Observations of Cygnus X-3 Binary and Challenges to the Conventional Black Hole Model

Cygnus X-3 is a high energy X ray binary in the Milky Way. Observations confirm that this binary system maintains stable orbits for a long time and does not undergo rapid inspiral and merger. The conventional black hole model adopts a Schwarzschild radius of 30 km and an equivalent dynamical mass of ten solar masses. When these parameters are combined with classical gravitational laws, the theory predicts a fast gravitational merger of the close binary, which conflicts with long term observational facts and reveals internal inconsistency within the traditional singularity black hole framework. This paper does not revise the mass parameters of the conventional model, recalculate gravitational strength, or set quantitative corrections. It only presents the observational contradictions inherent in the existing theory. Based on the Photon Origin Theory, a three layered spherical structure of black holes is constructed. The formation mechanism of high energy gamma ray photons inside a black hole, their penetration through successive layers, and the escape path of 30 PeV ultra high energy gamma photons are clearly illustrated. A new physical explanation is provided for the periodic high energy radiation detected from Cygnus X-3.