The spectral distribution of blackbody radiation, also known as the blackbody spectrum, describes the intensity of radiation emitted by a blackbody at different wavelengths or frequencies. A blackbody is an idealized object that absorbs all incident radiation and emits radiation across the entire electromagnetic spectrum.

The spectral distribution of blackbody radiation is characterized by several important features:

- Planck’s Law: The spectral distribution of blackbody radiation is described by Planck’s law, formulated by physicist Max Planck in 1900. Planck’s law provides the mathematical expression for the intensity of blackbody radiation as a function of wavelength or frequency.
- Shape of the Spectrum: The blackbody spectrum is continuous and exhibits a characteristic shape that depends on temperature. At higher temperatures, the spectrum shifts towards shorter wavelengths and higher frequencies, resulting in a more pronounced intensity at higher energies. The shape of the spectrum is bell-shaped and has a peak at a particular wavelength or frequency.
- Wien’s Displacement Law: Wien’s displacement law states that the wavelength at which the blackbody spectrum reaches its peak intensity is inversely proportional to the absolute temperature of the blackbody. Mathematically, this relationship can be expressed as λ_max * T = constant, where λ_max is the wavelength of maximum intensity and T is the temperature.
- Stefan-Boltzmann Law: The total radiant power emitted by a blackbody is given by the Stefan-Boltzmann law. It states that the total power emitted per unit surface area is proportional to the fourth power of the temperature. The law is represented by the equation P = σ * A * T^4, where P is the power, A is the surface area, T is the temperature, and σ is the Stefan-Boltzmann constant.

The spectral distribution of blackbody radiation has profound implications in several areas of physics, such as astrophysics, cosmology, and quantum mechanics. It provides a fundamental basis for understanding the behavior of thermal radiation and the interaction of matter with electromagnetic waves. The blackbody spectrum is directly related to the temperature of the emitting object, allowing scientists to determine the temperature of celestial bodies, study the early universe, and explore the quantum nature of electromagnetic radiation.

Experimental measurements of blackbody radiation closely match the predictions of Planck’s law, confirming its validity and the existence of discrete energy levels associated with electromagnetic radiation. The study of blackbody radiation has played a pivotal role in the development of quantum mechanics and the understanding of fundamental concepts like quantization of energy and the wave-particle duality of light.