Photon emission in classical physics occurs when electrons transition between energy states, while in nuclear fusion, photons are produced during nuclear de-excitations rather than directly from neutron decay. Neutron decay involves a neutron transforming into a proton, emitting a W boson, which subsequently decays into an electron and an anti-neutrino, not a photon. The photons that eventually escape from stars like the Sun are generated through fusion reactions, involving numerous interactions that convert high-energy gamma photons into lower-energy optical frequencies. Understanding these processes requires careful study of reputable scientific sources rather than relying solely on videos. The discussion emphasizes the complexity of photon production in nuclear fusion and the importance of accurate scientific communication.