Identifying the Spatial Structure of Black Hole and Tropical Cyclone Based on a Theoretical Analysis of Orthogonal Interaction

Abstract

Black holes are recognized by Newton’s gravitational theory and Einstein’s general relativity, but there is still a lack of understanding the spatial structure of events, especially the nature of event horizon. In this paper, a theoretical analysis is used to compare the structures of tropical cyclone in the atmosphere and black hole in the astronomy so that five results are: 1) Both of them share the similar spatial structure, with tropical cyclone and black hole having the outflow cloud shield and the horizon sphere in the central part, respectively, while four spiral material bands exist in the rotating plane around them; 2) In theoretically, the energy density formed by the orthogonal interaction of the four spiral material bands is as times as the total kinetic energy of the head-on interaction; 3) This region of high energy density can lead to the conversion from mass to energy and the creation of new physical states of matter, which is a black hole event; 4) The outer horizon of a black hole is the outermost interface of events, or the orthogonal interaction interface of particles; 5) High-speed plasma jets extended at the poles of the black hole are directly associated with the shear stress of orthogonal interaction.