Quantum Gravity and String Theory

   

The Thermodynamic Properties of Zero Oscillations of a Homogeneous Universe Are Specified

Authors: Miheeev Sergey Vladimirovich

It is shown that the share of zero-point oscillations ¾ in the energy of a homogeneous universe does not depend on the chosen shape factor. The temperature of zero-point oscillations is weak and indirectly depends on the shape factor, through the minimum wavelength. It is shown that the coefficient of the form must be taken equal to the classical value - 8π. At the same time, in a homogeneous universe with a gravitational radius of 4.4 × 1026 m, the temperature of zero-point oscillations is T = 2,76 K.

Comments: 5 Pages.

Download: PDF

Submission history

[v1] 2018-11-26 22:04:04

Unique-IP document downloads: 12 times

Vixra.org is a pre-print repository rather than a journal. Articles hosted may not yet have been verified by peer-review and should be treated as preliminary. In particular, anything that appears to include financial or legal advice or proposed medical treatments should be treated with due caution. Vixra.org will not be responsible for any consequences of actions that result from any form of use of any documents on this website.

Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.

comments powered by Disqus