Relativity and Cosmology


Addressing Strength of GW Radiation Affected by Additional Dimensions

Authors: A. Beckwith

We examine whether gravitational waves would be generated during the initial phase, δ0 of the universe when triggered by changes in space-time geometry; i.e. We hope to find traces of the breakdown of the Entropy/QM space-time regime during δ0. In particular, we look at if higher dimensions affect the relative strength of ΩGW , and comment as to how this magnitude may affect opportunities for detection of GW from relic sources. In particular, we will explain the reason why GW O of the pre big bang model is so strong, up to 10 to the - 6 power, while the ΩGW of ordinary inflation is so weak. In relic conditions.

Comments: 15 pages, 3 tables, two figures.; Has arguments in simplified form as to what will be brought up for presentation by the author in rencontres de Moriond, in a GW symposium

Download: PDF

Submission history

[v1] 16 Mar 2011

Unique-IP document downloads: 75 times 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. 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