Given the non-graph-changing Hamiltonian H[N ] in Loop Quantum Gravity (LQG), H[N ] , the coherent state expectation value of H[N ], admits an semiclassical expansion in 2 p . In this paper, as presenting the detailed derivations of our previous work [1], we explicitly compute the expansion of H[N ] to the linear order in 2 p on the cubic graph with respect to the coherent state peaked at the homogeneous and isotropic data of cosmology. In our computation, a powerful algorithm is developed, supported by rigorous proofs and several theorems, to overcome the complexity in the computation of H[N ] . Particularly, some key innovations in our algorithm substantially reduce the complexity in computing the Lorentzian part of H[N ] . Additionally, some quantum correction effects resulted from H[N ] in cosmology are discussed at the end of this paper.