Relativity and Cosmology

    

Limitations of Possibility to Detect Gravitational Waves Caused by Gravitational Barrier

Authors: Miroslav Súkeník, Jozef Šima

Modern detectors intended to detect gravitational waves are in function from 2002. Their figure of merith has reached h = 10‒21 from 2007 approaching current values h = 10‒23. Given the number of existing detectors, several hundreds of events involving gravitational waves should be registered to the present day. In reality, there is no one such an event, in spite of the fact that the existence of gravitationa waves has been evidenced indirectly through the binary pulsar PSR 1913+16. One of the modes of explanation the given state lies in a presumption that due to a non-stationary gravitational field, gravitational radiation is formed creating a barrier for gravitational waves detection. Based on our Expansive Nondecelerative Universe model we declare that only extremely strong sources exceeding the limiting value h = 10‒16 may be detected.

Comments: 3 Pages.

Download: PDF

Submission history

[v1] 2014-11-30 11:27:31

Unique-IP document downloads: 283 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