Note on the Optogeometric Interpretation of Black Hole Radiation

A new perspective on black hole physics is proposed by extending the concept of the optogeometric factor, originally introduced in radiometry and pixel-level imaging, to gravitational systems. The event horizon of a black hole is interpreted as an optogeometric sensor, whose spatial--angular throughput limits the number of accessible quantum modes. This yields a natural connection between Hawking radiation, black hole entropy, and the growth of horizon volume. It is hypothesized that quantum gravity is inherently tied to the optogeometric properties of space itself, rather than reducible to a particle-mediated interaction.