Astrophysics

    

Peeking under the Event Horizon

Authors: Francois Zinserling

It is shown mathematically with Newtonian physics that a particle or photon can exit from underneath the event horizon of a singularity or black hole, where it can be observed, even though it may never fully escape the gravitational field. The radius of the event horizon is only an observed effect, dependent on the distance of the observer from the singularity, where Rs (Schwarzchild radius) is the event horizon observed from a distance approaching infinity. We will show that it is possible for matter to exit from the event horizon, and be observed outside the event horizon, as has been observed in many instances. While we may not be able to observe objects under the event horizon, we may observe how objects nearer the event horizon are affected from within.

Comments: 11 Pages. To be presented at the ASSA symposium 24-27 September 2014

Download: PDF

Submission history

[v1] 2014-08-07 05:56:56

Unique-IP document downloads: 224 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