Astrophysics

    

Investigation of the Gravitational Wave of the Binary Star System J0651+2844

Authors: Herbert Weidner

The binary star system J0651 is expected to be be one of the brightest sources of gravitational waves in our galaxy. Despite its known frequency, the radiation could not be detected so far. A new method eliminates the strong phase modulation caused by the Earth's orbit and drastically reduces the bandwidth. Therefore, the GW may be identified in the records of numerous superconducting gravimeters. The determined parameters of GW agree well with the results of previous observations in the optical domain and the predictions of relativity.

Comments: 12 Pages.

Download: PDF

Submission history

[v1] 2022-08-21 16:16:04

Unique-IP document downloads: 193 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