The Kaver Horizon Equation: A Phenomenological Model for Quantum Energy Attenuation Near Gravitational Horizons

This work introduces the Kaver Horizon Equation, a phenomenological relation intended to explore possible interactions between quantum energy scales and gravitational horizons. The proposed framework suggests an exponential attenuation mechanism associated with Schwarzschild horizons and discusses its conceptual implications within quantum field theory in curved spacetime, black hole thermodynamics, and strong gravitational environments. The relation is presented as a preliminary phenomenological and heuristic framework intended for future theoretical development and analysis. (A revised and expanded version of this work is currently under development, with ongoing efforts focused on improving the theoretical consistency, mathematical formulation, and physical interpretation of the proposed framework).