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en/5.11.3.md
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| + | ### Statement | ||
| + | |||
| + | $5.11.3.$ [Insert the problem statement] | ||
| + | |||
| + | ### Solution | ||
| + | |||
| + | ### Statement | ||
| + | |||
| + | $5.11.3.$ Determine the energy density of thermal radiation in the cavity of a body with temperature $T$. The speed of light is $c = 3 \cdot 10^8 \text{ m/s}$. | ||
| + | |||
| + | ### Solution | ||
| + | |||
| + | The energy density of thermal radiation (equilibrium black-body radiation) in a cavity is related to the radiant emittance by the formula: | ||
| + | $$u = \frac{4\sigma}{c} T^4$$ | ||
| + | where: | ||
| + | * $\sigma = 5.67 \cdot 10^{-8} \text{ W/(m}^2 \cdot \text{K}^4\text{)}$ is the Stefan-Boltzmann constant, | ||
| + | * $c = 3 \cdot 10^8 \text{ m/s}$ is the speed of light, | ||
| + | * $T$ is the absolute temperature. | ||
| + | |||
| + | Let us substitute the numerical values of the constants to obtain the final calculation formula: | ||
| + | $$u = \frac{4 \cdot 5.67 \cdot 10^{-8}}{3 \cdot 10^8} T^4 = 7.56 \cdot 10^{-16} T^4 \text{ J/m}^3$$ | ||
| + | *(Note: the numerical coefficient $7.56 \cdot 10^{-16}$ itself has units of $\text{J}/(\text{m}^3 \cdot \text{K}^4)$).* | ||
| + | |||
| + | #### Answer | ||
| + | $u \approx 7.56 \cdot 10^{-16} T^4 \text{ J/m}^3$ | ||
| + | |||
| + | #### Answer | ||
| + | |||
| + | [Insert a concise answer or boxed result] | ||
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| ### Statement | |||
| $5.11.3.$ [Insert the problem statement] | |||
| ### Solution | |||
| ### Statement | |||
| $5.11.3.$ Determine the energy density of thermal radiation in the cavity of a body with temperature $T$. The speed of light is $c = 3 \cdot 10^8 \text{ m/s}$. | |||
| ### Solution | |||
| The energy density of thermal radiation (equilibrium black-body radiation) in a cavity is related to the radiant emittance by the formula: | |||
| $$u = \frac{4\sigma}{c} T^4$$ | |||
| where: | |||
| * $\sigma = 5.67 \cdot 10^{-8} \text{ W/(m}^2 \cdot \text{K}^4\text{)}$ is the Stefan-Boltzmann constant, | |||
| * $c = 3 \cdot 10^8 \text{ m/s}$ is the speed of light, | |||
| * $T$ is the absolute temperature. | |||
| Let us substitute the numerical values of the constants to obtain the final calculation formula: | |||
| $$u = \frac{4 \cdot 5.67 \cdot 10^{-8}}{3 \cdot 10^8} T^4 = 7.56 \cdot 10^{-16} T^4 \text{ J/m}^3$$ | |||
| *(Note: the numerical coefficient $7.56 \cdot 10^{-16}$ itself has units of $\text{J}/(\text{m}^3 \cdot \text{K}^4)$).* | |||
| #### Answer | |||
| $u \approx 7.56 \cdot 10^{-16} T^4 \text{ J/m}^3$ | |||
| #### Answer | |||
| [Insert a concise answer or boxed result] | |||