Conformable Fractional Models of the Stellar Helium Burning via Artificial Neural Networks

Figure 5

Convergence of the weights of input, bias, and output layers for the training of the NN used to simulate helium burning network. (a) The convergence of input layer weights (). (b) The convergence of bias (β_i). (c) Convergence of output layer weights ().

(a)

(b)

(c)