The equation of state (EOS) of radiation, specifically for a photon gas, is established as P = 1/3 * energy density due to the isotropic pressure derived from momentum components. This factor of 1/3 arises from the relationship between pressure and energy density in a photon gas, where the average momentum contributes equally across three spatial dimensions. The EM stress tensor for radiation is traceless, leading to the identity for a perfect fluid, which confirms the isotropic nature of pressure in such a gas. Discussions also highlight the need for a detailed derivation of the energy-momentum tensor for radiation, which can be found in general relativity textbooks. Understanding these principles is crucial for analyzing the behavior of radiation around black holes.