is regulated by the choice of initial plasma temperature Θ. We explore different values of Θ and of the background magnetism. throughout the simulations, plasmoid torus is generated in the central region of the stellar layer, and they evolve at different rates, achieving a wide range of sizes. The gaps between plasmoid torus are filled by smooth relativistic outflows called radiation minijets, whose contribution to the observed radiation is very limited due to their low particle densities. Small-sized stellar plasmoid torus and are rapidly accelerated, however, they have lower gravity contributions to the simulated mass-data construct, despite stronger relativistic tidal forces. Stellar-sized plasmoids are slow, but produce most of the observed synchrotron emission, with major part of their radiation produced within the central cores, the density of which is enhanced by radiative cooling and mass-data stacking and lower dimensions. Synchrotron space-time lightcurves show rapid bright flares that can be identified as originating from tail-on mergers between small/fast plasmoids and large/slow targets. Key words: stellar plasmoid torus acceleration of particles – stellar magnetic principles of stellar plasmoids – space-time data-stacking methods