Applied Physics, Vol. 1, Issue 1, Jul  2018, Pages 12-20; DOI: 10.31058/j.ap.2018.11002 10.31058/j.ap.2018.11002

A Square-Root Approach for Cosmic Temperature Evolution in the Early Formation of Stars in the Young Universe

Applied Physics, Vol. 1, Issue 1, Jul  2018, Pages 12-20.

DOI: 10.31058/j.ap.2018.11002

Johann Michael Köhler 1*

1 Techn. Univ. Ilmenau, Institute for Micro- Und Nanotechnologies/Institute for Chemistry and Microreaction Technology, Dept. Phys. Chem. and Microreaction Technology, Ilmenau, Germany

Received: 21 June 2018; Accepted: 12 July 2018; Published: 27 July 2018

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Abstract

In this paper, a simple approach for general temperature decay function in the early phase of cosmic evolution is studied. New findings on the age of early developed galaxies demand for a re-thinking of the fate of young universe. The square-root scenario is compatible with an early aggregation of masses and an early beginning of the formation of galaxies and stars.

Keywords

Early Developed Galaxies, Young Universe, Linearly Increasing Energy, Square-Root Scenario, Formation of Galaxies and Stars

Copyright

© 2017 by the authors. Licensee International Technology and Science Press Limited. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

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