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Distortion of the Microwave Background by Dust from Population III

Published online by Cambridge University Press:  04 August 2017

Michael Rowan-Robinson*
Affiliation:
Queen Mary College, Mile End Road, London, E.1

Abstract

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Population III has been invoked to explain the missing mass in the haloes of galaxies, the first heavy elements in our Galaxy and even to explain the whole microwave background. However there are alternative explanations for each of these phenomena. The most compelling evidence for the existence of a pregalactic generation of objects is the observed distortion of the microwave background in the millimetre range, which can be explained as radiation from Population III objects absorbed and re-emitted by dust grains. If the distortion is confirmed, we can probably conclude that the density fluctuations in the early universe were isothermal and that no neutrino can have a mass in the astrophysically interesting range 1–100 eV.

Type
Research Article
Copyright
Copyright © Reidel 1983 

References

Barrow, J.D., & Turner, M.S., 1981, Nature 291, 469.CrossRefGoogle Scholar
Bond, J.R., Efstathiou, G., & Silk, J., 1980, Phys. Rev. Lett. 45, 1980.CrossRefGoogle Scholar
Carr, B.J., 1981, Mon. Not. R, Astr. Soc. 195, 669.CrossRefGoogle Scholar
Danese, L., & de Zotta, G., 1977, Riv. Nuovo Cim. 7, 277.CrossRefGoogle Scholar
Gush, H.P., 1981, Phys. Rev. Lett. 47, 745.CrossRefGoogle Scholar
Klapp, J., 1982, , Oxford Univ. Google Scholar
Nanopoulos, D., 1981, ‘Cosmology & Particles’, ed. Audouze, J. et al, p. 89.Google Scholar
Narlikar, J.V., Edmunds, M.G., & Wickramasinghe, N.C., 1976, ‘Far Infrared Astronomy’, ed. Rowan-Robinson, M. (Pergamon, Oxford), p. 131.Google Scholar
Negroponte, J., Rowan-Robinson, M. & Silk, J., 1981, Astrophs. J. 248, 38 CrossRefGoogle Scholar
Rana, N.C., 1981 Mon. Not. R. Astr. Soc. 197, 1125.CrossRefGoogle Scholar
Rees, M., 1978, Nature 275, 35.CrossRefGoogle Scholar
Rowan-Robinson, M., 1982, Varenna Summer School on ‘Gamov Cosmology’.Google Scholar
Rowan-Robinson, M., & Tarbet, P.J., 1982 ‘Progress in Cosmology’, ed. Wolfendale, A. (Reidel, Dordrecht) p. 101.CrossRefGoogle Scholar
Tarbet, P.J., & Rowan-Robinson, M. 1982, Nature (in press).Google Scholar
Truran, J.W., & Cameron, A.G.W., 1974, Astrophys. J. 190, 605.Google Scholar
White, S.D.M., & Rees, M.J., 1978, Mon. Not. R. Astro. Soc. 183, 347.CrossRefGoogle Scholar
Woody, D.P., & Richards, P.L., 1979, Phys. Rev. Lett. 42, 925.CrossRefGoogle Scholar
Woody, D.P., & Richards, P.L., Astrophys. J. 248, 18.CrossRefGoogle Scholar
Wright, E.L., 1982 Astrophys. J. 255, 401.CrossRefGoogle Scholar