The inverse square law for point light sources inside an opaque medium

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Discussion Overview

The discussion revolves around the behavior of light emitted from a point source within an opaque medium, specifically how the radiant intensity changes with distance when accounting for a spatially varying absorption coefficient. Participants explore the mathematical formulation of this relationship, contrasting it with the well-known inverse square law applicable in a vacuum.

Discussion Character

  • Exploratory
  • Technical explanation
  • Mathematical reasoning

Main Points Raised

  • One participant, manuel, seeks to understand the general law for light intensity in an opaque medium, suggesting that the relationship will still depend on distance but will not follow the inverse square law.
  • Another participant proposes that the intensity is affected by both the inverse square law and the absorption per meter traveled.
  • A subsequent reply questions the validity of an effective absorption coefficient that incorporates the inverse square term, highlighting the inconsistency in an optically transparent medium.
  • Further clarification is provided that absorption is exponential with distance, in addition to the spreading loss associated with the inverse square law.
  • Another viewpoint suggests that in a vacuum, the total power remains constant across spherical shells, while in an opaque medium, the power decreases exponentially with distance, leading to a modified expression for power per unit area.
  • The original poster expresses gratitude for the insights, indicating a newfound understanding of the relationship between inverse square law and absorption in the medium.

Areas of Agreement / Disagreement

Participants present differing views on how to mathematically express the relationship between light intensity and distance in an opaque medium, with no consensus reached on a single formulation. The discussion remains unresolved regarding the precise nature of the relationship.

Contextual Notes

Participants reference the light transport equation and the role of the absorption coefficient, but the discussion does not resolve the assumptions or dependencies on specific definitions of the absorption coefficient across different scenarios.

mgamito
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Hello all,

I already know that the radiant intensity of a point light source falls off with the inverse square of the distance to the source. This, however, only happens in a vacuum. My question is, what is the more general law for a point source inside an opaque medium with a known absorption coefficient σ(x) that may vary across space. From symmetry considerations alone, I would expect that the result will still be a function only of the distance to the light source, as before, just not an inverse square power anymore. The actual function will, of course, depend on σ(x) and should be the outcome of some 1D differential equation whose control variable is the distance to the source - it is the form of this 1D equation that I am looking for.

To clarify a bit further, the above absorption coefficient occurs in the light transport equation when stating that the derivative of radiance L(t) along a light ray parameterised by t is:

dL(t)/dt = -σ(t) L(t)

or stating the same in 3D space:

(ω.∇) L(x, ω) = -σ(x) L(x, ω)

where L(x, ω) is the radiance at point x in the direction ω.

Thank you,
manuel
 
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Both factors apply. The inverse square plus (or, rather, multiplied by) the absorption per metre travelled.
 
Hi Sophie, you mean that there is an effective absorption coefficient given by σ(t)/t^2 ? I don't see how that would work because in an optically transparent medium (σ = 0), the inverse square term would vanish together with the σ, which we know is not true.

manuel
 
Absorption PER METRE. It's exponential with distance (in addition to the spreading loss).
 
Better way to look at it, perhaps, is that in vacuum, the total power of the radiation passing through a spherical shell around a point source is a constant regardless of shell radius. This gives you inverse square per unit area. In opaque medium, the total power drops of as exp(-λr). Therefore, power per unit area drops as exp(-λr)/r²
 
Thank you both - I understand it now. I didn't imagine the solution was so simple as to just multiply the inverse square with the absorption (after application of the exponential to the latter).
 

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