The amount of radiation emitted by a perfectly black body is proportional to

Question

The amount of radiation emitted by a perfectly black body is proportional to (A) temperature oh ideal gas scale (B) fourth root of temperature on ideal gas scale (C) fourth power of temperature on ideal gas scale (D) square of temperature on ideal gas scale

Tardigrade Admin · Accepted Answer

According to the Stefan’s law the radiant energy emitted by a perfectly black body per unit area per second is directly proportional to the fourth power of its absolute temperature

R \propto T^{4}

or

R = σ T^{4}

where

σ

is a Stefan’s constant

Q. The amount of radiation emitted by a perfectly black body is proportional to

temperature oh ideal gas scale

fourth root of temperature on ideal gas scale

fourth power of temperature on ideal gas scale

square of temperature on ideal gas scale

According to the Stefan’s law the radiant energy emitted by a perfectly black body per unit area per second is directly proportional to the fourth power of its absolute temperature R∝T4 or R=σT4 where σ is a Stefan’s constant

According to the Stefan’s law the radiant energy emitted by a perfectly black body per unit area per second is directly proportional to the fourth power of its absolute temperature
$R \propto T^{4}$
or $R = σ T^{4}$
where $σ$ is a Stefan’s constant