law of black-body radiation

The law of black-body radiation describes how an idealized object emits electromagnetic radiation with an intensity and spectrum that depend solely on its temperature, as quantified by Planck’s radiation formula.

Observed surface forms (3)

• blackbody radiation ×1
• classical limit of Planck’s law ×1
• radiation law ×1

Instances (5)

• Hawking radiation via concept surface "blackbody radiation"
• Rayleigh–Jeans law at low frequencies via concept surface "classical limit of Planck’s law"
• Wien displacement law
• Stefan–Boltzmann law via concept surface "radiation law"
• Planck radiation law