Skip to main content
Log in

Rate of H2 formation on amorphous grains

  • Published:
Astrophysics and Space Science Aims and scope Submit manuscript

Abstract

The rate of formation of molecular hydrogen from hydrogen atoms adsorbed on grains is analyzed, assuming that the grains are single crystals, polycrystalline or amorphous. On polycrystalline grains, and on graphite platelets, this rate could be orders of magnitude lower than on single crystal grains. The same is true for amorphous grains because there, at low temperatures, only atoms absorbed on neighboring sites can form molecules. Suitable formulae are derived and compared with the classical results for single crystal grains. Quantitative results are given for crystalline and amorphous ice, but with small changes these should also be valid for other solids. The rates for amorphous grains can approximate, within a factor of 10 or so, those for crystalline grains if the density of H atoms is high and the density of H2 molecules is low and only when the temperature of the grains satisfies a relation which for ice and graphite leads to a value in the proximity of 15–17 K. This maximum rate occurs only a degree or so above the temperature at which the grains are totally covered by an H2 layer and the reaction ceases. Furthermore, for a constant number density of grains, the rates on amorphous grains are second order while those on crystalline grains are first order. Both these circumstances predict amorphous grains to lead to H2 clouds with irregular and sharply delineated features in contrast to more uniform clouds formed on crystalline grains.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Ainslie, N. C., Morelock, C. R., and Turnbull, D.: 1962, inSymposium on Nucleation and Crystallization in Glasses and Metals, Amer. Ceram. Soc., Columbus, Ohio, p. 97.

    Google Scholar 

  • Brownlee, D. E., Horz, F., Tomandl, D. A., and Hodge, P. W.: 1976,IAU Colloq. 25, 962.

    Google Scholar 

  • Czyzak, S. J. and Santiago, J. J.: 1973,Astrophys. Space Sci. 23, 443.

    Google Scholar 

  • Czyzak, S. J., Meese, J. M., and Santiago, J. J.: 1976,Astrophys. J. 207, 425.

    Google Scholar 

  • Draine, B. T.: 1979,Astrophys. Space Sci. 65, 313.

    Google Scholar 

  • Gilra, D. P.: 1972, NASA SP-310, p. 295.

  • Goodman, F. O.: 1978,Astrophys. J. 226, 87.

    Google Scholar 

  • Hollenbach, D. J. and Salpeter, E. E.: 1970,J. Chem. Phys. 53, 79.

    Google Scholar 

  • Hollenbach, D. J. and Salpeter, E. E.: 1971,Astrophys. J. 163, 155.

    Google Scholar 

  • Hollenbach, D. J., Werner, M. W., and Salpeter, E. E.: 1971,Astrophys. J. 163, 165.

    Google Scholar 

  • Jura, M.: 1974,Astrophys. J. 191, 375.

    Google Scholar 

  • Konnert, J. H. and Karle, J.: 1973,Acta Cryst. A29, 702.

    Google Scholar 

  • Mathis, J. S., Rumpl, W., and Nordsieck, K. N.: 1977,Astrophys. J. 217, 425.

    Google Scholar 

  • McLean, D.: 1957,Grain Boundaries in Metals, Clarendon Press, Oxford.

    Google Scholar 

  • Montroll, E. W. and Weiss, G. H.: 1965,J. Math. Phys. 6, 167.

    Google Scholar 

  • Mott, N. F.: 1969,Phil. Mag. 19, 835.

    Google Scholar 

  • Mott, N. F. and Davis, E. A.: 1979,Electronic Processes in Non-crystalline Materials, Clarendon Press. Oxford.

    Google Scholar 

  • Narten, A. H., Venkatesh, C. G., and Rice, S. A.: 1976,J. Chem. Phys. 64, 1106.

    Google Scholar 

  • Purcell, E. M.: 1976,Astrophys. J. 206, 685.

    Google Scholar 

  • Rosenstock, H. B.: 1980,J. Math. Phys. 21, 1643.

    Google Scholar 

  • Savage, B. D.: 1975,Astrophys. J. 199, 92.

    Google Scholar 

  • Smoluchowski, R.: 1952,Phys. Rev. 87, 482.

    Google Scholar 

  • Smoluchowski, R.: 1978,Science 201, 809.

    Google Scholar 

  • Smoluchowski, R.: 1979,Astrophys. Space Sci. 65, 29.

    Google Scholar 

  • Spitzer, L. and Cochran, W.: 1973,Astrophys. J. 186, L23.

    Google Scholar 

  • Stephens, J. R. and Russell, B. W.: 1979,Astrophys. J. 228, 780.

    Google Scholar 

  • Watson, W. D.: 1976,Rev. Mod. Phys. 48, 513.

    Google Scholar 

  • Watson, W. D. and Salpeter, E. E.: 1972,Astrophys. J. 174, 321.

    Google Scholar 

  • Willner, S. P., Puetter, R. C., Russell, R. W., and Soifer, B. T.: 1979,Astrophys. Space Sci. 65, 95.

    Google Scholar 

  • Ziman, J. M.: 1979,Models of disorder, Cambridge University Press, Cambridge.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Smoluchowski, R. Rate of H2 formation on amorphous grains. Astrophys Space Sci 75, 353–363 (1981). https://doi.org/10.1007/BF00648648

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00648648

Keywords

Navigation