Photons per Unit Volume (Quantum)

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SUMMARY

The discussion focuses on calculating the number of photons per unit volume in a blackbody within a specific wavelength interval, represented by the equation ρ(λ)dλ = (8πhc/λ⁵)(dλ/(e^(hc/(λKT)) - 1)). Participants clarify that this function defines the energy per unit volume in the infinitesimal wavelength interval dλ, and that integrating from 0 to ∞ is unnecessary for this specific calculation. The correct expression for the number of photons per unit volume is (8π/λ⁴)(dλ/(e^(hc/(λKT)) - 1)).

PREREQUISITES
  • Understanding of blackbody radiation and Planck's law
  • Familiarity with quantum mechanics concepts, particularly photon energy
  • Knowledge of calculus, specifically integration techniques
  • Basic grasp of thermodynamic principles related to temperature (T) and Boltzmann's constant (k)
NEXT STEPS
  • Study Planck's Law for blackbody radiation in detail
  • Learn about the derivation of the Stefan-Boltzmann Law
  • Explore applications of quantum mechanics in thermodynamics
  • Investigate the implications of photon statistics in different physical systems
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Students and researchers in physics, particularly those focusing on quantum mechanics, thermodynamics, and astrophysics, will benefit from this discussion.

trevor51590
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Homework Statement


\rho(\lambda)d\lambda=\frac{8(\pi)hc}{\lambda^{5}}\frac{d\lambda}{e^{hc/(\lambda)KT}-1}

What does this represent?
Calculate the number of photons per unit volume in a blackbody from \lambda to d\lambda


Homework Equations


N/A


The Attempt at a Solution


I believe this represents the energy per unit volume in wavelength \lambda to d\lambda. To calculate the number of photons per unit volume, would I just calculate

\int^{d\lambda}_{\lambda}\frac{8(\pi)hc}{\lambda^{5}}\frac{d\lambda}{e^{hc/(\lambda)KT}-1}? It seems pretty messy
 
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If rho is the energy per unit volume (and per unit frequency interval), then to get the number of photons per unit volume and per unit frequency interval, you'd have to divide by the energy per photon.

Also, you're thinking about the integral wrong. It doesn't make sense to have lambda and d(lambda) as limits in an integral, since the whole point of d(lambda) is that it represents an "infinitesimal" wavelength interval (it's not a number). You integrate once you want to get the change over some finite wavelength interval, like between lambda1 and lambda2. Conceptually, at least, this operation corresponds to adding up all the changes in all the little infinitesimal intervals within that finite wavelength range.
 
Using your hint I believe I need to integrate from 0→∞

\frac{8(\pi)hc}{\lambda^{5}}\frac{d\lambda}{e^{hc/(\lambda)KT}-1}\frac{\lambda}{hc}

I used E=\frac{hc}{\lambda} for the energy of a photon. My final integral appears to be

8\pi\int^{\infty}_{0}\frac{1}{\lambda^{4}}\frac{d\lambda}{e^{hc/(\lambda)KT}-1}

It appears to be a pretty messy integral. Am I on the right track?

Thank you!
 
trevor51590 said:
Using your hint I believe I need to integrate from 0→∞

\frac{8(\pi)hc}{\lambda^{5}}\frac{d\lambda}{e^{hc/(\lambda)KT}-1}\frac{\lambda}{hc}

I used E=\frac{hc}{\lambda} for the energy of a photon. My final integral appears to be

8\pi\int^{\infty}_{0}\frac{1}{\lambda^{4}}\frac{d\lambda}{e^{hc/(\lambda)KT}-1}

It appears to be a pretty messy integral. Am I on the right track?

Thank you!

I don't think you need to integrate at all. It only asks for the number of photons per volume in infinitesimal wavelength interval dλ, which is precisely what this function is defined to be. ρ(λ) is the energy per unit volume in the infinitesimal wavelength interval dλ.

If you integrated from 0 to ∞, you'd be finding the amount of energy (or number of photons) per unit volume due to photons at ALL POSSIBLE WAVELENGTHS, which is not what the question is asking.
 
I see what you're saying. Then the number of photons per volume in a black body from \lambda to d\lambda should be simply

\frac{8\pi}{\lambda^{4}}\frac{d\lambda}{e^{hc/(\lambda)KT}-1}?

It seems too easy though
 

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