We present a complete calculation of radiative corrections to the inverse beta decay reaction, ${\overline{\nu }}_e+p\to e^{+}+n$, at reactor antineutrino energies using heavy-baryon chiral perturbation theory. Our analysis consistently incorporates quantum electrodynamics, chromodynamics, and electroweak contributions for the first time within this framework. We provide updated, high-precision cross-section predictions with a full error budget and present the positron energy spectrum, including radiative effects. The results are essential for normalizing the reactor antineutrino flux, determining neutrino oscillation parameters with sub-percent accuracy, and searching for new physics at nuclear power plants.