Integrating monochromatic luminosity to get total luminosity

In summary, the conversation is about integrating the monochromatic luminosity of a blackbody model star over all wavelengths to obtain an expression for the total luminosity. The given equations involve u-substitution and the definite integral of u^3/(e^u-1) from 0 to infinity. A mistake in the u-substitution results in a negative factor in the final expression for luminosity. This is corrected by properly substituting out the limits.
  • #1
btouellette
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Homework Statement



Integrate the monochromatic luminosity (of a blackbody model star) over all wavelengths to obtain an expression for the total luminosity. This is 3.14(a) from An Introduction to Modern Astrophysics 2e by Carroll and Ostlie.

Homework Equations



## L_\lambda d\lambda = \frac{8 \pi^2 R^2 h c^2 / \lambda^5}{e^{h c / \lambda k T} - 1} d\lambda ##

## \int_0^\infty \frac{u^3}{e^u - 1} \, du = \frac{\pi^4}{15} ##

The Attempt at a Solution



So we need to evaluate

## L = \int_0^\infty L_\lambda \, d\lambda = \int_0^\infty \frac{8 \pi^2 R^2 h c^2 / \lambda^5}{e^{h c / \lambda k T} - 1} \, d\lambda ##

## L = 8 \pi^2 R^2 h c^2 \int_0^\infty \frac{1}{\lambda^5 (e^{h c / \lambda k T} - 1)} \, d\lambda ##

Using u-substitution with

## u = \frac{hc}{\lambda k T} ##
## du = \frac{-hc}{\lambda^2 k T} d\lambda ##

results in

## L = 8 \pi^2 R^2 h c^2 \int_0^\infty \frac{1}{e^{h c / \lambda k T} - 1} \frac{1}{\lambda^5} \, d\lambda = 8 \pi^2 R^2 h c^2 \int_0^\infty \frac{1}{e^u - 1} \frac{u^3 k^3 T^3}{h^3 c^3} \frac{-k T}{h c} \, du ##

so that makes

## L = \frac{-8 \pi^2 R^2 k^4 T^4}{c^2 h^3} \int_0^\infty \frac{u^3}{e^u - 1} \, du ##

and using the definition of the definite integral from the givens we get

## L = \frac{-8 \pi^6 R^2 k^4 T^4}{15 c^2 h^3} ##

Everything here makes sense and is in agreement with the solution I've seen as well as the followup problems except for the negative factor. It also doesn't make much sense to have a negative luminosity in this context. I expect I've botched something small in the u-substitution but for the life of me I can't spot it.
 
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  • #2
btouellette said:

Homework Statement



Integrate the monochromatic luminosity (of a blackbody model star) over all wavelengths to obtain an expression for the total luminosity. This is 3.14(a) from An Introduction to Modern Astrophysics 2e by Carroll and Ostlie.

Homework Equations



## L_\lambda d\lambda = \frac{8 \pi^2 R^2 h c^2 / \lambda^5}{e^{h c / \lambda k T} - 1} d\lambda ##

## \int_0^\infty \frac{u^3}{e^u - 1} \, du = \frac{\pi^4}{15} ##

The Attempt at a Solution



So we need to evaluate

## L = \int_0^\infty L_\lambda \, d\lambda = \int_0^\infty \frac{8 \pi^2 R^2 h c^2 / \lambda^5}{e^{h c / \lambda k T} - 1} \, d\lambda ##

## L = 8 \pi^2 R^2 h c^2 \int_0^\infty \frac{1}{\lambda^5 (e^{h c / \lambda k T} - 1)} \, d\lambda ##

Using u-substitution with

## u = \frac{hc}{\lambda k T} ##
## du = \frac{-hc}{\lambda^2 k T} d\lambda ##

results in

## L = 8 \pi^2 R^2 h c^2 \int_0^\infty \frac{1}{e^{h c / \lambda k T} - 1} \frac{1}{\lambda^5} \, d\lambda = 8 \pi^2 R^2 h c^2 \int_0^\infty \frac{1}{e^u - 1} \frac{u^3 k^3 T^3}{h^3 c^3} \frac{-k T}{h c} \, du ##



Ignoring all the constants, you have an integral with limits ##\int_0^\infty## and a ## \frac 1 \lambda## and some other stuff in it. When you do a substitution like ##u = \frac 1 \lambda## and ##du = -\frac1 {\lambda^2}~d\lambda## and change the limits from ##\lambda## limits to ##u## limits, note that ##\lambda = 0## gives ##u = \infty## and ##\lambda = \infty## gives ##u=0##. So you have the ##u## limits reversed and that will fix your minus sign.
 
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  • #3
Thank you! That's it exactly, forgot that I have to substitute out the limits as well.
 

Related to Integrating monochromatic luminosity to get total luminosity

1. What is monochromatic luminosity?

Monochromatic luminosity refers to the amount of light radiated by an object at a specific wavelength, often measured in units of watts per square meter.

2. How is monochromatic luminosity different from total luminosity?

Total luminosity refers to the overall amount of light radiated by an object at all wavelengths, while monochromatic luminosity only refers to the amount of light at a specific wavelength.

3. Why is integrating monochromatic luminosity necessary to calculate total luminosity?

Integrating monochromatic luminosity allows us to account for the contributions of all wavelengths of light, as total luminosity takes into account the light emitted at all wavelengths.

4. What factors can affect the accuracy of integrating monochromatic luminosity?

The accuracy of integrating monochromatic luminosity can be affected by factors such as the distance of the object, the distribution of light within the object, and any absorption or scattering of light that may occur.

5. How is integrating monochromatic luminosity used in scientific research?

Integrating monochromatic luminosity is often used in research to study the properties of stars and galaxies, as well as to understand the processes that govern the emission of light from various astronomical objects.

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