The spacetime singularity resolution of Schwarichild-de Sitter black hole in loop quantum gravity

By using the analog variable of the holonomy variable of loop quantum gravity and the corresponding quantization method, the gravity field near the center of the Schwarichild de Sitter black hole is processed though quantization. The spectrums of 1/r and the curvature invariant are computed near the black hole center and the result that the both spectrums is bounded from above are obtained. Following the above quantization method and by computing the quantum Hamiltonian constraint equation of the gravity field near the classical singularity r = 0, the evolution formula of the black hole wave function is obtained and the result that the wave function can evolve though the classical singularity is obtained.