Perturbation in closed systems tends to amass the energy unavailable to do work. The capacity for equilibrium within this dynamic is likely radiational and not thermal or gravitational. Gravitational and thermal sinks of any polarity do not probably contribute to systemic field or boundary parameters. The variability in field conditions is itself the system tending towards equilibrium. Radiational free energy is most likely the ground state of this equilibrium, the spatial directionality of which is totally uncertain.

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