Open AccessAbout Black Holes
Author(s) -
Sankar Palchoudhury
Publication year - 2021
Publication title -
international journal of fundamental physical sciences
Language(s) - English
Resource type - Journals
ISSN - 2231-8186
DOI - 10.14331/ijfps.2021.330144
Subject(s) - black hole (networking) , physics , radius , quiet , astrophysics , gravitational wave , gravitational field , field (mathematics) , gravitation , binary black hole , astronomy , pure mathematics , link state routing protocol , routing protocol , routing (electronic design automation) , computer security , mathematics , computer science , computer network
All kinds of waves occur for the disturbances in the quiet gravitational field. Different waves powered differently and propagated in the gravitational field. A black hole is the higher GFI (Gravitational Field Intensity) area. The rays do not possess, coming from a distant source when pass by the black holes, adequate strength to disturb in the higher GFI area of the black holes. Naturally, the rays take on a curve path as the provision in a circular area depends on the radius (distance), keeping distance according to the lower GFI area around the black holes’ centre.