Abstract
The hot-big-bang picture emerges from a FL model, where the expansion factor R (t) approaches zero towards the limit (t → 0) of the cosmic time t. The presence of a uniform radiation field implies a “hot” singularity, i.e. an ever-increasing temperature as t → 0. (This is true as long as the constituent particles of the radiation background can be treated as non-interacting. There are model theories of elementary particles where the interactions limit the temperature to a maximum, finite value, which is, however, large when compared with the energy scales discussed in this chapter; cf. also Chap. 7.)
“The present universe is something like the old professor nearing retirement with his brilliant future behind him.”
A. Sandage (1984)
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© 1993 Springer-Verlag Berlin Heidelberg
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Börner, G. (1993). Thermodynamics of the Early Universe in the Classical Hot-Big-Bang Picture. In: The Early Universe. Texts and Monographs in Physics. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-02918-3_3
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DOI: https://doi.org/10.1007/978-3-662-02918-3_3
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-56729-5
Online ISBN: 978-3-662-02918-3
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