WHAT IS PLANCK'S RADIATION LAW? WHNERE THE VIDEOS FOR IT? PLZ EXPALIN

I would like to mention that Planck’s radiation law and Planck’s quantum theory are different and incase you still want information precisely on Plank's radiation law here is it and i am also sending you the link of our web page where you would find all the relevant details of Plank's quantum theory/Einstein plank photoelectric effect: 

Plank's radiation law a mathematical relationship formulated in 1900 by German physicist Max Planck to explain the spectral-energy distribution of radiation emitted by a blackbody (a hypothetical body that completely absorbs all radiant energy falling upon it, reaches some equilibrium temperature, and then re emits that energy as quickly as it absorbs it). Planck assumed that the sources of radiation are atoms in a state of oscillation and that the vibrational energy of each oscillator may have any of a series of discrete values but never any value between. Planck further assumed that when an oscillator changes from a state of energy E1 to a state of lower energy E2, the discrete amount of energy E1E2, or quantum of radiation, is equal to the product of the frequency of the radiation, symbolized by the Greek letter ν and a constant h, now called Planck’s constant, that he determined from blackbody radiation data; i.e., E1E2 = hν.

Planck’s law for the energy Eλ radiated per unit volume by a cavity of a blackbody in the wavelength interval λ to λ + Δλ (Δλ denotes an increment of wavelength) can be written in terms of Planck’s constant (h), the speed of light (c), the Boltzmann constant (k), and the absolute temperature (T):

The wavelength of the emitted radiation is inversely proportional to its frequency, or λ = c/ν. The value of Planck’s constant is found to be 6.62606957 × 10−34 joule∙second, with a standard uncertainty of 0.00000029 × 10−34 joule∙second.

For a blackbody at temperatures up to several hundred degrees, the majority of the radiation is in the infrared radiation region of the electromagnetic spectrum. At higher temperatures, the total radiated energy increases, and the intensity peak of the emitted spectrum shifts to shorter wavelengths so that a significant portion is radiated as visible light....

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The behavior of blackbody radiation is described by the Planck Law, but we can derive from the Planck Law two other radiation laws that are very useful, these are Wien Displacement Law, and the Stefan-Boltzmann Law.

The hotter an object is, the shorter the wavelength at which it will emit most of its radiation, and, further, that the wavelength for maximum or peak radiation power is found by dividing Wien's constant by the temperature in Kelvins. This relationship can be seen in the graphs below. The peak of each curve moves to the left.

Black body thermal emission intensity as a function of wavelength for various (absolute) temperatures.

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