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Use Stefan's law to find the intensity of the cosmic background radiation emitted by the fireball of the Big Bang at a temperature of 2.81 K.

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Complete Question

Use Stefan's law to find the intensity of the cosmic background radiation emitted by the fireball of the Big Bang at a temperature of 2.81 K. Remember that Stefan's Law gives the Power (Watts) and Intensity is Power per unit Area (W/m2).

Answer:

The intensity is
I = 3.535 *10^(-6) \ W/m^2

Step-by-step explanation:

From the question we are told that

The temperature is
T = 2.81 \ K

Now According to Stefan's law


Power(P) = \sigma * A * T^4

Where
\sigma is the Stefan Boltzmann constant with value
\sigma = 5.67*10^(-8) m^2 \cdot kg \cdot s^(-2) K^(-1)

Now the intensity of the cosmic background radiation emitted according to the unit from the question is mathematically evaluated as


I = (P)/(A)

=>
I = (\sigma * A * T^4)/(A)

=>
I = \sigma * T^4

substituting values


I = 5.67 *10^(-8) * (2.81)^4


I = 3.535 *10^(-6) \ W/m^2

User Eric Pigeon
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