Accelerating electrons in synchrotrons emit significant X-rays due to their relativistic Lorentz factor, which increases the emission power dramatically compared to protons in cyclotrons. While protons also emit synchrotron radiation, the power is much lower, making it less significant at equivalent energies. In high-energy environments like the LHC, proton synchrotron radiation can lead to issues such as vacuum pressure rises due to desorption of gas atoms from beam tube walls. This phenomenon can result in proton residual gas scattering and subsequent beam loss. Understanding the differences in radiation emission between electrons and protons is crucial for optimizing particle accelerator performance.