A Possible Evolution of Black Holes by Using a Hydrodynamic Analogy

Author:

BERBENTE Corneliu1,BERBENTE Sorin2

Affiliation:

1. “POLITEHNICA” University of Bucharest, Faculty of Aerospace Engineering, Department of Aerospace Sciences “Elie Carafoli”, Str. Polizu 1-7, sector 1, 011061 Bucharest, Romania, berbente@yahoo.com

2. “POLITEHNICA” University of Bucharest, Faculty of Aerospace Engineering, Department of Aerospace Sciences “Elie Carafoli”, Str. Polizu 1-7, sector 1, 011061 Bucharest, Romania and INCAS – National Institute for Aerospace Research “Elie Carafoli”, B-dul Iuliu Maniu 220, 061126 Bucharest, Romania, berbente.sorin@incas.ro

Abstract

The creation of black holes starts with the implosion of a star after the fuel to power the thermonuclear reactions from inside was consumed. Then more and more mass is added until a critical value of the ratio mass/radius was obtained. This ratio contains the Schwarzschild radius, the general relativity being taken in consideration as well. Mainly, the definition of the black hole implies the impossibility of light to leave the black hole/ Essentially, the definition of a black hole implies that light cannot leave the black hole. In this paper, we show that the inability of HD-gravitons to leave a black holes will affect the black hole evolution. In this paper, we show that the inability of HD gravitons to leave a black hole will affect the evolution of the black hole.

Publisher

INCAS - National Institute for Aerospace Research Elie Carafoli

Subject

Aerospace Engineering,Control and Systems Engineering

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