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Nature of Black Holes and Space-Time around Them

Author:

tavajoh, amir ali

Category:

Research Papers

Sub-Category:

Relativity Theory

Language:

English

Date Published:

January 29, 2017

File:

/Research Papers-Relativity Theory/Download/6768

Downloads:

755

Keywords:

General Relativity, Geodesic, Rafini-Weeler Diagram, Strange Stars, Einstein-Rosen Bridge, Schwarzschild’s Sphere, Ergo Sphere, Space-Time Curvature, Time Warp, Special Relativity, Mach’s Principle

Abstract:

Based on the Mach’s principle, black holes warp the space time in a way that geodesic for every object which is moving toward black hole starts to bend and object starts to rotate around the black hole. Even light cannot be able to escape from the strong gravitational field of black hole and all the light like paths will warp so as to fall farther to the hole. Before arriving to the Schwarzschild’s Sphere, object faces with length extension because of the difference between amount of tidal forces on the nearest and furthest points of object that take the object apart and after passing the Schwarzschild’s sphere, based on the Special relativity of Einstein, the parts of object face with length contraction. In comparison between strange stars and black holes we conclude that core of strange stars has a temperature and pressure not sufficient for up and down quarks and they turn into strange ones. However, in core of black holes, because of massive stars and hot gases falling into it, they are always in a high temperature and pressure. So they can be made up of up and down quarks. At the Ergo sphere Region of black hole, a particle that gets into it will divide into 2 pieces, one of them falls into the black hole and another gets out of the Schwarzschild sphere very fast and it’s called the black hole radiation....

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