Table of Contents
The Boltzmann Constant is the ratio between Heat Particles and Aether Particles.
The Stefan-Boltzmann Constant (σ Heat-Aetherspace): The Power of Heat Radiation
The Stefan-Boltzmann constant is a macroscopic constant that describes how much thermal radiation (heat energy in the form of electromagnetic waves) is emitted by a hot object.
It is built from the Boltzmann constant and the Stefan-Boltzmann law states that the total energy radiated per unit surface area of a black body (a perfect emitter) is proportional to the fourth power of its absolute temperature:
P=σAT4P=σAT4
Where:
PP is the total power (energy per second) radiated.
AA is the surface area of the emitting object.
TT is the absolute temperature (in Kelvin).
σσ is the Stefan-Boltzmann constant.
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