The Boltzmann Constant: Heat-Aether

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.