Kirchhoff's law of thermal radiation/Infinitesimal volume

In summary, Kirchhoff's law of thermal radiation states that the ratio of emissive power to absorptive power in a body at thermal equilibrium is equal to the ratio of its emissivity to absorptivity. This law is closely related to the concept of blackbody radiation and is significant in thermodynamics as it helps us understand the relationship between a body's properties and its ability to absorb and emit radiation. Additionally, the law applies to all types of radiation and is related to the concept of entropy in the second law of thermodynamics.
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em3ry
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Is there a form of Kirchhoff's law of thermal radiation that applies to infinitesimal volumes rather than optical surfaces of materials?
 
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No, Kirchhoff's law of thermal radiation applies only to optical surfaces of materials and not to infinitesimal volumes. The law states that the ratio of the radiant exitance (or emittance) to the absorptance of a surface is equal to the emissivity of that surface. This means that the amount of radiation emitted by the surface is directly proportional to the amount of radiation absorbed by it.
 

Related to Kirchhoff's law of thermal radiation/Infinitesimal volume

1. What is Kirchhoff's law of thermal radiation?

Kirchhoff's law of thermal radiation states that the ratio of emissive power to absorptive power of a material at thermal equilibrium is constant and independent of temperature or wavelength.

2. How does Kirchhoff's law apply to infinitesimal volumes?

Kirchhoff's law can be applied to infinitesimal volumes by considering the emission and absorption of radiation within a small volume. The law states that the ratio of the emission and absorption coefficients for a given material will be the same for all wavelengths and temperatures within this volume.

3. What is the significance of Kirchhoff's law in thermal radiation studies?

Kirchhoff's law is significant in thermal radiation studies because it provides a fundamental understanding of the relationship between emission and absorption of radiation in materials. It allows for the prediction of thermal radiation behavior and can be used to design and optimize thermal systems.

4. How is Kirchhoff's law related to the Stefan-Boltzmann law?

Kirchhoff's law is related to the Stefan-Boltzmann law, which states that the total emissive power of a blackbody is proportional to the fourth power of its absolute temperature. This is because Kirchhoff's law states that the emissivity of a material is equal to its absorptivity, and a blackbody is a material with an emissivity and absorptivity of 1.

5. Are there any exceptions to Kirchhoff's law of thermal radiation?

While Kirchhoff's law is generally applicable to most materials, there are some exceptions. Some materials, such as selective surfaces, have different emissivity and absorptivity values for different wavelengths, violating the law. Additionally, Kirchhoff's law does not hold for non-equilibrium systems or for materials with strong electric or magnetic fields.

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