Relativity and Cosmology


Source Signal Observability at Hyper Light Velocity

Authors: Harvey Scribner

Abstract—In [1] an observer at rest and perpendicular to moving source will detect a difference in the time of arrival of the initial τ0 and final τ' waves as τ' > τ0 a transverse relative time shift. The position of the observer in [1] for source velocities near the speed of light has the disadvantage of having to wait a long time to detect τ'. The observer cannot detect τ' for velocities equal to or greater than the speed of light. This work shows that moving the observer to a strategic position downstream from the τ' signal has the advantage of introducing observability of τ'. The transverse relative time shift formulas are derived for the stationary observer perpendicular to and also on the path axis for velocities less than and much greater than c. Also, a method to calculate transverse relative length is proposed.

Comments: 32 Pages. Version 2 includes Section IX - "The Meaning of Area K3"

Download: PDF

Submission history

[v1] 2019-01-23 01:08:16
[v2] 2019-02-10 19:49:31

Unique-IP document downloads: 48 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