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On the computation of optical properties of heterogeneous grains

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Abstract

The Maxwell-Garnet (MG) expression for the effective dielectric function of a composite medium consisting of small spherical inclusions embedded in a homogeneous matrix is derived. It is shown that the MG theory accounts for dipole-dipole interactions among the inclusions and that the validity of the theory does not depend on the matrix being non-absorbing. Moreover, by comparing the Mie theory with the MG theory it is shown that the MG dielectric function is correct at least to terms linear in the volume fraction of inclusions. For a sphere ‘carved out’ of such a medium we then have a prescription for calculating cross sections and scattering phase functions. The scattering properties of a small heterogeneous sphere described by the MG dielectric function are identical to those of a small layered sphere with the same outer radius and volumes of the two constituents. In the small particle (Rayleigh) limit we discuss two illustrative examples: (a) a porous sphere, (b) spherical inclusions in a ‘waxy’ dielectric matrix. In both cases we obtain the conditions for resonance absorption. Finally, we apply these results to evaluate the role of porosity in individual graphite grains, and of a waxy matrix containing small spherical graphite inclusion, on the graphite particle resonance absorption at 2200 Å. Increasing porosity and increasing the volume fraction of matrix material have similar effects in shifting the resonance to longer wavelengths.

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References

  • Abadi, H. and Wickramasinghe, N. C.: 1976,Astrophys. Space Sci. 39, L31.

    Google Scholar 

  • Abadi, H., Joshi, P., Ramadurai, S., and Wickramasinghe, N. C.: 1976,Nature 263, 214.

    Google Scholar 

  • Abelès, B. and Gittleman, J. I.: 1976,Appl. Opt. 15, 2328.

    Google Scholar 

  • Alfvén, H., and Mendis, D. A.: 1973,Nature 246, 410.

    Google Scholar 

  • Barker, A. S.: 1973,Phys. Rev. B7, 2507.

    Google Scholar 

  • Bless, R. C. and Savage, B. D.: 1972,Astrophys. J. 171, 293.

    Google Scholar 

  • Bohren, C. F. and Gilra, D. P.: 1977, in preparation.

  • Cohen, J. G.: 1973,Astrophys. J. 186, 149.

    Google Scholar 

  • de Groot, S. R.: 1969,The maxwell Equations, North-Holland, Amsterdam.

    Google Scholar 

  • Genzel, L.: 1974,Adv. Sol. State Phys. 14, 183.

    Google Scholar 

  • Genzel, L. and Martin, T. P.: 1972,Phys. Stat. Sol. B51, 91.

    Google Scholar 

  • Genzel, L. and Martin, T. P.: 1972,Surface Science 34, 33.

    Google Scholar 

  • Gilra, D. P.: 1972, in A. D. Code (ed.),The Scientific Results from the Orbiting Astronomical Observatory OAO-2, NASA-SP 310, p. 295.

  • Hoyle, F. and Wickramasinghe, N. C.: 1962,Monthly Notices Roy. Astron. Soc. 124, 417.

    Google Scholar 

  • Hoyle, F. and Wickramasinghe, N. C.: 1976,Nature,264, 45.

    Google Scholar 

  • Maxwell-Garnet, J. C.: 1904,Phil. Trans. Roy. Soc. A203, 385.

    Google Scholar 

  • Millman, P. M.: 1972, in A. Elvius (ed.), ‘From Plasma to Planet’,Nobel Symp. 21, 157.

    Google Scholar 

  • Ruppin, R. and Engelman, R.: 1970,Rep. Prog. Phys. 33, 149.

    Google Scholar 

  • Shah, G. A.: 1976,Bull. Astron. Soc. India 4, 20.

    Google Scholar 

  • Soifer, B. T., Russell, R. W., and Merrill, K. M.: 1976,Astrophys. J. 210, 334.

    Google Scholar 

  • Stroud, D.: 1975,Phys. Rev. B12, 3368.

    Google Scholar 

  • Taft, E. A. and Philipp, H. R.: 1965,Phys. Rev. 138, A197.

    Google Scholar 

  • Unsöld, A.: 1964,Publ. Roy. Obs. Edinburgh 4, 35.

    Google Scholar 

  • van de Hulst, H. C.: 1946,Rech. Astron. Obs. Utrecht 11, pt. 1.

    Google Scholar 

  • van de Hulst, H. C.: 1949,Rech. Astron. Obs. Utrecht 11, pt. 2.

    Google Scholar 

  • van de Hulst, H. C.: 1957,Light Scattering by Small Particles, Wiley, New York.

    Google Scholar 

  • Wasson, J. T.: 1974,Meteorites, Springer-Verlag, New York.

    Google Scholar 

  • Wickramasinghe, N. C., Ireland, J. G., Nandy, K., Seddon, H., and Wolstencroft, R. D.: 1968,Nature 217, 412.

    Google Scholar 

  • Wickramasinghe, N. C.: 1973,Light Scattering Functions for Small Particles, Adam Hilger, London.

    Google Scholar 

  • Woolf, H. J.: 1973, in J. M. Greenberg and H. C. van de Hulst (eds), ‘Interstellar Dust and Related Topics’,IAU Symp. 52, 485.

    Google Scholar 

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Bohren, C.F., Wickramasinghe, N.C. On the computation of optical properties of heterogeneous grains. Astrophys Space Sci 50, 461–472 (1977). https://doi.org/10.1007/BF00641750

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