Proving Maclaurin Series for 1st Law of Blackbody Radiation

In summary, the Maclaurin series for the 1st Law of Blackbody Radiation is an infinite series representation of the relationship between the intensity of radiation emitted by a blackbody and its temperature. It is derived using Taylor series expansion and has numerous applications in physics and engineering. However, there are limitations to its use, as it is an approximation and assumes a perfect emitter. The series can also be extended to higher orders for a more accurate representation, but this increases the complexity of the equation.
  • #1
Pietervv
6
0
My homework question is about the first law of blackbody radiation. I have to prove an expansion when
for KT≫ℏw.
After some rewriting of the formula i have (ex-1)-1

because KT≫ℏw, x is close to zero, so i think i should use the maclaurin series.

According Wolfram Alpha the series expansion is [PLAIN]http://www5b.wolframalpha.com/Calculate/MSP/MSP32441h2h6354114hd8ba00002hih32dh1h5ch337?MSPStoreType=image/gif&s=14&w=174.&h=59. and this is exactly what i have to prove. But i have no idea how to come here. I tried to use all my knowledge but i don't even come close to the expansion that it should be...

So my question is: what are the steps from (ex-1)-1 to [PLAIN]http://www5b.wolframalpha.com/Calculate/MSP/MSP32441h2h6354114hd8ba00002hih32dh1h5ch337?MSPStoreType=image/gif&s=14&w=174.&h=59.
 
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  • #2
Pietervv said:
My homework question is about the first law of blackbody radiation. I have to prove an expansion when
for KT≫ℏw.
After some rewriting of the formula i have (ex-1)-1


because KT≫ℏw, x is close to zero, so i think i should use the maclaurin series.

According Wolfram Alpha the series expansion is [PLAIN]http://www5b.wolframalpha.com/Calculate/MSP/MSP32441h2h6354114hd8ba00002hih32dh1h5ch337?MSPStoreType=image/gif&s=14&w=174.&h=59. and this is exactly what i have to prove. But i have no idea how to come here. I tried to use all my knowledge but i don't even come close to the expansion that it should be...

So my question is: what are the steps from (ex-1)-1 to [PLAIN]http://www5b.wolframalpha.com/Calculate/MSP/MSP32441h2h6354114hd8ba00002hih32dh1h5ch337?MSPStoreType=image/gif&s=14&w=174.&h=59.


First, find the expansion for ##e^x - 1##. Then think Binomial.
 
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  • #3
Pietervv said:
My homework question is about the first law of blackbody radiation. I have to prove an expansion when
for KT≫ℏw.
After some rewriting of the formula i have (ex-1)-1


because KT≫ℏw, x is close to zero, so i think i should use the maclaurin series.

According Wolfram Alpha the series expansion is [PLAIN]http://www5b.wolframalpha.com/Calculate/MSP/MSP32441h2h6354114hd8ba00002hih32dh1h5ch337?MSPStoreType=image/gif&s=14&w=174.&h=59. and this is exactly what i have to prove. But i have no idea how to come here. I tried to use all my knowledge but i don't even come close to the expansion that it should be...

So my question is: what are the steps from (ex-1)-1 to [PLAIN]http://www5b.wolframalpha.com/Calculate/MSP/MSP32441h2h6354114hd8ba00002hih32dh1h5ch337?MSPStoreType=image/gif&s=14&w=174.&h=59.
What do KT and ℏw have to do with (ex - 1)-1?

Per Physics Forums rules, homework questions need to be posted using the homework template, which includes a complete problem statement. I am locking this thread. Please start a new thread with the information that's needed.
 
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1. What is the Maclaurin series for the 1st Law of Blackbody Radiation?

The Maclaurin series for the 1st Law of Blackbody Radiation is an infinite series representation of the relationship between the intensity of radiation emitted by a blackbody and its temperature. It is given by the equation I = aT + bT^3 + cT^5 + ..., where I is the intensity, T is the temperature, and a, b, c, etc. are constants.

2. How is the Maclaurin series derived for the 1st Law of Blackbody Radiation?

The Maclaurin series for the 1st Law of Blackbody Radiation can be derived using Taylor series expansion, which is a method for expressing a function as an infinite sum of terms. The coefficients of the series are obtained by taking derivatives of the function at a specific point, in this case, the temperature of the blackbody.

3. What is the significance of the Maclaurin series for the 1st Law of Blackbody Radiation?

The Maclaurin series provides a mathematical representation of the 1st Law of Blackbody Radiation, which states that the intensity of radiation emitted by a blackbody is directly proportional to its temperature. This series allows for the prediction and calculation of the intensity of radiation at different temperatures, which has numerous applications in physics and engineering.

4. Are there any limitations to using the Maclaurin series for the 1st Law of Blackbody Radiation?

Yes, there are limitations to using the Maclaurin series for the 1st Law of Blackbody Radiation. Firstly, it is an approximation and becomes less accurate as the temperature increases. Additionally, it assumes that the blackbody is a perfect emitter, which is not always the case in real-world scenarios.

5. Can the Maclaurin series for the 1st Law of Blackbody Radiation be extended to higher orders?

Yes, the Maclaurin series for the 1st Law of Blackbody Radiation can be extended to higher orders by including more terms, such as T^7, T^9, etc. This results in a more accurate representation of the relationship between intensity and temperature, but also increases the complexity of the equation.

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