Linearizing Stefan-Boltzmann equation

In summary, the goal of this problem is to linearize both the Stefan-Boltzmann equation and the adiabatic relation in order to find a relationship between δL/L(0) and δR/R(0). Using a Taylor Expansion, the equations are simplified to δL/L(0) = (2δR/R(0)) + (4δT/T(0)), which can be used to solve the problem.
  • #1
J_I_F
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Homework Statement


I want to linearize both the Stefan-Boltzmann equation and the adiabatic relation to draw a relationship between δL/L(0) and δR/R(0).


Homework Equations


Stefan-Boltzmann equation in the form of L=4πσ(R^2)(T^4)
Adiabatic relation TV^(γ-1) = constant


The Attempt at a Solution


I have L(0) + δL = 4πσ((R(0) + δR)^2)*((T(0) + δT)^4) for the S-B part, but don't know how to get it into this desired form:

δL/L(0) = (2δR/R(0)) + (4δT/T(0))
 
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  • #2
J_I_F said:
I have L(0) + δL = 4πσ((R(0) + δR)^2)*((T(0) + δT)^4)

δL/L(0) = (2δR/R(0)) + (4δT/T(0))

So you have:

[tex]L_0+\delta L=4\pi\sigma(R_0+\delta R)^2(T_0+\delta T)^4[/tex]

You will have to use a Taylor Expansion to expand the terms that can be considered very small. For example:

[tex](a+x)^4=a^4(1+\frac{x}{a})^4 \approx a^4(1+\frac{4x}{a})[/tex]

This only works when [tex]\frac{x}{a}[/tex] is very small compared to 1, as is the case in your example. If you're still having trouble, show your work and we can go from there.
 
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  • #3
That helped a bunch, thanks.
 

FAQ: Linearizing Stefan-Boltzmann equation

What is the Stefan-Boltzmann equation?

The Stefan-Boltzmann equation is a fundamental law of physics that describes the relationship between the temperature and the total energy radiated by a blackbody. It states that the total energy radiated per unit time by a blackbody is proportional to the fourth power of its absolute temperature.

Why is it important to linearize the Stefan-Boltzmann equation?

Linearizing the Stefan-Boltzmann equation is important because it allows us to simplify complex relationships between temperature and energy radiation into a linear equation, making it easier to analyze and manipulate mathematically.

How is the Stefan-Boltzmann equation linearized?

The Stefan-Boltzmann equation can be linearized by taking the natural logarithm of both sides, which transforms the fourth-power relationship into a linear relationship. This allows for easier interpretation and analysis of the data.

What are the applications of the linearized Stefan-Boltzmann equation?

The linearized Stefan-Boltzmann equation has many applications in fields such as astrophysics, thermodynamics, and materials science. It can be used to calculate the energy output of stars, predict the behavior of materials at high temperatures, and determine the efficiency of thermal systems.

Are there any limitations to the linearized Stefan-Boltzmann equation?

While the linearized Stefan-Boltzmann equation is a useful tool for many applications, it is only accurate for idealized blackbodies. Real-world objects may have different properties that can affect energy radiation, such as reflectivity and emissivity, which can lead to deviations from the linearized equation.

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