For nearly a century, the incompatibility between General Relativity (GR) and Quantum Mechanics (QM) has persisted due to the absence of a unified theoretical framework that seamlessly integrates both. GR describes gravity as the curvature of spacetime—a smooth, continuous fabric—while QM operates on principles of quantization and uncertainty, governing interactions at atomic and subatomic scales.

The challenge lies in reconciling these fundamentally different descriptions: GR breaks down under extreme conditions such as singularities, where quantum effects dominate, while QM lacks a mechanism to incorporate the dynamic geometry of spacetime.

A successful unification would require either quantizing gravity, modifying the structure of spacetime at quantum scales, or deriving both GR and QM from a deeper underlying theory.

This theoretical tension has also shaped the way we interpret astrophysical phenomena. A recent experiment involving a curved smoke layer illustrates how a spatially varying refractive index can bend and subtly magnify light, mimicking the effects of gravitational lensing. This raises an intriguing question: To what extent might refractive index gradients — such as those found in the Sun’s chromosphere — contribute to the observed bending of starlight?

If both gravitational curvature and optical refraction influence light deflection in celestial observations, the implications could be profound. It may reshape our understanding of mass distributions in the universe, offer alternative explanations for quasar anomalies, and challenge conventional models of dark matter. Exploring the interplay between gravitational and optical effects could open new avenues for refining cosmological models and deepening our understanding of the fundamental nature of space and light.

Please see at:

https://www.ej-physics.org/index.php/ejphysics/article/view/374/421

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