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Galaxy formation from tepid inflation

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Abstract

It is argued that the primordial density fluctuations needed for galaxy formation may have been of thermal origin in a quasi-exponential state of inflation.

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Authors and Affiliations

  1. Central Research Institute for Physics, Budapest, Hungary

    B. Lukács

  2. Konkoly Observatory of the Hungarian Academy of Sciences, Budapest, Hungary

    G. Paál

Authors
  1. B. Lukács
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  2. G. Paál
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Lukács, B., Paál, G. Galaxy formation from tepid inflation. Astrophys Space Sci 146, 347–354 (1988). https://doi.org/10.1007/BF00637584

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  • DOI: https://doi.org/10.1007/BF00637584

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