How Does Particle Size Influence Emissivity in Circumstellar Dust?

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    Dust Emissivity
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Discussion Overview

The discussion centers around the influence of particle size on the emissivity of circumstellar dust, particularly in relation to the relationship between visual and infrared emissivity. Participants explore the physical justification for the expression involving the particle radius and its connection to blackbody radiation and emissivity.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • One participant references a 1984 paper discussing the condition that the ratio of visual to infrared emissivity must be near unity for the dust shell model to be consistent with observations.
  • The same participant questions the origin and physical justification of the expression ##\lambda_p / 2\pi## in relation to particle size and emissivity.
  • Another participant suggests consulting the latest Planck mission results for relevant information on dust properties.
  • A different participant expresses difficulty in navigating the extensive Planck publications and requests specific references related to the original question.
  • One participant provides a link to a paper titled "Astrophysics of Dust in Cold Clouds" as a potential resource for further research.
  • The original poster acknowledges the helpfulness of the provided article but feels there is a fundamental aspect they are missing regarding the topic.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the specific origin of the expression or its implications, and multiple viewpoints regarding the relevance of available resources remain. The discussion is ongoing and unresolved.

Contextual Notes

Participants express uncertainty about the foundational concepts related to emissivity and blackbody radiation, indicating potential gaps in understanding that are not fully addressed in the discussion.

robotopia
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In this 1984 paper on circumstellar dust, the author says, speaking of the emissivity/absorption of dust grains at visual and infrared wavelengths:
The dust shell model is consistent with the observed shape of the [IR] excess and the observed size of the ##60 \, \mu \text{m}## source, provided that ##(\varepsilon_\text{vis}/\varepsilon_\text{IR})## is near unity. Since ##\varepsilon_\text{vis}## for most material is near unity... it follows that ##\varepsilon_\text{IR}## also has to be near unity. This condition will normally be satisfied if the particle radius, ##a##, is comparable to or larger than ##\lambda_p / 2\pi##, where ##\lambda_p## is the wavelength of the peak emission.

My question is: where did the expression ##\lambda_p / 2\pi## come from, and what is the physical justification for it? I understand that small objects whose size is comparable to the wavelength of the incident light can't be resolved by that light, but what does that have to do with blackbody radiation and emissivity?
 
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Read the latest Planck mission results. They have some good information on this.
 
Planck Mission results seem vast...

Thanks, Chronos, for the reply.

I made my way to http://www.sciops.esa.int/index.php?project=PLANCK&page=Planck_Published_Papers, tried to find something specifically relating to my question, and failed, feeling overwhelmed by the sheer amount of their publications. I can see that the Planck Mission is obviously very concerned with dust and its properties, and I'm sure the answer is buried in there somewhere, but in the meantime, is there a specific paper, or webpage that you could send me a link for?
 
I too could find nothing specifically relevant to your question. I took the liberty of doing some additional research and came up with this: Astrophysics of Dust in Cold Clouds, http://arxiv.org/abs/astro-ph/0304488. Hope that helps
 
Thanks again, Chronos. The article is helpful, but will require more careful reading to find the answer I'm looking for. I feel as though there's something basic that I'm missing, but I can't quite put my finger on it.
I'll post again if I have any luck.
 

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