Version 1
: Received: 31 March 2024 / Approved: 1 April 2024 / Online: 2 April 2024 (15:44:00 CEST)
How to cite:
Haug, E.; Tatum, E. How a Thermodynamic Version of the Friedmann Equation Appears to Solve the Early Galaxy Formation Problem. Preprints2024, 2024040159. https://doi.org/10.20944/preprints202404.0159.v1
Haug, E.; Tatum, E. How a Thermodynamic Version of the Friedmann Equation Appears to Solve the Early Galaxy Formation Problem. Preprints 2024, 2024040159. https://doi.org/10.20944/preprints202404.0159.v1
Haug, E.; Tatum, E. How a Thermodynamic Version of the Friedmann Equation Appears to Solve the Early Galaxy Formation Problem. Preprints2024, 2024040159. https://doi.org/10.20944/preprints202404.0159.v1
APA Style
Haug, E., & Tatum, E. (2024). How a Thermodynamic Version of the Friedmann Equation Appears to Solve the Early Galaxy Formation Problem. Preprints. https://doi.org/10.20944/preprints202404.0159.v1
Chicago/Turabian Style
Haug, E. and Eugene Tatum. 2024 "How a Thermodynamic Version of the Friedmann Equation Appears to Solve the Early Galaxy Formation Problem" Preprints. https://doi.org/10.20944/preprints202404.0159.v1
Abstract
Based on our recent thermodynamic formulation of the Friedmann equation, we demon- strate how the age of the universe must be approximately 14.6 billion years. This is about 800 million years older than predicted by the Λ-CDM model and therefore greatly alleviates the early galaxy formation problem.
Copyright:
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.